Ultimate Fast Gyrosynchrotron Codes
Alexey A. Kuznetsov, Gregory D. Fleishman

TL;DR
This paper introduces advanced fast gyrosynchrotron codes that handle arbitrary electron distribution functions, significantly enhancing the flexibility and accuracy of plasma diagnostics and solar flare modeling.
Contribution
We extended existing fast gyrosynchrotron codes to support arbitrary numerical electron distributions, removing previous limitations and improving modeling capabilities.
Findings
Codes can now process arbitrary distribution functions.
Enhanced accuracy in spectral calculations.
Broader applicability to realistic plasma conditions.
Abstract
The past decade has seen a dramatic increase of practical applications of the microwave gyrosynchrotron emission for plasma diagnostics and three-dimensional modeling of solar flares and other astrophysical objects. This break-through turned out to become possible due to apparently minor, technical development of Fast Gyrosynchrotron Codes, which enormously reduced the computation time needed to calculate a single spectrum, while preserving accuracy of the computation. However, the available fast codes are limited in that they could only be used for a factorized distribution over the energy and pitch-angle, while the distributions of electrons over energy or pitch-angle are limited to a number of predefined analytical functions. In realistic simulations, these assumptions do not hold; thus, the codes free from the mentioned limitations are called for. To remedy this situation, we…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
