Titlebook: Cosmic Magnetic Fields; Richard Wielebinski,Rainer Beck Book 2005 Springer-Verlag Berlin Heidelberg 2005 astrophysics.cosmic magnetic fiel

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書(shū)目名稱(chēng)Cosmic Magnetic Fields影響因子(影響力)




書(shū)目名稱(chēng)Cosmic Magnetic Fields影響因子(影響力)學(xué)科排名




書(shū)目名稱(chēng)Cosmic Magnetic Fields網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱(chēng)Cosmic Magnetic Fields網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書(shū)目名稱(chēng)Cosmic Magnetic Fields被引頻次




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書(shū)目名稱(chēng)Cosmic Magnetic Fields年度引用




書(shū)目名稱(chēng)Cosmic Magnetic Fields年度引用學(xué)科排名




書(shū)目名稱(chēng)Cosmic Magnetic Fields讀者反饋




書(shū)目名稱(chēng)Cosmic Magnetic Fields讀者反饋學(xué)科排名

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978-3-642-42130-3Springer-Verlag Berlin Heidelberg 2005

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Structuralism and Postmodernism the Sun either as optical streamers during solar eclipses and by using remote sensing methods. Magnetic fields of the solar planets have been studied in situ by measurements made by magnetometers on various spacecraft. Stars, supernova remnants and pulsars have been shown to harbour magnetic fields

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Structuralism and Postmodernisms supernovae and stellar winds. This energy stimulates turbulence in the H., which cascades up the turbulent wavenumber spectrum. The spectral wavelengths extend all the way down to scales most easily quoted in Astronomical Units. H. and molecular clouds enjoy a synergistic relationship, with turbul

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The Foundations of Postmodernismpre-main sequence and on late- and early-type main sequence stars, with some discussion also of red giants and white dwarfs, and with a brief reference to neutron stars. The current observational situation is reviewed, and some of the consequences for our ideas on star formation, on stellar structur

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