Preliminary Reduction of Data Obtained with a Full Disk Magnetograph

Details Preliminary Reduction of Data Obtained with a Full Disk Magnetograph Preliminary Reduction of Data Obtained with a Full Disk Magnetograph

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp..413l&link_type=abstract

In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.413-416.

Astronomy and Astrophysics

Astronomy

Scientific paper

A new full disk magnetograph with high spatial and temporal resolution has been established at Huairou Solar Observing Station of Beijing Astronomical Observatory. Comparing its observing data with the relevant data obtained by the Solar Magnetic Field Telescope(SMFT)(Ai, 1987) at Huairou Station, we find that they are very similar in both respects of magnetic field morphology and intensity. This demonstrates that the observing results obtained by the full disk magnetograph are reliable. Obvious correlations between radio emission flux and absolute magnetic field flux at the photosphere, and between full disk magnetograms and plages appeared IN calcium monochromatic images have been shown.

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