LOFAR imaging spectroscopy and anisotropic scattering simulations indicate that compact apparent sizes of diverse fine structures in a solar noise storm arise primarily from emission within closed magnetic field structures rather than intrinsic emission differences.
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This review summarizes particle acceleration models in solar flares and how SKAO observations will enable better characterization of nonthermal particle populations and coronal properties.
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.
citing papers explorer
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Frequency-time-resolved Imaging Spectroscopy of Fine Structures in a Solar Radio Noise Storm
LOFAR imaging spectroscopy and anisotropic scattering simulations indicate that compact apparent sizes of diverse fine structures in a solar noise storm arise primarily from emission within closed magnetic field structures rather than intrinsic emission differences.
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Radio Diagnostics of Particle Acceleration in Solar Flares with SKAO Observations
This review summarizes particle acceleration models in solar flares and how SKAO observations will enable better characterization of nonthermal particle populations and coronal properties.
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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.