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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3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
years
2026 3verdicts
UNVERDICTED 3representative citing papers
MHD simulation of a CME reveals that spacecraft connect to different regions of an inhomogeneous shock, reproducing the observed SEP flux differences among Earth, STA, and SolO.
SPADE demonstrates a small, fully digital phased array spectrograph for decameter solar radio observations, with first 2024 data showing temporal and frequency resolution suitable for coronal turbulence and propagation studies.
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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The Small Phased Array DEmonstrator (SPADE) -- Description and first results
SPADE demonstrates a small, fully digital phased array spectrograph for decameter solar radio observations, with first 2024 data showing temporal and frequency resolution suitable for coronal turbulence and propagation studies.