Motion 发表于 2025-3-21 17:55:49
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https://doi.org/10.1007/978-94-009-7958-1Variation; atmosphere; chromosphere; solar physics; solar windgrandiose 发表于 2025-3-22 10:28:52
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 frCollected 发表于 2025-3-22 14:55:16
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).nerve-sparing 发表于 2025-3-22 19:17:23
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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.单调性 发表于 2025-3-23 04:55:18
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.AMITY 发表于 2025-3-23 09:31:06
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