Astronomical observation Books
Springer London Ltd Illustrated Dictionary of Practical Astronomy
Book SynopsisA unique dictionary of astronomy specifically written for practical amateur astronomers. In addition to definitions, it provides an invaluable reference source for terms, techniques, instruments, formulas and processes for practising observers, both amateur and professional. A special feature of this dictionary is extended definitions for many topics; they give sufficient information for many of the techniques and items of instrumentation to be used as well as understood. With over 200 illustrations and extensive appendices, this is an essential reference book for every astronomer.Trade ReviewFrom the reviews: "This publication is wide-ranging with over 1,800 entries and 273 illustrations. It also provides web addresses for relevant organizations … . There are extensive appendices including the Messier and Caldwell catalogues, relevant addresses of organizations and even the Greek alphabet. … it is undoubtedly an invaluable reference tool for the dedicated practical astronomer." (Sharon Hough, Astronomy & Space, April, 2004) "This book is primarily aimed at the practicing amateur observer. There is most certainly a need for a reference work of this sort, and the author has managed to go some way towards filling a glaring gap in the market. … this dictionary is a mandatory addition to the practical astronomer’s bookshelf." (T. J. Mahoney, The Observatory, Vol. 124 (1179), 2004) "It does an excellent job of covering the basics and many not so basic aspects of astronomy. In fact, it provides more depth than would be considered normal for a dictionary in most cases, and nicely bridges the gap between a pure dictionary and an encyclopaedia. … A worthwhile addition to one’s reference library … . for an advanced amateur, this might just be the eclectic mix for which they yearn." (Roger Feasey, Auckland Astronomical Society Journal, May, 2003) "The emphasis in this dictionary is very much on the word ‘practical’ contained in the title. … many practical astronomers will find the book useful. It deals in some detail with techniques and instrumentation, offering many useful charts and diagrams. … The book is well cross-referenced and includes a number of useful appendices. … The dictionary finishes with a listing of astronomical societies worldwide and a bibliography which covers major journals, yearbooks, star catalogues, reference books, introductory books on astronomy and practical guides." (L. J. Anthony, Reference Reviews, Vol. 17 (1), 2003)Table of ContentsA.- B.- C.- D.- E.- F.- G.- H.- I.- J.- K.- L.- M.- N.- O.- P.- Q.- R.- S.- T.- U.- V.- W.- X.- Y.- Z.
£44.99
Springer London Ltd The Continuing Story of The International Space Station
Book SynopsisIn this fascinating and well-written text Peter Bond describes the development and evolution of space stations. Particular emphasis is placed on the International Space Station, beginning with the revolution that began in 1970, when Salyut 1, the world's first space station was sent into orbit by the Soviet Union. Defeated in the race to the Moon, the Soviets redirected their efforts towards the conquest of near-Earth space. In the next three decades, their increasingly large and sophisticated structures rewrote the history books as cosmonauts continued to push back all space endurance records. In clear and concise language the book explains how the human exploitation of low-Earth orbit is about to change.Trade ReviewFrom the reviews: "This book describes the development and evolution of the idea and concept of space stations with the chief emphasis on the International Space Station. … This is the story of a truly monumental project, from the dream to the reality and can be recommended as useful contribution to general space history." (Spaceflight, Vol. 45 (12), 2003) "In his new book, Peter Bond takes the reader on an astonishing journey. … it portrays origin and development of the International Space Station. It is a story of both technological and intercultural achievement, turning the ISS into a challenging human outpost in space." (Science in Africa, October, 2002) "This book begins with a description of the ISS at the end of 2001 and a view of how it will look on completion sometime after 2006 … . The book is illustrated throughout … . There are three appendices … and there are also lists of interesting web sites and books. This is an interesting and easy-to-read account of the ISS, the people involved with it, and the many problems it has faced and will face in the future." (Helen Close, Astronomy & Space, February, 2003) "Now four years old, the International Space Station has yet to inspire much affection. … This extremely detailed yet readable reference book might cause people to think differently. With sheer accumulation of fact, Bond succeeds in spelling out the scale of achievement the … ISS really represents." (Sean Blair, Astronomy Now, January, 2003) "‘How can anyone make the endless saga of the International Space Station interesting?’ However, Peter Bond has done a pretty good job of telling this … story. … this is a good history of a complex programme, well illustrated and quite readable. There are several appendices … . Adding these to more than 330 pages of text, a reading list, and a selection of web-sites, this is a useful addition to the space enthusiast’s bookshelf." (John Davies, The Observatory, Vol. 122 (1172), 2003) "Expecting a catalogue of cold facts, I was pleasantly surprised to find this book written with feeling and at times, an undercurrent of humour. It is structured chronologically, but more so by topic allowing the subject matter to flow naturally. … The book both supplies answers I have not been able to find previously and is a record of the ISS up to the beginning of 2002. I thoroughly recommend it." (R. W. Evans, Southern Stars, September, 2002) "This book does an excellent job of looking back at the history of various space station projects, including the short-lived Skylab and the long-lived Mir, before detailing the science, politics, training and finance behind the current ISS. … the content carries it through, making it the definitive story of the ISS to date." (John Mather, Focus, August, 2002)Table of ContentsIntroduction.- Building a giant.- Space stations - from dream to reality.- Handshake in space.- Metamorphosis.- Coming and going.- Construction site in space.- Life on the space station.- Value for money?- Future uncertain.- Appendices: ISS Assembly November 1998 - December 2001.- Future Assembly Schedule.- Biographies of ISS resident crew members.
£31.34
Springer London Ltd The New Amateur Astronomer
Book SynopsisAmateur astronomy has changed beyond recognition in less than two decades. The reason is, of course, technology. Affordable high-quality telescopes, computer-controlled 'go to' mountings, autoguiders, CCD cameras, video, and (as always) computers and the Internet, are just a few of the advances that have revolutionized astronomy for the twenty-first century. Martin Mobberley first looks at the basics before going into an in-depth study of what’s available commercially. He then moves on to the revolutionary possibilities that are open to amateurs, from imaging, through spectroscopy and photometry, to patrolling for near-earth objects - the search for comets and asteroids that may come close to, or even hit, the earth. The New Amateur Astronomer is a road map of the new astronomy, equally suitable for newcomers who want an introduction, or old hands who need to keep abreast of innovations. From the reviews: "This is one of several dozen books in Patrick Moore's "Practical Astronomy" series. Amid this large family, Mobberley finds his niche: the beginning high-tech amateur. The book's first half discusses equipment: computer-driven telescopes, CCD cameras, imaging processing software, etc. This market is changing every bit as rapidly as the computer world, so these details will be current for only a year or two. The rest of the book offers an overview of scientific projects that serious amateurs are carrying out these days. Throughout, basic formulas and technical terms are provided as needed, without formal derivations. An appendix with useful references and Web sites is also included. Readers will need more than this book if they are considering a plunge into high-tech amateur astronomy, but it certainly will whet their appetites. Mobberley's most valuable advice will save the book's owner many times its cover price: buy a quality telescope from a reputable dealer and install it in a simple shelter so it can be used with as little set-up time as possible. A poor purchase choice and the hassle of setting up are why most fancy telescopes gather dust in their owners' dens. Summing Up: Highly recommended. General readers; lower- and upper-division undergraduates."( T. D. Oswalt, CHOICE, March 2005)Trade ReviewFrom the reviews: "The book … serves not only as an informative guide but also as a source of ideas and inspiration. … is a solid guide to high-tech amateur astronomy by an author who is better at explaining his subject matter than most people. The book is ideal for anyone who is attracted to the technical side … . It will also prove useful to those with some experience … . it offers a great snapshot depicting part of amateur astronomy’s culture today. It’s a refreshing and welcome addition to my bookshelf." (Jeff Medkeff, Sky & Telescope, July, 2005) "The New Amateur Astronomer reflects the change in technology that has taken place in the last ten years. Astronomers can now observe the skies on a PC monitor … . shows the possibilities that are open to amateurs and introduces some of them, their equipment, and their results." (Book News on the Internet, January 27, 2005) "This is a remarkable book. … The author is very well known to the amateur fraternity and has a wealth of experience of using the equipment he describes, and so is highly qualified to write this book, which is well illustrated … . there is more than enough here to guide you through making the correct choice, not just now, but for a few years into the future. Highly recommended." (Roger Pickard, The Observatory, Vol. 125 (1187), 2005) "This book is designed to help the amateur astronomer to choose his or her telescope, to get the best use out of this telescope, and to better define his or her field of astronomical observation. … reading this book was a pleasant experience because of the light writing style adopted by the author. I gladly recommend the book not only to amateur astronomers and their associates but also to physics teachers and to any man or woman who enjoys the beauty of the night sky." (Fernande Grandjean, Physicalia Magazine, Vol. 28 (1), 2006)Table of ContentsIntroduction - Why Amateur Astronomy?.- Part I - Equipment.- Optical Fundamentals.- Buying a Commercial Telescope.- Navigating the Rotating Spherical Sky.- ‘Go To’ Telescopes and Mountings.- Digicams and Video Astronomy.- Cooled CCD Cameras.- Image Processing Software.- Part II - The People.- CCD Planetary Imagers.- Supernova Discoverers.- Deep-sky Perfectionists.- Cataclysmic.- Variable Observers & Gamma Ray Burster Hunters.- Saving the World - Near Earth Object Chasers.-Armchair Comet Hunters.- Backyard Spectroscopists.- Appendix I
£28.49
Springer London Ltd Visual Astronomy in the Suburbs: A Guide to Spectacular Viewing
Book SynopsisThe only practical guide to observing truly spectacular astronomical objects from less than perfect locations. The only book to deal in depth with the application of image intensifiers to real-time astronomy. Gives advice on viewing objects, and on making realistic images by drawing or video. Includes extensive catalogs of spectacular objects that can be seen from suburban sites in both hemispheres. Trade ReviewFrom the reviews: "This book is clear, well laid out … and is divided into sections on equipment, techniques for seeing and results of actual observations and captured images. … It is good in what it sets out to do … ." (David Fox, Astronomy & Space, May, 2005) "In a series of ten chapters, the author describes how the Moon, planets and deep sky objects can be observed in real time by using a telescope equipped with auxiliary equipment designed to counteract the deleterious effects of light pollution. As the many excellent images in the book attest, it is now possible to enjoy the thrills of deep space exploration from the comfort of your urban backyard … . This book is a must buy for the city astronomer." (Neil English, Astronomy Now, May, 2004) "Visual Astronomy in the Suburbs is aimed squarely at today’s observer who is often confined to the rosy glow of city living. It is a comprehensive guide to getting the most out of your evenings under the stars. The book is dedicated purely to ‘real time’ observing. … is a fantastic companion to a good star atlas and should be considered an essential for today’s amateur who has to endure light pollution. … Buy the book and take your observing to the next level." (Cameron Jack, Southern Stars, Vol. 43 (1), March, 2004) "Because the whole gamut of observing is so huge, the author has restricted the content to ‘live’ visual observing only, and expressly visual observing from a typical light polluted suburban environment. … The author has very definite ideas about these subjects, and these are expressed clearly throughout. … this distinctive book remains full of great ideas and insight relevant to visual observers who are keen to use a bit of technology in support of their hobby/obsession, for observers at all locations." (Roger Feasey, AAS - Auckland Astronomical Society Journal, April, 2004) "Every backyard skygazer cherishes skies so dark they look deep, deep gray due to unresolved, faint starlight. But the reality for most of us is a suburban site full of compromises. California amateur astronomer Anthony Cooke has written a valuable book that accepts these limitations and shows how you can explore the heavens from home." (www.Astronomy.com, August, 2004)Table of ContentsPurpose and Fundamentals.- Practical Applications and Viewing Aids.- Techniques for Seeing.- to Drawings and Real Time Video.- The Moon.- The Planets.- Deep Space — Visual Impressions and Expectations: The Primary Catalog.- Second Viewing Catalog.- Supplementary Catalog for the Southern Hemisphere.- Postscript.
