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Magnetoclinicity Instability

In strongly compressible magnetohydrodynamic turbulence, obliqueness between the large-scale density gradient and magnetic field gives an electromotive force mediated by density variance (intensity of density fluctuation). This effect is named ``magnetoclinicity'', and is expected to play an important role in large-scale magnetic-field generation in astrophysical compressible turbulent flows. Analysis of large-scale instability due to the magnetoclinicity effect shows that the mean magnetic-field perturbation is destabilised at large scales in the vicinity of strong mean density gradient in the presence of density variance.

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Co-authorshipAuthorshipAuthorshipTopic signalTopic signalTopic signalRelated contextWMagnetoclinicity Instabilitypreprint / 2022ANobumitsu YokoiResearcherASteven M. TobiasResearcherTastro-ph.SR7966 worksTphysics.flu-dyn4653 worksTphysics.plasm-ph2285 works
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Magnetoclinicity Instability

preprint / 2022

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