Type II radio burst sources align with quasi-perpendicular shock regions of enhanced Mach number in the simulation, with fundamental-harmonic offsets matching the projected shock-surface magnetic field direction.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
UNVERDICTED 2representative citing papers
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.
citing papers explorer
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Radio Spectral Imaging and MHD Modeling of a CME-Driven Shock: Connecting Solar Type II Radio Bursts with Shock-Surface Magnetic Geometry
Type II radio burst sources align with quasi-perpendicular shock regions of enhanced Mach number in the simulation, with fundamental-harmonic offsets matching the projected shock-surface magnetic field direction.
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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.