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Cited article:

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Center-to-Limb Variation of Solar Bursts Polarization at Millimeter Wavelengths

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Solar Flare Loops: Observations and Interpretations

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Flare parameters inferred from a 3D loop model data base

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The 6 September 2017 X9 Super Flare Observed From Submillimeter to Mid‐IR

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Simulation of Microwave Emission from the Magnetic Arch with Growing Millimeter Spectrum

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THREE-DIMENSIONAL RADIO AND X-RAY MODELING AND DATA ANALYSIS SOFTWARE: REVEALING FLARE COMPLEXITY

Gelu M. Nita, Gregory D. Fleishman, Alexey A. Kuznetsov, Eduard P. Kontar and Dale E. Gary
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Simulations of Gyrosynchrotron Microwave Emission from an Oscillating 3D Magnetic Loop

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Solar Burst Analysis with 3D Loop Models

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THREE-DIMENSIONAL SIMULATIONS OF GYROSYNCHROTRON EMISSION FROM MILDLY ANISOTROPIC NONUNIFORM ELECTRON DISTRIBUTIONS IN SYMMETRIC MAGNETIC LOOPS

Alexey A. Kuznetsov, Gelu M. Nita and Gregory D. Fleishman
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NEW EXPLANATIONS FOR SOME OBSERVATION PHENOMENA OF THE PEAK FREQUENCY OF SOLAR RADIO BURSTS

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The Astrophysical Journal 708 (1) 445 (2010)
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Gyrosynchrotron Emission from Anisotropic Pitch-Angle Distribution of Electrons in 3-D Solar Flare Sources

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Evidence that Synchrotron Emission from Nonthermal Electrons Produces the Increasing Submillimeter Spectral Component in Solar Flares

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Spatial Characterization of a Flare Using Radio Observations and Magnetic Field Topology

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Solar Physics 240 (2) 271 (2007)
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