Determination of the line-of-sight magnetic field based on the solar rotation.

Details Determination of the line-of-sight magnetic field based on the solar rotation. Determination of the line-of-sight magnetic field based on the solar rotation.

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995arbei..26...37l&link_type=abstract

Astrophysics Reports, Publications of the Beijing Astronomical Observatory, No. 26, p. 37 - 44

Astronomy and Astrophysics

Astrophysics

Solar Photosphere: Magnetograms, Solar Chromosphere: Magnetograms

Scientific paper

The authors calibrate consistently the magnetograms and Dopplergrams on the photosphere and chromosphere obtained by the Solar Magnetic Field Telescope (SMFT) at Huairou Solar Observing Station, based on solar rotation. There is a good agreement between the new calibration parameters with the theoretically calculated parameters used earlier. However, the parameters for Dopplergrams are much larger than the former ones.

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