Description

Book Synopsis

The volume of data being collected in solar astronomy has exponentially increased over the past decade and we will be entering the age of petabyte solar data. Deep learning has been an invaluable tool exploited to efficiently extract key information from the massive solar observation data, to solve the tasks of data archiving/classification, object detection and recognition.

Astronomical study starts with imaging from recorded raw data, followed by image processing, such as image reconstruction, inpainting and generation, to enhance imaging quality. We study deep learning for solar image processing. First, image deconvolution is investigated for synthesis aperture imaging. Second, image inpainting is explored to repair over-saturated solar image due to light intensity beyond threshold of optical lens. Third, image translation among UV/EUV observation of the chromosphere/corona, Ha observation of the chromosphere and magnetogram of the photosphere is realized by using GAN, exhibiting powerful image domain transfer ability among multiple wavebands and different observation devices. It can compensate the lack of observation time or waveband. In addition, time series model, e.g., LSTM, is exploited to forecast solar burst and solar activity indices.

This book presents a comprehensive overview of the deep learning applications in solar astronomy. It is suitable for the students and young researchers who are major in astronomy and computer science, especially interdisciplinary research of them.



Trade Review
“Each application is described with sufficient detail to give the reader an understanding of how AI is used and how its use compares with older tools used for the same purposes. The writing is clear … and an excessive use of acronyms. Relevant images and tables enhance the reader’s understanding; many references accompany each chapter. This book should appeal to those interested in either AI or the field of solar astronomy.” (G. R. Mayforth, Computing Reviews, November 22, 2023)

Table of Contents

Chapter 1: Introduction

Chapter 2: Classical deep learning models

Chapter 3: Deep learning in solar image classification tasks

Chapter 4: Deep learning in solar object detection tasks

· Active Region (AR) detection

· EUV waves detection

Chapter 5: Deep learning in solar image generation tasks

· Deconvolution of aperture synthesis

· Recovering over-exposed solar image

· Generating magnetogram from EUV image

· Generating magnetogram from H-alpha

Chapter 6: Deep learning in solar forecasting tasks

· Flare forecast

· F10.7c forecast

Deep Learning in Solar Astronomy

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£42.74

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RRP £44.99 – you save £2.25 (5%)

Order before 4pm tomorrow for delivery by Sat 27 Dec 2025.

A Paperback / softback by Long Xu, Yihua Yan, Xin Huang

5 in stock


    View other formats and editions of Deep Learning in Solar Astronomy by Long Xu

    Publisher: Springer Verlag, Singapore
    Publication Date: 28/05/2022
    ISBN13: 9789811927454, 978-9811927454
    ISBN10: 9811927456

    Description

    Book Synopsis

    The volume of data being collected in solar astronomy has exponentially increased over the past decade and we will be entering the age of petabyte solar data. Deep learning has been an invaluable tool exploited to efficiently extract key information from the massive solar observation data, to solve the tasks of data archiving/classification, object detection and recognition.

    Astronomical study starts with imaging from recorded raw data, followed by image processing, such as image reconstruction, inpainting and generation, to enhance imaging quality. We study deep learning for solar image processing. First, image deconvolution is investigated for synthesis aperture imaging. Second, image inpainting is explored to repair over-saturated solar image due to light intensity beyond threshold of optical lens. Third, image translation among UV/EUV observation of the chromosphere/corona, Ha observation of the chromosphere and magnetogram of the photosphere is realized by using GAN, exhibiting powerful image domain transfer ability among multiple wavebands and different observation devices. It can compensate the lack of observation time or waveband. In addition, time series model, e.g., LSTM, is exploited to forecast solar burst and solar activity indices.

    This book presents a comprehensive overview of the deep learning applications in solar astronomy. It is suitable for the students and young researchers who are major in astronomy and computer science, especially interdisciplinary research of them.



    Trade Review
    “Each application is described with sufficient detail to give the reader an understanding of how AI is used and how its use compares with older tools used for the same purposes. The writing is clear … and an excessive use of acronyms. Relevant images and tables enhance the reader’s understanding; many references accompany each chapter. This book should appeal to those interested in either AI or the field of solar astronomy.” (G. R. Mayforth, Computing Reviews, November 22, 2023)

    Table of Contents

    Chapter 1: Introduction

    Chapter 2: Classical deep learning models

    Chapter 3: Deep learning in solar image classification tasks

    Chapter 4: Deep learning in solar object detection tasks

    · Active Region (AR) detection

    · EUV waves detection

    Chapter 5: Deep learning in solar image generation tasks

    · Deconvolution of aperture synthesis

    · Recovering over-exposed solar image

    · Generating magnetogram from EUV image

    · Generating magnetogram from H-alpha

    Chapter 6: Deep learning in solar forecasting tasks

    · Flare forecast

    · F10.7c forecast

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