A constant-turn flux rope MHD simulation reproduces the rotating magnetic field of a stealth ICME observed at radially aligned Solar Orbiter and Earth, with +/-5 hour arrival time errors.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Magnetohydrodynamic Simulation of a Coronal Mass Ejection Observed During the Near-radial Alignment of Solar Orbiter and Earth
A constant-turn flux rope MHD simulation reproduces the rotating magnetic field of a stealth ICME observed at radially aligned Solar Orbiter and Earth, with +/-5 hour arrival time errors.