£26.59
Springer London Ltd Digital Astrophotography: The State of the Art
Book SynopsisProvides novice to accomplished amateur astronomers with a firm grounding in the basics and successful use of digital astrophotography. Provides examples of the best images, and gives readers hints and tips about how to get the best out of this extraordinary technology. Experts in CCD astronomy from North America and Europe have contributed to this book, illustrating their help and advice with many beautiful colour images – the book is in full color throughout. Techniques range from using simple webcams to highly technical aspects such as supernovae patrolling. Computer processing, stacking and image-enhancement are detailed, along with many hints and tips from the experts.Trade ReviewFrom the reviews: "This colourful book is yet another addition to the forty-strong library of ‘Patrick Moore’s Practical Astronomy Series’ produced by Springer. … it is a very interesting book and the colour illustrations are excellent and beautifully reproduced. Undoubtedly it will inspire many beginners to find out much more information about astronomical imaging." (Martin Mobberley, Astronomy Now, February, 2006) "This compendium by S&T contributing editor David Ratledge offers a mother lode of practical information for imaging neophytes, but expert sky shooters can pick up a lot of useful tips as well. Its 11 chapters are lavishly illustrated, often in color, and they cover a wide range of techniques … . Ratledge’s ambitious goal of covering ‘the state of art’ is laudable … ." (Edwin Aguirre, Sky & Telescope, March, 2008) "This is certainly a book to inspire. Ratledge has used many of the acknowledged experts in the field, each of whom has written a chapter on their own particular specialisation. … I can thoroughly recommend this book. Many excellent images are included and the reproduction in colour is very good. If you are new to digital imaging it will help you get started. If you are already an ‘expert’ it will inspire you to higher things … ." (Nick James, Journal of the British Astronomical Association, Vol. 116 (4), 2006)Table of ContentsPreface Introduction Section 1: Getting Started Afocal Photography with Digital Cameras An Introduction to Webcam Imaging Long Exposure Webcams and Image Stacking Techniques Deep-Sky Imaging with a Digital SLR Section 2: Getting Serious IRIS: Astronomical Image Processing Software High-Resolution Imaging of the Planets High-Resolution Color Imaging Out-Smarting Light Pollution Section 3: Advanced The Hybrid Image – A New Astro-imaging Philosophy Amateur Spectroscopy in the 21st Century Successful Patrolling for Supernovae
£20.90
Springer London Ltd The Moon and How to Observe It
Book SynopsisThis revolutionary new book is written for practical amateur astronomers who not only want to observe, but want to know the details of exactly what they are looking at. The Moon is the most commonly observed of all astronomical objects. This is the first book to deal equally with the Moon itself - its formation, geology, and history - as well as the practical aspects of observation. The concept of the book - and of the series - is to present an up-to-date detailed description of the Moon, including its origins, history, and geology (part one); and then (part two) to consider how best to observe and record it successfully using commercially-available equipment. The Moon and How to Observe It is a mine of information for all levels of amateur observers, from the beginner to the experienced Trade ReviewFrom the reviews: "Books on the Moon tend to be either photographic or cartographic collections, observing guides or text books … . This book conveniently provides elements of all three … . Production quality is very good, with high quality semi-gloss paper, 134 figures, many in colour. … These are followed with a glossary, a list of resources including organisations, internet resources and bibliography … . If you are looking for a lunar guide with some nice clear maps … you would be hard pressed to find better." (Roger Feasey, Journal of Auckland Astronomical, July, 2005) "Grego provides a refreshingly clear explanation of how the Moon’s surface and interior reached their present state … . The section comparing the Earth’s moon to the moons of the other planets in the Solar System is particularly interesting, leaving the reader with many easily remembered facts … . The book was obviously produced with great care. … this thoroughly up-to-date book may prove to be well suited for the intermediate amateur astronomer seeking more specialized knowledge of a timely subject." (Brian Chapel, The Observatory, Vol. 126 (1193), 2006) "The Moon and How to Observe It is the latest of Springer-Verlag’s Astronomers’ Observing Guides. Described as ‘an advanced handbook for students of the Moon’, it is in fact suitable for amateur astronomers of all levels, beginner as well as advanced. … The book is illustrated by about 100 photographs and drawings, many of them by Grego himself. … a detailed and up-to-date guide, ideal for the amateur astronomer who wishes to observe the Moon or simply learn more about it." (Brendan K Ward, Astronomy and Space, June, 2006) "Refreshingly, Peter Grego’s book explores every aspect of the Moon … . It also includes recent theories on the possibilities of the existence of lunar ice in deep polar craters. … Outline drawings, photographs and descriptions illustrate the lunar surface … . This publication would be a good addition to the library of anyone interested in the Moon." (Alan Wells, BBC SkyatNight, February, 2006) "The current crop range from scholarly discourses on lunar geology to popular tours of lunar features. Grego has attempted to include all of this and more in his book … . Grego does an excellent job of describing the wide range of features that are visible in moderate telescopes and he includes several interesting projects that will encourage beginners. … this discussion of the visual treats available to naked eye, binocular and telescopic workers is very valuable. … I would recommend this book … ." (Nick James, Journal of the British Astronomical Association, Vol. 116 (2), 2006)Table of ContentsIntroduction.- PART 1 - The Moon.- 1. The Moon’s origin.- 2. The Measure of the Moon 3. Worlds in comparison.- PART 2 - Observing the Moon.- 4. Observing and recording the Moon 5. Viewing the Moon with the Unaided Eye.- 6. Lunar showcase - a binocular tour.- 7. A Survey of the Moon’s Near Side.- 8. Advanced Lunar Research.- 9. Lunar Observer’s Equipment.- Glossary
£28.49
Springer London Ltd Double & Multiple Stars, and How to Observe Them
Book SynopsisWritten specially for practical amateur astronomers who not only want to observe, but want to know and understand the details of exactly what they are looking at. Presents an up-to-date detailed description of the objects, their physics and their evolution (part one); and then (part two) to consider how to observe and record them successfully. Delivers a wealth of information for all levels of amateur observers, from the beginner to the experienced; it is equally fascinating for practical astronomers, and also for those who simply want to find out more about these unusual star systems.Trade ReviewJames Mullaney's book Double and Multiple Stars and How to Observe Them exceeds what anyone has done with this topic before--by a whole qualitative level or two. Mullaney is one of the world's most experienced observers of double stars and "deep-sky objects." His writing is always clear, accurate and enthusiastic and this book is no exception. Double and Multiple Stars, along with Mullaney's other writings on the topic, may end up almost singlehandedly winning over a new generation of observers to the joy of double-star observing.—Fred Schaaf ...I can recommend Double and Multiple Stars and How to Observe Them to those who delight in seeing close points of light and those who can imagine the huge variety of suns they represent. —Leif J. Robinson, in Sky & Telescope, October 2006Table of ContentsPreface Acknowledgements PART 1 Introduction PART II Types of Double Stars Astrophysics of Double Stars Observing Techniques Tools of the Trade Observing Projects Double & Multiple Star Observing Lists Conclusion Appendices Index About the Author
£33.24
Springer London Ltd Visual Astronomy Under Dark Skies: A New Approach to Observing Deep Space
Book SynopsisProvide the reader with everything he needs to know about what to observe, and using some of today’s state-of-the-art technique and commercial equipment, how to get superb views of faint and distant astronomical objects.Only guide to live observation of deep space, utilizing modern image enhancement techniques (image intensifiers and CCD video monitors) Detailed information supplied on the image intensifiers and CCD video monitors Explains how to select and prepare sites for live viewing. Trade ReviewCooke is full of great ideas and insight relevant to visual observers who are keen to use a bit of technology in support of their hobby / obsession, for observers at all locations. Highly recommended for visual observers who want to push their eyeball observing to the limit. --Roger Feasey, in the Journal of the Auckland Astronomical SocietyTable of ContentsForeword Introduction New tools The Dark Sky Site So, what can we expect to see? Our Neighbourhood in Space: The Milky Way The Great Beyond Eyes on the Future Appendices Recommended equipment manufacturers Resources Real Time visual astronomy using image intensifiers and data modelling StellaCam II Highlights and Description Index
£28.49
Springer Nature Switzerland AG High Energy Cosmic Rays
Book SynopsisOffers an accessible text and reference (a cosmic-ray manual) for graduate students entering the field and high-energy astrophysicists will find this an accessible cosmic-ray manual Easy to read for the general astronomer, the first part describes the standard model of cosmic rays based on our understanding of modern particle physics. Presents the acceleration scenario in some detail in supernovae explosions as well as in the passage of cosmic rays through the Galaxy. Compares experimental data in the atmosphere as well as underground are compared with theoretical modelsTable of Contents Overview Part I:The Standard Model of Cosmic Rays.- Cosmic ray interactions.- The birth of cosmic rays.- Cosmic rays in the Galaxy.- Cosmic rays at the top of the atmosphere.- Cosmic rays in the atmosphere.- Cosmic rays underground.- Part II Contemporary Challenges.- Cosmic ray showers.- The end of the cosmic ray spectrum.- High energy neutrino and gamma-ray astronomy. Appendix References Index
£94.99
Springer Nature Switzerland AG Our Place in the Universe - II: The Scientific
Book SynopsisStarting from Newton’s times this follow-up to the author’s Springer book “Our Place in the Universe - Understanding Fundamental Astronomy from Ancient Discoveries” addresses the question of “our place in the Universe” from astronomical, physical, chemical, biological, philosophical and social perspectives.Using the history of astronomy to illustrate the process of discovery, the emphasis is on the description of the process of how we learned and on the exploration of the impacts of discoveries rather than on the presentation of facts. Thus readers are informed of the influence of science on a broad scale.Unlike the traditional way of teaching science, in this book, the author begins by describing the observations and then discusses various attempts to find answers (including unsuccessful ones). The goal is to help students develop a better appreciation of the scientific process and learn from this process to tackle real-life problems.Trade Review“My overall impression is of a very carefully organized book in which clear explanations are seen as the key to understanding the process by which scientific discoveries are made. ... this book is a mostly excellent, carefully constructed, step-by-step educational path through the development of the process of doing science and resulting discoveries. Sun Kwok’s book provides an all-embracing view of how science has enabled a detailed description of our place in the Universe ... .” (Barry Kent, The Observatory, Vol. 142 (1291), December, 2022)Table of ContentsFrom Copernicus to Enlightenment.- Empirical Evidence for the Heliocentric Model.- Resolution of the Theoretical Objections to the Heliocentric Theory.- Size of the Solar System.- Celestial Navigation and Exploration of the Heavens.- New Members of the Solar System.- Is the Sun a Star?.- A New Way of Thinking.- What Are Stars Made of?.- Origin of the Solar System.- Plurality of the World.- The Nature of Nebulae.- Are all Motions Relative?.- The Nature of Light and Matter.- The Human Star Connection.- Is the Universe Finite?.- Early History of the Earth.- Common Ancestors.- Origin of Life.- Complexity in the Universe.- Evolution of the Earth through the Ages.- Earth as an Integrated System.- Life Cycles of Stars.- Life in other Worlds.- Our Place in the Universe.- The Common Link in Our Journey.- Further Reading.- Appendix I: Brightest Stars in the Sky.- Appendix II: Units of Measurement.- Appendix III: Astronomical Measurements.- Appendix IV: Photometric Method to Estimate the Distances of Stars.- Appendix V: Mass of the Milky Way.- Appendix VI: Examples of Inertial Forces.- Appendix VII: Astronomy from other Planetary Systems.- Review Exercises.- Glossary.
£23.74
Springer Radio Astronomy in Canada
£123.49
Springer DataIntensive Radio Astronomy
Book SynopsisPreface.- Introduction - Concepts and challenges of data-intensive radio astronomy.- Part 1. DATA CREATION, STORAGE AND ARCHIVES.- CHAPTER 1: From the data generation to the archive.- CHAPTER 2: Storage and archives.- CHAPTER 3: Computing infrastructure.- Part 2. DATA PROCESSING.- CHAPTER 4: Challenges of radio data processing (big radio data processing).- CHAPTER 5: Implementations for specific radio observatories.- CHAPTER 6: Co-design and software architecture.- CHAPTER 7: Lesson learned from SKA pathfinders regarding processing.- PART 3. POST-PROCESSING AND DATA ANALYSIS.- CHAPTER 8: Continuum Source extraction and identification.- CHAPTER 9: Other types of source extraction and identification.- CHAPTER 10: Using AI for radio (big) data.- CHAPTER 11: Visualisation for analysis.- PART 4. DATA ACCESS AND REUSE (accessibility, VR/VO FAIR).- CHAPTER 12: Exploitation platforms & Virtual Observatory.- CHAPTER 14: Data documentation beyond provenance: metadata, Research Data Management (RDM), FAIR.- Epilogue and future outlook.- Glossary.- Index.
£113.99
Springer Comete
Book SynopsisIntroduzione.- Cos'è e come è fatta una cometa.- Le tappe fondamentali della ricerca.- Le comete nell'antichità.- Dal medioevo all'illuminismo.- Arriva Edmond Halley.- Comete famose.- La cometa di Halley.- Comete interessanti del nostro secolo.- Come si osservano e come si scoprono.- Denominazioni e sigle.- Nascita e orbite.- Le comete visitate dalle sonde.- Incontri ravvicinati e rischi di impatto con la Terra.- Glossario.- Personaggi importanti nel campo delle comete.
£23.99
Springer International Publishing AG Astrophotography on the Go: Using Short Exposures with Light Mounts
Book SynopsisNo longer are heavy, sturdy, expensive mounts and tripods required to photograph deep space. With today's advances in technology, all that is required is an entry-DSLR and an entry level GoTo telescope. Here is all of the information needed to start photographing the night sky without buying expensive tracking mounts. By using multiple short exposures and combining them with mostly ‘freeware’ computer programs, the effect of image rotation can be minimized to a point where it is undetectable in normal astrophotography, even for a deep-sky object such as a galaxy or nebula. All the processes, techniques, and equipment needed to use inexpensive, lightweight altazimuth and equatorial mounts and very short exposures photography to image deep space objects are explained, step-by-step, in full detail, supported by clear, easy to understand graphics and photographs.Currently available lightweight mounts and tripods are identified and examined from an economic versus capability perspective to help users determine what camera, telescope, and mount is the best fit for them. A similar analysis is presented for entry-level telescopes and mounts sold as bundled packages by the telescope manufacturers. This book lifts the veil of mystery from the creation of deep space photographs and makes astrophotography affordable and accessible to most amateur astronomers.Table of ContentsIntroduction.- Short Review of Astronomy Basics.- Planetary and Lunar Imaging.- Very Short Exposure Astrophotography.- Computers.- Lightweight Altzimuth and Equatorial Mount Economics.- Altazimuth Astrophotography System.- Chapter 8: Astrophotography with a Lightweight Equatorial Mount.- Piggy-back Photography.- Astrophotography in Light-polluted Urban Areas.- DeepSky Stacker.- Processing Very Short Exposures.- Objects in the Night Sky to Photograph.- Portable Observatories.- How to Get 45 to 90 Second Exposures with a 4/5SE Mount.- How to Strengthen Tripods.- Index.
£39.99
Springer International Publishing AG Astronomical Discoveries You Can Make, Too!: Replicating the Work of the Great Observers
Book SynopsisYou too can follow in the steps of the great astronomers such as Hipparchus, Galileo, Kepler and Hubble, who all contributed so much to our modern understanding of the cosmos. This book gives the student oramateur astronomer the following tools to replicate some of these seminal observations from their own homes: With your own eyes: Use your own observations and measurements to discover and confirm the phenomena of the seasons, the analemma and the equation of time, the logic behind celestial coordinates, and even the precession of the equinoxes. With a consumer-grade digital camera: Record the changing brightness of an eclipsing binary star and show that a pulsating star changes color as it brightens and dims. Add an inexpensive diffraction grating to your camera and see the variety of spectral features in the stars, and demonstrate that the Sun’s spectrum is similar to one particular type of stellar spectrum. With a backyard telescope: Add a CCD imager and you can measure the scale of the Solar System and the distance to a nearby star. You could even measure the distance to another galaxy and observe the cosmological redshift of the expanding universe. Astronomical Discoveries You Can Make, Too! doesn’t just tell you about the development of astronomy; it shows you how to discover for yourself the essential features of the universe.Trade Review“This is one of the most genuinely exciting new astronomy books I’ve seen in a long time. It shows you, for example, how you can use Galileo’s method to work out the height of mountains on the moon. … The time commitment and equipment requirements for each project are well set out, and the projects are well explained. … this book a treat for the armchair astronomer, but a real treasure trove for a team of committed explorers.” (Andy Sawers, Astronomy Now, February, 2016)Table of ContentsMotions and Positions in the Sky.- The Moon.- The Planets.- The Stars.- Astrophysics and Cosmology.- Appendices.
£43.29
Springer International Publishing AG The Physical Processes and Observing Techniques of Radio Astronomy: An Introduction
Book SynopsisThis is a textbook for undergraduate courses on radio astronomy. Written by an active professor and researcher in the field, it begins by explaining why conducting observations at radio frequencies is so important, then reviews essential physics concepts corresponding to a sophomore-level curriculum or higher. Next, the book introduces students to single dish telescopes and interferometers. The most commonly encountered emission mechanisms seen in radio astronomy are then explained, along with examples of astronomical sources broadly divided into the types of sources seen in galactic and extragalactic observations. Each chapter provides examples and exercises suitable for homework assignments. Also included is an appendix of useful supplementary material. Altogether, the book is a comprehensive, yet digestible starting point for physics and astronomy undergraduates looking to understand the basics of radio astronomy.Trade Review“Radio astronomy is increasingly accessible as part of the undergraduate teaching curriculum, both as a practical activity and as part of the broader study of astrophysics. … it is well illustrated with colour figures, has a good set of sample problems with answers … . For those looking for a short one-volume text, it is certainly worth considering.” (Martin Hardcastle, The Observatory, Vol. 141 (1284), October, 2021)Table of ContentsChapter1. Introduction: Why Make Observations at Radio Frequencies?.- Chapter2. Angles, Gravity, Light, The Bohr Model of the Atom and Relativity.- Chapter3. Emission Mechanisms: Blackbody Radiation, An Introduction to Radiative Transfer, Synchrotron Radiation, Thermal Bremsstrahlung and Molecular Transitions.- Chapter4. Radio Observations: An Introduction to Fourier Transforms, Observing Through Earth’s Atmosphere, Single Dish Telescopes and Interferometers.- Chapter5. Solar System Radio Astronomy: The Sun, The Planets, The Moon and Minor Bodies.- Chapter6. Galactic Radio Astronomy: Galactic Structure, HII Regions, Supernova Remnants, Neutron Stars and Pulsars.- Chapter7. Extragalactic Radio Astronomy: Galaxy Classification, Active Galactic Nuclei, Superluminal Motion, Galaxy Clusters and the Microwave Background.
£44.99
Springer International Publishing AG Deep Sky Observing: An Astronomical Tour
Book SynopsisThis updated second edition has all of the information needed for your successful forays into deep sky observing. Coe uses his years of experience to give detailed practical advice about how to find the best observing site, how to make the most of the time spent there, and what equipment and instruments to take along. There are comprehensive lists of deep sky objects of all kinds, along with Steve's own observations describing how they look through telescopes with apertures ranging from 4 inches to 36 inches (0.1 - 0.9 meters).Binocular observing also gets its due, while the lists of objects have been amended to highlight only the best targets. A new index makes finding targets easier than ever before, while the selection of viewing targets has been revised from the first edition. Most of all, this book is all about how to enjoy astronomy. The author's enthusiasm and sense of wonder shine through every page as he invites you along on a tour of some of the most beautiful and fascinating sites in the deep sky, with the improved object list making sure your choice of a faint cluster, hazy nebula or distant galaxy will all be equally rewarding.Trade Review“The definitive guide to observing deep sky objects such as globular clusters, galaxies, planetary nebulae and supernova remnants. … it gives answers to lots of practical questions that you haven't even realized you wanted to know such as why you should invite other people to observe with you, or share your hobby with others, or how could a computer be helpful with deep sky objects.” (AstroMadness.com, December, 2016)“This is a book aimed at fairly serious stargazers, even though the tone and some chapters seem suited for beginners. … Summing Up: Recommended. Professionals and practitioners.” (D. J. Van Domelen, Choice, Vol. 54 (3), November, 2016)Table of ContentsWho Can Benefit from This Book?.- Why Should You Listen to Me?.- How Do I Find the Best Observing Site?.- How Do I Maximize My Time While Observing?.- What Other Accessories Are Useful?.- Why Should I Take Notes While Observing?.- How Can I Find All These Deep-Sky Goodies when the Sky is So Huge?.- Any Other Tips?.- What Can I Observe in Galaxies Beyond the Milky Way?.- What Can I Observe in a Cluster of Galaxies?.- What Are All These Different Types of Nebulae, and What Details Can I See in Them with My Telescope?.- What Can Be Seen Within Planetary Nebulae?.- What Can Be Seen in an Open Star Cluster?.- What Can Be Observed in Globular Clusters?.- Why Would I Want to Use Binoculars to View the Sky?.- How Can I Use a Computer to Help Me Enjoy Deep-Sky Observing?.- Why Should I Set Up the Scope for a Public Viewing Session?.- Which Books on Astronomy Should I Get?.- A Magical Evening.
