Exact 1D solutions show ambipolar diffusion carrying flux in an inner layer between external advection and an Ohmic core, with B scaling as x to the 1/3 in the diffusion region and eigenmodes evolving toward lowest-order states.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Hybrid simulations of tearing reconnection show magnetic energy converts to ion bulk flows and heating in the nonlinear phase, with island contraction driving parallel ion temperature anisotropy that firehose instabilities regulate by redistributing energy to the perpendicular direction.
Low-angular-momentum test-particle models of HVCs originating at tens of kpc in a rotating halo reproduce observed kinematics and imply an accretion rate of several solar masses per year sufficient for long-term star formation.
citing papers explorer
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The Singular Behaviour of Ambipolar Diffusion Revealed by 1D Cartesian Solutions
Exact 1D solutions show ambipolar diffusion carrying flux in an inner layer between external advection and an Ohmic core, with B scaling as x to the 1/3 in the diffusion region and eigenmodes evolving toward lowest-order states.
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Tearing Driven Reconnection: Energy Conversion Involving Firehose Kinetic Instabilities (2D Hybrid M\"obius Simulations)
Hybrid simulations of tearing reconnection show magnetic energy converts to ion bulk flows and heating in the nonlinear phase, with island contraction driving parallel ion temperature anisotropy that firehose instabilities regulate by redistributing energy to the perpendicular direction.
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Modeling the Accretion of High-Velocity Clouds from a Rotating Halo
Low-angular-momentum test-particle models of HVCs originating at tens of kpc in a rotating halo reproduce observed kinematics and imply an accretion rate of several solar masses per year sufficient for long-term star formation.