Statistics – Computation
Scientific paper
Dec 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...141...67k&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 141, no. 1, Dec. 1984, p. 67-76.
Statistics
Computation
48
Computational Astrophysics, Gyromagnetism, Solar Electrons, Solar Flares, Solar Radio Bursts, Synchrotron Radiation, Brightness Distribution, Centimeter Waves, Decimeter Waves, Electron Distribution, Radio Spectra, Solar Magnetic Field, Stellar Models
Scientific paper
A computation of gyrosynchrotron emission from electrons radiating in an inhomogeneous source is presented. For the purpose of illustration, it is applied to a simple model with parameters typical of some types of solar flare-associated radio emission from microwaves to the decameter band. The source morphology at discrete frequencies, and the spatially integrated spectrum, are represented in their dependence on parameters such as the observer's location relative to the source, the magnetic field, and the density of the ambient medium. It is shown that even a simple model can account for a variety of features observed in spectra and maps of flaring regions at radio wavelengths. The results are discussed in comparison with previous calculations.
Klein Karl-Ludwig
Trottet Gerard
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