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Titlebook: Advanced Topics on Astrophysical and Space Plasmas; Proceedings of the A Elisabete M. Gouveia Dal Pino,Anthony L. Peratt,Ab Conference proc

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發(fā)表于 2025-3-21 18:20:02 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
期刊全稱(chēng)Advanced Topics on Astrophysical and Space Plasmas
期刊簡(jiǎn)稱(chēng)Proceedings of the A
影響因子2023Elisabete M. Gouveia Dal Pino,Anthony L. Peratt,Ab
視頻videohttp://file.papertrans.cn/147/146385/146385.mp4
圖書(shū)封面Titlebook: Advanced Topics on Astrophysical and Space Plasmas; Proceedings of the A Elisabete M. Gouveia Dal Pino,Anthony L. Peratt,Ab Conference proc
影響因子In June of 1996, at the idyllic seaside resort ofGuarujá, Brazil, a renowned group of researchers in space andastrophysical plasmas met to provide a forum on Advanced Topics onAstrophysical and Space Plasmas at a school consisting of some 60students and teachers, mainly from Brazil and Argentina, but also fromall the other parts of the globe. The purpose was to provide an updateon the latest theories, observations, and simulations ofspace-astrophysical plasma phenomena. .The topics covered included space plasma mechanisms for particleacceleration, nonthermal emission in cosmic plasma,magnetohydrodynamic instabilities in solar, interstellar, and othercosmic objects, magnetic field line reconnection and merging, thenonlinear and often chaotic structure of astrophysical plasmas, andthe advances in high performance supercomputing resources to replicatethe observed phenomena. The lectures were presented by Professor MarkBirkinshaw of the Harvard-Smithsonian Center for Astrophysics and theUniversity of Bristol; Dr Anthony Peratt, Los Alamos NationalLaboratory Scientific Advisor to the United States Department ofEnergy; Dr Dieter Biskamp of the Max Planck Institute for PlasmaPhysics, Garc
Pindex Conference proceedings 1997
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Axel Borsdorf,Michael Jungmeiernd on acceleration by shock waves. Radiation processes in astrophysical and space plasmas are reviewed with emphasis on plasma emission from the solar corona and electron cyclotron maser emission from planets and stars.
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Günter K?ck,Arne Arnberger,Lutz M?llerThis information is then used in a theoretical treatment of the Kelvin-Helmholtz instability of the flows, and the relevance of this instability to the persistence of the observed structures is emphasised.
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Florian Weber,Friedericke Weberimportant contribution to make in understanding the connection between microscopic and macroscopic phenomena. Plasma is a system composed of a large number of particles which interact primarily, but not exclusively, through the electromagnetic field. The problem of understanding the linkages and cou
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Axel Borsdorf,Michael Jungmeiernd on acceleration by shock waves. Radiation processes in astrophysical and space plasmas are reviewed with emphasis on plasma emission from the solar corona and electron cyclotron maser emission from planets and stars.
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