| 书目名称 | Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes | | 副标题 | First Kodai-Trieste | | 编辑 | S. S. Hasan,R. T. Gangadhara,V. Krishan | | 视频video | | | 概述 | Provides and up to date review of the field.Each chapter presents research problems and contains a pedagogical component.Includes supplementary material: | | 丛书名称 | Astrophysics and Space Science Proceedings | | 图书封面 |  | | 描述 | .It is well established and appreciated by now that more than 99% of the baryonic matter in the universe is in the plasma state. Most astrophysical systems could be approximated as conducting fluids in a gravitational field. It is the combined effect of these two that gives rise to the mind boggling variety of configurations in the form of filaments, loops, jets and arches. The plasma structures that cannot last for more than a second or less in a laboratory remain intact for astronomical time and spatial scales in an astrophysical setting. The case in point is the well known extragalactic jets whose collimation and stability has remained an enigma inspite of the efforts of many for many long years. The high energy radiation sources such as the active galactic nuclei again summon the coherent plasma radiation processes for their exceptionally large output from regions of relatively small physical sizes. The generation of magnetic field, anomalous transport of angular momentum with decisive bearing on star formation processes, the ubiquitous MHD turbulence under conditions irreproducible in terrestrial laboratories are some of the generic issues still awaiting a concerted effort for | | 出版日期 | Conference proceedings 2008 | | 关键词 | Astophysical Plasmas; Astrophysical Turbulence; Galactic Dynamos; Geomagnetic field; Ionized Plasmas; MHD | | 版次 | 1 | | doi | https://doi.org/10.1007/978-1-4020-8868-1 | | isbn_softcover | 978-90-481-8011-0 | | isbn_ebook | 978-1-4020-8868-1Series ISSN 1570-6591 Series E-ISSN 1570-6605 | | issn_series | 1570-6591 | | copyright | Springer Science+Business Media B.V. 2008 |
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发表于 2025-3-21 18:39:19
