Relationship between the mean solar magnetic field strength and the stokes V-parameter distribution

Details Relationship between the mean solar magnetic field strength and the stokes V-parameter distribution Relationship between the mean solar magnetic field strength and the stokes V-parameter distribution

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26at...20..525z&link_type=abstract

Astronomical and Astrophysical Transactions, vol. 20, Issue 3, pp.525-529

Astronomy and Astrophysics

Astronomy

Sun, Sun-As-A-Star, Magnetic Fields, Stokes Parameters

Scientific paper

This paper examines some of the properties of the Solar mean magnetic field (SMMF) that are brought to light by Stokesmeter (Stokes V-parameter) observations in the FeI line 525.02 nm. Stokesmeter SMMF measurements are compared with magnetographic data, based on observations from the STOP telescope at the Sayan solar observatory as well as from the J.Wilcox Solar Observatory. It is shown that the character of the Stokes V-parameter distribution in the line profile is determined by the distribution of large-scale fields across the solar disk, especially in the central zone.

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