dagger 发表于 2025-3-25 06:09:34
http://reply.papertrans.cn/88/8714/871387/871387_21.png规范就好 发表于 2025-3-25 08:18:13
http://reply.papertrans.cn/88/8714/871387/871387_22.png卵石 发表于 2025-3-25 15:43:17
http://reply.papertrans.cn/88/8714/871387/871387_23.png会议 发表于 2025-3-25 19:13:04
http://reply.papertrans.cn/88/8714/871387/871387_24.pngAnticoagulants 发表于 2025-3-25 22:22:43
978-90-277-0663-8D. Reidel Publishing Company, Dordrecht, Holland 1976可能性 发表于 2025-3-26 03:29:03
http://reply.papertrans.cn/88/8714/871387/871387_26.png节约 发表于 2025-3-26 06:41:10
http://reply.papertrans.cn/88/8714/871387/871387_27.png不透气 发表于 2025-3-26 08:29:07
Particle Emission From Solar Flares, their transit over the visible hemisphere of the Sun. The particle flux sets in on about the second day after the appearance of the region on the eastern solar limb (cf. Figure 100) and continues until the region moves to about 40° behind the western limb (Fan .., 1968). Figure 90 shows an exampleMITE 发表于 2025-3-26 15:18:06
http://reply.papertrans.cn/88/8714/871387/871387_29.pngPulmonary-Veins 发表于 2025-3-26 20:28:45
The High-Temperature Flare,regions. The reason for this is that thermal and non-thermal effects are coupled in the high temperature flare regions in the solar corona; non-thermal effects arise from pre-heated plasma and eventually become thermalized.