LANCE
发表于 2025-3-30 11:50:01
http://reply.papertrans.cn/32/3151/315026/315026_51.png
Outshine
发表于 2025-3-30 12:35:43
http://reply.papertrans.cn/32/3151/315026/315026_52.png
synovium
发表于 2025-3-30 17:03:02
http://reply.papertrans.cn/32/3151/315026/315026_53.png
accomplishment
发表于 2025-3-30 21:36:35
http://reply.papertrans.cn/32/3151/315026/315026_54.png
四指套
发表于 2025-3-31 02:22:36
http://reply.papertrans.cn/32/3151/315026/315026_55.png
绝缘
发表于 2025-3-31 07:25:42
http://reply.papertrans.cn/32/3151/315026/315026_56.png
失败主义者
发表于 2025-3-31 10:08:51
Plasma parameters derived from MSDP observations of cool flare loops, been detected in the Hα line just after the flare maximum and they appeared in absorption against the disk. Using the first-order differential cloud model (DCM1) technique, we derive empirically some basic plasma parameters at 15 points along one loop leg. The flow velocities and true heights have
显微镜
发表于 2025-3-31 17:00:13
http://reply.papertrans.cn/32/3151/315026/315026_58.png
Commentary
发表于 2025-3-31 21:07:21
http://reply.papertrans.cn/32/3151/315026/315026_59.png
PATHY
发表于 2025-4-1 01:17:40
http://reply.papertrans.cn/32/3151/315026/315026_60.png