£34.99
Springer International Publishing AG The NexStar User’s Guide II: For the LCM, SLT, SE, CPC, SkyProdigy, and Astro Fi
Book SynopsisMichael Swanson’s online discussions with literally thousands of NexStar owners made it clear that there was a desperate need for a book such as this – one that provides a complete, detailed guide to buying, using and maintaining NexStar telescopes. Although this book is highly comprehensive, it is suitable for beginners – there is a chapter on "Astronomy Basics" – and experts alike.Celestron’s NexStar telescopes were introduced in 1999, beginning with their first computer controlled "go to" model, a 5-inch. More models appeared in quick succession, and Celestron’s new range made it one of the two dominant manufacturers of affordable "go to" telescopes. Trade ReviewFrom the reviews of the first edition: “Swanson includes thorough, model-specific descriptions of the all the telescope functions, care and maintenance, accessories, and numerous advanced topics. You’ll find advice on how to fine-tune your alignment so that a new target will fall within the eyepiece’s field of view every time you slew. I used to be pleased if that happened two or three times in a night. … I was surprised by the difference these small improvements made in the pleasure of my observing experience. … true advantage comes from its friendly approach and sound advice based on the personal experiences of the author and other avid NexStar users.” (Sky & Telescope, December, 2004)Table of ContentsChapter 1 - Introduction.- Chapter 2 - Astronomy Basics.- Chapter 3 - Overview of Celestron's Alt-Az Computerized Telescopes.- Chapter 4 - Alignment.- Chapter 5 - NexStar and StarSense Hand Control Operation.- Chapter 6 - SkyPortal Operation.- Chapter 7 - Connecting a PC, Mac, Tablet, or Smartphone to Your 'Scope.- Chapter 8- Expanding Your Horizons - Choosing Objects to View.- Chapter 9 - accessories for Your Telescope.- Chapter 10 - Firmware Updates.- Chapter 11.- Collimation, Maintenance, Care, and Cleaning.- Chapter 12 - Tips, Solutions, and Troubleshooting Common problems.- Appendix A - Internet Resources.- Appendix B - Glossary.- Index.
£31.34
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Astroparticle Physics
Book SynopsisDescribes the branch of astronomy in which processes in the universe are investigated with experimental methods employed in particle-physics experiments. After a historical introduction the basics of elementary particles, Explains particle interactions and the relevant detection techniques, while modern aspects of astroparticle physics are described in a chapter on cosmology. Provides an orientation in the field of astroparticle physics that many beginners might seek and appreciate because the underlying physics fundamentals are presented with little mathematics, and the results are illustrated by many diagrams. Readers have a chance to enter this field of astronomy with a book that closes the gap between expert and popular level.Trade ReviewFrom the reviews: "In astroparticle physics techniques known from particle physics experiments are applied to investigate the universe … . Grupen presents an introduction and overview of the main ideas and concepts of this rapidly growing field of research. Written in a very clear and readable fashion it is accessible to a broad audience. … is enriched with many diagrams and illustrations, increasing the readability of the text. … Grupen’s book is really a must-have for anyone looking for a good starting point in … astroparticle physics." (Michael Tytgat, Physicalia, Vol. 28 (4-6), 2006) "Astroparticle Physics is a timely attempt to describe the status of a booming field at the interface of astrophysics, particle physics, and cosmology that has produced so many exciting results over the past few years. The format of the book, with the wide margin for keywords and figures, the extensive glossary, and the problems for each section (with detailed solutions), make it very readable and provide a good starting point for undergraduate and postgraduate students interested in astroparticle physics." (Johannes Knapp, The Observatory, Vol. 126 (1192), 2006) "This book … covers a wide range and requires a good grounding in modern physics to be useful. … Included are a mathematical appendix and an appendix on the results from statistical physics necessary to understand the thermodynamics of the early universe. These additions make the book a good introduction to this rapidly moving subject. Each chapter offers problems with solutions, and a 26-page comprehensive index and references are included. A very useful book for the right reader. Summing Up: Recommended." (K. W. Ogilvie, CHOICE, March, 2006) "Claus Grupen provides a comprehensive and up-to-date introduction to the main ideas and terminology of the study of elementary particles originating from astrophysical objects. … The style and presentation of the material make the book accessible to a broad audience … . A good selection of simple exercises with solution increases its pedagogical value and makes it suitable as a textbook for an undergraduate course. Non-specialists who want to follow the main issues of current research in the field … also benefit from Grupen’s book." (Marcello Lissia, CERN Courier, Vol. 46 (1), 2006) "In the present context, Astroparticle Physics consists of the studies of charged cosmic rays, neutrinos, gamma rays, X-rays and cosmology. … The index is magnificent and there is a good, relevant, mathematical appendix plus a glossary of terms which is actually useful. Best of all, there are worthwhile problems at the end of each chapter, complete with full solutions at the end of the book. … this is a well written, well produced, text for a new field at a reasonable price." (Roger Clay, Australian Physics, Vol. 42 (5), 2005)Table of ContentsHistorical Introduction.- The Standard Model of Elementary Particles.- Kinematics and Cross Sections.- Physics of Particle and Radiation Detection.- Acceleration Mechanisms.- Primary Cosmic Rays.- Secondary Cosmic Rays.- Cosmology.- The Early Universe.- Big Bang Nucleosynthesis.- The Cosmic Microwave Background.- Inflation.- Dark Matter.- Astrobiology.- Outlook.- Solutions.
£54.99
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Theory of Orbits: Volume 1: Integrable Systems
Book SynopsisHalf a century ago, S. Chandrasekhar wrote these words in the preface to his l celebrated and successful book: In this monograph an attempt has been made to present the theory of stellar dy namics as a branch of classical dynamics - a discipline in the same general category as celestial mechanics. [ ... J Indeed, several of the problems of modern stellar dy namical theory are so severely classical that it is difficult to believe that they are not already discussed, for example, in Jacobi's Vorlesungen. Since then, stellar dynamics has developed in several directions and at var ious levels, basically three viewpoints remaining from which to look at the problems encountered in the interpretation of the phenomenology. Roughly speaking, we can say that a stellar system (cluster, galaxy, etc.) can be con sidered from the point of view of celestial mechanics (the N-body problem with N » 1), fluid mechanics (the system is represented by a material con tinuum), or statistical mechanics (one defines a distribution function for the positions and the states of motion of the components of the system).Trade ReviewFrom the reviews "The book is ... didactically written and contains topics from classical to most modern ones, treated rigorously by indicating where complete proofs are to be found."Zentralblatt für Mathematik, 1999Table of Contents— The Theory of Orbits from Epicycles to “Chaos”.- 1. Dynamics and Dynamical Systems — Quod Satis.- 2. The Two-Body Problem.- 3. The N-Body Problem.- 4. The Three-Body Problem.- 5. Orbits in Given Potentials.- Mathematical Appendix.- A.1 Spherical Trigonometry.- A.2 Curvilinear Coordinate Systems.- A.3 Riemannian Geometry.- Bibliographical Notes.- Name Index.
£75.99
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Tools of Radio Astronomy
Book SynopsisThis 6th edition of “Tools of Radio Astronomy”, the most used introductory text in radio astronomy, has been revised to reflect the current state of this important branch of astronomy. This includes the use of satellites, low radio frequencies, the millimeter/sub-mm universe, the Cosmic Microwave Background and the increased importance of mm/sub-mm dust emission. Several derivations and presentations of technical aspects of radio astronomy and receivers, such as receiver noise, the Hertz dipole and beam forming have been updated, expanded, re-worked or complemented by alternative derivations. These reflect advances in technology. The wider bandwidths of the Jansky-VLA and long wave arrays such as LOFAR and mm/sub-mm arrays such as ALMA required an expansion of the discussion of interferometers and aperture synthesis. Developments in data reduction algorithms have been included. As a result of the large amount of data collected in the past 20 years, the discussion of solar system radio astronomy, dust emission, and radio supernovae has been revisited. The chapters on spectral line emission have been updated to cover measurements of the neutral hydrogen radiation from the early universe as well as measurements with new facilities. Similarly the discussion of molecules in interstellar space has been expanded to include the molecular and dust emission from protostars and very cold regions. Several worked examples have been added in the areas of fundamental physics, such as pulsars. Both students and practicing astronomers will appreciate this new up-to-date edition of Tools of Radio Astronomy. Trade ReviewAus den Rezensionen zur 6.Auflage: “... Studenten und Absolventen einschlägiger Fachrichtungen ist das Buch auch fur Quereinsteiger und Amateure geeignet, die ernsthaft in dieses Fachgebiet eindringen wollen.“ (in: Funkamateur, Heft 5, 2014)Table of ContentsRadio Astronomical Fundamentals.- ElectromagneticWave Propagation Fundamentals.- Wave Polarization.- Signal Processing and Receivers: Theory.- Practical Receiver Systems.- Fundamentals of Antenna Theory.- Practical Aspects of Filled Aperture Antennas.- Single Dish Observational Methods.- Interferometers and Aperture Synthesis.- Emission Mechanisms of Continuous Radiation.- Some Examples of Thermal and Nonthermal Radio Sources.- Spectral Line Fundamentals.- Line Radiation from Atoms.- Radio Recombination Lines.- Overview of Molecular Basics.- Molecules in Interstellar Space.- Some Useful Vector Relations & Fourier Transforms.- The Van Vleck Clipping Correction: One Bit Quantization.- Conventional Derivation of Square Law Detector Response & Receiver Noise.- The Reciprocity Theorem.- Filled Aperture Antennas.- The Hankel Transform.- Lists of Calibration Radio Sources.- The Mutual Coherence Function and van Cittert-Zernike Theorem.- Bibliography.- Index.
£49.99
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Fundamental Astronomy
Book SynopsisFundamental Astronomy is a well-balanced, comprehensive introduction to classical and modern astronomy. While emphasizing both the astronomical concepts and the underlying physical principles, the text provides a sound basis for more profound studies in the astronomical sciences. This is the fifth edition of the successful undergraduate textbook and reference work. It has been extensively modernized and extended in the parts dealing with extragalactic astronomy and cosmology. You will also find augmented sections on the solar system and extrasolar planets as well as a new chapter on astrobiology. Long considered a standard text for physical science majors, Fundamental Astronomy is also an excellent reference work for dedicated amateur astronomers.Trade Review"For the book to reach the fourth edition, it must be hitting a niche in the market. The preface to the first edition in 1987 identifies that market as a ‘university textbook for a first course in astronomy’ which is also suited for serious amateurs who ‘find the popular texts too trivial’. In my opinion, that description from the original preface is ‘spot on’ and makes this volume a must-buy for any serious amateur looking for a comprehensive overview of matters astronomical." (Roger Feasey, Auckland Astronomical Society Journal, March 2004) "This work remains a most excellent textbook for the student as well as the dedicated amateur astronomer." (ORION 62/321, ) "If you are looking for a solid undergraduate text outlining the physics which underpins so much of modern astronomy then this book will be a very useful addition to your personal library." (Astronomy Now, May 2004) "… The wide range of expertise gives the book an authority that would be almost impossible for a single-author text ... There are other aids to the reader: worked examples ... starred sections in small print take the inquisitive reader beyond the general level of the book." (Nature) "… Unique among available texts and has so much to offer ... No one involved in astronomy teaching will want to be without a copy." (The Physics Teacher) "Gives a solid foundation to the basic ideas of astronomy in a clear and accessible fashion … Fundamental ideas are developed clearly and applied to real problems, and solutions are worked out." (Sky & Telescope) From the reviews of the fourth edition: "This book will well serve its readership which includes both undergraduate physical science and mathematics students … . covers all the important subjects of an introductory course in astronomy. … is beautifully illustrated with many black and white and color photographs, which will be most appealing … . they have produced a book that will prove useful for many years … . As such it is highly recommended … to the general reader who wants to be pleasantly and highly informed about astronomy." (Fernande Grandjean, Gary J. Long, Physicalia, Vol. 26(1), 2004) "The book remains a calculus-based textbook and reference source containing many exercises … for the proper comprehension of the subjects treated. … This work remains a most excellent textbook for the student as well as the dedicated amateur astronomer. … can considerably widen the vision of the student … ." (Noël Cramer, ORIAN-Zeitschrift der Schweizerischen Astronomischen Gesellschaft Vol. 62(321), 2004) "Fundamental Astronomy is both the title and an excellent description of the content … . is also suited for serious amateurs who "find the popular texts too trivial". In my opinion … this volume a must-buy for any serious amateur looking for a comprehensive overview of matters astronomical. … Its usefulness for education purposes is enhanced by worked examples in each section followed by exercises." (AAS Journal, March, 2004) "This is the 4th edition of this well known and well tested undergraduate-level text on astronomy. … All the derivations are well done and the problems selected for student work are interesting and will undoubtedly help the student in his or her studies. … if you are looking for a solid undergraduate text outlining the physics which underpins so much of modern astronomy then this book will be a very useful addition to your personal library." (Kevin P. Marshall, Astronomy Now, May, 2004) From the reviews of the fifth edition: “This textbook, suitable for a university first course in astronomy, is the outgrowth of a long and outstanding astronomical tradition in Finland, and the result of an extensive collaborative effort, which included also teaching and interaction with many people. … I highly recommend this book for class use … it will be useful for professionals as well.” (Bruno Bertotti, Prometeo, Vol. 24 (3-4), 2008)Table of ContentsSpherical Astronomy.- Observations and Instruments.- Photometric Concepts and Magnitudes.- Radiation Mechanisms.- Celestial Mechanics.- The Solar System.- Stellar Spectra.- Binary Stars and Stellar Masses.- Stellar Structure.- Stellar Evolution.- The Sun.- Variable Stars.- Compact Stars.- The Interstellar Medium.- Star Clusters and Associations.- The Milky Way.- Galaxies.- Cosmology.- Astrobiology.
£54.99
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG What are the Stars?
Book SynopsisThe outstanding question in astronomy at the turn of the twentieth century was: What are the stars and why are they as they are? In this volume, the story of how the answer to this fundamental question was unravelled is narrated in an informal style, with emphasis on the underlying physics. This book discusses recent developments in the context of discussing the nature of the stars, their stability and the source of the energy they radiate. Reading this book will get young students excited about the presently unfolding revolution in astronomy and the challenges that await them in the world of physics, engineering and technology. General readers will also find the book appealing for its highly accessible narrative of the physics of stars.Table of ContentsThe Present Revolution in Astronomy: An Overview.- What Are the Stars?.- Stars as Globes of Gas.- Eddington’s Theory of the Stars.- Why Are the Stars as They Are?.- Energy Generation in the Stars.- Sounds of the Sun.- The Smoking Gun is Finally Found.
