Stereoscopic HXR and EOVSA microwave data constrain source heights in a data-driven MHD simulation of the 2024 Oct 1 X7.1 flare, confirming consistency and associating a secondary source with southward reconnection in a current sheet that exhibits a higher electron low-energy cutoff.
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Numerical MHD and test-particle simulations indicate that unsteady loop-top dynamics enhance electron acceleration efficiency compared to quasi-steady cases by mitigating betatron cooling at compressed field edges.
citing papers explorer
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Non-thermal Sources from Stereoscopic Hard X-ray and Earth-based Microwave Observations in a Data-Constrained Magnetohydrodynamic Simulation
Stereoscopic HXR and EOVSA microwave data constrain source heights in a data-driven MHD simulation of the 2024 Oct 1 X7.1 flare, confirming consistency and associating a secondary source with southward reconnection in a current sheet that exhibits a higher electron low-energy cutoff.
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Numerical Investigation of Efficient Electron Acceleration at an Unsteady Solar Flare Loop-Top
Numerical MHD and test-particle simulations indicate that unsteady loop-top dynamics enhance electron acceleration efficiency compared to quasi-steady cases by mitigating betatron cooling at compressed field edges.