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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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21#
發(fā)表于 2025-3-25 03:34:14 | 只看該作者
Theory of Anisotropic Collisional Relaxation,rbers having no nuclear spin and no hyperfine structure of the quantum states, will be examined in this chapter. Using a kinetic approach, the effect of collisions in this case can be qualitatively interpreted as the transformation of an ordering of the distribution of the relative velocity vectors
22#
發(fā)表于 2025-3-25 11:03:38 | 只看該作者
23#
發(fā)表于 2025-3-25 12:08:37 | 只看該作者
Observations of Polarization Effects at the Irkutsk Institute of Solar and Terrestrial Physics (Rusarge amount of research was undertaken on turbulent electric fields in plasmas under laboratory conditions. Since most theories and models of solar flares rely on the concept of the turbulent state of a flare plasma, the Irkutsk group made some initial attempts to study plasma turbulence with the up
24#
發(fā)表于 2025-3-25 19:13:22 | 只看該作者
Solar Flare Observations at Meudon Observatory (France),group. The significance of these data and general conclusions are very important in connection with the fact that detailed spectropolarimetric information was obtained and analyzed together with X-ray observations. Such a comprehensive approach can provide a clearer and deeper understanding of the e
25#
發(fā)表于 2025-3-25 20:12:28 | 只看該作者
26#
發(fā)表于 2025-3-26 00:38:00 | 只看該作者
27#
發(fā)表于 2025-3-26 07:48:06 | 只看該作者
Impact Spectropolarimetric Diagnostics of Nonthermal Phenomena in the Solar Atmosphere,solar atmosphere are of the utmost importance for the clarification of energy transport modes from the corona, where primary energy release takes place, to the lower parts of the solar atmosphere. The upper layer of the chromosphere is an optically active region, where most emission lines are formed
28#
發(fā)表于 2025-3-26 12:33:28 | 只看該作者
29#
發(fā)表于 2025-3-26 12:57:07 | 只看該作者
, and the evident potential applications of this technique to environmental physics, astrophysics, and hot plasma. This is a practically oriented book, describing theoretical fundamentals and implementation of this new interdisciplinary remote sensing technique. A basic phenomenon for impact spectro
30#
發(fā)表于 2025-3-26 20:09:07 | 只看該作者
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