£44.99
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Astrophysics of Neutron Stars
Book SynopsisThe existence of neutron stars was not only a brilliant theoretical prediction, but also one of the most unexpected and astonishing discoveries of all heavenly bodies. Twenty-five years after the remarkable event of their discovery, neutron stars, which are the densest, the most strongly magnetized, and the most rapid ly rotating bodies in the Galaxy, remain objects of intense interest. This book is a revised and enlarged version of the original Russian edition. The last five years were marked by the discovery of a supernova in the closest galaxy and dozens of X-ray sources and millisecond pulsars, which apparently confirm the validity of the basic ideas underlying these discoveries. The author has concentrated on the astrophysical manifestations of neutron stars, which are believed mainly to be associated with the nature of their interaction with their surroundings. Naturally, this approach does not leave much room for a detailed description of the internal structure of these stars. Fortunately, there exists an excellent monograph by S. L. Shapiro and S. A. Teukolsky (Black Holes, White Dwarfs, and Neutron Stars, Wiley, New York 1985) which deals mainly with the purely physical problems. Moreover, the publication of such a book in the West partly makes amends for the lack of information about the work being done by Soviet scientists in this field.Table of Contents1. Theoretical and Observational Principles of the Astrophysics of Neutron Stars.- 1.1 Prediction.- 1.2 Accretion.- 1.3 Rotation and Magnetic Field.- 1.4 Radiopulsars.- 1.5 New Ideas.- 1.6 X-Ray Pulsars.- 1.7 X-Ray Bursters.- 1.8 Bursts and Other Sources of Gamma Rays.- 1.9 General View.- 2. Structure of Neutron Stars.- 2.1 Equilibrium of Stars.- 2.2 Exact Equilibrium Equations for Cold Stars.- 2.3 Physical Conditions Inside Neutron Stars.- 2.4 Parameters of Neutron Stars.- 2.5 Mass of Neutron Stars.- 2.6 Rotational Effects.- 3. Fluid Dynamics of Accretion.- 3.1 Spherically Symmetric Accretion.- 3.2 The Role of Radiation and Ejection.- 3.3 Spherical Accretion to a Neutron Star Without a Magnetic Field.- 3.4 Capture of Matter by a Moving Star.- 3.5 Fluid Dynamics of Cylindrical Accretion.- 3.6 Disk Accretion.- 3.7 Luminosity and Spectrum of Accretion Disks.- 3.8 Supercritical Disk Accretion.- 3.9 Accretion in Binary Systems.- 3.9.1 Overflow Through the Inner Lagrangian Point.- 3.9.2 Accretion from Stellar Wind.- 3.10 Two-Stream Accretion.- 3.11 Accretion of Magnetic Fields.- 4. Classification of Neutron Stars.- 4.1 Magnetic Dipole.- 4.2 Stopping Radius.- 4.3 Stopping Radius in the Supercritical Case.- 4.4 The Effect of a Magnetic Field.- 4.5 Gravimagnetic Parameter.- 4.6 Corotation Radius.- 4.7 Nomenclature.- 4.8 Critical Periods. The p-y and p-L Diagrams.- 5. Boundaries. Magnetospheres of Slowly Rotating Neutron Stars.- 5.1 Physical Conditions in the Alfvén Zone.- 5.2 Formulation of the Problem.- 5.3 Simple Configurations.- 5.4 Magnetosphere in Spherically Symmetric Accretion.- 5.5 Pascal’s Pressure Law.- 5.5.1 Two-Dimensional Solutions.- 5.5.2 Three-Dimensional Solutions.- 5.6 A Dipole Confined by an Ideally Conducting Disk.- 5.6.1 Two-Dimensional Model.- 5.6.2 Three-Dimensional Problem.- 5.6.3 Dipole Rotation.- 5.7 Magnetosphere in a Plane-parallel Plasma Flow.- 5.7.1 Two-Dimensional Solution.- 5.7.2 Three-Dimensional Solution.- 5.8 Two-Stream Accretion.- 6. Accreting Neutron Stars.- 6.1 Boundary Stability.- 6.1.1 Spherically Symmetric Accretion.- 6.1.2 Disk Accretion onto a Magnetized Neutron Star.- 6.1.3 Torsion of an Accretion Disk by Magnetic Forces.- 6.1.4 Magnetosphere Boundary Stability for Two-Stream Accretion.- 6.2 The Polar Column.- 6.3 Spin-up, Spin-down and Induced Precession of Accreting Stars.- 6.3.1 Spin-up Torque.- 6.3.2 Spin-down Torque.- 6.3.3 Analytical Model of Torques Applied to a Magnetized Accreting Star.- 6.3.4 Equilibrium Period.- 6.4 Observed Properties of X-Ray Pulsars.- 6.5 Energy Parameters of Pulsars and Transport of Matter in Binary Systems.- 6.6 Spectrum and Magnetic Fields.- 6.7 Periods of X-Ray Pulsars and Their Variation.- 6.7.1 Equilibrium of X-Ray Pulsars.- 6.7.2 Magnetic Fields of X-Ray Pulsars.- 6.7.3 Reasons Behind the Average Spin-up of X-Ray Pulsars.- 6.7.4 Rapid Fluctuation of Periods and Internal Structure of Neutron Stars.- 6.8 Variability of X-Ray Sources. Transients.- 6.9 Generation of Relativistic Particles.- 6.10 X-Ray Bursters.- 6.10.1 Localization and Spatial Distribution.- 6.10.2 Periodic Variations of X-Ray Flux. X-Ray Eclipses.- 6.10.3 Luminosity and Spectra of Bursters.- 6.11 Nuclear Burning at the Surface of Neutron Stars. Spherically Symmetric Model.- 6.12 Accretion to X-Ray Bursters.- 6.12.1 Accretion for ? Stars.- 7. The “Propeller” Regime.- 7.1 Quasistatic Shells.- 7.1.1 Supersonic Propeller.- 7.1.2 Subsonic Propeller.- 7.1.3 Very Rapid Propeller.- 7.1.4 Nongravitating Propeller.- 7.2 Spinning-down in the Boundary Layer.- 7.3 Two-Stream Flow Formation due to the Propeller Effect.- 7.3.1 Stationary Flow from Disks.- 7.3.2 Time-Dependent Solution.- 7.4 Dead Disks and Accumulator Disks.- 7.5 Nonstationary Disk Accretion. Model of Transient X-Ray Sources.- 7.6 Relativistic Propeller.- 7.7 Objects That Can Become Propellers.- 7.7.1 Binary Systems.- 7.7.2 Single Neutron Stars.- 8. Ejecting Stars.- 8.1 Observed Characteristics of Radiopulsars.- 8.1.1 Periods and Their Variation.- 8.1.2 Pulse Structure.- 8.1.3 Spectrum and Luminosity.- 8.1.4 Distribution of Pulsars in Space.- 8.1.5 Spatial Velocity of Radiopulsars.- 8.1.6 Pulsars and Binary Systems.- 8.2 Radiopulsars as Ejecting Neutron Stars.- 8.3 Pulsar Electrodynamics and Generation of Relativistic Particles.- 8.3.1 Vacuum Approximation.- 8.3.2 Magnetosphere in the Presence of Plasma.- 8.4 Mechanisms of Radiation.- 8.5 Caverns Around Neutron Stars.- 8.5.1 Caverns in Binary Systems.- 8.5.2 Caverns Around a Single Neutron Star.- 8.5.3 Effect of Relativistic Wind on Accretion Flow Parameters.- 8.6 Change in Radiopulsar Period.- 8.6.1 Spin-down of Pulsars and Their Magnetic Fields.- 8.6.2 Spin-up Episodes and Internal Structure of Neutron Stars.- 8.7 Evolution of Radiopulsars.- 8.7.1 Origin and Age of Pulsars.- 8.7.2 Evolution of the Radiopulsar Period.- 8.8 Spatial Velocities of Radiopulsars.- 8.9 Ejecting Stars in Binary Systems.- 8.9.1 Radiopulsars Forming Pairs with Degenerate Stars.- 8.9.2 “Reflection” Effect.- 8.9.3 Observational Evidence of the Existence of Ejecting Stars in Binary Systems.- 9. Supercritical Regimes.- 9.1 Superaccretor.- 9.1.1 Accretion Pattern.- 9.1.2 Neutrino Pulsar.- 9.1.3 Spin-up and Spin-down.- 9.2 Superejectors and Superpropellers.- 9.3 Is SS 433 a Superaccretor?.- 9.4 Other Candidates.- 10. Stars with an Anomalously Low Value of Gravimagnetic Parameter.- 10.1 Georotators.- 10.2 Binary Magnetic Systems (Magnetors).- 11. Evolution of Stars.- 11.1 Normal Stars.- 11.1.1 Single Stars.- 11.1.2 Binary Stars.- 11.2 Evolution of Neutron Stars.- 11.2.1 Evolution Equation.- 11.2.2 Statistical Description of the Ensemble of Neutron Stars.- 11.3 Neutron Star Tracks.- 11.4 Numerical Simulation of the Joint Evolution of Normal and Neutron Stars.- 11.4.1 Computational Method.- 11.4.2 Evolutionary Tracks.- 11.4.3 Simulation of X-Ray Pulsars (Stage IIA) and the Choice of Optimal Parameters.- 11.4.4 Abundance of Different Types of Systems in the Galaxy.- 11.4.5 Physical Characteristics of Neutron Stars at Various Stages of Evolution.- 11.4.6 Two Types of Radiopulsars.- 11.5 Possible Candidates.- 11.5.1 “Runaway” Stars.- 11.5.2 The SS 433 Object.- 11.5.3 “Single” Wolf-Rayet Stars.- 11.5.4 Collapse Anisotropy.- 11.5.5 Other Numerical Models.- Magnetohydrodynamic Instabilities.- Rayleigh-Taylor (RT) Instability.- Commutation Instability.- References.
£64.99
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Physics of Gravitating Systems I: Equilibrium and Stability
Book SynopsisIt would seem that any specialist in plasma physics studying a medium in which the interaction between particles is as distance-dependent as the inter action between stars and other gravitating masses would assert that the role of collective effects in the dynamics of gravitating systems must be decisive. However, among astronomers this point of view has been recog nized only very recently. So, comparatively recently, serious consideration has been devoted to theories of galactic spiral structure in which the dominant role is played by the orbital properties of individual stars rather than collec tive effects. In this connection we would like to draw the reader's attention to a difference in the scientific traditions of plasma physicists and astrono mers, whereby the former have explained the delay of the onset of controlled thermonuclear fusion by the "intrigues" of collective processes in the plasma, while many a generation of astronomers were calculating star motions, solar and lunar eclipses, and a number of other fine effects for many years ahead by making excellent use of only the laws of Newtonian mechanics. Therefore, for an astronomer, it is perhaps not easy to agree with the fact that the evolution of stellar systems is controlled mainly by collective effects, and the habitual methods of theoretical mechanics III astronomy must make way for the method of self-consistent fields.Table of Contents(Volume I).- § 1. Basic Concepts and Equations of Theory.- § 2. Equilibrium States of Collisionless Gravitating Systems.- § 3. Small Oscillations and Stability.- §4. Jeans Instability of a One—Component Uniform Medium.- §5. Jeans Instability of a Multicomponent Uniform Medium.- 5.1. Basic Theorem (on the Stability of a Multicomponent System with Components at Rest).- 5.2. Four Limiting Cases for a Two—Component Medium.- 5.3. Table of Jeans Instabilities of a Uniform Two—Component Medium.- 5.4. General Case of n Components.- §6. Non—Jeans Instabilities.- § 7. Qualitative Discussion of the Stability of Spherical, Cylindrical (and Disk—Shaped) Systems with Respect to Radial Perturbations.- I Theory.- I Equilibrium and Stability of a Nonrotating Flat Gravitating Layer.- § 1. Equilibrium States of a Collisionless Flat Layer.- § 2. Gravitational (Jeans) Instability of the Layer.- § 3. Anisotropic (Fire—Hose) Instability of a Collisionless Flat Layer.- 3.1. Qualitative Considerations.- 3.2. Derivation of the Dispersion Equation for Bending Perturbations of a Thin Layer.- 3.3. Fire—Hose Instability of a Highly Anisotropic Flat Layer.- 3.4. Analysis of the Dispersion Equation.- 3.5. Additional Remarks.- § 4. Derivation of Integra—Differential Equations for Normal Modes of a Flat Gravitating Layer.- § 5. Symmetrical Perturbations of a Flat Layer with an Isotropic Distribution Function Near the Stability Boundary.- § 6. Perpendicular Oscillations of a Homogeneous Collisionless Layer.- 6.1. Derivation of the Characteristic Equation for Eigenfrequencies.- 6.2. Stability of the Model.- 6.3. Permutational Modes.- 6.4. Time—Independent Perturbations (? = 0).- Problems.- II Equilibrium and Stability of a Collisionless Cylinder.- §1. Equilibrium Cylindrical Configurations.- § 2. Jeans Instability of a Cylinder with Finite Radius.- 2.1. Dispersion Equation for Eigenfrequencies of Axial-Symmetrical Perturbations of a Cylinder with Circular Orbits of Particles.- 2.2. Branches of Axial—Symmetrical Oscillations of a Rotating Cylinder with Maxwellian Distribution of Particles in.- 2.3. Longitudinal Velocities.- 2.4. Oscillative Branches of the Rotating Cylinder with a Jackson Distribution Function (in Longitudinal Velocities).- 2.5. Axial—Symmetrical Perturbations of Cylindrical Models of a More General Type.- § 3. Nonaxial Perturbations of a Collisionless Cylinder.- 3.1. The Long—Wave Fire-Hose Instability.- 3.2. Nonaxial Perturbations of a Cylinder with Circular Particle Orbits 100§ 4. Stability of a Cylinder with Respect to Flute—like Perturbations.- § 5. Local Analysis of the Stability of Cylinders (Flute—like Perturbations).- 5.1. Dispersion Equation for Model (2), § 1.- 5.2. Maxwellian Distribution Function.- § 6. Comparison with Oscillations of an Incompressible Cylinder.- 6.1. Flute—like Perturbations (kz = 0).- § 7. Flute—like Oscillations of a Nonuniform Cylinder with Circular Orbits of Particles.- Problems.- III Equilibrium and Stability of Collisionless Spherically Symmetrical Systems.- § 1. Equilibrium Distribution Functions.- § 2. Stability of Systems with an Isotropic Particle Velocity Distribution.- 2.1. The General Variational Principle for Gravitating Systems with the Isotropic Distribution of Particles in Velocities (f0 = f0(E), f’0 = df0|dE ? 0).- 2.2. Sufficient Condition of Stability.- 2.3. Other Theorems about Stability. Stability with Respect to Nonradial Perturbations.- 2.4. Variational Principle for Radial Perturbations.- 2.5. Hydrodynamical Analogy.- 2.6. On the Stability of Systems with Distribution Functions That Do Not Satisfy the Condition f’0 (E) ? 0.- § 3. Stability of Systems of Gravitating Particles Moving On Circular Trajectories.- 3.1. Stability of a Uniform Sphere.- 3.2. Stability of a Homogeneous System of Particles with Nearly Circular Orbits.- 3.3. Stability of a Homogeneous Sphere with Finite Angular Momentum.- 3.4. Stability of Inhomogeneous Systems.- § 4. Stability of Systems of Gravitating Particles Moving in Elliptical Orbits.- 4.1. Stability of a Sphere with Arbitrary Elliptical Particle Orbits.- 4.2. Instability of a Rotating Freeman Sphere.- § 5. Stability of Systems with Radial Trajectories of Particles.- 5.1. Linear Stability Theory.- 5.2. Simulation of a Nonlinear Stage of Evolution.- § 6. Stability of Spherically Symmetrical Systems of General Form.- 6.1. Series of the Idlis Distribution Functions.- 6.2. First Series of Camm Distribution Functions (Generalized Poly tropes).- 6.3. Shuster’s Model in the Phase Description.- §7. Discussion of the Results.- Problems.- IV Equilibrium and Stability of Collisionless Ellipsoidal Systems.- § 1. Equilibrium Distribution Functions.- 1.1 Freeman’s Ellipsoidal Models.- 1.2. “Hot” Models of Collisionless Ellipsoids of Revolution.- § 2. Stability of a Three—Axial Ellipsoid and an Elliptical Disk.- 2.1. Stability of a Three-Axial Ellipsoid.- 2.2. Stability of Freeman Elliptical Disks.- § 3. Stability of Two—Axial Collisionless Ellipsoidal Systems.- 3.1. Stability of Freeman’s Spheroids.- 3.2. Peebles—Ostriker Stability Criterion. Stability of Uniform Ellipsoids, “Hot” in the Plane of Rotation.- 3.3. The Fire-Hose Instability of Ellipsoidal Stellar Systems.- 3.4. Secular and Dynamical Instability. Characteristic Equation for Eigenfrequencies of Oscillations of Maclaurin Ellipsoids.- Problems.- V Equilibrium and Stability of Flat Gravitating Systems.- § 1. Equilibrium States of Flat Gaseous and Collisionless Systems.- 1.3. Systems with Circular Particle Orbits.- 1.4. Plasma Systems with a Magnetic Field.- 1.5. Gaseous Systems.- 1.6. “Hot” Collisionless Systems.- § 2. Stability of a “Cold” Rotating Disk.- 2.1. Membrane Oscillations of the Disk.- 2.2. Oscillations in the Plane of the Disk.- § 3. Stability of a Plasma Disk with a Magnetic Field.- 3.1. Qualitative Derivation of the Stability Condition.- 3.2. Variational Principle.- 3.3. Short—Wave Approximation.- 3.4. Numerical Analysis of a Specific Model.- § 4. Stability of a “Hot” Rotating Disk.- 4.1. Oscillations in the Plane of the Disk.- 4.2. Bending Perturbations.- 4.3. Methods of the Stability Investigation of General Collisionless Disk Systems.- 4.4. Exact Spectra of Small Perturbations.- 4.5. Global Instabilities of Gaseous Disks. Comparison of Stability Properties of Gaseous and Stellar Disks.- Problems.- References.- Additional References.
