Please use this identifier to cite or link to this item: http://library.iigm.res.in:8080/xmlui/handle/123456789/139
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dc.contributor.authorButi, B.
dc.contributor.authorLakhina, G.S.
dc.date.accessioned2015-06-01T11:01:18Z
dc.date.accessioned2021-02-12T09:29:52Z-
dc.date.available2015-06-01T11:01:18Z
dc.date.available2021-02-12T09:29:52Z-
dc.date.issued1973
dc.identifier.citationJ. Plasma Physics, v.10/2, p.249-263, 1973, doi: 10.1017/S0022377800007832en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/139-
dc.description.abstractElectromagnetic waves propagating perpendicular to an external magnetic field in a non-uniform anisotropic plasma can become unstable due to the excitation of either resonant ion instability or resonant electron instability. The former instability can exist in the absence of both the temperture anisotropy and the temperature gradients, whereas for the excitation of resonant electron instability the presence of at least one of them is necessary. An off-resonance drift cyclotron instability can also get excited if the temperature gradients are much stronger than the magnetic field gradients.en_US
dc.language.isoenen_US
dc.subjectElectromagnetic wavesen_US
dc.subjectMagnetic fielden_US
dc.subjectAnisotropic plasmasen_US
dc.subjectSolar activityen_US
dc.titleElectromagnetic instabilities in non-uniform anisotropic plasmasen_US
dc.typeArticleen_US
dcterms.sourcedoi: 10.1017/S0022377800007832
dc.identifier.accession090656
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