| 書目名稱 | Plasma Astrophysics, Part II | | 副標(biāo)題 | Reconnection and Fla | | 編輯 | Boris V. Somov | | 視頻video | http://file.papertrans.cn/750/749098/749098.mp4 | | 概述 | In the book, brief historical remarks demonstrate that the outstanding discoveries in cosmic physics were by no means governed by chance.Distinguishing feature of the proposed book is the consecutive | | 叢書名稱 | Astrophysics and Space Science Library | | 圖書封面 |  | | 描述 | Magnetic ?elds are easily generated in astrophysical plasma owing to its ?6 high conductivity. Magnetic ?elds, having strengths of order few 10 G, correlated on several kiloparsec scales are seen in spiral galaxies. Their origin could be due to ampli?cation of a small seed ?eld by a turbulent galactic dynamo. In several galaxies, like the famous M51, magnetic ?elds are well correlated (or anti-correlated) with the optical spiral arms. These are the weakest large-scale ?elds observed in cosmic space. The strongest magnets in space are presumably the so-called magnetars, the highly mag- 15 netized (with the strength of the ?eld of about 10 G) young neutron stars formed in the supernova explosions. The energy of magnetic ?elds is accumulated in astrophysical plasma, and the sudden release of this energy – an original electrodynamical ‘burst’ or‘explosion’–takesplaceunderde?nitebutquitegeneralconditions(P- att, 1992; Sturrock, 1994; Kivelson and Russell, 1995; Rose, 1998; Priest and Forbes, 2000; Somov, 2000; Kundt, 2001). Such a ‘?are’ in ast- physical plasma is accompanied by fast directed ejections (jets) of plasma, powerful ?ows of heat and hard electromagnetic radiation as well as | | 出版日期 | Book 20071st edition | | 關(guān)鍵詞 | Accretion; Flares; Plasma; Somov; astrophysics; space science | | 版次 | 1 | | doi | https://doi.org/10.1007/978-0-387-68894-7 | | isbn_softcover | 978-1-4419-2245-8 | | isbn_ebook | 978-0-387-68894-7Series ISSN 0067-0057 Series E-ISSN 2214-7985 | | issn_series | 0067-0057 | | copyright | Springer-Verlag New York 2007 |
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書目名稱Plasma Astrophysics, Part II影響因子(影響力)
書目名稱Plasma Astrophysics, Part II影響因子(影響力)學(xué)科排名
書目名稱Plasma Astrophysics, Part II網(wǎng)絡(luò)公開度
書目名稱Plasma Astrophysics, Part II網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Plasma Astrophysics, Part II被引頻次
書目名稱Plasma Astrophysics, Part II被引頻次學(xué)科排名
書目名稱Plasma Astrophysics, Part II年度引用
書目名稱Plasma Astrophysics, Part II年度引用學(xué)科排名
書目名稱Plasma Astrophysics, Part II讀者反饋
書目名稱Plasma Astrophysics, Part II讀者反饋學(xué)科排名
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