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Titlebook: Coronal Physics from Radio and Space Observations; Proceedings of the C Gérard Trottet Conference proceedings 1997 Springer-Verlag Berlin H

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11#
發(fā)表于 2025-3-23 11:20:20 | 只看該作者
12#
發(fā)表于 2025-3-23 16:46:07 | 只看該作者
Parity Violating Effects in Atoms,rrelator (Stokes I and V, 576 channels). Calibration has also been improved. The multifrequency operation remains almost unchanged. It allows simultaneous observations of up to 10 frequencies in the range 150–450 MHz. Integrated data will be available on the internet, and special observing modes may
13#
發(fā)表于 2025-3-23 21:15:22 | 只看該作者
https://doi.org/10.1007/978-1-4684-2193-4orders of magnitude over current facilities operating at frequencies between about 200 MHz and a few GHz. Such a leap in performance is motivated by a wide range of fundamental astrophysical questions which we hope to address in the first decades of the next millenium. Some of the myriad possibiliti
14#
發(fā)表于 2025-3-24 01:03:34 | 只看該作者
15#
發(fā)表于 2025-3-24 05:36:03 | 只看該作者
https://doi.org/10.1007/BFb0106448astronomy; energy release; interferometer; large-scale disturbances; measurement; particle beams; radio in
16#
發(fā)表于 2025-3-24 07:52:18 | 只看該作者
978-3-662-14120-5Springer-Verlag Berlin Heidelberg 1997
17#
發(fā)表于 2025-3-24 13:12:01 | 只看該作者
Coronal Physics from Radio and Space Observations978-3-540-68693-4Series ISSN 0075-8450 Series E-ISSN 1616-6361
18#
發(fā)表于 2025-3-24 16:47:05 | 只看該作者
Molecular Distribution Functions,ent results of X-ray bright-points, transient brightenings and jets are reviewed, and diagnostics that result from bulk plasma motions are discussed. Finally, three events are examined in detail and the implications of the observation discussed in relation to flare models.
19#
發(fā)表于 2025-3-24 22:38:35 | 只看該作者
Molecular Distribution Functions,oblem of coronal heating. Radio observations provide powerful diagnostics of the physical conditions in the transition region and the corona. Recent observational and theoretical results are presented and their implications are discussed. The prospects of further observations, in conjunction with other wavelength ranges are given.
20#
發(fā)表于 2025-3-25 03:06:52 | 只看該作者
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