£44.99
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Physics of Gravitating Systems II: Nonlinear Collective Processes: Nonlinear Waves, Solitons, Collisionless Shocks, Turbulence. Astrophysical Applications
Table of Contents(Volume II).- Non-Jeans Instabilities of Gravitating Systems.- VI Non-Jeans Instabilities of Gravitating Systems.- § 1. Beam Instability of a Gravitating Medium.- 1.1. Theorem of a Number of Instabilities of the Heterogeneous System with Homogeneous Flows.- 1.2. Expression for the Growth Rate of the Kinetic Beam Instability in the Case of a Beam of Small Density (for an Arbitrary Distribution Function).- 1.3. Beam with a Step Function Distribution.- 1.4. Hydrodynamical Beam Instability. Excitation of the Rotational Branch.- 1.5. Stabilizing Effect of the Interaction of Gravitating Cylinders and Disks.- 1.6. Instability of Rotating Inhomogeneous Cylinders with Oppositely Directed Beams of Equal Density.- § 2. Gradient Instabilities of a Gravitating Medium.- 2.1. Cylinder of Constant Density with Radius-Dependent Temperature. Hydrodynamical Instability.- 2.2. Cylinder of Constant Density with a Temperature Jump. Kinetic Instability.- 2.3. Cylinder with Inhomogeneous Density and Temperature.- § 3. Hydrodynamical Instabilities of a Gravitating Medium with a Growth Rate Much Greater than that of Jeans.- 3.1. Hydrodynamical Instabilities in the Model of a Flat Parallel Flow.- 3.2. Hydrodynamical Instabilities of a Gravitating Cylinder.- §4. General Treatment of Kinetic Instabilities.- 4.1. Beam Effects in the Heterogeneous Model of a Galaxy.- 4.2. Influence of a “Black Hole” at the Center of a Spherical System on the Resonance Interactions Between Stars and Waves.- 4.3. Beam Instability in the Models of a Cylinder and a Flat Layer.- VII Problems of Nonlinear Theory.- § 1. Nonlinear Stability Theory of a Rotating, Gravitating Disk.- 1.1. Nonlinear Waves and Solitons in a Hydrodynamical Model of an Infinitely Thin Disk with Plane Pressure.- 1.2. Nonlinear Waves in a Gaseous Disk.- 1.3. Nonlinear Waves and Solitons in a Stellar Disk.- 1.4. Explosive Instability.- 1.5. Remarks on the Decay Processes.- 1.6. Nonlinear Waves in a Viscous Medium.- § 2. Nonlinear Interaction of a Monochromatic Wave with Particles in Gravitating Systems.- 2.1. Nonlinear Dynamics of the Beam Instability in a Cylindrical Model.- 2.2. Nonlinear Saturation of the Instability at the Corotation Radiusin the Disk.- § 3. Nonlinear Theory of Gravitational Instability of a Uniform Expanding Medium.- § 4. Foundations of Turbulence Theory.- 4.1. Hamiltonian Formalism for the Hydrodynamical Model of a Gravitating Medium.- 4.2. Three-Wave Interaction.- 4.3. Four-Wave Interaction.- §5. Concluding Remarks.- 5.1. When Can an Unstable Gravitating Disk be Regarded as an Infinitesimally Thin One?.- 5.2. On Future Soliton Theory of Spiral Structure.- Problems.- II Astrophysical Applications.- VIII General Remarks.- § 1. Oort’s Antievolutionary Hypothesis.- § 2. Is There a Relationship Between the Rotational Momentum of an Elliptical Galaxy and the Degree of Oblateness?.- § 3. General Principles of the Construction of Models of Spherically Symmetric Systems.- § 4. Lynden-Bell’s Collisionless Relaxation.- § 5. Estimates of “Collisionlessness” of Particles in Different Real Systems.- IX Spherical Systems.- § 1. A Brief Description of Observational Data.- 1.1. Globular Star Clusters.- 1.2. Spherical Galaxies.- 1.3. Compact Galactic Clusters.- § 2. Classification of Unstable Modes in Scales.- § 3. Universal Criterion of the Instability.- § 4. Specificity of the Effects of Small-Scale and Large-Scale Perturbations on the System’s Evolution.- § 5. Results of Numerical Experiments for Systems with Parameters Providing Strong Supercriticality.- § 6. Example of Strongly Unstable Model.- § 7. Can Lynden-Bell’s Intermixing Mechanism Be Observed Against a Background of Strong Instability ?.- § 8. Is the “Unstable” Distribution of Stellar Density Really Unstable (in the Hydrodynamical Sense) in the Neighborhood of a “Black Hole”?.- X Ellipsoidal Systems.- § 1. Objects Under Study.- § 2. Elliptical Galaxies.- 2.1. Why Are Elliptical Galaxies More Oblate than E7 Absent?.- 2.2. Comparison of the Observed Oblatenesses of S- and SO-Galaxies with the Oblateness of E-Galaxies.- 2.3. Two Possible Solutions of the Problem.- 2.4. The Boundary of the Anisotropic (Fire-Hose) Instability Determines the Critical Value of Oblateness.- 2.5. Universal Criterion of Instability.- §3. SB-Galaxies.- 3.1. The Main Problem.- 3.2. Detection in NGC 4027 of Counterflows as Predicted by Freeman.- 3.3. Stability of Freeman Models of SB-Galaxies with Observed Oblateness.- XI Disk-like Systems. Spiral Structure.- § 1. Different Points of View on the Nature of Spiral Structure.- § 2. Resonant Interaction of the Spiral Wave with Stars of the Galaxy.- 2.1. Derivation of Expressions for the Angular Momentum and Energy of the Spiral Wave.- 2.2. Physical Mechanisms of Energy and Angular Momentum Exchange Between the Spiral Waves and the Resonant Stars.- § 3. The Linear Theory of Stationary Density Waves.- 3.1. The Primary Idea of Lin and Shu of the Stationary Density Waves.- 3.2. The Spiral Galaxy as an Infinite System of Harmonic Oscillators.- 3.3. On “Two-Armness” of the Spiral Structure.- 3.4. The Main Difficulties of the Stationary Wave Theory of Lin and Shu.- §4. Linear Theory of Growing Density Waves.- 4.1. Spiral Structure as the Most Unstable Mode.- 4.2. Gravitational Instability at the Periphery of Galaxies.- 4.3. Waves of Negative Energy Generated Near the Corotation Circle and Absorbed at the Inner Lindblad Resonance—Lynden-BellKalnaj’s Picture of Spiral Pattern Maintenance.- 4.4. Kelvin–Helmholz Instability and Flute-like Instability in the Near-Nucleus Region of the Galaxy as Possible Generators of Spiral Structure.- 4.5. The “Trailing” Character of Spiral Arms.- § 5. Comparison of the Lin–Shu Theory with Observations.- 5. 1 The Galaxy.- 5.2. M33, M51, M81.- § 6. Experimental Simulation of Spiral Structure Generation.- 6. 1 In a Rotating Laboratory Plasma.- 6.2. In Numerical Experiment.- § 7. The Hypothesis of the Origin of Spirals in the SB-Galaxies.- XII Other Applications.- § 1 On the Structure of Saturn’s Rings.- l.1. Introduction.- 1.2. Model. Basic Equations.- 1.3. Jeans Instability.- 1.4. Dissipative Instabilities.- 1.5. Modulational Instability.- Appendix. Derivation of the Expression for the Perturbation Energy of Maclaurin’s Ellipsoid.- § 2. On the Law of Planetary Distances.- §3. Galactic Plane Bending.- 3.1. Quasistationary Tidal Deformation.- 3.2. Free Modes of Oscillations.- 3.3. Close Passage.- § 4. Instabilities in Collisions of Elementary Particles.- § 1. Collisionless Kinetic Equation and Poisson Equation in Different Coordinate Systems.- § 2. Separation of Angular Variables in the Problem of Small Perturbations of Spherically Symmetrical Collisionless Systems.- § 3. Statistical Simulation of Stellar Systems.- 3.1. Simulation of Stellar Spheres of the First Camm Series.- 3.2. Simulation of Homogeneous Nonrotating Ellipsoids.- § 4. The Matrix Formulation of the Problem of Eigenoscillations of a Spherically-Symmetrical Collisionless System.- § 5. The Matrix Formulation of the Problem of Eigenoscillations of Collisionless Disk Systems.- 5.1. The Main Ideas of the Derivation of the Matrix Equation.- 5.2. “Lagrange” Derivation of the Matrix Equation.- § 6. Derivation of the Dispersion Equation for Perturbations of the Three-Axial Freeman Ellipsoid.- § 7. WKB Solutions of the Poisson Equation Taking into Account the Preexponential Terms and Solution of the Kinetic Equation in the Postepicyclic Approximation.- 7.1. The Relation Between the Potential and the Surface Density.- 7.2. Calculations of the Response of a Stellar Disk to an Imposed Perturbation of the Potential.- § 8. On the Derivation of the Nonlinear Dispersion Equation for Collisionless Disk.- § 9. Calculation of the Matrix Elements for the Three-Waves Interaction.- § 10. Derivation of the Formulas for the Boundaries of Wave Numbers Range Which May Take Part in a Decay.- §11. Derivation of the Kinetic Equation for Waves.- § 12. Table of Non-Jeans Instabilities (with a Short Summary).- References.- Additional References.
£44.99
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Astronomy on the Personal Computer
Book SynopsisA thorough introduction to the computation of celestial mechanics, covering everything from astronomical and computational theory to the construction of rapid and accurate applications programs. The book supplies the necessary knowledge and software solutions for determining and predicting positions of the Sun, Moon, planets, minor planets and comets, solar eclipses, stellar occultations by the Moon, phases of the Moon and much more. This completely revised edition takes advantage of C++, and individual applications may be efficiently realized through the use of a powerful module library. The accompanying CD-ROM contains the complete, fully documented and commented source codes as well as executable programs for Windows 98/2000/XP and LINUX.Table of Contents1 Introduction.- 2 Coordinate Systems.- 3 Calculation of Rising and Setting Times.- 4 Cometary Orbits.- 5 Special Perturbations.- 6 Planetary Orbits.- 7 Physical Ephemerides of the Planets.- 8 The Orbit of the Moon.- 9 Solar Eclipses.- 10 Stellar Occultations.- 11 Orbit Determination.- 12 Astrometry.- A.1 The Accompanying CD-ROM.- A.1.1 Contents.- A.1.2 System Requirements.- A.1.3 Executing the Programs.- A.2 Compiling and Linking the Programs.- A.2.1 General Advice on Computer-Specific Modifications.- A.2.2 Microsoft Visual C++ for Windows 98/2000/XP.- A.2.3 GNU C++ for Linux.- A.3 List of the Library Functions.- Symbols.
£94.99
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Spectroscopic Instrumentation: Fundamentals and Guidelines for Astronomers
Book SynopsisIn order to analyze the light of cosmic objects, particularly at extremely great distances, spectroscopy is the workhorse of astronomy. In the era of very large telescopes, long-term investigations are mainly performed with small professional instruments. Today they can be done using self-designed spectrographs and highly efficient CCD cameras, without the need for large financial investments.This book explains the basic principles of spectroscopy, including the fundamental optical constraints and all mathematical aspects needed to understand the working principles in detail. It covers the complete theoretical and practical design of standard and Echelle spectrographs. Readers are guided through all necessary calculations, enabling them to engage in spectrograph design. The book also examines data acquisition with CCD cameras and fiber optics, as well as the constraints of specific data reduction and possible sources of error. In closing it briefly highlights some main aspects of the research on massive stars and spectropolarimetry as an extension of spectroscopy. The book offers a comprehensive introduction to spectroscopy for students of physics and astronomy, as well as a valuable resource for amateur astronomers interested in learning the principles of spectroscopy and spectrograph design.Trade Review“It is a comprehensive volume that includes all the fundamental optics concerned with the components of spectrographs and their construction. … this is a text that will readily find a place on my bookshelf. It is a volume to which I expect to refer frequently, particularly in my efforts to develop spectrographs for future space missions.” (Martin Barstow, The Observatory, Vol. 135 (1249), December, 2015)Table of ContentsPrologue.- Fundamentals of standard spectroscopy.- The construction of a grating spectrograph.- Fundamentals of Echelle spectroscopy.- The construction of an Echelle spectrograph.- Other designs.- Practical examples.- Image Slicer.- CCD.- Fiber optics.- Data reduction.- Measurement errors and statistics.- Practical Observations.- The next step – Polarization.- Epilogue.- Acknowledgements.- Appendices.
£85.49
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Tools of Radio Astronomy
Book SynopsisThis 6th edition of “Tools of Radio Astronomy”, the most used introductory text in radio astronomy, has been revised to reflect the current state of this important branch of astronomy. This includes the use of satellites, low radio frequencies, the millimeter/sub-mm universe, the Cosmic Microwave Background and the increased importance of mm/sub-mm dust emission. Several derivations and presentations of technical aspects of radio astronomy and receivers, such as receiver noise, the Hertz dipole and beam forming have been updated, expanded, re-worked or complemented by alternative derivations. These reflect advances in technology. The wider bandwidths of the Jansky-VLA and long wave arrays such as LOFAR and mm/sub-mm arrays such as ALMA required an expansion of the discussion of interferometers and aperture synthesis. Developments in data reduction algorithms have been included. As a result of the large amount of data collected in the past 20 years, the discussion of solar system radio astronomy, dust emission, and radio supernovae has been revisited. The chapters on spectral line emission have been updated to cover measurements of the neutral hydrogen radiation from the early universe as well as measurements with new facilities. Similarly the discussion of molecules in interstellar space has been expanded to include the molecular and dust emission from protostars and very cold regions. Several worked examples have been added in the areas of fundamental physics, such as pulsars. Both students and practicing astronomers will appreciate this new up-to-date edition of Tools of Radio Astronomy. Trade ReviewAus den Rezensionen zur 6.Auflage: “... Studenten und Absolventen einschlägiger Fachrichtungen ist das Buch auch fur Quereinsteiger und Amateure geeignet, die ernsthaft in dieses Fachgebiet eindringen wollen.“ (in: Funkamateur, Heft 5, 2014)Table of ContentsRadio Astronomical Fundamentals.- ElectromagneticWave Propagation Fundamentals.- Wave Polarization.- Signal Processing and Receivers: Theory.- Practical Receiver Systems.- Fundamentals of Antenna Theory.- Practical Aspects of Filled Aperture Antennas.- Single Dish Observational Methods.- Interferometers and Aperture Synthesis.- Emission Mechanisms of Continuous Radiation.- Some Examples of Thermal and Nonthermal Radio Sources.- Spectral Line Fundamentals.- Line Radiation from Atoms.- Radio Recombination Lines.- Overview of Molecular Basics.- Molecules in Interstellar Space.- Some Useful Vector Relations & Fourier Transforms.- The Van Vleck Clipping Correction: One Bit Quantization.- Conventional Derivation of Square Law Detector Response & Receiver Noise.- The Reciprocity Theorem.- Filled Aperture Antennas.- The Hankel Transform.- Lists of Calibration Radio Sources.- The Mutual Coherence Function and van Cittert-Zernike Theorem.- Bibliography.- Index.
£34.99
Springer Position and Motion of Celestial Bodies
Book SynopsisPart I Position of Celestial Bodies.- Measurement of Position.- Representation of Position.- Part II Motion of Celestial Bodies.- Fundamentals of Celestial Mechanics.- Orbital Motion.- Rotational Motion.- Appendix A. Constants.- Appendix B. Mathematical Formulae.- Appendix C. Symbols.- Appendix D. Model Answers to Exercises.
