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New Millennium Solar Physics

  • Markus J.¬†Aschwanden
Book

Part of the Astrophysics and Space Science Library book series (ASSL, volume 458)

Table of contents

  1. Front Matter
    Pages i-xv
  2. Markus J. Aschwanden
    Pages 1-49
  3. Markus J. Aschwanden
    Pages 51-88
  4. Markus J. Aschwanden
    Pages 89-131
  5. Markus J. Aschwanden
    Pages 133-173
  6. Markus J. Aschwanden
    Pages 175-217
  7. Markus J. Aschwanden
    Pages 219-259
  8. Markus J. Aschwanden
    Pages 261-302
  9. Markus J. Aschwanden
    Pages 303-342
  10. Markus J. Aschwanden
    Pages 343-382
  11. Markus J. Aschwanden
    Pages 383-421
  12. Markus J. Aschwanden
    Pages 423-461
  13. Markus J. Aschwanden
    Pages 463-502
  14. Markus J. Aschwanden
    Pages 503-541
  15. Markus J. Aschwanden
    Pages 543-584
  16. Markus J. Aschwanden
    Pages 585-624
  17. Markus J. Aschwanden
    Pages 625-662
  18. Back Matter
    Pages 663-714

About this book

Introduction

This is a follow-on book to the introductory textbook "Physics of the Solar Corona" previously published in 2004 by the same author, which provided a systematic introduction and covered mostly scientific results from the pre-2000 era. Using a similar structure as the previous book the second volume provides a seamless continuation of numerous novel research results in solar physics that emerged in the new millennium (after 2000) from the new solar missions of RHESSI, STEREO, Hinode, CORONAS, and the Solar Dynamics Observatory (SDO) during the era of 2000-2018. The new solar space missions are characterized by unprecedented high-resolution imaging, time resolution, spectral capabilities, stereoscopy and tomography, which reveal the intricate dynamics of magneto-hydrodynamic processes in the solar corona down to scales of 100 km. The enormous amount of data streaming down from SDO in Terabytes per day requires advanced automated data processing methods. The book focuses exclusively on new research results after 2000, which are reviewed in a comprehensive manner, documented by over 3600 literature references, covering theory, observations, and numerical modeling of basic physical processes that are observed in high-temperature plasmas of the Sun and other astrophysical objects, such as plasma instabilities, coronal heating, magnetic reconnection processes, coronal mass ejections, plasma waves and oscillations, or particle acceleration. 

Keywords

Data Processing Methods Models of Physical Processes in High-temperature Plasmas RHESSI, STEREO, Hinode, CORONAS, SDO Solar Corona Physics Solar Corona Results from 21st Century Missions Solar Physics Instrumentation

Authors and affiliations

  • Markus J.¬†Aschwanden
    • 1
  1. 1.Solar & Astrophysics LaboratoryPalo AltoUSA

Bibliographic information

  • DOI https://doi.org/10.1007/978-3-030-13956-8
  • Copyright Information Springer Nature Switzerland AG 2019
  • Publisher Name Springer, Cham
  • eBook Packages Physics and Astronomy
  • Print ISBN 978-3-030-13954-4
  • Online ISBN 978-3-030-13956-8
  • Series Print ISSN 0067-0057
  • Series Online ISSN 2214-7985
  • Buy this book on publisher's site