The Sun as a magnetic star: on the manifestation of different surface structures in disk-integrated observations

Details The Sun as a magnetic star: on the manifestation of different surface structures in disk-integrated observations The Sun as a magnetic star: on the manifestation of different surface structures in disk-integrated observations

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009iaus..259..229d&link_type=abstract

Cosmic Magnetic Fields: From Planets, to Stars and Galaxies, Proceedings of the International Astronomical Union, IAU Symposium,

Astronomy and Astrophysics

Astronomy

Sun: Magnetic Fields, Sun: Activity, Polarization

Scientific paper

A reality of solar global magnetic fields Stokes-meter observations with polarimetric accuracy as high as 10-5 - 10-6, and the dependence of Stokes V profiles on distribution of surface magnetic fields in the central zone of the disk are demonstrated. A possibility to use solar disk-integrated and spatially resolved magnetic fields measurements for testing of magnetic fields mapping methods on Sun-like stars is suggested.

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