Astronomical observation Books
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
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG The Chang’E-1 Topographic Atlas of the Moon
Book SynopsisThis atlas is based on the lunar global Digital Elevation Models (DEM) of Chang'E-1 (CE-1), and presents CCD stereo image data with digital photogrammetry. The spatial resolution of the DEM in this atlas is 500m, with horizontal accuracy of 192m and vertical accuracy of 120m. Color-shaded relief maps with contour lines are used to show the lunar topographical characteristics. The topographical data gathered by CE-1 can provide fundamental information for the study of lunar topographical, morphological and geological structures, as well as for lunar evolution research.Trade Review“This lovely, featured book will have you easily finding your way about the lunar surface. … I recommend ‘The Chang’E-1 Topographic Atlas of the Moon’ by Chunlai Li, Jianjun Liu, Lingli Mu, Xin Ren and Wei Zuo. It may guide you to all sorts of interesting features and finds.” (Mark Mortimer, Universe Today, universetoday.com, March, 2016)Table of ContentsPart I Introduction of the CCD Stereo Camera.- Part II Global topographic map of the Moon by CD-1.- Part III Subdivision topographic maps of the Moon.- Appendix – Gazetteer.
£123.49
Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Im Kosmos zu Hause: Wie astronomische Fotografien
Book SynopsisWir Menschen wissen bereits seit über 400 Jahren, dass wir uns unverschämterweise nicht im Zentrum des Universums befinden. Dennoch war die Überraschung groß, als mit Beginn der Raumfahrt die ersten Fotografien der blauen Erdkugel auftauchten. Umweltaktivisten erschraken vor der Fragilität der Atmosphäre, Philosophinnen distanzierten sich vom Menschen und Landschaftsfotografen entdeckten fremde Welten in der bereits bekannten. Bernd Pröschold hat in Wüstenlandschaften, im Erdorbit und sogar in der Tiefsee außerirdisch anmutende Motive aufgespürt und zu einem essayistischen Bildband im Querformat verarbeitet. Vor kosmischer Kulisse zeichnet er die Konturen eines zweibeinigen Wesens, dessen Schicksal viel enger mit dem Weltall verwoben ist, als unsere Alltagserfahrung es erahnen lässt. Wir begeben uns auf einen visuellen Streifzug durch extraterrestrische Bildwelten, bereichert durch Zitate und Anekdoten – ein Muss für alle Naturfreunde, Philosophen und Weltraum-Fans.Table of Contents1 Ein neues Weltbild.- 2 Der Overview-Effekt.- 3 Entgrenzungserfahrung.- 4 Entgrenzungsphysik.- 5 Der Underview-Effekt.- 6 Kosmische Landschaften.- 7 Lichter der Nacht.
£31.34
Springer Spacecraft Attitude Determination and Control
Book SynopsisRoger D. Werking Head, Attitude Determination and Control Section National Aeronautics and Space Administration/ Goddard Space Flight Center Extensiye work has been done for many years in the areas of attitude determination, attitude prediction, and attitude control. During this time, it has been difficult to obtain reference material that provided a comprehensive overview of attitude support activities. This lack of reference material has made it difficult for those not intimately involved in attitude functions to become acquainted with the ideas and activities which are essential to understanding the various aspects of spacecraft attitude support. As a result, I felt the need for a document which could be used by a variety of persons to obtain an understanding of the work which has been done in support of spacecraft attitude objectives. It is believed that this book, prepared by the Computer Sciences Corporation under the able direction of Dr. James Wertz, provides this type of reference. This book can serve as a reference for individuals involved in mission planning, attitude determination, and attitude dynamics; an introductory textbook for stu dents and professionals starting in this field; an information source for experimen ters or others involved in spacecraft-related work who need information on spacecraft orientation and how it is determined, but who have neither the time nor the resources to pursue the varied literature on this subject; and a tool for encouraging those who could expand this discipline to do so, because much remains to be done to satisfy future needs.Table of ContentsI—Background.