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The atmosphere of the sun
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ISBN: 0852743750 9780852743751 Year: 1988 Publisher: Bristol: Hilger,

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Book
Physics of the sun and its atmosphere
Authors: ---
ISBN: 9812832726 9789812832726 9789812832719 9812832718 Year: 2008 Publisher: Hackensack, NJ Singapore World Scientific

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This book presents a pedagogical, updated and modern view of the Sun from its interior to its exterior as well as the Sun-Earth system. Written by eminent scientists in solar physics, the chapters deal with recent advances in solar physics, seismic Sun, solar magnetic field, waves and oscillations, spectroscopic diagnostics of solar plasmas, partially ionized lower atmosphere, coronal heating, coronal mass ejections, radio Sun, solar wind, and the Sun-Earth system. Each chapter is fully illustrated and has a comprehensive reference list. The book covers all major topics in solar physics, and p

Solar photosphere : structure, convection and magnetic fields : proceedings of the 138th symposium of the International Astronomical Union, held in Kiev, May 15-20, 1989
Authors: ---
ISBN: 0792305299 0792305302 9400910614 Year: 1990 Volume: 138 Publisher: Dordrecht Boston New York Kluwer

Solar influences on global change
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ISBN: 0309051487 9786610193134 1280193131 0309538122 0585024235 9780585024233 6610193134 9780309051484 Year: 1994 Publisher: Washington, D.C. National Academy Press


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MHD waves in the solar atmosphere
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ISBN: 9781108427661 1108427669 9781108633581 9781108613774 Year: 2019 Publisher: Cambridge, UK : Cambridge University Press,

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This volume presents a full mathematical exposition of the growing field of coronal seismology which will prove invaluable for graduate students and researchers alike. Roberts' detailed and original research draws upon the principles of fluid mechanics and electromagnetism, as well as observations from the TRACE and SDO spacecraft and key results in solar wave theory. The unique challenges posed by the extreme conditions of the Sun's atmosphere, which often frustrate attempts to develop a comprehensive theory, are tackled with rigour and precision; complex models of sunspots, coronal loops and prominences are presented, based on a magnetohydrodynamic (MHD) view of the solar atmosphere, and making use of Faraday's concept of magnetic flux tubes to analyse oscillatory phenomena. The rapid rate of progress in coronal seismology makes this essential reading for those hoping to gain a deeper understanding of the field.

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