Coronal Heating and Microwave Emission from the Solar Active Region NOAA 0139

Details Coronal Heating and Microwave Emission from the Solar Active Region NOAA 0139 Coronal Heating and Microwave Emission from the Solar Active Region NOAA 0139

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...3e..38t&link_type=abstract

Solar Active Regions and 3D Magnetic Structure, 26th meeting of the IAU, Joint Discussion 3, 16-17 August, 2006, Prague, Czech R

Computer Science

Scientific paper

Dynamics and structure of the active region NOAA 0139 on the basis of microwave observations at RT-22, SSRT, and RATAN-600 have been investigated. As appears from the wavelet analysis the observed behavior of the S-component of microwave emission is determined by elementary flare events. It has been shown that accelerated electrons can play an important role in heating the plasma of the transition region and upper chromosphere.

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