SLAY
发表于 2025-3-23 10:20:44
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猛然一拉
发表于 2025-3-23 14:11:11
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让步
发表于 2025-3-23 19:47:24
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遭遇
发表于 2025-3-24 00:50:54
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为敌
发表于 2025-3-24 05:02:34
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evaculate
发表于 2025-3-24 07:59:38
https://doi.org/10.1007/978-3-030-55704-1 In this paper, recent results on the solar origin of 1-300 keV electrons and 0.1-6 MeV protons are reviewed. The main findings are that one class of electron events escaping into interplanetary space are related to the impulsive phase of the flare (radio type III burst related events), but there is
PACT
发表于 2025-3-24 14:43:11
https://doi.org/10.1007/978-3-030-51610-9 heliosphere, processes in the solar corona associated with flares and coronal mass ejections (CMEs) are the most energetic natural particle accelerators, sometimes accelerating electrons and ions to relativistic energies. The observation of these particles offers the unique opportunity to study fun
杀死
发表于 2025-3-24 16:35:54
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–DOX
发表于 2025-3-24 22:48:39
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Hemoptysis
发表于 2025-3-25 00:07:45
https://doi.org/10.1007/978-94-007-0585-2ch was focused on radio observations and related modeling. Progress reached in the following areas is summarized: (1) diagnostics of coronal magnetic fields and the morphology of the field in flares and filament eruptions; (2) evidence of magnetic reconnection and MHD turbulence in radio emissions;