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Titlebook: Dynamics of the Magnetosphere; Proceedings of the A S.-I. Akasofu Conference proceedings 1980 D. Reidel Publishing Company, Dordrecht, Holl

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發(fā)表于 2025-3-21 19:57:16 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Dynamics of the Magnetosphere
副標題Proceedings of the A
編輯S.-I. Akasofu
視頻videohttp://file.papertrans.cn/285/284207/284207.mp4
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Dynamics of the Magnetosphere; Proceedings of the A S.-I. Akasofu Conference proceedings 1980 D. Reidel Publishing Company, Dordrecht, Holl
描述The Los Alamos Chapman Conference on Magnetospheric Substorms and Related Plasma Processes can be considered the fourth in a series devoted to magnetospheric substorms, after the Moscow (1971), Houston (1972), and Bryce Mountain (1974) meetings. The main motivation for organizing the Los Alamos Conference was that magnetospheric substorm studies have advanced enough to the point of bringing experimenters, analysts and theorists together to discuss major substorm problems with special emphasis on theoretical interpretations in terms of plasma processes. In spite of an extremely heavy schedule from 8:30 A.M. to 10:00 P.M., every session was conducted in an enjoyable and spirited atmosphere. In fact, during one of the afternoons that we had put aside for relaxation, John Winckler led a group of the attendees in a climb to the ceremonial cave of a prehistoric Indian ruin at Bandelier National Monument, near Los Alamos under a crystal blue sky and a bright New Mexico sun. There, they danced as the former dwellers of the pueblo had, perhaps as an impromptu evocation of a magnetospheric event.
出版日期Conference proceedings 1980
關(guān)鍵詞Planet; Solar wind; ionosphere; magnetosphere; solar; transport
版次1
doihttps://doi.org/10.1007/978-94-009-9519-2
isbn_softcover978-94-009-9521-5
isbn_ebook978-94-009-9519-2Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1980
The information of publication is updating

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Electric Fields and Currents in the Earth’s Magnetospherech . -field is a result of deviation from the normal level of solar wind velocity or density or of either IMF component..A concept of magnetospheric substorms, divided into convection-driven and anticonvectional disturbances, is outlined.
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Searching Your Phone and Using Speech, substorms appear to be associated with an increase of the region of the tail-like field or an increase of magnetospheric stresses and associated increase of magnetopause currents. We suggest the dayside field reconfiguration results from an increase of near-tail magnetopause currents which are connected through the night-side electrojet.
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Investing in Sales and Marketing Too Earlyto support the view that tearing modes grow to finite amplitudes. Future work will have to determine whether collision-free or collision-dominated (based on microturbulence) processes play the major role.
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Magnetic Substorm Characteristics Described by Magnetic Potential Maps for 26 – 28 March 1976ll into three categories, morning, evening and midnight, which may occur simultaneously or independently. During recovery of these ten substorms the westward electrojet is always in the morning sector.
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