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arXiv · 0906.0192

Dynamic Magnetography of Solar Flaring Loops

Gregory D. Fleishman·Gelu M. Nita·Dale E. Gary
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Abstract

We develop a practical forward fitting method based on the SIMPLEX algorithm with shaking, which allows the derivation of the magnetic field and other parameters along a solar flaring loop using microwave imaging spectroscopy of gyrosynchrotron emission. We illustrate the method using a model loop with spatially varying magnetic field, filled with uniform ambient density and an evenly distributed fast electron population with an isotropic, power-law energy distribution.

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Gregory D. Fleishman, Gelu M. Nita, Dale E. Gary. 2009-06-01. Dynamic Magnetography of Solar Flaring Loops. https://doi.org/10.1088/0004-637x%2F698%2F2%2Fl183

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