Solar Activity and Classical Physics

Details Solar Activity and Classical Physics Solar Activity and Classical Physics

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001chjaa...1...99p&link_type=abstract

Chinese Journal of Astronomy & Astrophysics, Vol. 1, p. 99-124

Astronomy and Astrophysics

Astrophysics

12

Sun: Activity, Magnetohydrodynamics, Radiative Transfer

Scientific paper

This review of solar physics emphasizes several of the more conspicuous scientific puzzles posed by contemporary observational knowledge of the magnetic activity of the Sun. The puzzles emphasize how much classical physics we have yet to learn from the Sun. The physics of solar activity is based on the principles of Newton, Maxwell, Lorentz, Boltzmann, 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.

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