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Titlebook: Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond; Tetsuya Watanabe,Takeo Kosugi,Alphonse C. Sterling Book 1998 Springer

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發(fā)表于 2025-3-21 19:30:04 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond
編輯Tetsuya Watanabe,Takeo Kosugi,Alphonse C. Sterling
視頻videohttp://file.papertrans.cn/701/700365/700365.mp4
叢書(shū)名稱Astrophysics and Space Science Library
圖書(shū)封面Titlebook: Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond;  Tetsuya Watanabe,Takeo Kosugi,Alphonse C. Sterling Book 1998 Springer
描述Since its launch in 1991, the Yohkoh satellite has beenreturning unprecedented observations of solar flares and the dynamicsolar corona. This book is a collection of papers presented at ameeting held in: Yoyogi, Tokyo, on the occasion of Yohkoh‘s fifthanniversary of operation. The papers constitute a summary ofobservations and results over the five years, including contributionsbased on data from Yohkoh‘s hard and soft X-ray telescopes and itsspectrometer experiments. The five years of data, coveringapproximately one-half of a solar cycle, reveal a fresh perspective onsolar science, with a new picture of solar flares and the active Sunemerging. Also, for the first time there are extensive results fromYohkoh observations of the Sun during the solar minimum period. .This wide-ranging volume will be of interest to workers in solarphysics and X-ray astronomy. It also contains material appropriate forsupplemental reading for graduate students in solar physics.
出版日期Book 1998
關(guān)鍵詞Corona; Plasma; Solar flare; astrophysics; solar
版次1
doihttps://doi.org/10.1007/978-94-011-5220-4
isbn_softcover978-94-010-6198-8
isbn_ebook978-94-011-5220-4Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media Dordrecht 1998
The information of publication is updating

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發(fā)表于 2025-3-22 00:14:06 | 只看該作者
0067-0057 s book is a collection of papers presented at ameeting held in: Yoyogi, Tokyo, on the occasion of Yohkoh‘s fifthanniversary of operation. The papers constitute a summary ofobservations and results over the five years, including contributionsbased on data from Yohkoh‘s hard and soft X-ray telescopes
板凳
發(fā)表于 2025-3-22 03:30:12 | 只看該作者
Studies of Coronal Temperaturee is observed to increase with height (Sturrock, Wheatland and Acton, 1996, Foley, Culhane and Acton, 1997). Here we present a full-sun temperature map to illustrate these and other features of the temperature structure of the corona.
地板
發(fā)表于 2025-3-22 08:16:13 | 只看該作者
Deep Survey of Solar Nano-Flares with Yohkoharker 1988) using the soft X-ray position-dependent time profiles. For details, please refer to the full-length paper published in the 1997 September issue of the . with the same title (Shimizu and Tsuneta 1997).
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發(fā)表于 2025-3-22 10:47:02 | 只看該作者
Book 1998a collection of papers presented at ameeting held in: Yoyogi, Tokyo, on the occasion of Yohkoh‘s fifthanniversary of operation. The papers constitute a summary ofobservations and results over the five years, including contributionsbased on data from Yohkoh‘s hard and soft X-ray telescopes and itsspe
6#
發(fā)表于 2025-3-22 14:03:33 | 只看該作者
The Behavior of Coronal Holes the minimum of the cycle. In this paper we discuss the role of fine structures in the solar corona with densities comparable to CHs, their relations with photospheric fields, and the connection with the global behavior of CHs through the solar cycle.
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發(fā)表于 2025-3-22 21:02:53 | 只看該作者
Coronal and Interplanetary Disturbances Associated with an Eruptive Prominence of 28 August 1992rmation of the CME (and its interplanetary manifestation). An interplanetary disturbance was observed via interplanetary scintillation technique in the region to the east of the sun-Earth line on 29–30 August 1992.
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