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Titlebook: High Energy Density Laboratory Astrophysics; Sergey V. Lebedev Conference proceedings 2007 Springer Science+Business Media B.V. 2007 Accre

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樓主: Diverticulum
21#
發(fā)表于 2025-3-25 06:02:43 | 只看該作者
22#
發(fā)表于 2025-3-25 10:55:28 | 只看該作者
23#
發(fā)表于 2025-3-25 13:38:10 | 只看該作者
Astrophysical Jets of Blazars and Microquasars for some time that extragalactic jets found in radio galaxies, quasars, and BL Lac objects are the site of ultrarelativistic particle acceleration, the recent identification of the Galactic jet source and microquasar LS 5039 as a source of very-high-energy gamma-ray emission has underlined the stri
24#
發(fā)表于 2025-3-25 18:04:40 | 只看該作者
Simulation of the Magnetothermal Instabilityal stability criterion for convective stability, the Schwarzschild criterion, which depends on entropy gradients, is modified. In the magnetized long mean free path regime, instability occurs for small wavenumbers when (? ./?.)(? ln ./?.) > 0, which we refer to as the Balbus criterion. We refer to t
25#
發(fā)表于 2025-3-25 23:44:16 | 只看該作者
26#
發(fā)表于 2025-3-26 00:35:58 | 只看該作者
How to Produce a Plasma Jet Using a Single and Low Energy Laser Beamuced using a relatively low energy laser pulse, below 500 J and it presents similarities with astrophysical protostellar jets. It lasts more than 10 ns, extends over several millimeters, has velocity more than 500 km/s, the Mach number more than 10 and the density above 10. cm.. The mechanism of jet
27#
發(fā)表于 2025-3-26 06:30:11 | 只看該作者
28#
發(fā)表于 2025-3-26 09:40:07 | 只看該作者
29#
發(fā)表于 2025-3-26 16:23:54 | 只看該作者
Plasma Jet Experiments Using LULI 2000 Laser Facilitysured quantities related to the jet such as its propagation velocity, temperature and emissive radius evolution are presented. We also performed analytical work, which explains the jet evolution in some cases.
30#
發(fā)表于 2025-3-26 17:56:42 | 只看該作者
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