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发表于 2025-3-25 05:52:47
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generic
发表于 2025-3-25 09:06:59
Joseph V. Montvilleresonance emission of the electrons in the presence of a magnetic field (mainly in the microwave domain). Thermal emissions originate from regions with distinct physical parameters, and their detection will depend on the observing frequency. The different classes of radio bursts are presented in Sec
audiologist
发表于 2025-3-25 14:51:57
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peritonitis
发表于 2025-3-25 17:28:31
Michael L. Perlin,Alison J. Lynch are narrowband, short peaks of emission. Narrowband spikes are seen sometimes at frequencies above the start of metric type III events. There is mounting evidence for the hypothesis that these spikes coincide with the energy release region. Much less clear is the situation for decimetric spikes, wh
蜈蚣
发表于 2025-3-25 21:00:37
Connie Dawsonions through stochastic forcing and nonlinear effects. The book concludes with an overview of the major challenges in understanding stellar magnetic fields and their evolution in terms of various dynamo models, global MHD simulations, and fossil fields. Each chapter is accompanied by an annotated bi
LAY
发表于 2025-3-26 00:25:23
duration events are consistent with diffusive shock acceleration taking place high in the corona. Electron spectra of short-duration flares are well reproduced by the distribution functions derived from a model assuming simultaneous second-order Fermi acceleration and Coulomb losses operating in clo
植物茂盛
发表于 2025-3-26 05:36:32
Daniel Rothbartmicroquasars inour own galaxy, astrophysical jets from nearby galaxies, or remoteactive galactic nuclei and quasars, probably fuelled by supermassiveblack holes978-94-010-6603-7978-94-009-0265-7Series ISSN 1389-2185
Inflammation
发表于 2025-3-26 11:43:23
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Meditate
发表于 2025-3-26 14:10:23
by an order of magnitude in several dimensions at once (frequency coverage, spatial reso- tion,dynamicrange,timeresolution,polarizationprecision)—thatitchalleng978-90-481-6725-8978-1-4020-2814-4Series ISSN 0067-0057 Series E-ISSN 2214-7985
敲诈
发表于 2025-3-26 17:30:22
David Y. F. Ho of the major challenges in understanding stellar magnetic fields and their evolution in terms of various dynamo models, global MHD simulations, and fossil fields. Each chapter is accompanied by an annotated bi978-3-642-43047-3978-3-642-32093-4Series ISSN 1861-7980 Series E-ISSN 1861-8227