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.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.SR 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Energy-conserving numerics in CME simulations yield >2x higher kinetic energy by extending flare reconnection duration compared to non-conservative schemes.
citing papers explorer
-
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.
-
The Effects of Energy Conservation in Simulating Solar Eruptions
Energy-conserving numerics in CME simulations yield >2x higher kinetic energy by extending flare reconnection duration compared to non-conservative schemes.