Some of the main properties of the fine structure of solar magnetic fields as deduced from low spatial resolution stokesmeter observations at the stop telescope of the sayan observatory

Details Some of the main properties of the fine structure of solar magnetic fields as deduced from low spatial resolution stokesmeter observations at the stop telescope of the sayan observatory Some of the main properties of the fine structure of solar magnetic fields as deduced from low spatial resolution stokesmeter observations at the stop telescope of the sayan observatory

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26at...20..439p&link_type=abstract

Astronomical and Astrophysical Transactions, vol. 20, Issue 3, pp.439-444

Astronomy and Astrophysics

Astronomy

Sun, Magnetic Fields, Stokes Parameters

Scientific paper

With the purpose of gaining a better understanding of large-scale solar magnetic fields, we investigated some of the main properties of their fine structure. The study was based on using stokesmeter observations of the Stokes I- and V-parameters in the line of FeI 525.02 nm from the STOP telescope of the Sayan observatory covering a time interval from April to November 1999. Using extensive statistical material (totaling over 120 full-disk stokesgrams with a resolution of 2 arc min) we determined the most informative parameters of the V-profiles such as the asymmetry in amplitudes and areas, and Doppler shifts with respect to the I-profiles of the observed spectral line. The results are compared with findings reported by other authors.

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