Magnetic field in active regions of the sun at coronal heights

Details Magnetic field in active regions of the sun at coronal heights Magnetic field in active regions of the sun at coronal heights

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009iaus..257..349b&link_type=abstract

Universal Heliophysical Processes, Proceedings of the International Astronomical Union, IAU Symposium, Volume 257, p. 349-352

Astronomy and Astrophysics

Astronomy

Sun: Radio Radiation Methods: Data Analysis

Scientific paper

A method is developed for estimation of the vertical structure of the magnetic field in active regions using multi-wave spectral-polarization measurements of radio waves which gives not only the dependence of magnetic field strength on height but also determines two-dimensional form of a magnetic flux tube, emitted in the microwave range of wavelengths.

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