Detection and characterization of 613 repeating radio burst pairs in the solar corona at 30-50 MHz, with delayed components interpreted as turbulent echoes of harmonic emission via imaging spectroscopy and propagation simulations.
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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.
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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Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona
Detection and characterization of 613 repeating radio burst pairs in the solar corona at 30-50 MHz, with delayed components interpreted as turbulent echoes of harmonic emission via imaging spectroscopy and propagation simulations.
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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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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.