- 1. Introduction.- 1.1 Representative Mission Profile.- 1.2 Representative Examples of Attitude Determination and Control.- 1.3 Methods of Attitude Determination and Control.- 1.4 Time Measurements.- 2. Attitude Geometry.- 2.1 The Spacecraft-Centered Celestial Sphere.- 2.2 Coordinate Systems.- 2.3 Elementary Spherical Geometry.- 3. Summary of Orbit Properties and Terminology.- 3.1 Keplerian Orbits.- 3.2 Planetary and Lunar Orbits.- 3.3 Spacecraft Orbits.- 3.4 Orbit Perturbations.- 3.5 Viewing and Lighting Conditions.- 4. Modeling the Earth.- 4.1 Appearance of the Earth at Visual Wavelengths.- 4.2 Appearance of the Earth at Infrared Wavelengths.- 4.3 Earth Oblateness Modeling.- 4.4 Modeling the Structure of the Upper Atmosphere.- 5. Modeling the Space Environment.- 5.1 The Earth’s Magnetic Field.- 5.2 The Earth’s Gravitational Field.- 5.3 Solar Radiation and the Solar Wind.- 5.4 Modeling the Position of the Spacecraft.- 5.5 Modeling the Positions of the Sun, Moon, and Planets.- 5.6 Modeling Stellar Positions and Characteristics.- II—Attitude Hardware and Data Acquisition.- 6. Attitude Hardware.- 6.1 Sun Sensors.- 6.2 Horizon Sensors.- 6.3 Magnetometers.- 6.4 Star Sensors.- 6.5 Gyroscopes.- 6.6 Momentum and Reaction Wheels.- 6.7 Magnetic Coils.- 6.8 Gas Jets.- 6.9 Onboard Computers.- 7. Mathematical Models of Attitude Hardware.- 7.1 Sun Sensor Models.- 7.2 Horizon Sensor Models.- 7.3 Sun Sensor / Horizon Sensor Rotation Angle Models.- 7.4 Modeling Sensor Electronics.- 7.5 Magnetometer Models.- 7.6 Star Sensor Models.- 7.7 Star Identification Techniques.- 7.8 Gyroscope Models.- 7.9 Reaction Wheel Models.- 7.10 Modeling Gas Jet Control Systems.- 8. Data Transmission and Preprocessing.- 8.1 Data Transmission.- 8.2 Spacecraft Telemetry.- 8.3 Time Tagging.- 8.4 Telemetry Processors.- 9. Data Validation and Adjustment.- 9.1 Validation of Discrete Telemetry Data.- 9.2 Data Validation and Smoothing.- 9.3 Scalar Checking.- 9.4 Data Selection Requiring Attitude Information.- III—Attitude Determination.- 10. Geometrical Basis of Attitude Determination.- 10.1 Single-Axis Attitude.- 10.2 Arc-Length Measurements.- 10.3 Rotation Angle Measurements.- 10.4 Correlation Angles.- 10.5 Compound Measurements—Sun to Earth Horizon Crossing Rotation Angle.- 10.6 Three-Axis Attitude.- 11. Single-Axis Attitude Determination Methods.- 11.1 Methods for Spinning Spacecraft.- 11.2 Solution Averaging.- 11.3 Single-Axis Attitude Determination Accuracy.- 11.4 Geometrical Limitations on Single-Axis Attitude Accuracy.- 11.5 Attitude Uncertainty Due to Systematic Errors.- 12. Three-Axis Attitude Determination Methods.- 12.1 Parameterization of the A ttitude.- 12.2 Three-Axis Attitude Determination.- 12.3 Covariance Analysis.- 13. State Estimation Attitude Determination Methods.- 13.1 Deterministic Versus State Estimation Attitude Methods.- 13.2 State Vectors.- 13.3 Observation Models.- 13.4 Introduction to Estimation Theory.- 13.5 Recursive Least-Squares Estimators and Kaiman Filters.- 14. Evaluation and Use of State Estimators.- 14.1 Prelaunch Evaluation of State Estimators.- 14.2 Operational Bias Determination.- 14.3 Limitations on State Vector Observability.- IV—Attitude Dynamics and Control.- 15. Introduction to Attitude Dynamics and Control.- 15.1 Torque-Free Motion.- 15.2 Response to Torques.- 15.3 Introduction to Attitude Control.- 16. Attitude Dynamics.- 16.1 Equations of Motion.- 16.2 Motion of a Rigid Spacecraft.- 16.3 Spacecraft Nutation.- 16.4 Flexible Spacecraft Dynamics.- 17. Attitude Prediction.- 17.1 Attitude Propagation.- 17.2 Environmental Torques.- 17.3 Modeling Internal Torques.- 17.4 Modeling Torques Due to Orbit Maneuvers.- 18. Attitude Stabilization.- 18.1 A utomatic Feedback Control.- 18.2 Momentum and Reaction Wheels.- 18.3 Autonomous Attitude Stabilization Systems.