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Titlebook: Solar Magnetohydrodynamics; Eric R. Priest Book 1982 D. Reidel Publishing Company, Dordrecht, Holland 1982 Variation.atmosphere.chromosphe

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书目名称Solar Magnetohydrodynamics
编辑Eric R. Priest
视频videohttp://file.papertrans.cn/872/871401/871401.mp4
丛书名称Geophysics and Astrophysics Monographs
图书封面Titlebook: Solar Magnetohydrodynamics;  Eric R. Priest Book 1982 D. Reidel Publishing Company, Dordrecht, Holland 1982 Variation.atmosphere.chromosphe
描述I have felt the need for a book on the theory of solar magnetic fields for some time now. Most books about the Sun are written by observers or by theorists from other branches of solar physics, whereas those on magnetohydrodynamics do not deal extensively with solar applications. I had thought of waiting a few decades before attempting to put pen to paper, but one summer Josip Kleczek encouraged an im­ mediate start ‘while your ideas are still fresh‘. The book grew out of a postgraduate lecture course at St Andrews, and the resulting period of gestation or ‘being with monograph‘ has lasted several years. The Sun is an amazing object, which has continued to reveal completely unexpected features when observed in greater detail or at new wavelengths. What riches would be in store for us if we could view other stars with as much precision! Stellar physics itself is benefiting greatly from solar discoveries, but, in tum, our understanding of many solar phenomena (such as sunspots, sunspot cycles, the corona and the solar wind) will undoubtedly increase in the future due to their observation under different conditions in other stars. In the ‘old days‘ the solar atmosphere was regarded as
出版日期Book 1982
关键词Variation; atmosphere; chromosphere; solar physics; solar wind
版次1
doihttps://doi.org/10.1007/978-94-009-7958-1
isbn_softcover978-90-277-1833-4
isbn_ebook978-94-009-7958-1
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1982
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书目名称Solar Magnetohydrodynamics影响因子(影响力)




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https://doi.org/10.1007/978-94-009-7958-1Variation; atmosphere; chromosphere; solar physics; solar wind
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Book 1982rists from other branches of solar physics, whereas those on magnetohydrodynamics do not deal extensively with solar applications. I had thought of waiting a few decades before attempting to put pen to paper, but one summer Josip Kleczek encouraged an im­ mediate start ‘while your ideas are still fr
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A Description of the Sun,ver, we begin with a list of earlier developments, many of which took place before the solar magnetic field was discovered. Section 1.2 continues by describing the overall characteristics of the solar interior and atmosphere, and is followed by a more detailed account of both the quiet Sun (Section 1.3) and the active Sun (Section 1.4).
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Shock Waves,e is revealed by a Type II radio burst. On a smaller scale, shock waves are probably generated by ., . and the continual granular motion of the solar surface (Sections 6.3 and 6.4.1). Some of the applications are discussed elsewhere in the book, while the present chapter develops the basic theory for both hydrodynamic and magnetic shocks.
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Dynamo Theory,nobservable depths of the convective zone, but the details of such an interaction between plasma and magnetic field are not yet fully understood. The problems are first of all to show that a magnetic field may, in act, be maintained and then to reproduce the above features of the solar cycle.
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