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Titlebook: Radio Continua During Solar Flares; Selected Contributio Arnold O. Benz Book 1986 Springer Science+Business Media Dordrecht 1986 Corona.Pla

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31#
發(fā)表于 2025-3-26 22:42:47 | 只看該作者
32#
發(fā)表于 2025-3-27 03:50:19 | 只看該作者
https://doi.org/10.1007/978-94-009-4710-8Corona; Planet; Population; Solar flare; Variation; solar
33#
發(fā)表于 2025-3-27 07:17:57 | 只看該作者
34#
發(fā)表于 2025-3-27 13:01:24 | 只看該作者
35#
發(fā)表于 2025-3-27 14:09:23 | 只看該作者
Discussion on the Classification of Fine Structures in ContinuaA short discussion on classification and terminology connected with fine structures in solar continuum emission at radio frequencies was arranged on Monday, 27 May with C. Slottje acting as chairman.
36#
發(fā)表于 2025-3-27 20:15:13 | 只看該作者
Occurrence of Solar Decimetric Spike Bursts over a Period of 4 Years During the 21st CycleA total number of 460 DCIM events, single or groups, were observed during the period of October 1980 to December 1984 with the Weissenau spectrograph as dynamic film spectra. Several parameters describing these data were evaluated statistically and the main features were discussed in context with associated burst types.
37#
發(fā)表于 2025-3-27 23:08:59 | 只看該作者
38#
發(fā)表于 2025-3-28 03:46:14 | 只看該作者
39#
發(fā)表于 2025-3-28 07:17:25 | 只看該作者
A Model of Ultra-Fast Fine Structures of Microwave Bursts electron cyclotron frequency and electron velocity as well as Landau damping and cyclotron damping) to excite the UFFS (Ultra-Fast Fine Structures) of microwave bursts and adopting a nonlinear density wave as a trigger mechanism to explain the millisecond time structure of the UFFS.
40#
發(fā)表于 2025-3-28 11:23:37 | 只看該作者
Alberto Abrami,Mauro Messerotti,Paolo Zlobecfuture. It will appeal to both beginners and seasoned researchers in nonlinear science, numerous areas of physics (optics, quantum physics, biophysics), and applied mathematics (ODEs, PDEs, dynamical systems, machine learning) as well as engineering..978-3-030-44992-6Series ISSN 2195-9994 Series E-ISSN 2196-0003
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