The influence of flows on the fine structure of sunspots

Details The influence of flows on the fine structure of sunspots The influence of flows on the fine structure of sunspots

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990chjss..10...66z&link_type=abstract

Chinese Journal of Space Science (ISSN 0254-6124), vol. 10, Jan. 1990, p. 66-71. In Chinese, with abstract in English.

Physics

2

Magnetohydrodynamic Flow, Solar Activity Effects, Sunspots, Magnetic Diffusion, Wave Functions

Scientific paper

The dispersion equation of linear disturbance MHD equations is an algebraic equation of third power of frequency when the magnetic diffusivity is considered as a function of temperature. The magnetic diffusion instability can be obtained when the dispersion equation is solved. In this paper, the influence of small flows on the magnetic diffusion instability is discussed.

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