£66.49
Springer The Dynamic Sun Astrophysics Space Science
Book SynopsisOur Sun is the nearest star and thus an ideal laboratory to study dynamic processes which are related to solar terrestrial physics.Table of ContentsPreface. List of Participants. Invited Lectures. Highlights from SOHO and Future Space Missions; B. Fleck. Solar Instrumentation; O. von der Lühe. Solar Activity Monitoring; M. Messerotti. Space Weather and the Earth's Climate; N.B. Crosby. Solar Magnetohydrodynamics; R.W. Walsh. The Navier-Stokes Equations and their Solution: Convection and Oscillation Excitation; M.P. Rast. Solar Polarimetry and Magnetic Field Measurements; J.C. del Toro Iniesta. Contributed Papers. High-Resolution Solar Imaging Using Blind Deconvolution; K. Hartkorn. The Trieste Solar Radio System: A Surveillance Facility for the Solar Corona; M. Messerotti, et al. Deconvolutions and Power Spectra of Solar Granulation; K.N. Pikalov, A. Hanslmeier. Computational Methods Concerning the Solar Granulation; W. Pötzi, et al. Solar Activity Monitoring and Flare Alerting at Kanzelhöhe Solar Observatory; M. Steinegger, et al. Analytical Modeling of Composed Cylindrical Magnetic Structures in the Corona; V.M. Cadez, et al. Physical Conditions in Solar Coronal Holes on the Base of Non-LTE Calculations; E. Malanushenko, E. Baranovsky. X-Ray Limb Flares with Plasma Ejections; K. Mikurda, et al. Coincidences between Magnetic Oscillations and Halpha Bright Points; P.F. Moretti, et al. Chromospheric Dynamics as can be Inferred from Sumer/SOHO Observations; J. Rybák, et al. Formation of Coronal Shock Waves; B. Vrsnak. Onset of Metric and Kilometric Type II Bursts; B. Vrsnak. Observations of NOAA 8210 Using MOF and DHC of Kanzelhöhe Solar Observatory; A. Warmuth, et al. On the Rigid Component in the Solar Rotation; R. Brajsa, et al. The Location of Solar Oscillations in the Photosphere; A. Hanslmeier, et al. High ResolutionObservations of a Photospheric Light Bridge; J. Hirzberger, et al. Phases of the 5-min Photospheric Oscillations above Granules and Intergranular Lanes; E.V. Khomenko. A Photometric and Magnetic Analysis of the Wilson Effect; M. Steinegger, et al. Modeling VIRGO Spectral and Bolometric Irradiances with MDI Data; M. Steinegger, et al. Generated Langmuir Wave Distribution of an Electron Beam Group; C. Estel, G. Mann. Magnetoacoustic Surface Waves at the Base of the Convection Zone; C. Foullon, B. Roberts. Small-Scale Magnetic Elements in 2-D Nonstationary Magnetogranulation; A.S. Gadun, S.K. Solanki. Multi-Mode Kink Instability as a Mechanism for &dgr;-Spot Formation; M.G. Linton. A Numerical Method for Studies of 3D Coronal Field Structures; Z. Romeou, T. Neukirch. Numerical Modeling of Transition Region Dynamics; L. Teriaca, J.G. Doyle. The Effect of Azimuthal Magnetic Field on the Magnetostatic Models of Sunspots; P.B. Tiwari. Comparison of Local and Global Fractal Dimension Determination Methods; A. Veronig, et al. Author Index.
£123.49
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Gesammelte Werke / Collected Works: Volume 2
Book SynopsisDer bekannte Astronom Karl Schwarzschild (1873-1916) gilt als der Begr}nder der Astrophysik und als hervorragender Forscher mit einer erstaunlichen Bandbreite seiner Interessen. Arbeiten zur Himmelsmechanik, Elektrodynamik und Relativit{tstheorie weisen ihn als vorz}glichen Mathematiker und Physiker seiner Zeit aus. Untersuchungen zur Photographischen Photometrie, Optik und Spektroskopie zeigen den versierten Beobachter, der sein Me~instrument beherrscht. Schlie~lich arbeitete Schwarzschild als Astrophysiker und an Sternatmosph{ren, Kometen, Struktur und Dynamikvon Sternsystemen. Die in seinem kurzen Leben entstandene F}lle von wissenschafltichen Arbeiten ist in drei B{nden der Gesamtausgabe gesammelt, erg{nzt durch biographisches Material und ein Essay des Nobelpreistr{gers S. Chandrasekhar und Annotationen von Fachleuten in jedem der drei B{nde.Table of Contents5. Astronomical Positioning.- 5.1 Ueber photographische Ortsbestimmung / On Photographic Position Determination.- 5.2 Über photographische Breitenbestimmung mit Hilfe eines hängenden Zenitkollimators / On Determining Latitude Using a Suspended Zenith Collimator.- 5.3 Über Breitenbestimmung mit Hilfe einer hängenden Zenitkamera / On Latitude Determination Using a Suspended Zenith Camera.- 5.4 Bestimmung der Polhöhe von Göttingen u. der Deklinationen von 375 Zenithsternen mit der hängenden Zenithkamera / Determination of the Altitude of the Pole at Göttingen and the Declination of 375 Zenith Stars Using the Suspended Zenith Camera (with W. Dziewulski).- 5.5 Über einen Transformator zur Auflösung sphärischer Dreiecke, besonders für Zwecke der Ortsbestimmung im Luftballon / On a Transformer for the Solution of Spherical Triangles, Especially for Position Determination in Air Balloons.- 5.6 Tafeln zur astronomischen Ortsbestimmung im Luftballon bei Nacht, sowie zur leichten Bestimmung der mitteleuropäischen Zeit an jedem Orte Deutschlands / Tables for Astronomical Position Determination in Air Balloons at Night and for Easy Determination of Central-European Time at any Point in Germany (with o. Birck).- 5.7 Künstlicher Horizont and Ballonsextant / Artificial Horizon and Balloon Sextant.- 5.8 Libellenhorizont und Libellensextant / Bubble Horizon and Bubble Sextant.- 6. Photographie Photometry.- 6.1 Die Bestimmung von Sternhelligkeiten aus extrafocalen photographischen Aufnahmen / The Determination of Stellar Magnitudes from Extrafocal Exposures.- 6.2 Beiträge zur photo graphischen Photometrie der Gestirne / Contributions on the Photographic Photometry of Stars.- 6.3 Ueber Abweichungen vom Reciprocitätsgesetz für Bromsilbergelatine / On Departures from the Reciprocity Law for Silver-Bromide Gelatine.- 6.4 Ueber die Wirkung intermittirender Belichtung auf Bromsilbergelatine / On the Effects of Intermittent Exposures on Silver-Bromide Gelatine.- 6.5 Bemerkungen zur Sensitometrie / Remarks on Sensitometry.- 6.6 über die photographische Vergleichung der Helligkeit verschiedenfarbiger Sterne / On the Photographic Comparison of the Magnitudes of Stars of Different Colours.- 6.7 Ueber sensitometrische Regeln und ihre astronomische Anwendung / On Sensitometry Laws and Their Astronomical Application.- 6.8 Professor G. Jägers Theorie des photographischen Prozesses / Professor G. Jäger’sf Theory of the Photographic Process.- 6.9 Plan zur Durchführung einer photographisch-photometrischen Durchmusterung des nördlichen Himmels / Plan for Carrying Out a Photographic-Photometric Survey of the Northern Sky.- 6.10 Über eine Schraffierkassette zur Aktinometrie der Sterne / On a Schraffierkassette for Stellar Actinometry (with Br. Meyermann).- 6.11 Über eine Interpolationsaufgabe der Aktinometrie / On an Interpolation Problem in Actinometry.- 6.12 Aufnahmen des Sternhaufens h Persei mit Spiegeln von sehr großem öffnungsverhältnis / Exposures of the Cluster h Persei Using Mirrors with Very Large Aperture Ratios (with W. Villiger).- 6.13 Über eine neue Schraffierkassette / On a New Schraffierkassette (with Br. Meyermann).- 6.14 Über die Farbentönung der Sterne / On the Colour Tints of the Stars.- 6.15 Remarque sur la determination des grandeurs photographiques absolues / Note on the Determination of Absolute Photographic Magnitudes.- 6.16 Über die Bestimmung absoluter photographischer Helligkeiten / On the Determination of Absolute Photographic Magnitudes.- 6.17 Aktinometrie der Sterne der B.D. bis zur Grösse 7.5 in der Zone 0 ° bis + 20 ° Deklination. Teil A / Actinometry of B.D. Stars down to Magnitude 7.5 in the Zone between Declinations 0 ° and + 20 ° , Part A (with Br. Meyermann, A. Kohlschütter and O. Birck).- 6.18 Aktinometrie der Sterne der B.D. bis zur Grösse 7.5 in der Zone 0 ° bis + 20 ° Deklination. Teil B / Actinometry of B.D. Stars down to Magnitude 7.5 in the Zone between Declinations 0 ° and +20 ° , Part B (with Br. Meyermann, A. Kohlschütter, O. Birck and W. Dziewulski).- 6.19 Buchbesprechung / Book Review: J.A. Parkhurst, Yerkes Actinometry, Zone + 73 ° to + 90 °.- 6.20 Über die Schleierkorrektion bei der Halbgittermethode zur Bestimmung photographischer Sterngrößen / On the Correction for Fogging in the Half-Grating Method of Determining Photographic Stellar Magnitudes.- 6.21 Vorbemerkung zu / Introduction to: W. Dziewulski, Photographische Größen von Sternen in der Nähe des Nordpols / Photographic Magnitudes of Stars Near the North Pole.- 7. Measuring Techniques, Binary Stars, Variable Stars and Spectroscopy.- 7.1 Ueber Messung von Doppelsternen durch Interferenzen / On Measuring Double Stars by Interference Methods.- 7.2 Zur Bestimmung der Theilungsfehler von Maassstäben / On Determining Dividing Errors of Graduated Scales.- 7.3 Beitrag zur Bestimmung von Radialgeschwindigkeiten mit dem Objektivprisma / Contribution on the Determination of Radial Velocities with an Objective Prism.- 7.4 Einige Beobachtungen der Radialgeschwindigkeit von 0: Coronae borealis mit dem Objektivprisma / Some Observations of the Radial Velocity of 0: Coronae borealis with an Objective Prism.- 7.5 über die Radialgeschwindigkeit des Sterns 63 Tauri / On the Radial Velocity of the Star 63 Tauri.- 7.6 Präzisionstechnik und wissenschaftliche Forschung / Precision Engineering and Scientific Research.- 7.7 Spectral Classification of Stars (in German).- 7.8 Ein Verfahren der Bahnbestimmung bei spectroskopischen Doppelsternen / A Procedure for Deterrnining the Orbits of Spectroscopic Binaries.- 7.9 Beobachtungen von Veränderlichen Sternen und der Nova Aurigae / Observations of Variable Stars and of Nova Aurigae.- 7.10 Ein neuer Veränderlicher (41.1910 Tauri) in den Hyaden / A New Variable (41.1910 Tauri) in the Hyades.- 7.11 über den Lichtwechsel des Veränderlichen 41.1910 Tauri / On the Variations in Brightness of the Variable 41.1910 Tauri.- 7.12 Nova 18.1912 Geminorum (Bemerkung zum Spektrum der Eneboschen Nova) /Nova 18.1912 Geminorum (Remark on the Spectrum of Enebo’s Nova).- 7.13 Der neue Stern in den Zwillingen / The New Star in the Constellation Gemini.- for Volume 1.- for Volume 3.
£119.99
Springer Calibration of Fundamental Stellar Quantities: Proceedings of the 111th Symposium of the International Astronomical Union held at Villa Olmo, Como, Italy, May 24–29, 1984
Book SynopsisIAU Symposium No. 111, "Calibration of Fundamental Stellar Quanti- ties", was held at Villa Olmo, Como, Italy, on May 24-29, 1984. Meet- ings held in the past ten years on related topics include: IAU Symposium No. 109, '*Astrometric Techniques", held at the University of Florida in Jan. , 1984, "The MK Process and Stellar Classification", held at the University of Toronto in June, 1983, "Stellar Absolute Energy Distri- butions", an unpublished Joint Meeting (Commissions 25 and 45), held at the General Assembly of the IAU in Patras, Greece in August, 1982, IAU Colloquium No. 62, "Current Techniques in Double and Multiple Star Re- search", held at Northern Arizona University in May, 1981, the ESO Work- fl shop: "Methods of Abundance Determination for Stars , held in Geneva in March, 1980, "Problems of Calibration of Multicolor Photometric Sys tems", held at Dudley Observatory in March, 1979, IAU Colloquium No. 48, "Modern Astrometry", held at the University of Vienna in Sept. , 1978, IAU Colloquium No. 50, "High Angular Resolution Stellar Interferometry" held at the University of Maryland in Aug. , 1978, "Spectral Classifice. - tion of the Future", held at the Vatican in July, 1978 and IAU Sympos- ium No. 72, "Abundance Effects in Classification", held at the Univer- sity of Lausanne in July, 1975. The present meeting was the first to cover the broad range of the calibration of fundamental stellar qU8T". ti- ties in one meeting. Nine commissions of the IAU co-sponsored the meeting.Table of Contents1. Review Papers.- 1.1 Standard Stars.- The Choice of Standard Stars.- (Papers on stellar radial velocities may be found on pp. 583 and 587.).- The Use and Abuse of Standard Stars.- (Related papers may be found on pp. 353 and 357.).- 1.2 Parallaxes and Proper Motions.- Trigonometric Parallaxes and Their Calibration.- The Determination of Fundamental Proper Motions.- (Related papers may be found on pp. 36 – 381 and 601.).- 1.3 Information Obtained from Binary Systems.- Positional Astronomy and Stellar Masses.- Masses, Radii and Luminosities from Analysis of Eclipsing Binaries.- The Calibration of Interferometrically Determined Properties of Binary Stars.- (Related papers may be found on pp. 385 – 401.).- 1.4 Stellar Classification.- The MK Classification and Its Calibration.- (Related papers may be found on pp. 403 – 415.).- 1.5 Abundances.- How Precise are Spectroscopic Abundance Determinations Today?.- (Related papers may be found on pp. 417 – 443.).- 1.6 Stellar Rotation.- Determination of Stellar Rotational Velocities.- 1.7 Angular Diameters.- Measuring Stars with High Angular Resolution: Results from Narrabri Observatory.- Measuring Stars with High Angular Resolution: Current Status and Future Prospects.- (Related papers may be found on pp. 447 – 459.).- 1.8 Spectrophotometry.- The Role of Space Observations in the Calibration of Fundamental Stellar Quantities.- Stellar Absolute Fluxes and Energy Distributions from 0.32 to 4.0 ?m.- (Related papers may be found on pp. 463 – 479.).- 1.9 Photometry.- Approaches to Photometric Calibrations.- Calibration in Temperature of Photometric Parameters.- The Calibration of Photometric Determinations of Abundance.- (Related papers may be found on pp. 485 – 565.).- 1.10 Model Atmospheres.- Fundamental Parameters and Models Of Stellar Atmospheres.- (Related papers may be found on pp. 569 – 581.).- 1.11 Data Banks and Summary.- Standard Values and Information in Data Banks.- Calibration of Fundamental Stellar Quantities: Summary and Conclusions.- 2. Contributed Papers.- The Microfiche of Standard Stars.- Standard Astronomical Sources for the Space Telescope.- The Open Cluster M67 as A Fundamental Standard of Reference for Stellar Properties.- White Dwarf Candidates for Trigonometrical Parallax Determinations.- The Absolute Magnitudes of the Nearby Stars: Calibrations of Mean Luminosity Relations.- Fifteen Years of Statistical Parallaxes by the Principle of Maximum Likelihood.- An Empirical H? -Luminosity Calibration.- The Wilson-Bappu Effect for Mg II k-Line Emission Widths.- The Influence of an Outflowing Gaseous Stream on the Determination of Masses of Semidetached Binary Systems.- The Absolute Dimensions and Masses of IQ Persei.- Un Diagramme Fondamental Luminosite-Type Spectral Pour Les Etoiles Doubles.- Visual Binaries and the Calibration of the Main Sequence.- Rotational Properties and Synchronization in Early-Type Close Binaries.- UV Standard Stars by the Variable Procrustean Bed Approach.- MKJ and MSS Classification of Solar-Type Stars within 100 Parsecs of the Sun: Preliminary Results.- UV Spectral Classification of B Stars.- Spectral Anomalies in the Hyades and Pleiades and in Field Stars with Active Chromospheres.- A New Analysis of the Abundance Standards ? Herculis and ? Scorpii.- Elemental Abundances of Normal Sharp-Lined B and A Stars from Optical Region Analyses.- The Relation between the Anomalous Cn Strength, ? Cn, and [Fe/H] Abundances.- On the Gravity Determination from Carbon Star Spectra.- A Note on the Calibration of Effective Temperatures.- The Be II ? 3l30 A Region in the Spectra of Vega and Sirius.- Mount Wilson Spectra of Standard Stars.- About the Photometric Calibration of IUE High Resolution Spectra: Quantification of the Order-Overlap for the SWP Camera.- Determination des diametres stellaires par occultations. Technique de reduction.- Standard Stars for the Comparison of Methods of Diameter Determination.- A Comparison of Direct and Indirect Methods of Determination of Stellar Angular Diameters.- Problems Concerning Planck’s Blackbody Law.- Effective Temperatures of Stars with “Standard” Angular Diameters.- Faint Secondary Standards for Spectrophotometry and the Energy Distributions of Horizontal-Branch A-Stars.- High Precision Solar Radiation Data for ??3300 – 12500 Å.- The New Observing Station at the Pic Du Midi Observatory for the Absolute Calibration of Stellar Radiation.- The Status of the Absolute Calibration of Stellar Fluxes between 912 and 1200 Å.- Secondary Standard Stars in the Four-Color System.- A Preliminary Luminosity Calibration of the uvby,? Systems for Supergiant F-Type Stars.- On Photometric Standards and Color Transformation.- An Empirical Calibration of the Strömgren System for Late-Type Stars.- Analysis of uvby Photometry and Low-Resolution Spectrophotometry of B-Stars.- The Stability and Accuracy of the uvby System.- On the Calibration of the uvby Photometric System for Late-Type Stars.- Steps toward A Physical Calibration of UBV Photometry.- Calibration of Photometric Systems from Homogeneous Spectrophotometric Data.- An Improvement in the Visual Surface-Brightness Scale for B5 — F5 Main-Sequence Stars.- The Response Function S(?) of the UBV Color System — A Problem Again and again?.- On the Observational Determination of OB Standards.- An Effective Temperature Calibration of A uv-Visual Photometric Index for “Normal” Non-Supergiant Stars.- The Determination of Teff for Candidate Standard Stars Based on Comparison with Model Atmospheres.- The Effect of Metallicity and Pulsation on the Infrared Colors of Luminous M Giants.- The Temperature Scale of G and K Subgiants.- On the Accuracy of Infrared Photometry.- Mv and Teff of B-Type Stars as Derived from 13-Color Photometry.- The Estimation of the Electron Density ne with a Narrow-Band Photometric System Calibrated by Model Atmospheres.- A Reddening and Metallicity-Free Temperature Estimator for Late M Giants.- On the Homogenization of Photometric Data.- Spectroscopic Gravity Estimates for Late-Type Giants: Arcturus as an Example.- The Temperatures of G and K Stars.- The Chemical Evolution of the Galactic Disc, Investigated by Abundance Analysis of F Stars: A Progress Report.- LTE-Blanketed and Unblanketed Models for SDO Stars.- The Zero-Point of the IAU Standard Velocity System.- Precise Radial Velocities and Radial Velocity Standards.- Standard Pulsars: Probes for the Calibration of the Galactic Continuum Background Temperature and the Electron Density of the Interstellar Medium.- The Calibration of Stellar Spectra Used in Measurements of the Generalized Compton Shift.- Recent Trigonometric Parallax Measurements of Mk Late-Type Spectral Standard Giant Stars.- The Determination of Extinction and Temperature for the Central Star of the Planetary Nebula NGC 40.- The Microfiche of Standard Stars.- Resolution Passed by the Participants; Discussion of Suggestion by Code.- Closing Remarks by R. Hanbury Brown, President of the IAU.- Pictures of participants.- Random Quotes.- Name Index.- Object Index.
