Magnetic probing of the solar interior

Details Magnetic probing of the solar interior Magnetic probing of the solar interior

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985colo.rept.....b&link_type=abstract

Final Report, 1 Jan. 1983 - 31 Jul. 1985 Colorado Univ., Boulder. Dept. of Astrophysical, Planetary, and Atmospheric Sciences.

Astronomy and Astrophysics

Astrophysics

Coronas, Helioseismology, Magnetic Field Configurations, Magnetic Probes, Photosphere, Solar Interior, Solar Magnetic Field, Magnetohydrodynamic Turbulence, Magnetometers, Mathematical Models, Solar Oscillations, Sunspots

Scientific paper

The magnetic field patterns in the region beneath the solar photosphere is determined. An approximate method for downward extrapolation of line of sight magnetic field measurements taken at the solar photosphere was developed. It utilizes the mean field theory of electromagnetism in a form thought to be appropriate for the solar convection zone. A way to test that theory is proposed. The straightforward application of the lowest order theory with the complete model fit to these data does not indicate the existence of any reasonable depth at which flux conservation is achieved.

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