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Titlebook: Handbook of the Solar-Terrestrial Environment; Y. Kamide,A. Chian Book 2007 Springer-Verlag Berlin Heidelberg 2007 Climatology.Storm.Weath

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樓主: Cyclone
41#
發(fā)表于 2025-3-28 16:20:23 | 只看該作者
Substormsnhanced energy input from the solar wind into the magnetosphere and ends with a decrease of that energy input to its original value. The study of substorms breaks down into three major thrusts. First of all, there are the observations which have been well documented since the latter part of the 19th
42#
發(fā)表于 2025-3-28 20:01:41 | 只看該作者
Solar Radio Emissionss of radio bursts reveal various forms of activity and acceleration processes which are associated to large scale eruptive phenomena including flares, filament eruptions, CMEs and shocks. CMEs and the interplanetary shock waves are the most spectacular large-scale manifestations in the solar corona
43#
發(fā)表于 2025-3-28 23:00:08 | 只看該作者
Ionospheremics of the Earth’s magnetosphere are discussed, with a particular emphasis on the energization and transport of ionospheric particles. At the end of the chapter some ground-based powerful tools that are routinely used to sound the ionosphere are briefly introduced.
44#
發(fā)表于 2025-3-29 06:20:32 | 只看該作者
Thermospherevered, requiring novel understanding of TID which may imply inconsistency with simple manifestation of GW as understood so far. Thermosphere global winds are little known observationally but GCM simulation now presents a plausible model. Intense vertical motion as highly fluctuating and with large a
45#
發(fā)表于 2025-3-29 11:10:35 | 只看該作者
46#
發(fā)表于 2025-3-29 12:27:05 | 只看該作者
47#
發(fā)表于 2025-3-29 16:55:21 | 只看該作者
48#
發(fā)表于 2025-3-29 20:13:58 | 只看該作者
keV to more than ? GeV. It is convenient satellite observations and computer simulations over to group these particles into lower-energy particles and thepasttwo decades, it hasbecomepossibleto analyze higher-e978-3-642-07968-9978-3-540-46315-3
49#
發(fā)表于 2025-3-30 01:37:29 | 只看該作者
50#
發(fā)表于 2025-3-30 07:11:13 | 只看該作者
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