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Titlebook: Jets From Young Stars III; Numerical MHD and In S. Massaglia,G. Bodo,P. Rossi Book 2008 Springer-Verlag Berlin Heidelberg 2008 Computationa

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21#
發(fā)表于 2025-3-25 06:12:12 | 只看該作者
22#
發(fā)表于 2025-3-25 08:27:39 | 只看該作者
E.F. Toroe suggestiveness of some of its results, experi-mental philosophy has been criticized almost from its very beginnings. In this chapter, we focus on a methodological objection due to Antti Kauppinen (Kauppinen, 2007). According to Kauppinen, experimental philosophy (in any of its possible formulation
23#
發(fā)表于 2025-3-25 12:59:55 | 只看該作者
ial for verifying the predictions of general relativity and comparing it with alternative theories of gravitation. After a quick recap of the astrophysical models for a pulsar, we provide an overview of the techniques that are implemented to record the arrival times of the radio pulses, including th
24#
發(fā)表于 2025-3-25 18:46:38 | 只看該作者
25#
發(fā)表于 2025-3-25 20:49:48 | 只看該作者
Shock-Capturing Schemes in Computational MHD). The shock-capturing framework developed for the Euler equations of gasdynamics is extended to MHD by illustrating differences and additional complexities introduced by the presence of magnetic fields. In particular, we focus our attention on the characteristic structure of the equations by invest
26#
發(fā)表于 2025-3-26 04:10:50 | 只看該作者
The Kelvin–Helmholtz Instabilitysses that rule the dynamics of collimated outflows in various astronomical scenarios (AGN, Young Stellar Objects, compact galactic bodies, etc.). We outline here the main physical properties of the KHI following linear and non linear treatments, and considering typical conditions in astrophysical co
27#
發(fā)表于 2025-3-26 06:49:52 | 只看該作者
28#
發(fā)表于 2025-3-26 11:22:23 | 只看該作者
Thermal Instabilitiesrst give a derivation of the instability conditions by using a simple physical analysis and then I will give a more formal derivation. I will finally briefly discuss the effects of cooling-heating processes on the Kelvin-Helmholtz instability.
29#
發(fā)表于 2025-3-26 14:14:16 | 只看該作者
The Oscillatory Instability of Radiative Shock Waveshock speed. In the limit of optically thin plasma, the linear stability analysis of planar shocks with a power-law cooling function ^;∝ ρ.T. is reviewed. It is shown that the shock front can oscillate around its stationary position with increasing quantized frequencies resembling the modes of a pipe
30#
發(fā)表于 2025-3-26 20:13:20 | 只看該作者
iety of engineering disciplines.Helps students to bridge theThis textbook provides comprehensive, in-depth coverage of the fundamental concepts of electrical engineering. It is written from an engineering perspective, with special emphasis on circuit functionality and applications. Reliance on highe
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