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Magnetic field in active regions of the sun at coronal heights
Published online by Cambridge University Press: 01 September 2008
Abstract
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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 4 , Symposium S257: Universal Heliophysical Processes , September 2008 , pp. 349 - 352
- Copyright
- Copyright © International Astronomical Union 2009