An empirical model of the small-scale magnetic element of the solar quiet region

Details An empirical model of the small-scale magnetic element of the solar quiet region An empirical model of the small-scale magnetic element of the solar quiet region

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kfnt....5...50l&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 5, Jan.-Feb. 1989, p. 50-58, 62. In Russian.

Astronomy and Astrophysics

Astronomy

5

Astronomical Models, Solar Activity, Solar Magnetic Field, Background Radiation, Field Strength, Gas Pressure, Solar Spectra, Spatial Resolution, Sunspots

Scientific paper

Magnetographic observations of the longitudinal magnetic fields carried out with a high spatial resolution on a magnetograph are analyzed. Six magnetosensitive lines were used: Fe I 480.8, 523.3, 525.0, 525.3, 630.2 nm and Mg I 518.4 nm. The data obtained are interpreted within the framework of a two-component model, which includes spatially unresolved flux tubes and background fields. It is shown that the magnetic field strength in the flux tubes is 220 mT at the Fe I 525.0 nm line formation level.

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