The temperature influence on the relation between magnetic field strength and equivalent width of solar spectral lines

Details The temperature influence on the relation between magnetic field strength and equivalent width of solar spectral lines The temperature influence on the relation between magnetic field strength and equivalent width of solar spectral lines

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998atsir1557...30b&link_type=abstract

Astronomicheskij Tsirkulyar, no. 1557

Astronomy and Astrophysics

Astronomy

Scientific paper

The model of the solar atmosphere with a small temperature gradient and
a temperature higher than its photospheric value may explain the
relation between magnetic field strength and equivalent width of the
spectral lines if we infer the presence of fine-structure magnetic
elements in the photosphere.

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