强制性 发表于 2025-3-27 00:03:09
http://reply.papertrans.cn/24/2383/238296/238296_31.png毗邻 发表于 2025-3-27 02:36:44
http://reply.papertrans.cn/24/2383/238296/238296_32.pngLigneous 发表于 2025-3-27 07:26:27
Conference proceedings 1997hock waves and coronal mass ejections; particle beams in the solar corona and in the interplanetary medium; and explosive energy-release phenomena and particle acceleration. The different articles give a well-balanced presentation of relevant observations based upon various techniques, models and th星星 发表于 2025-3-27 11:10:15
http://reply.papertrans.cn/24/2383/238296/238296_34.png不妥协 发表于 2025-3-27 17:09:31
The Nature of Liquids and Gases,es are also reviewed. The knowledge of the electron energy spectra deduced at low and high energies from both hard X-ray and centimeter/millimeter observations is discussed. The experimental data is compared with the predictions of the avalanche model for solar flares and further tests of the model proposed.Minatory 发表于 2025-3-27 20:56:59
http://reply.papertrans.cn/24/2383/238296/238296_36.pngBureaucracy 发表于 2025-3-27 23:19:30
http://reply.papertrans.cn/24/2383/238296/238296_37.png占线 发表于 2025-3-28 02:28:11
High Energy Neutrino Interactions,relation to coronal beams, using recent spacecraft data from . and .. Interplanetary electron beams can often be traced back to coronal type III sources, while there is no such relation for interplanetary ion beams. In the third part, we briefly review acceleration mechanisms for coronal and interplanetary beams, separately for electrons and ions.菊花 发表于 2025-3-28 07:41:42
http://reply.papertrans.cn/24/2383/238296/238296_39.png木讷 发表于 2025-3-28 14:07:29
http://reply.papertrans.cn/24/2383/238296/238296_40.png