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Titlebook: Coronal Holes and Solar Wind Acceleration; John L. Kohl,Steven R. Cranmer Book 1999 Springer Science+Business Media B.V. 1999 Corona.Plane

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发表于 2025-3-21 18:57:03 | 显示全部楼层 |阅读模式
书目名称Coronal Holes and Solar Wind Acceleration
编辑John L. Kohl,Steven R. Cranmer
视频video
图书封面Titlebook: Coronal Holes and Solar Wind Acceleration;  John L. Kohl,Steven R. Cranmer Book 1999 Springer Science+Business Media B.V. 1999 Corona.Plane
描述The SOHO-7 Workshop was held from 28 September through 1 October 1998 at the Asticou Inn in Northeast Harbor, Maine. The primary topic of this Workshop was the impact of SOHO observations on our understanding of the nature and evolution of coronal holes and the acceleration and composition of the solar wind. The presentations and discussions occasionally went beyond this topic to include the impact of the reported research on other solar structures and the heliosphere. SOHO (the Solar and Heliospheric Observatory), a project of international cooperation between ESA and NASA, was launched in December 1995 and began its science operations during the first few months of 1996. To many solar and space physicists, it was a great advantage that SOHO began itscomprehensive look at the Sun during the 1996 solar minimum. The qualitatively simple two-phase corona, with polar coronal holes expanding into the high-speed solar wind, and a steady equatorial streamer belt related somehow to the stochastic slow-speed solar wind, allowed various SOHO diagnostics to be initiated with a reasonably well­ understoodcircumsolar geometry. The analysis of subsequentSOHO measurements made during the rising
出版日期Book 1999
关键词Corona; Planet; Solar wind; Variation; solar
版次1
doihttps://doi.org/10.1007/978-94-015-9167-6
isbn_softcover978-90-481-5267-4
isbn_ebook978-94-015-9167-6
copyrightSpringer Science+Business Media B.V. 1999
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发表于 2025-3-21 23:00:33 | 显示全部楼层
expanding into the high-speed solar wind, and a steady equatorial streamer belt related somehow to the stochastic slow-speed solar wind, allowed various SOHO diagnostics to be initiated with a reasonably well­ understoodcircumsolar geometry. The analysis of subsequentSOHO measurements made during the rising 978-90-481-5267-4978-94-015-9167-6
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978-90-481-5267-4Springer Science+Business Media B.V. 1999
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is Workshop was the impact of SOHO observations on our understanding of the nature and evolution of coronal holes and the acceleration and composition of the solar wind. The presentations and discussions occasionally went beyond this topic to include the impact of the reported research on other sola
发表于 2025-3-23 04:21:34 | 显示全部楼层
Wavelet Theory and Its Applicationsrmation about the boundary conditions for the wind in the inner solar corona and about the plasma conditions prevailing in the transition region and chromospheric sources of the wind plasma. These results are presented, and then some key questions and scientific issues are identified.
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Solar Wind Models from the Sun to 1 AU: Constraints by in Situ and Remote Sensing Measurementsrmation about the boundary conditions for the wind in the inner solar corona and about the plasma conditions prevailing in the transition region and chromospheric sources of the wind plasma. These results are presented, and then some key questions and scientific issues are identified.
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