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.
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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.