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Effect of magnetic perturbation on the magneto-active plasma

dc.contributor.authorSingh R.P.; Singh R.N.
dc.date.accessioned2025-05-24T09:57:45Z
dc.description.abstractThe effect of magnetic perturbation on the magneto-active plasma has been considered. The collisionless Boltzmann transport equation has been solved for an assumed perturbation in the Maxwellian velocity distribution function. An expression for energy transfer has been derived in terms of perturbed distribution function. Using the magnitude of perturbation for certain astrophysical and laboratory conditions, the heating or cooling of the magneto-active plasma has been studied. © 1970 Società Italiana di Fisica.
dc.identifier.doihttps://doi.org/10.1007/BF02710357
dc.identifier.urihttp://172.23.0.11:4000/handle/123456789/22529
dc.relation.ispartofseriesIl Nuovo Cimento B Series 10
dc.titleEffect of magnetic perturbation on the magneto-active plasma

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