Non-reflecting MHD boundaries can severely distort a magnetic spheromak passing through them at sub-Alfvenic speeds, causing it to bounce or accelerate, because they discard the incoming information needed to preserve force balance.
Title resolution pending
1 Pith paper cite this work, alongside 20 external citations. Polarity classification is still indexing.
1
Pith paper citing it
20
external citations · OpenAlex
citation-role summary
background 1
citation-polarity summary
fields
astro-ph.SR 1years
2025 1verdicts
CONDITIONAL 1roles
background 1polarities
unclear 1representative citing papers
citing papers explorer
-
Simulating the photospheric to coronal plasma using magnetohydrodyanamic characteristics II: reflections on non-reflecting boundary conditions
Non-reflecting MHD boundaries can severely distort a magnetic spheromak passing through them at sub-Alfvenic speeds, causing it to bounce or accelerate, because they discard the incoming information needed to preserve force balance.