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Titlebook: Impact Spectropolarimetric Sensing; S. A. Kazantsev,A. G. Petrashen,N. M. Firstova Book 1999 Kluwer Academic / Plenum Publishers 1999 Chro

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31#
發(fā)表于 2025-3-27 00:42:32 | 只看該作者
Observations of Polarization Effects at the Irkutsk Institute of Solar and Terrestrial Physics (Rusper chromospheric layers of a solar flare by different spectroscopic techniques, in particular by the Berange—Mozer method, based on satellites of the forbidden Hel line(228,229) and estimates of linear polarization,
32#
發(fā)表于 2025-3-27 03:12:51 | 只看該作者
Physical Introduction: Concepts, Phenomenology, Retrospectives, Applications, principles governing the polarization spectroscopy of ionized gases, the quantitative spectropolarimetric sensing of various gas discharges, and the first steps toward exploiting this method in diagnostic problems of the solar atmosphere have been presented in the book . by S. A. Kazantsev and J.-C. Hénoux.
33#
發(fā)表于 2025-3-27 05:58:30 | 只看該作者
34#
發(fā)表于 2025-3-27 12:18:41 | 只看該作者
Solar Flare Observations at Meudon Observatory (France),tion was obtained and analyzed together with X-ray observations. Such a comprehensive approach can provide a clearer and deeper understanding of the evolution of a flare and the determination of the flare phase.
35#
發(fā)表于 2025-3-27 17:33:53 | 只看該作者
36#
發(fā)表于 2025-3-27 20:33:00 | 只看該作者
Solar Flare Observations at the Crimean Astrophysical Observatory (Ukraine),ms. This aspect of solar flare emission was quite poorly studied at that time. Therefore, the Crimean group during the 1970s and 1980s undertook systematic and careful observations of linear polarization in solar flare emissions.
37#
發(fā)表于 2025-3-28 00:25:29 | 只看該作者
38#
發(fā)表于 2025-3-28 02:58:53 | 只看該作者
39#
發(fā)表于 2025-3-28 06:32:28 | 只看該作者
Physics of Atoms and Moleculeshttp://image.papertrans.cn/i/image/462348.jpg
40#
發(fā)表于 2025-3-28 14:12:46 | 只看該作者
978-1-4613-7194-6Kluwer Academic / Plenum Publishers 1999
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