Global Energetics of Solar Flares. XII. Energy Scaling Laws
Markus J. Aschwanden

TL;DR
This paper tests 30 variants of five physical scaling laws against observational data from approximately 400 solar flares, confirming the validity of 10 variants and supporting the theoretical models of solar flare energetics.
Contribution
It systematically evaluates multiple scaling law variants against real data, identifying which theoretical models are consistent with observations of solar flares.
Findings
10 out of 30 scaling law variants are consistent with observations.
The validated scaling laws support existing theoretical models of solar flare energetics.
The study confirms the applicability of specific energy scaling laws to real solar flare data.
Abstract
In this study we test 30 variants of 5 physical scaling laws that describe different aspects of solar flares. We express scaling laws in terms of the magnetic potential field energy , the mean potential field strength , the free energy , the dissipated magnetic flare energy , the mean loop length scale , the mean helically twisted flux tube radius , the sunspot radius , the emission measure-weighted flare temperature , the electron density , and the total emission measure , measured from a data set of GOES M- and X-class flare events. The 5 categories of physical scaling laws include (i) a scaling law of the potential-field energy, (ii) a scaling law for helical twisting, (iii) a scaling law for Petschek-type magnetic reconnection, (iv) the Rosner-Tucker-Vaiana scaling law, and (v) the Shibata-Yokoyama scaling law. 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.
