克制
发表于 2025-3-25 05:17:26
Stellar Flare Spectral Diagnotics: Present and Future,ons and ground-based observatories, with new techniques for obtaining high spectral and temporal resolution, are discussed in light of their possible contribution to our understanding of solar and stellar flares.
粉笔
发表于 2025-3-25 11:13:29
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jaundiced
发表于 2025-3-25 11:57:54
Electron Beam as Origin of White-Light Solar Flares, enhanced white-light emission both at chromospheric and photospheric level, due to Paschen and H. continua emission, respectively. We then obtain white-light contrasts compatible with observations, obviously showing the link between white-light flares and atmospheric bombardment by electron beams.
slow-wave-sleep
发表于 2025-3-25 17:27:26
Radio Emission from Stellar Flares,sion for the flare process in classic and compact stars. In particular we discuss the possible production of radio flares from interactions between an accretion disk and the magnetic field of the central object.
Presbycusis
发表于 2025-3-25 21:02:23
Preface,ways: various aspects of solar flares were observed but hardly ever white-light events, whereas on the stellar side optical flaring was virtually the only observable phenomenon. With the first X-ray detections of flares on UV Ceti, YZ CMi, and Proxima Centauri in the mid-1970’s things changed dramat
暂时过来
发表于 2025-3-26 03:06:36
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nonplus
发表于 2025-3-26 07:17:10
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esoteric
发表于 2025-3-26 11:40:54
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GNAW
发表于 2025-3-26 15:04:15
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防水
发表于 2025-3-26 20:18:01
Electron Acceleration in Solar Flares,pacecraft detected electrons above 10 MeV. Combining our data with those from the ULEWAT spectrometer (MPI Garching and University of Maryland) electron spectra in the range from 0.1 to 100 MeV were obtained. The observed spectral shapes can be divided into two classes. The spectra of the one class