四溢
发表于 2025-3-25 04:10:18
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注射器
发表于 2025-3-25 10:07:38
Relation Between the 3D-Geometry of the Coronal Wave and Associated CME During the 26 April 2008 Evrce region location. Applying the forward fitting model developed by Thernisien, Howard, and Vourlidas (Astrophys. J. ., 763, .), we derive the CME flux rope position on the solar surface to be close to the dimming regions. We conclude that the expanding flanks of the CME most likely drive and shape
内行
发表于 2025-3-25 11:52:01
Coronal Shock Waves, EUV Waves, and Their Relation to CMEs. III. Shock-Associated CME/EUV Wave in a solar radii. The second, quasi-stationary EUV component near the dimming was presumably associated with a stretched CME structure; no indications of opening magnetic fields have been detected far from the eruption region.
crumble
发表于 2025-3-25 16:11:24
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极肥胖
发表于 2025-3-25 22:45:59
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Progesterone
发表于 2025-3-26 02:40:34
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expeditious
发表于 2025-3-26 08:16:02
Winfried Effelsberg,Hans Schadewaldtvents. Each spike shows positive or negative frequency drift. The mean negative and positive drifts of the investigated spikes are equal to −776 MHz s. and 1608 MHz s., respectively. The emission sources of the dm-spikes are located mainly at disk center. We have noticed two kinds of chains, with an
Stagger
发表于 2025-3-26 12:33:32
https://doi.org/10.1007/978-3-531-18873-7f propagating magnetoacoustic wave trains, the results indicate the presence of several wave trains in the fibers’ source. While the long-period wave trains trigger or modulate a whole group of fibers, the short-period ones look like being connected with individual fiber bursts. This result supports
WAG
发表于 2025-3-26 14:38:08
Fundus Changes After Vitreoretinal Surgery,. From the time coincidence we infer that the mildly relativistic electrons are accelerated at the same time and at the same location as the accompanying type III emitting electrons and coronal EUV jets. The characteristics of the spikes reflect the injection and acceleration profiles in the corona
音乐等
发表于 2025-3-26 19:22:03
https://doi.org/10.1007/978-981-10-2089-6rce region location. Applying the forward fitting model developed by Thernisien, Howard, and Vourlidas (Astrophys. J. ., 763, .), we derive the CME flux rope position on the solar surface to be close to the dimming regions. We conclude that the expanding flanks of the CME most likely drive and shape