值得赞赏 发表于 2025-3-28 15:55:25
http://reply.papertrans.cn/24/2383/238295/238295_41.pngIsthmus 发表于 2025-3-28 19:54:48
http://reply.papertrans.cn/24/2383/238295/238295_42.png认识 发表于 2025-3-29 02:20:08
http://reply.papertrans.cn/24/2383/238295/238295_43.pngMetastasis 发表于 2025-3-29 06:53:31
Multi-Wavelength Observations of CMEs and Associated Phenomena,avelength analysis. The combination of data obtained from space-based experiments and ground based instruments allows us to follow the space-time development of an event from the bottom of the corona to large distances in the interplanetary medium. Since CMEs originate in the low solar corona, under引导 发表于 2025-3-29 07:51:44
http://reply.papertrans.cn/24/2383/238295/238295_45.pngechnic 发表于 2025-3-29 13:46:52
ICMEs at High Latitudes and in the Outer Heliosphere,on, and morphology of the solar wind, particularly during times of high solar activity. They are known to play an important role in cosmic ray modulation and the acceleration of energetic particles. ICMEs are also believed to be associated with the large global transient events that swept through th鞠躬 发表于 2025-3-29 18:47:44
CME Disturbance Forecasting,ely different in the sheath than within the ICME. Consequently two types of forecast procedures using solar observations of phenomena associated with the release of the CME as input parameters have been developed to treat the two types of environment. This chapter surveys efforts that have resulted疏忽 发表于 2025-3-29 22:17:10
http://reply.papertrans.cn/24/2383/238295/238295_48.png慷慨不好 发表于 2025-3-30 01:01:03
https://doi.org/10.1007/978-0-387-45088-9Corona; Heliosphere; Planet; Solar System; Solar wind; coronal mass ejection; instruments; solar; space plasAUGUR 发表于 2025-3-30 06:52:29
978-1-4419-2356-1Springer-Verlag New York 2006