£42.74
The University of Chicago Press Galileos Instruments of Credit
Book SynopsisFocusing on the aspects of Galileo's scientific life that extended beyond court culture and patronage, this title offers an account of the different systems of exchanges, communication, and credibility at work in Galileo's career. It is intended for readers interested in the history of astronomy and the history of science in general.Trade Review"Biagioli reinterprets key episodes of Galileo's career and shows how his tactics rapidly shifted to match his changing circumstances. His study presents a fresh and interesting view of the challenges faced by the seventeenth-century scientist." - Antony Anderson, New Scientist"
£26.00
John Wiley & Sons Inc Interpreting Astronomical Spectra Paper
Book SynopsisInterpreting Astronomical Spectra D.Table of ContentsRadiative Transfer and Model Atmospheres. Microscopic Processes and Statistical Equilibrium. Line Profiles. Line Formation. Stellar Spectra. Photoionized Clouds-Gaseous Nebulae and AGN. Photoionized Clouds-AGN. The Spectrum of the Cold Interstellar Medium. Masers. Wind and Circumstellar Shells. Very Hot Thin Gases and Coronae. Appendices. Select Bibliography. Index.
£111.56
MP-NMX Uni of New Mexico The Adaptive Optics Revolution A History
Book SynopsisA compilation of a unique history of the invention of laser guide stars and other contributions to adaptive optics made by the Department of Defense.
£26.96
Springer New York Binocular Astronomy
Book Synopsis“Binocular Astronomy”, 2nd edition, extends its coverage of small and medium binoculars to large and giant (i.e., up to 300mm aperture) binoculars and also binoviewers, which brings the work into the realm of serious observing instruments.Table of ContentsWhy Binoculars?.- Binocular Optics and Mechanics.- Choosing Binoculars.- Evaluating Binoculars.- Care and Maintenance of Binoculars.- Mounting Binoculars.- Binocular Telescopes.- Accessories.- Observing Techniques.- 200 Objects for Binoculars.
£37.99
Chelsea House Publishers Edward Pickering and His Women Computers: Analyzing the Stars
£29.71
ISTE Ltd and John Wiley & Sons Inc Observers of the Aurora Borealis in Europe:
Book SynopsisThe spectacular reappearance of the aurora borealis at the beginning of the 18th century, often observed simultaneously from different observatories in Europe, mobilized and federated a large community of astronomers on a European scale. It encouraged them to communicate the results of their observations and, in compiling exhaustive catalogs of information, has helped to establish a system of the aurora borealis that can be further studied in the future, according to the experimental method inherited from the previous century. This book is dedicated to some of the main aurora observers in Europe and to the human, institutional and philosophical context in which they evolved in the first half of the 18th century. Its reading should be seen as a retrospective journey through the scholarly world of the Enlightenment, during which the same scholars are frequently encountered and reencountered, yet each time in different contexts, or from different angles, with the aim of compiling an account of the swarming of ideas and encounters that constituted the development of experimental science in this pivotal period.Table of ContentsIntroduction ix Chapter 1 The Aurora Borealis Issue of the Affirmation of the Cartesian Mechanism and the Dispute Between Paris and Montpellier: The French Choice 1 1.1 Introduction 1 1.2 The two main systems of the aurora borealis 2 1.2.1 Halley’s system 2 1.2.2 Mairan’s system 5 1.3 History of the aurora borealis in the volumes of the Académie Royale des Sciences between 1716 and 1733 8 1.3.1 The silence on Halley’s system in Mémoires and Histoire 8 1.3.2. The memoir refused by the Parisian Academy of François de Plantade .. 13 1.4 The Montpellier actors: François de Plantade and the Société Royale des Sciences 20 1.4.1 François de Plantade, founder of the Société Royale de Montpellier 20 1.4.2 The Société Royale des Sciences de Montpellier 21 1.5 The Parisian actors: Bernard le Bovier de Fontenelle and Jean-Jacques Dortous de Mairan, the Académie Royale des Sciences 26 1.5.1 The Académie Royale des Sciences 26 1.5.2 The permanent secretary Bernard le Bovier de Fontenelle 30 1.5.3 Jean-Jacques Dortous de Mairan 37 1.6 The London actors: Hans Sloane and Edmond Halley, the Royal Society 43 1.6.1 Hans Sloane 43 1.6.2 Edmond Halley 45 1.6.3 The Royal Society and its relations with the Académie Royale des Sciences 49 1.7 Discussion of the reasons for rejecting Plantade’s submission 51 Chapter 2 Joseph-Nicolas Delisle: Grandeur and Vicissitudes of a Newtonian Scientist with Thwarted Ambitions 55 2.1 Introduction 55 2.2 Delisle in the period before his departure for Russia (1710–1725) 61 2.2.1 Delisle’s beginnings in astronomy and optics, a Newtonian 61 2.2.2 Delisle’s setbacks at the Académie Royale des Sciences 71 2.2.3 Delisle’s great project: Histoire Céleste 83 2.2.4 Epilogue concerning the Parisian period 89 2.3 The invitation to St Petersburg and Delisle’s Russian period (1726–1747) 90 2.3.1 The cartographic objective of Delisle’s mission 90 2.3.2 Delisle’s means at the St Petersburg Observatory 97 2.4 Brief synthesis of Delisle’s scientific trajectory 109 2.5 Conclusion 112 Chapter 3 The Creation Ex-nihilo and the Beginnings of the Imperial Russian Academy of Sciences: The Influence of Christian Wolff 115 3.1 Introduction 115 3.2 The foundation of the Imperial Academy of Sciences in St Petersburg 117 3.2.1 Historical context 117 3.2.2 Peter the Great’s Imperial Academy of Sciences project 120 3.2.3 The birth of astronomy in Russia 122 3.3 Christian Wolff, the aurora borealis and their first observers at the Academy of Sciences in St Petersburg 125 3.3.1 Historical context 125 3.3.2 Christian Wolff’s conference 126 3.3.3 The quartet of aurora observers at the Academy of Sciences of St Petersburg 131 3.3.4 The rejection of aurora observations by Mayer 135 3.3.5 Euler’s physical–mathematical explanation 143 3.3.6 Mayer’s philosophical position and possible reasons for his abandonment of aurora observation 146 3.4 The Imperial Academy of Sciences of St Petersburg 149 3.4.1 The setting up of the Academy 149 3.4.2 The clerical and noble opposition 151 3.4.3 Wolffians versus Newtonians 155 3.4.4. The problems of the functioning of the Academy in the decades 1730–1740 161 3.4.5 The regulation of 1748 refounding the Academy 164 3.5 Conclusion 167 Chapter 4 Anders Celsius and the European Observation Networks, Setting Up a Science Society and an Astronomical Observatory in Uppsala 171 4.1 Introduction 171 4.2 The life of Celsius 173 4.2.1 The first years 173 4.2.2 The European journey 176 4.2.3 Maupertuis’ expedition in Lapland 179 4.2.4 The last few years 181 4.3 Three European networks for the observation of natural phenomena 184 4.3.1 The observations of the aurora borealis around de Mairan 185 4.3.2 Monitoring the variations of the magnetic needle according to Anders Celsius 190 4.3.3 Thermometry and meteorological records around Joseph-Nicolas Delisle 199 4.4 The Royal Society of Uppsala and Celsius’ legacy 211 4.4.1 Historical context of the Enlightenment in Sweden 211 4.4.2 Birth and development of the Royal Society of Sciences in Uppsala 214 4.4.3 Relations between the Royal Society and the University 219 4.4.4 Celsius’ legacy 222 4.5 Conclusion 228 Chapter 5 Genesis of the Academies of Bologna and Berlin, the Involvement of Women in Astronomy and the Gender Issue 231 5.1 Introduction 231 5.2 Three examples of “astronomical households” 236 5.2.1. The Kirchs: an artisanal-type household inspired by the guild tradition 238 5.2.2 The Manfredis: a household with a humanistic coloration inherited from the Renaissance 247 5.2.3 The Delisle family: an artisanal household where women took care of the family scientific heritage 255 5.3 Two examples of astronomical institutions: the academies of Bologna and Berlin and their observatories 259 5.3.1 The Academy and the Bologna Observatory 262 5.3.2 The Academy and the Observatory of Berlin 270 5.4 Astronomical households, institutions and gender in Bologna and Berlin 280 5.5 Conclusion 287 Conclusion 289 Appendix 301 References 313 Index 331
£118.80
Springer International Publishing AG The Barnard Objects: Then and Now
Book SynopsisThe Barnard Objects have fascinated professional and amateur astronomers for over one hundred years. Many of those objects first imaged by E.E. Barnard on black-and-white photographic plates are now being captured daily in thousands of color astrophotographs. This book tells of Barnard’s story; describing his life and work as well as how the fields of astronomy and astrophotography have transformed ever since.The chapters in this book are equal parts history and science. It will provide readers with an introduction to nebula science and the incredible discoveries made in this field over the decades; including an overview of popular astronomical catalogues and a detailed look at how astronomical imaging has advanced since Barnard’s time, from early plates to digital imaging and chips. In addition, the book features a comprehensive guide to viewing and imaging these objects yourself. A glossary of astronomical and photographic terms is provided, along with detailed references. And, an updated table displaying the locations of these Barnard Objects; including the missing twenty-five objects from E.E. Barnard’s original catalogue.Richly researched and illustrated, this fascinating reference will attract astronomers of all skill levels interested in astrophotography and how it has changed over the past hundred years.Table of ContentsPreface Chapter 1. Introduction Chapter2. Nebulae – an overview Bright nebulae Dark nebulae Classical nebulae: HII regions, planetary nebulae, supernova remnants Diffuse nebulae Bok globules Chapter 3. Astronomical Catalogs – an overview Messier NGC IC Sharpless Cederblad DG Lynds Chapter 4. EE Barnard, his life, observations, and his catalogs Max Wolf (1863-1932) Objects discovered and named after Barnard Barnard’s awards and honors Catherine Wolfe Bruce (1816-1900) Bruce photographic telescopes (Yerkes, Mt. Wilson, Heidelberg) Comet observations, Comet Halley Planet observations Barnard’s star Barnard Objects Chapter 5. Visual Observation of Barnard Objects Astronomical League Dark Nebulae Observing Program Chapter 6. Modern Imaging of the Barnard Objects: images and imaging technique What to look for – nova, variable stars, change in nebulosity, astrometry, B&W and color imaging, history of color imaging Imaging techniques Chapter 7. Selected Important Barnard Objects Chapter 8. Filling in the Missing Barnard Objects- #176-200 Chapter 9. Conclusions Glossary and Table of Astronomical Catalogs Acknowledgements Index
£34.32
Springer International Publishing AG The NexStar Evolution and SkyPortal User's Guide
Book SynopsisThis book serves as a comprehensive guide for using a Nexstar Evolution mount with WiFi SkyPortal control, walking the reader through the process for aligning and operating the system from a tablet or smartphone. The next generation Go-To mount from Celestron, this is compatible not only with the Nextstar Evolution but also with older mounts. It is the ideal resource for anyone who owns, or is thinking of owning, a Nexstar Evolution telescope, or adapting their existing Celestron mount. Pros and cons of the system are thoroughly covered with a critical depth that addresses any possible question by users.Beginning with a brief history of Go-To telescopes and the genesis of this still new technology, the author covers every aspect of the newly expanding capability in observing. This includes the associated Sky Portal smartphone and tablet application, the transition from the original Nexstar GoTo system to the new SkyPortal system, the use of the Sky Portal application with its Sky Safari 4 basic software and Celestron WiFi adaptations, and discussions on the use of SkyPortal application using the Celestron adapter on older Celestron mounts. Comments and recommendations for equipment enable the reader to successfully use and appreciate the new WiFi capability without becoming overwhelmed. Extensively illustrated using actual screenshots from the program interface, this is the only guide to the Nextstar SkyPortal an observer will need.Table of ContentsPreface.- Chapter 1: A Brief History of Computerized Telescope Mounts for Amateurs.- Chapter 2: A Review of Celestron GoTo Computerized Telescopes.- Chapter 3: Introduction to the Celestron NexStar Evolution and Sky Portal.- Chapter 4: Basic Operation of the Celestron NexStar Evolution and SkyPortal App.- Chapter 5: Basic Operation of the Celestron NexStar Evolution and NexStar+ Hand Control.- Chapter 6: Lessons Learned in Using the Celestron NexStar Evolution and SkyPortal.- Chapter 7: Introduction to the SkyPortal WiFi Module.- Chapter 8: Advanced WiFi Tricks.- Chapter 9: Accessories for the Celestron NexStar Evolution.- Chapter 10: Mounting Other Optical Tubes on the NexStar Evolution Mounts.- Chapter 11: Maintenance and Care of the NexStar Evolution Mounts and Electronics.- Appendix 1: Troubleshooting Checklist.- Appendix 2: Celestron Timeline.- Appendix 3: Celestron NexStar Evolution Schmidt-Cassegrain Telescope Specifications.- Appendix 4: Messier Catalog.- Appendix 5: The Caldwell Catalog.- Appendix 6: Selected Non-Messier Catalog NGC Objects.- Appendix 7: The Herschel 400.- Appendix 8: Current Sky Portal WiFi Module Compatible Celestron Mount Specifications.- Appendix 9: Glossary.- Bibliography.- Biographies.- Index.
