Acquisition and reduction procedures for MOF Doppler-magnetograms

Details Acquisition and reduction procedures for MOF Doppler-magnetograms Acquisition and reduction procedures for MOF Doppler-magnetograms

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..185c&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 185-188 (SEE N89-25819 19-92)

Physics

Optics

5

Doppler Effect, Magnetic Signatures, Magneto-Optics, Solar Observatories, Data Acquisition, Data Reduction, Solar Corona, Solar Gravitation, Velocity Distribution

Scientific paper

Defects in the first magneto-optical filter (MOF) magnetograms, particularly the problem of the apparent contamination between velocity and magnetic fields, are discussed. It is found that a correct acquisition and reduction procedure gives cleaner results. A vector magnetograph is suggested. The vector field at coronal levels is calculated, using one MOF longitudinal magnetogram.

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