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Titlebook: Atomic Processes in Basic and Applied Physics; Viacheslav Shevelko,Hiro Tawara Book 2012 Springer-Verlag Berlin Heidelberg 2012 Astrophysi

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樓主: Garfield
51#
發(fā)表于 2025-3-30 12:17:57 | 只看該作者
52#
發(fā)表于 2025-3-30 15:33:17 | 只看該作者
Microprozessoren, Hybridsysteme, Softwareroblem in the framework of the probabilistic approach to be used for the temperature diagnostics of hot plasma structures. We then demonstrate applications of our diagnostics methods to hot plasmas in laboratory (tokamak plasma) and astrophysical (solar corona) conditions.
53#
發(fā)表于 2025-3-30 18:52:08 | 只看該作者
Microprozessoren, Hybridsysteme, Softwaredischarge are given as an example. In addition, we introduce the line-intensity ratio method for plasma diagnostic, it can be a good example how atomic and molecular data can be used plasma diagnostics.
54#
發(fā)表于 2025-3-30 22:42:47 | 只看該作者
Unsolved Mystery of Ball Lightningh environment, and phenomena related to it. On a way of studying this phenomenon, there are a lot of difficulties, the basic of them is insufficiency of authentic, scientific data. The chapter sets as the purpose to interest the reader in the problem, to describe conditions of ball lightning occurre
55#
發(fā)表于 2025-3-31 03:01:10 | 只看該作者
Unravelling the Mysteries of Matter Surrounding Supermassive Black Holes recombination of iron ions in connection with X-ray spectra from active galactic nuclei, and we explain how new dielectronic recombination rate coefficients from storage-ring experiments have helped to remove previous inconsistencies in the astrophysical modeling of such spectra.
56#
發(fā)表于 2025-3-31 05:56:15 | 只看該作者
Large Hot X-Ray Sources in the Solar Coronaof Kelvin. For this reason, the study of hot coronal plasma is the key for understanding mechanisms of heating of the corona and nature of solar flares. In this chapter, we analyze observation of Mg XII line (10 MK) in series of experiments onboard CORONAS satellites. We studied configuration, dynam
57#
發(fā)表于 2025-3-31 10:16:35 | 只看該作者
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