£28.49
Springer International Publishing AG Interferometry and Synthesis in Radio Astronomy
Book SynopsisThis book is open access under a CC BY-NC 4.0 license.The third edition of this indispensable book in radio interferometry provides extensive updates to the second edition, including results and technical advances from the past decade; discussion of arrays that now span the full range of the radio part of the electromagnetic spectrum observable from the ground, 10 MHz to 1 THz; an analysis of factors that affect array speed; and an expanded discussion of digital signal-processing techniques and of scintillation phenomena and the effects of atmospheric water vapor on image distortion, among many other topics.With its comprehensiveness and detailed exposition of all aspects of the theory and practice of radio interferometry and synthesis imaging, this book has established itself as a standard reference in the field. It begins with an overview of the basic principles of radio astronomy, a short history of the development of radio interferometry, and an elementary discussion of the operation of an interferometer. From this foundation, it delves into the underlying relationships of interferometry, sets forth the coordinate systems and parameters to describe synthesis imaging, and examines configurations of antennas for multielement synthesis arrays. Various aspects of the design and response of receiving systems are discussed, as well as the special requirements of very-long-baseline interferometry (VLBI), image reconstruction, and recent developments in image enhancement techniques and astrometric observations. Also discussed are propagation effects in the media between the source and the observer, and radio interference, factors that limit performance. Related techniques are introduced, including intensity interferometry, optical interferometry, lunar occultations, tracking of satellites in Earth orbit, interferometry for remote Earth sensing, and holographic measurements of antenna surfaces. This book will benefit anyone who is interested in radio interferometry techniques for astronomy, astrometry, geodesy, or electrical engineering.Trade Review“The authors of the book under review here to present a comprehensive discussion of the principles and applications of ‘Interferometry and Synthesis in Radio Astronomy.’ … the book delivers a comprehensive treatment of all aspects of interferometry and synthesis in a lucid and flowing tale that is a pleasure to read. The historical notes that are scattered throughout the text add flavor to the reading. … For all working in this field, the book is invaluable.” (Jacob W. M. Baars, The Radio Science Bulletin, Issue 361, June, 2017)Table of ContentsPreface.- Introduction and Historical Review.- Introductory Theory of Interferometry and Synthesis Imaging.- Analysis of the Interferometer Response.- Geometric Relationships and Polarimetry.- Antennas and Arrays.- Response of the Receiving System.- Design of the Analog Receiving System.- Digital Signal Processing.- Very-Long-Baseline Interferometry.- Calibration and Fourier Transformation of Visibility Data.- Deconvolution, Adaptive Calibration and Applications.- Interferometer Techniques for Astrometry and Geodesy.- Propagation Effects.- Van Cittert-Zernike Theorem, Spatial Coherence and Scattering.- Radio Interference.- Related Techniques.- Principal Symbols.- Index.
£41.79
Springer International Publishing AG Building and Using Binoscopes
Book SynopsisCovering both homemade and commercial products, this book provides the reader with simple and straightforward information about the modeling, building, and use of binoscopes. Binoscopes can be thought of as binoculars enlarged to the size of telescopes - essentially, a combination of the two. Constructing a binoscope is easier than most people think, but it still demands attention to detail and proper background knowledge. The author goes on to provide additional information about the products currently on the market, should the reader choose to purchase one instead of building it. Lastly, the book also compares binoscopes with telescopes in great detail, outlining the differences the reader can expect to see in the night sky from using both. The celestial views obtained with a binoscope, compared to a single telescope of the same aperture, are a very different experience.The new edition emphasizes the obvious advantages of viewing celestial objects through a binoscope. There are also many new photos and additional information on the latest equipment and some very special and rare equipment a collector might be interested in. Newly added cartoons and additional images of beautiful deep sky objects in each of the chapters makes reading the book a more enjoyable experience. Finally, there is a new comet discovery form and guide to follow for such discoveries, and a complete list of Messier objects for those interested in searching for these.Table of ContentsAbout the Author.- Why Binoscopes?- Optical Designs.- Binoculars Are Binoscopes.- Riverside Telescope Makers Conference (RTMC).- Homemade Binoscopes.- One of a Kind.- Odds and Ends.- Equatorial Drive Platforms.- Equatorial versus Altazimuth.- Binoculars of the Third Kind.- Appendix 1: Astronomical Formulae.- Appendix 2: Glossary.- Index.
£37.99
Springer International Publishing AG Astronomy of the Milky Way: The Observer’s Guide
Book SynopsisThis is the first of a two-volume set that deal with the entire Milky Way. This first volume looks at what can be seen predominantly from the Northern Skies. In addition to the descriptive text, there are many star charts and maps, as well as the latest up-to-date images made by observatories around the world and in space, as well as images taken by amateur astronomers.Trade Review“This updated edition … of Astronomy of the Milky Way is intended as a guide for amateur optical astronomers seeking interesting objects to investigate with their telescopes. … The book is recommended for amateur stargazers. … Summing Up: Recommended. General readers.” (D. E. Hogg, Choice, Vol. 55 (4), December, 2017)Table of Contents2nd Edition Preface.- 1st Edition Preface.- Acknowledgements.- Author's Note.- Chapter 1 The Milky Way.- Chapter 2 The Milky Way: July - August.- Chapter 3 The Milky Way: September - October.- Chapter 4 The Milky Way: November - December.- Appendices. Index of Objects.
£31.34
Springer Fachmedien Wiesbaden Sternbilderkunde: Himmelskarten, Himmelskörper,
Book SynopsisTable of Contents1 Himmelskarten.- Die Auswahl der richtigen Himmelskarte.- Wie man die Himmelskarte benutzt.- Die Helligkeit der Sterne.- Die scheinbare Bewegung der Fixsterne.- Der Sternenhimmel in verschiedenen geographischen Breiten.- Kartenteil.- Himmelskarten für geographische Breiten zwischen + 90° und + 60°.- Himmelskarten für geographische Breiten zwischen + 60° und + 30°.- Himmelskarten für geographische Breiten zwischen + 30° und 0°.- Himmelskarten für geographische Breiten zwischen 0° und - 30°.- Himmelskarten für geographische Breiten zwischen - 30° und - 60°.- Himmelskarten für geographische Breiten zwischen - 60° und - 90°.- 2 Himmelskörper.- Fixsterne und Planeten.- Kometen.- Sternschnuppen.- Größe des Sonnensystems.- Unsere Galaxie.- Veränderliche Sterne.- Planetarische Nebel.- Doppelsterne.- Sternhaufen.- Die Größe unserer Galaxie 89 Die anderen Galaxien.- 3 Die Sternbilder.- Kartenteil.- Achterschiff.- Adler.- Altar.- Andromeda.- Bärenhüter.- Becher.- Bildhauerwerkstatt.- Cepheus.- Chamäleon.- Chemischer Ofen.- Delphin.- Drache.- Dreieck.- Eidechse.- Einhorn.- Fernrohr.- Fische.- Fliege.- Fliegender Fisch.- Fluß Eridanus.- Fuchs.- Fuhrmann.- Füllen.- Giraffe.- Goldfisch.- Grabstichel.- Großer Bär.- Großer Hund.- Haar der Berenike.- Hase.- Herkules.- Inder.- Jagdhunde.- Jungfrau.- Kassiopeia.- Kiel des Schiffes.- Kleiner Bär.- Kleiner Hund.- Kleiner Löwe.- Kranich.- Krebs.- Kreuz.- Leier.- Löwe.- Luchs.- Luftpumpe.- Malerstaffelei.- Mikroskop.- Netz.- Nördliche Krone.- Nördliche Wasserschlange.- Oktant.- Orion.- Paradiesvogel.- Pegasus.- Pendeluhr.- Perseus.- Pfau.- Pfeil.- Phönix.- Rabe.- Schiffskompaß.- Schlange.- Schlangenträger.- Schütze.- Schwan.- Segel des Schiffes.- Sextant.- Skorpion.- Sobieskischer Schild.- Steinbock.- Stier.- Südliches Dreieck.- Südlicher Fisch.- Südliche Krone.- Südliche Wasserschlange.- Tafelberg.- Taube.- Tukan.- Waage.- Walfisch.- Wassermann.- Widder.- Winkelmaß.- Wolf.- Zentaur.- Zirkel.- Zwillinge.- Verzeichnisse und Zusammenstellungen.- Verzeichnis der Sternbildnamen.- Verzeichnis der Sternbilder.- Doppelsterne und Mehrfachsysteme.- Veränderliche Sterne.- Offene Sternhaufen, Kugelsternhaufen, Nebel, Galaxien.- Meteorströme.- Schrifttum und Quellen.- Register.- Gesamtregister.- Register der Sternbildnamen.- Register der Sternennamen und der besonderen.- Objekte.
£53.99
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Satellite Orbits: Models, Methods and
Book SynopsisThis modern presentation guides readers through the theory and practice of satellite orbit prediction and determination. Starting from the basic principles of orbital mechanics, it covers elaborate force models as well as precise methods of satellite tracking. The accompanying CD-ROM includes source code in C++ and relevant data files for applications. The result is a powerful and unique spaceflight dynamics library, which allows users to easily create software extensions. An extensive collection of frequently updated Internet resources is provided through WWW hyperlinks.Trade ReviewFrom the reviews: "Not many books on the topic of satellite orbits over the past decades have been informative, comprehensive and practical. I am happy to say that this publication does fall into that category. [...] This book should certainly be in the library of students and scientists working in the fields of navigation, geodesy, and spaceflight technology, as well as satellite engineers and operators focusing on spaceflight dynamics." (The Observatory, 2001) "Satellite Orbits: Models, Methods, and Application would be a valuable addition to the library of any engineer or scientist interested in the practical aspects of orbit prediction and determination. [...] The comprehensive reference list along with the CD supplied codes make this book unique in this area." (Applied Mechanics Reviews, 2002)Table of ContentsAround the World in a Hundred Minutes.- Introductory Astrodynamics.- Force Model.- Numerical Integration.- Time and Reference Systems.- Satellite Tracking and Observation Models.- Linearization.- Orbit Determination and Parameter Estimation.- Applications.
£66.49
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Principles of Star Formation
Book SynopsisUnderstanding star formation is one of the key fields in present-day astrophysics. This book treats a wide variety of the physical processes involved, as well as the main observational discoveries, with key points being discussed in detail. The current star formation in our galaxy is emphasized, because the most detailed observations are available for this case. The book presents a comparison of the various scenarios for star formation, discusses the basic physics underlying each one, and follows in detail the history of a star from its initial state in the interstellar gas to its becoming a condensed object in equilibrium. Both theoretical and observational evidence to support the validity of the general evolutionary path are presented, and methods for comparing the two are emphasized. The author is a recognized expert in calculations of the evolution of protostars, the structure and evolution of disks, and stellar evolution in general. This book will be of value to graduate students in astronomy and astrophysics as well as to active researchers in the field.Trade ReviewFrom the reviews:“This is an absolutely superb book, from the beginning of the preface, where the author provides a basic definition of star formation, to the last section where he reminds us that ‘efficiency’ of star formation can mean at least three different things, with three different numerical value … . The book concentrates on the interpretation of observations in star-forming regions relatively nearby, in our own Galaxy, at the present time, where the most detailed and accurate results can be obtained.” (Virginia Trimble, The Observatory, Vol. 132 (1226), February, 2012)Table of ContentsOverview.- Molecular Clouds and the Onset of Star Formation.- Protostar Collapse.- Rotating Protostars and Accretion Disks.- Massive Star Formation.- Formation of Binary Systems.- The Formation of the First Stars.- Pre-main-sequence Evolution.- Summary: Issues in Galactic Star Formation.- References.- Index.
£80.99
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Magnetosphere-Ionosphere Coupling
Book SynopsisIn the past two decades a succession of direct observations by satellites, and of extensive computer simulations, has led to the realization that the polar ionosphere plays a principal role in large-scale magnetospheric processes - a manifestation of the physics linkage involved in solar-terrestrial interactions. Spatial/temporal variations in high-latitude electromagnetic phenomena, such as dynamic aurorae, electric fields and currents, have proved to be extremely complex. Now the challenge is to comprehend the vast amount of complicated measurements made in this magnetosphere-ionosphere sysstem of the Earth. This book addresses the electrical coupling between the hot, but dilute, magnetospheric plasma and the cold, but dense, plasma in the ionosphere. In five major chapters, this book presents: - basic properties of magnetosphere-ionosphere coupling; - morphology of electric fields and currents at high latitudes; - global modeling of magnetosphere-ionosphere coupling; - modeling of ionospheric electrodynamics; - current issues, such as auroral particle acceleration, substorms, penetration of high-latitude fields into low latitudes.Table of Contents1 Implications of Magnetosphere-Ionosphere Coupling.- 1.1 Solar Wind, Magnetosphere, and Ionosphere.- 1.1.1 Entry of Energy into the Magnetosphere.- 1.1.2 Dissipation of Energy in Substorms.- 1.2 Basic Properties of Magnetosphere-Ionosphere Coupling.- 1.2.1 Global and Local Coupling Processes.- 1.2.2 Plasma Convection.- 1.2.3 Theoretical Approach.- 2 Morphology of Electric Fields and Currents at High Latitudes.- 2.1 Large-Scale Current Systems.- 2.1.1 Convection Electrojets.- 2.1.2 Substorm Current Wedge.- 2.1.3 Polar Cap and Cusp Currents.- 2.1.4 Eastward Current in the Dawn Sector.- 2.1.5 Current Closure in the Magnetosphere.- 2.1.6 Charge Carriers of Field-Aligned Currents.- 2.2 Electric Field and Currents Associated with Auroral Forms.- 2.2.1 Auroral Arcs.- 2.2.2 Westward Traveling Surges.- 2.2.3 Auroral Omega Bands.- 2.2.4 Pulsating Auroral Patches.- 3 Global Modeling of Magnetosphere-Ionosphere Coupling.- 3.1 Basic Concepts.- 3.2 Simulation of Magnetospheric Convection.- 3.2.1 Global Convection Model.- 3.2.2 Plasma Transport Model.- 3.3 Reproduction of Observed Features.- 3.4 Coupling Models with Specific Physical Aspects.- 4 Modeling of Ionospheric Electrodynamics.- 4.1 Ionospheric Parameters Controlled by Field-Aligned Currents.- 4.1.1 Basic Algorithm.- 4.1.2 Quiet Periods.- 4.1.3 Substorm Times.- 4.1.4 Cusp Structure.- 4.2 Magnetogram-Inversion Technique.- 4.2.1 Essence of the Scheme.- 4.2.2 Advantages and Limitations.- 4.2.3 Global Distribution of Ionospheric Parameters.- 4.2.4 Recent Improvements.- 4.3 Formation of Auroral Arcs.- 5 Current Issues in Magnetosphere-Ionosphere Coupling.- 5.1 The Westward Traveling Surge.- 5.1.1 Dynamics.- 5.1.2 Distortion of Convection Pattern.- 5.1.3 Pulsations.- 5.2 Auroral Particle Acceleration and Parallel Electric Fields.- 5.2.1 Observations.- 5.2.2 Theories and Computer Simulations.- 5.3 Penetration of High-Latitude Electric Fields / into Low Latitudes.- 5.3.1 Substorm Effects.- 5.3.2 Source Mechanisms.- 5.3.3 Global Patterns of Ionospheric Fields.- 5.3.4 Shielding of Convection Fields in the Magnetosphere.- 5.4 Relative Importance of Conductivities and Electric Fields..- 5.4.1 Simultaneous Measurements of Ionospheric Parameters.- 5.4.2 Two Electrojet Modes.- 5.4.3 Latitudinal Cross-Sections of the Auroral Electrojets.- 5.4.4 Implications for Substorm Dynamics.- 5.4.5 Future Problems.- References.
£42.74
