Joint vector magnetograph observations at BBSO, Huairou Station and Mees Solar Observatory

Details Joint vector magnetograph observations at BBSO, Huairou Station and Mees Solar Observatory Joint vector magnetograph observations at BBSO, Huairou Station and Mees Solar Observatory

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..142...11w&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 142, no. 1, p. 11-20.

Physics

33

Magnetic Signatures, Solar Magnetic Field, Solar Observatories, Faraday Effect, Instrument Errors

Scientific paper

Joint vector magnetograph observations were carried out at Big Bear Solar Observatory (BBSO), Huairou Solar Observing Station (Huairou), and Mees Solar Observatory (MSO) in late September 1989. Comparisons of vector magnetograms obtained at the three stations show a high degree of consistency in the morphology of both longitudinal and transverse fields. Quantitative comparisons show the presence of noise, cross-talk between longitudinal field and transverse field, Faraday rotation and signal saturation effects in the magnetograms. We have tried to establish how the scatter in measurements from different instruments is apportioned between these sources of error.

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