Non-thermal microwave solar radio emission from plage-associated coronal loops and their 3D modelling.
Abstract
On September 20-29, 1996, there was SOHO, Yohkoh and Meudon joint Observations of Filaments and Chromospheric Activity. The target active region was observed also with RATAN-600 radiotelescoope and Nobeyama radioheliograph in the frames of the SOHO ground-based support program. This active region was very stable and its radio emission was observed at least during five solar rotations. The authors present some results of observations and their modelling. The observation combined with the model show that there are the non-thermal processes continuously acting in the solar corona in the period of deep minimum of solar activity.
- Publication:
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JOSO Annu. Rep., 1997
- Pub Date:
- 1998
- Bibcode:
- 1998joso.proc...92K
- Keywords:
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- Solar Radio Radiation: Solar Coronal Loops;
- Solar Radio Radiation: Solar Active Regions