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Titlebook: Energetic Phenomena on the Sun; M. R. Kundu,B. Woodgate,E. J. Schmahl Book 1989 Springer Science+Business Media Dordrecht 1989 Corona.Plan

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发表于 2025-3-21 16:52:04 | 显示全部楼层 |阅读模式
书目名称Energetic Phenomena on the Sun
编辑M. R. Kundu,B. Woodgate,E. J. Schmahl
视频video
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Energetic Phenomena on the Sun; M. R. Kundu,B. Woodgate,E. J. Schmahl Book 1989 Springer Science+Business Media Dordrecht 1989 Corona.Plan
描述This publication is a result of three meetings, each 5 days long, held at the Goddard Space Flight Center on January 24-28, 1983, June 8-14, 1983, and February 13-17, 1984. The meetings were held in the interim between the full operations of the Solar Maximum Mission (SMM) in 1980, and the renewed operations after its repair in orbit in April 1984. Their general objectives were as follows: o Synthesize flare studies after three years of SMM data analysis. Many analyses of individual flares and individual phenomena, often jointly across many data sources had been published, but a need existed for a broader synthesis and updating of our understanding of solar flares since the Skylab Flare Workshops held several years earlier. o Encourage a broader participation in the SMM data anlysis and combine this more fully with theory and other data sources--data obtained with other spacecraft such as the HINOTORI, P78-1, and ISEE-3 spacecrafts, and with the Very Large Array (VLA) and many other ground-based instruments. Many coordinated data sets, unprecedented in their breadth of coverage and multiplicity of sources, had been obtained within the structure of the Solar Maximum Year (SMY). o St
出版日期Book 1989
关键词Corona; Planet; Solar flare; solar; solar activity
版次1
doihttps://doi.org/10.1007/978-94-009-2331-7
isbn_softcover978-94-010-7548-0
isbn_ebook978-94-009-2331-7Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media Dordrecht 1989
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Preflare Activity,dership of E. Schmahl and D. Webb. Its members were R. Bentley, F. Drago, S. Enome, V. Gaizauskas, R. Harrison, G. Hurford, B. Jackson, T. Kosugi, M. Kundu, K. Lang, A. Magun, P. Martens, G. Pneuman, E. Reichmann, A. Schadee, J. Schrijver, B. Schmieder, G. Simon, J. Smith, Jr., K. Strong, P. Waggett and B. Woodgate.
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Challenges to the Peace Accords,he SMM and HINOTORI satellites, particle detectors in several satellites and from ground based instruments and balloon flights and attempt to answer a number of fundamental questions that are stated below. We have also reviewed the progress made on the theory of mechanisms for particle acceleration in flares.
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https://doi.org/10.1007/978-3-642-99076-2e research performed during the SMM Workshop and reported here shows how successfully the SMM and collaborative observations have been used to advance our knowledge of the corona and how these observations have stimulated our theoretical understanding of why the corona is the way we observe it to be.
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