Derivation of flare magnetic field and density from two simultaneous frequency observations

Details Derivation of flare magnetic field and density from two simultaneous frequency observations Derivation of flare magnetic field and density from two simultaneous frequency observations

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mnras.329..567s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 329, Issue 3, pp. 567-571.

Astronomy and Astrophysics

Astronomy

Radiation Mechanisms: Non-Thermal, Methods: Numerical, Sun: Flares, Sun: Magnetic Fields, Sun: Radio Radiation

Scientific paper

We developed a simple model for a flare loop, which was used to fit the emission in the microwave (17GHz) and millimetre-wave (80GHz) ranges for the giant flare of 1991 June 4. The simplicity of the model enabled the exploration of a wide range of parameters in a reasonable time. It was possible, using the simple model, to derive from the 17- and 80-GHz data the magnetic field and the number density for every measurement point in the time range we chose to fit.

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