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.
Astronomy & Astrophysics , archivePrefix = "arXiv", eprint =
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Radio wave distortion effects serve as established probes of solar corona and wind turbulence parameters, with SKA expected to expand observational capabilities.
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 Wave Propagation as a Probe of the Solar Corona and Solar Wind
Radio wave distortion effects serve as established probes of solar corona and wind turbulence parameters, with SKA expected to expand observational capabilities.