| 書(shū)目名稱(chēng) | Magnetic Coupling between the Interior and Atmosphere of the Sun |
| 編輯 | S. Hasan,R. J. Rutten |
| 視頻video | http://file.papertrans.cn/622/621217/621217.mp4 |
| 概述 | Includes supplementary material: |
| 叢書(shū)名稱(chēng) | Astrophysics and Space Science Proceedings |
| 圖書(shū)封面 |  |
| 描述 | Solar physics in India has a tradition that can be traced to the setting up of the Kodaikanal Observatory in 1899 when the Madras Observatory was relocated to a high altitude site with a view to initiate observations of the sun. This conference on Magnetic Coupling between the Interior and the Atmosphere of the Sun during 2–5 December 2008 was planned to coincide with centenary of the Evershed effect discovery at Kodaikanal in 1909. The aim of this meeting was to bring to a critical focus a comprehensive - derstanding of the important issues pertaining to solar magnetism with particular emphasis on the various MHD processes that operate in the solar atmosphere. The current status of magnetic eld measurements and their implications in the light of recenttheoriesandnumericalmodelingthataddressthe fundamentalscalesandp- cessesinthehighlymagnetizedturbulentplasmawerereviewedduringthismeeting. The meeting was timely for the following reasons: Space observations such as from SOHO and TRACE have provided a wealth of multiwavelength observations onprocessesoccurringinregionsofthe atmosphereextendingfromthe photosphere up to the outer corona. With the launch of Hinode and STEREO in 2006 and |
| 出版日期 | Conference proceedings 2010 |
| 關(guān)鍵詞 | Chromosphere; Corona; Planet; Solar System; Solar flare; Solar wind; Sun; Sunspot; Tachocline; solar |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-3-642-02859-5 |
| isbn_softcover | 978-3-642-26274-6 |
| isbn_ebook | 978-3-642-02859-5Series ISSN 1570-6591 Series E-ISSN 1570-6605 |
| issn_series | 1570-6591 |
| copyright | Springer-Verlag Berlin Heidelberg 2010 |
|Archiver|手機(jī)版|小黑屋|
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