Aspects of the Zero Level Problem of Solar Magnetographs

Details Aspects of the Zero Level Problem of Solar Magnetographs Aspects of the Zero Level Problem of Solar Magnetographs

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996soph..164..381d&link_type=abstract

Solar Physics, Volume 164, Issue 1-2, pp. 381-388

Physics

7

Solar Magnetic Fields, Solar Magnetographs

Scientific paper

The zero level problem of solar magnetographs is particularly important for observations of large-scale magnetic fields on the Sun. Experiments conducted at the STOP telescope of the Sayan observatory show that, in addition to adjustment errors of the polarization analyzer and the spectrograph focusing, spurious signals of the magnetograph are caused by polarization effects in optical components preceding the polarization analyzer and aberration errors of the spectrograph.

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