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Titlebook: Magnetodynamic Phenomena in the Solar Atmosphere; Prototypes of Stella Yutaka Uchida,Takeo Kosugi,Hugh S. Hudson Book 1996 Springer Science

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發(fā)表于 2025-3-21 18:56:05 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Magnetodynamic Phenomena in the Solar Atmosphere
副標(biāo)題Prototypes of Stella
編輯Yutaka Uchida,Takeo Kosugi,Hugh S. Hudson
視頻videohttp://file.papertrans.cn/622/621420/621420.mp4
圖書封面Titlebook: Magnetodynamic Phenomena in the Solar Atmosphere; Prototypes of Stella Yutaka Uchida,Takeo Kosugi,Hugh S. Hudson Book 1996 Springer Science
描述These are the Proceedings of Colloquium No. 153 of the International Astro- nomical Union, held at Makuhari near Tokyo on May 22 - 26, 1995, and hosted by the National Astronomical Observatory. This meeting was intended to be an interdisciplinary meeting between re- searchers of solar and stellar activity, in order for them to exchange the newest information in each field. While each of these areas has seen remarkable advances in recent years, and while the researchers in each field have felt that information from the other‘s domain would be extremely useful in their own work, there have not been very many opportunities for intensive exchanges of information between these closely related fields. We therefore expected much from this meeting in pro- viding stellar researchers with new results of research on the counterparts of their targets of research, spatially and temporarily resolved, as observed on the Sun. Likewise we hoped to provide solar researchers with new results on gigantic ver- sions of their targets of research under the very different physical circumstances on other active stars. It was our greatest pleasure that we had wide attendance of experts and active researcher
出版日期Book 1996
關(guān)鍵詞Corona; Solar flare; Variation; solar
版次1
doihttps://doi.org/10.1007/978-94-009-0315-9
isbn_softcover978-94-010-6627-3
isbn_ebook978-94-009-0315-9
copyrightSpringer Science+Business Media Dordrecht 1996
The information of publication is updating

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Book 1996d by the National Astronomical Observatory. This meeting was intended to be an interdisciplinary meeting between re- searchers of solar and stellar activity, in order for them to exchange the newest information in each field. While each of these areas has seen remarkable advances in recent years, an
地板
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and hosted by the National Astronomical Observatory. This meeting was intended to be an interdisciplinary meeting between re- searchers of solar and stellar activity, in order for them to exchange the newest information in each field. While each of these areas has seen remarkable advances in recent
5#
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Book 1996as observed on the Sun. Likewise we hoped to provide solar researchers with new results on gigantic ver- sions of their targets of research under the very different physical circumstances on other active stars. It was our greatest pleasure that we had wide attendance of experts and active researcher
6#
發(fā)表于 2025-3-22 16:50:19 | 只看該作者
resolved, as observed on the Sun. Likewise we hoped to provide solar researchers with new results on gigantic ver- sions of their targets of research under the very different physical circumstances on other active stars. It was our greatest pleasure that we had wide attendance of experts and active researcher978-94-010-6627-3978-94-009-0315-9
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LTE. This SpringerBrief is suitable for telecom engineers, researchers, and academic professionals with valuable knowledge and potential working or research directions when designing and develo978-3-319-47345-1978-3-319-47346-8Series ISSN 2191-8112 Series E-ISSN 2191-8120
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發(fā)表于 2025-3-22 21:56:02 | 只看該作者
lined with both the . and . forms featuring. Finally, with reference to the critical inclination problem, the essential properties of the newer “fundamental” model are described and compared with the IRP. A strong correspondence is established between recent independent investigations of a variety o
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https://doi.org/10.1007/978-94-009-0315-9Corona; Solar flare; Variation; solar
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