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| Solar Activity and Classical Physics | |
| 引用本文： | E. N. Parker (Department of Physics,University of Chicago,Chicago,IL 60637). Solar Activity and Classical Physics[J]. 中国天文和天体物理学报, 2001, 1(2): 99-124 |
| 作者姓名： | E. N. Parker (Department of Physics University of Chicago Chicago IL 60637) |
| 作者单位： | Department of Physics，University of Chicago，Chicago，IL 60637 |
| 摘 要： | 1 INTRODUCTIONThe Sun is close enough to observe in some detail, and it shows that a star is more thanthe traditional stable self-gravitating thermonuclear body established half a celltury ago. Forthe fact is that out of sight beneath the visible surface the outward flow of heat from thethermonuclear core drives hydrodynamics that generates magnetic fields. It is the complicateddynamics of those magnetic fields that produces the modern mysteries of the active Sun. The… |
| 关 键 词： | 磁力计 辐射 太阳活动 太阳观测 |
Solar Activity and Classical Physics |
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| E.N.Parker. Solar Activity and Classical Physics[J]. Chinese Journal of Astronomy and Astrophysics, 2001, 1(2): 99-124 | |
| Authors: | E.N.Parker |
| Affiliation: | DepartmentofPhysics,UniversityofChiago,Chicago,IL60637 |
| Abstract: | This review of solar physics emphasizes several of the more comspicuous scientific puzzles posed by contemporary observational knowledge of the magnetic activity of the Sun.The physics of solar activity is based on the principles of Newton,Maxwell,Lorentz,Boltzmam,et.al.,along with the principles of radiative transfer.In the large,these principles are expressed by magnetohydrodynamics.A brief derivation of the magnetohydrodynamic induction and momentum equations is provided,with a discussion of popular misconceptions. |
| Keywords: | Sun: activety - Magnetohydro dynamics - radiative transfer |
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