A coupled nested-grid MHD framework with AMR to 700 km resolution and Boris correction for strong fields enables end-to-end simulation of CME emergence, eruption, and heliospheric propagation from realistic active-region scales.
Title resolution pending
3 Pith papers cite this work, alongside 257 external citations. Polarity classification is still indexing.
3
Pith papers citing it
257
external citations · OpenAlex
fields
astro-ph.SR 3years
2026 3verdicts
UNVERDICTED 3representative citing papers
Background magnetic field orientation affects eruption success and reconnection in MHD simulations of pre-existing flux ropes, with antiparallel fields enabling faster but shorter flare reconnection.
Observational data-driven MHD simulations reproduced an X1.6 flare's onset and showed that photospheric velocity input extends prediction lead time beyond one hour.
citing papers explorer
-
Modeling of Coronal Mass Ejection Originated from a Sheared Arcade of Realistic Active-Region Scale and Its Propagation in the Heliosphere: Methodology
A coupled nested-grid MHD framework with AMR to 700 km resolution and Boris correction for strong fields enables end-to-end simulation of CME emergence, eruption, and heliospheric propagation from realistic active-region scales.
-
Effects of the Background Magnetic Field on Flux Rope Eruptions
Background magnetic field orientation affects eruption success and reconnection in MHD simulations of pre-existing flux ropes, with antiparallel fields enabling faster but shorter flare reconnection.
-
Predictability of a solar flare in May 2024 using observational data-driven MHD simulations
Observational data-driven MHD simulations reproduced an X1.6 flare's onset and showed that photospheric velocity input extends prediction lead time beyond one hour.