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Titlebook: Solar and Interplanetary Dynamics; M. Dryer,E. Tandberg-Hanssen Book 1980 International Astronomical Union 1980 Variation.astrophysics.cos

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发表于 2025-3-21 17:55:10 | 显示全部楼层 |阅读模式
书目名称Solar and Interplanetary Dynamics
编辑M. Dryer,E. Tandberg-Hanssen
视频videohttp://file.papertrans.cn/872/871458/871458.mp4
丛书名称International Astronomical Union Symposia
图书封面Titlebook: Solar and Interplanetary Dynamics;  M. Dryer,E. Tandberg-Hanssen Book 1980 International Astronomical Union 1980 Variation.astrophysics.cos
描述Informal discussions in 1977 among a number of scientists asso­ ciated with solar and interplanetary physics revealed a need for a dialogue between the two often-divergent groups. It was clear that the latter group was dependent essentially on the sun for its raison d‘etre. On the other hand it was also clear that the former group could benefit in its search for insight vis-a-vis solar activity by looking beyond the shell of the inner corona. Needless to add that the combined solar/interplanetary topic is relevant to astrophysics when one considers stellar winds and binary star flows. It was felt, there­ fore, that a symposium was essential to bring together, for the first time, leading solar and interplanetary physicists from the interna­ tional community to discuss and record herein their own research. The fundamental physical processes underlying our own capricious star‘s activity can be understood only by the coupling of solar and interplan­ etary topics in an intimate observational and theoretical structure. This book, intended for active research scientists and advanced grad­ uate students, is an important step in this direction. The background of solar and interplanetary dyn
出版日期Book 1980
关键词Variation; astrophysics; cosmic ray; dynamics; galaxies; heliosphere; planet; solar activity; solar system; s
版次1
doihttps://doi.org/10.1007/978-94-009-9100-2
isbn_softcover978-90-277-1163-2
isbn_ebook978-94-009-9100-2Series ISSN 1743-9213 Series E-ISSN 2352-2186
issn_series 1743-9213
copyrightInternational Astronomical Union 1980
The information of publication is updating

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A Two-Level Solar Dynamo Based on Solar Activity, Convection, and Differential Rotationhere. It seems natural, therefore, to expect the reconnection aspect of conversion to be located there, where the least work needs to be performed. To transfer the generated flux there, we may add to conversion another spontaneous process: . of bipolar structure (Parker, 1955). To transfer the recon
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The Origin of Interplanetary Sectorsize the force-free condition, . × . = 0, and in fact make the more restrictive assumption that this region is current free. The magnetic field in this region can be derived from a solution to the Laplace equation.
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Stellar Mass Flux and Coronal Heating by Shock Wavese and dissipation terms. The input parameters are the base pressure, the base temperature and the mechanical flux introduced at chromospheric level in form of shock waves. If these three parameters allow a solar wind expansion, the output results are the radial variations of the density, of the temp
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Book 1980 be understood only by the coupling of solar and interplan­ etary topics in an intimate observational and theoretical structure. This book, intended for active research scientists and advanced grad­ uate students, is an important step in this direction. The background of solar and interplanetary dyn
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K. V. Sheridan,G. A. Dulkl ein besonders geschäftiges Jahr. Wie Richard Bellman es ausdrückte: „Man wußte nie, wo Erdös sich gerade aufhielt, nicht einmal das Land kannte man. Aber man konnte sicher sein, daß er im Laufe eines ganzen Jahres überall erschien. Er kam einem ergodischen Teilchen [eines, das schließlich alle phy
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