婚姻生活 发表于 2025-3-28 16:20:18
On the 24- and 155-Day Periodicity Observed in Solar H, Flares “activity”periods (∼150.–160.). We focus on the separate analysis of the northern and southern solar hemisphere as well as on an energy dependence of the flare events. Our findings suggest that the appearance of the “activity” periods might result due to superposition of two predominant periods of凝视 发表于 2025-3-28 20:01:32
He-D3 Polarization Observed in Prominences Locarno. Two different experimental techniques (ZIMPOL and beam exchange method) have been successfully employed to determine all four Stokes components. Both give compatible results. The preliminary results as well as the measurement techniques are reported.维持 发表于 2025-3-29 01:00:33
Solar Flares — Observations and Theory instabilities and particle acceleration process — are described as an indivisible part of the reconnection process. Finally, the interacting-flux flares and two-ribbon flares are used to illustrate some details of flare modeling.ARC 发表于 2025-3-29 04:00:07
http://reply.papertrans.cn/88/8714/871399/871399_44.png整理 发表于 2025-3-29 07:47:22
Physics of Solar Prominences transfer equations are described in some detail. Finally, new models resulting from a combination of magneto-hydrostatics and radiative transfer are outlined and their relevance for observations is discussed.重力 发表于 2025-3-29 12:47:46
http://reply.papertrans.cn/88/8714/871399/871399_46.pngEthics 发表于 2025-3-29 17:24:41
http://reply.papertrans.cn/88/8714/871399/871399_47.png消毒 发表于 2025-3-29 21:26:47
http://reply.papertrans.cn/88/8714/871399/871399_48.png捐助 发表于 2025-3-30 01:39:43
Arnold Hanslmeier,Astrid Veronig,Mauro MesserottiIs particularly useful for graduate students and young researchers working in solar physicsHighbrow 发表于 2025-3-30 04:30:34
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