Physics
Scientific paper
Mar 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..104..207a&link_type=abstract
(CNR, Workshop on Radio Continua during Solar Flares, Duino, Italy, May 27-31, 1985) Solar Physics (ISSN 0038-0938), vol. 104, M
Physics
29
Relativistic Electron Beams, Solar Flares, Solar Radio Bursts, Solar Radio Emission, Synchrotron Radiation, Brightness Temperature, Circular Polarization, Radiative Transfer, Solar Corona, Spatial Resolution, Stellar Models
Scientific paper
The current status of knowledge on the theory of radio emission from mildly relativistic electrons and its application in the interpretation of solar radio bursts are reviewed. The recent high spatial resolution microwave observations have given important information about the geometry of the emitting region and have helped in the computation of better inhomogeneous models that qualitatively reproduce several observational characteristics of the emission. The limitations of the observations and the theory (particularly the effect of mode coupling on the observed polarization) are pointed out and the potential of the gyrosynchrotron process as a diagnostic of the physical conditions is discussed. This will help one to obtain quantitative information about the changes of the magnetic field and the acceleration of particles in solar flares.
No associations
LandOfFree
Gyrosynchrotron emission of solar flares does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Gyrosynchrotron emission of solar flares, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gyrosynchrotron emission of solar flares will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-870640