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.
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Recent sub-second imaging spectroscopy of solar radio burst fine structures challenges existing theoretical models, with the SKA positioned to enable new frameworks for electron acceleration and coronal turbulence.
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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.
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Solar Radio Burst Fine Structures
Recent sub-second imaging spectroscopy of solar radio burst fine structures challenges existing theoretical models, with the SKA positioned to enable new frameworks for electron acceleration and coronal turbulence.