- 18.4 Nutation and Libration Damping.- 19. Attitude Maneuver Control.- 19.1 Spin Axis Magnetic Coil Maneuvers.- 19.2 Spin Plane Magnetic Coil Maneuvers.- 19.3 Gas Jet Maneuvers.- 19.4 Inertial Guidance Maneuvers.- 19.5 Attitude Acquisition.- V—Mission Support.- 20. Software System Development.- 20.1 Safeguards Appropriate for Mission Support Software.- 20.2 Use of Graphic Support Systems.- 20.3 Utility Subroutines.- 21. Software System Structure.- 21.1 General Structure for A ttitude Software Systems.- 21.2 Communications Technology Satellite Attitude Support System.- 21.3 Star Sensor Attitude Determination System.- 21.4 Attitude Data Simulators.- 22. Discussion.- VI—Appendices.- Appendix A—Spherical Geometry.- Appendix B—Construction of Global Geometry Plots.- Appendix C—Matrix and Vector Algebra.- Appendix D—Quaternions.- Appendix E—Coordinate Transformations.- Appendix F—The Laplace Transform.- Appendix G—Spherical Harmonics.- Appendix H—Magnetic Field Models.- Appendix I—Spacecraft Attitude Determination and Control Systems.- Appendix J—Time Measurement Systems.- Appendix K—Metric Conversion Factors.- Appendix L—Solar System Constants.- Appendix M—Fundamental Physical Constants.
£189.99
Springer Ultraviolet Stellar Spectra and Related Ground-Based Observations
Book SynopsisTwo years ago, just before the Prague meeting of the International Astronomical Union, Armin Deutsch made the bold suggestion that the space spectroscopists hold a joint symposium with the ground-based observers. At that time the rocket observa- tions of stellar spectra seemed too meagre to make such a meeting worthwhile, but we proceeded in the hope that there would be significant new results available by 1969. IAU Commissions 29 and 44, on Stellar Spectra and Observations from Outside the Terrestrial Atmosphere respectively, agreed to sponsor the symposium so that the organization was given to the Joint Working Group of these commissions. Conse- quently, the Organizing Committee, which met first in Prague, consisted of A. Deutsch, M. W. Feast, L. Houziaux, V. G. Kurt, N. G. Roman, J. Sahade, A. B. Underhill, and R. Wilson, with myself as Chairman. Later COSP AR was invited to join in spon- soring the symposium and T. Chubb was added as their representative. We were specially pleased when C. de Jager invited us to the Netherlands and offered the services of the Utrecht Observatory for the local organization. He suggested we hold the meeting at the new Lunteren Conference Centre located in a wooded area some 35 km east of Utrecht. The modern facilities of the Centre and the hospi- tality of its staff contributed much to the enjoyment of our four days there.Table of ContentsI / Stellar Fluxes.- A. Absolute Calibration.- 1. Absolute intensity calibration methods in the vacuum UV region.- 2. An investigation of the properties of vacuum-ultraviolet radiation detectors (Abstract).- 3. Recent absolute calibration work at Palomar Mountain.- 4. General discussion (On calibration methods).- B. Interstellar Extinction.- 1. Interstellar extinction (Introductory lecture).- 2. Ultraviolet interstellar extinction from a comparison of ? Persei and ? Pesei.- 3. Observations of interstellar extinction in the ultraviolet with the OAO satellite.- 4. On dielectric models of interstellar grains.- 5. Extinction curves for graphite-silicate grain mixtures.- 6. Measurement of interstellar extinction in emission line stars.- 7. The interstellar extinction curve from 4000 Å to 6500 Å.- C. Theoretical Models for Stellar Fluxes.- 1. The effective temperatures of the O stars.- 2. The effect of Silicon and Carbon opacity on ultraviolet stellar spectra.- D. Observed Stellar Fluxes.- 1. Review of ultraviolet and visual continuum observations and comparisons with models.- 2. The stellar temperature scale from 05 to A0.- 3. On ultraviolet fluxes, bolometric corrections and effective temperatures of late B to F stars.- 4. Far-ultraviolet intensities of Orion stars.- 5. Ultraviolet photometry of stars obtained with the Celescope experiment in the Orbiting Astronomical Observatory.