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Titlebook: High Energy Density Laboratory Astrophysics; G.A. Kyrala Book 2005 Springer Science+Business Media B.V. 2005 Accretion.MHD.Plasma.astrophy

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發(fā)表于 2025-3-21 18:56:03 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱High Energy Density Laboratory Astrophysics
編輯G.A. Kyrala
視頻videohttp://file.papertrans.cn/427/426236/426236.mp4
圖書封面Titlebook: High Energy Density Laboratory Astrophysics;  G.A. Kyrala Book 2005 Springer Science+Business Media B.V. 2005 Accretion.MHD.Plasma.astrophy
描述.During the past several years, research teams around the world have developed astrophysics-relevant utilizing high energy-density facilities such as intense lasers and z-pinches. Research is underway in many areas, such as compressible hydrodynamic mixing, strong shock phenomena, radiation flow, radiative shocks and jets, complex opacities, equations of stat, and relativistic plasmas. Beyond this current research and the papers it is producing, plans are being made for the application, to astrophysics-relevant research, of the 2 MJ National Ignition Facility (NIF) laser at Lawrence Livermore National Laboratory; the 600 kj Ligne d‘Intégration Laser (LIL) and the 2 MJ Laser Mégajoule (LMJ) in Bordeaux, France; petawatt-range lasers now under construction around the world; and current and future Z pinches. The goal of this conference and these proceedings is to continue focusing attention on this emerging research area. The conference brought together different scientists interested in this emerging new field, with topics covering:..- Hydrodynamic instabilities in astrophysics,.- Supernovae and supernova remnant evolution,.- Astrophysical shocks, blast waves, and jets,.- Stellar opa
出版日期Book 2005
關(guān)鍵詞Accretion; MHD; Plasma; astrophysics; relativistic jet
版次1
doihttps://doi.org/10.1007/1-4020-4162-4
isbn_softcover978-90-481-6880-4
isbn_ebook978-1-4020-4162-4
copyrightSpringer Science+Business Media B.V. 2005
The information of publication is updating

書目名稱High Energy Density Laboratory Astrophysics影響因子(影響力)




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發(fā)表于 2025-3-21 20:27:05 | 只看該作者
s such as intense lasers and z-pinches. Research is underway in many areas, such as compressible hydrodynamic mixing, strong shock phenomena, radiation flow, radiative shocks and jets, complex opacities, equations of stat, and relativistic plasmas. Beyond this current research and the papers it is p
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Laboratory Experiments of Stellar Jets from the Perspective of an Observer,ed jets with velocities and Mach numbers similar to those within stellar jets, and the field seems poised to make significant advances by connecting observations and theories with experiments. This article points out several aspects of stellar jets that might be clarified by such experiments.
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. These protocols are used for the evaluation of compounds that can be carried out by a single individual in a Category 3 containment laboratory. The number of compounds analyzed would be about 10, which is a convenient number to fill a single 96-well p24 enzyme-linked immunosorbent assay (ELISA) plate.
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Hypernovae and Gamma-Ray Bursts,. The abundance patterns of hypernovae are characterized by large ratios (Zn, Co)/Fe and small ratios (Mn, Cr)/Fe, indicating a significant contribution of hypernovae to the early Galactic chemical evolution.
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