Reduced drift-kinetics with thermal velocity distribution across magnetic field
Reviewed by Pithpith:TADI5FHCopen to challenge →
classification
astro-ph.SR
physics.plasm-ph
keywords
distributionequationsreducedacrossapproximateassumptioncoronaderive
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The goal of this study is to develop an approximate self-consistent description of particle motion in strongly magnetised solar corona. We derive a set of reduced drift-kinetic equations based on the assumption that the gyro-velocity distribution is Maxwellian. The equations are tested using simple 1D models.
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