- 6. Photographic magnitudes of 201 stars at 2600 Å.- 7. Spectrophotometrie integree des galaxies proches dans l’ultraviolet (expérience Persée).- 8. Low resolution stellar spectrophotometrie observations in the region 1500 Å–3000 Å.- 9. Absolute stellar photometry in the region 1200 Å–3000 Å.- 10. Preliminary note on the astronomical satellite Kosmos 215.- 11. Ultraviolet photometry of stars from OSO II.- 12. The ultraviolet solar opacity.- II / Stellar Line Spectra.- A. Rocket and Satellite Observations of Ultraviolet Spectra.- 1. Observations of ultraviolet stellar spectra.- 2. Photoelectric rocket spectra at 10 Å resolution (Abstract).- 3. Rocket spectroscopy of ? Puppis below 1100 Å.- 4. Observations of strong stellar lines with the OAO.- 5. The far-ultraviolet spectrum of ? Cassiopeiae.- 6. UV spectrophotometry of Canopus from Gemini XI.- B. Ground-Based Observations of Spectra Relevant to the Ultraviolet.- 1. Review of ground-based observations of spectra relevant to the ultraviolet.- 2. Chromospheric activity in red giants, and related phenomena.- 3. Mass loss from early-type stars.- C. Theory Relevant to UV Spectra.- 1. A discussion of the theory for interpreting ultraviolet stellar spectra.- 2. Possibility of fluorescence phenomena in the ultraviolet spectrum of symbiotic stars and long period variables.- 3. Radiative acceleration and ultraviolet resonance line profiles in OB supergiants.- 4. Stellar-wind theory for O and B stars (Abstract).- D. The Sun — a Typical G2V Star.- 1. Review of astrophysical conclusions from the UV solar spectra.- 2. Resonance lines in the solar chromosphere.- 3. On the contribution of solar activity to the ultraviolet spectrum of the Sun.- 4. Intensity distribution in the Lyman-? line at the solar limb.- 5. A high-resolution solar spectrum 2000 Å–2200 Å.- 6. Fabry-Pérot interferograms of the solar MgII resonance lines.- III / Interstellar Absorption and Emission.- A. Absorption Lines.- 1. Observations of interstellar Lyman-? absorption.- 2. Observations of interstellar Lyman-? with the Orbiting Astronomical Observatory.- 3. Interstellar lines other than hydrogen.- 4. Interstellar molecular hydrogen (Abstract).- 5. General discussion.- B. Emission.- 1. The night sky brightness measured from satellites Kosmos 51 and 213.- 2. Mariner 5 measurements of ultraviolet emission from the Galaxy.- 3. The ultraviolet background (intergalactic gas, the Galaxy, and subcosmic rays).- 4. Lyman-? radiation from nebular objects.- Space and ground-based stellar spectrophotometry: a summary.
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Springer Proceedings of the 7th International Workshop on the TianQin Science Mission 2526 April 2024 Hong Kong SAR China
Book Synopsis1. Ten Years of TianQin Project.- 2. A brief introduction to the TianQin project.- 3. Gravitational Wave Astrophysics with TianQin.- 4. Primordial Intermediate-mass Binary Black Holes as Targets for Space Laser Interferometers.- 5. Gravitational wave and radio observations of Galactic inspiraling double neutron stars.
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Book SynopsisAstrometry encompasses all that is necessary to provide the positions and motions of celestial bodies. This includes observational techniques, instrumentation, processing and analysis of observational data, reference systems and frames, and the resulting astronomical phenomena. This comprehensive reference will be invaluable for graduate students and research astronomers.Table of Contents1. Introduction; 2. New observational techniques; 3. Basic principles and coordinate systems; 4. Treatment of astronomical data; 5. Principles of relativity; 6. Apparent displacements of celestial objects; 7. Extragalactic reference frame; 8. Dynamical reference frame; 9. Terrestrial coordinate systems; 10. Earth orientation; 11. Stars; 12. Double and multiple star systems; 13. Astronomical phenomena; 14. Application of theory to observations; Appendices.
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