Magnetic field strength estimation in synchrotron radiation sources

Details Magnetic field strength estimation in synchrotron radiation sources Magnetic field strength estimation in synchrotron radiation sources

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.222..107z&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 222, no. 1-2, p. 107-111

Astronomy and Astrophysics

Astrophysics

3

Energetic Particles, Flux Density, Gamma Ray Bursts, Particle Interactions, Radio Bursts, Solar Flares, Solar Magnetic Field, Synchrotron Radiation, X Rays, Electron Distribution, Line Of Sight, Spectroscopy

Scientific paper

In this paper a method of estimating the magnetic field strength, B, in a homogeneous microwave burst source with simplified expressions for the synchrotron radiation is presented. An approximation formula of the magnetic field is obtained using the method. Once the magnetic field is estimated the total number of energetic electrons along the line of sight NL can be estimated also. The errors of B and NL have been given. It is found that this method is useful for semiquantitative investigations of models of radio burst sources.

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