Please use this identifier to cite or link to this item: http://library.iigm.res.in:8080/xmlui/handle/123456798/133
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dc.rights.licenseCC BY 4.0
dc.contributor.authorBarik, K.C.
dc.contributor.authorSingh, S.V.
dc.contributor.authorLakhina, G.S.
dc.date.accessioned2022-05-27T05:38:12Z
dc.date.available2022-05-27T05:38:12Z
dc.date.issued2020
dc.identifier.citationAstronomical Journal, v,897, https://doi.org/10.3847/1538-4357/ab962aen_US
dc.identifier.urihttp://library.iigm.res.in:8080/xmlui/handle/123456798/133
dc.description.abstractA nonresonant instability of kinetic Alfvén waves (KAWs) is studied in a three-component plasma system consisting of background cold ions, an ion beam, and hot electrons with a κ-distribution. The nonresonant KAW instability is produced by the combined sources of ion beam and velocity shear. It is found that the wave excitation by velocity shear alone will give rise to purely growing KAWs, whereas the ion beam velocity alone as a source cannot excite the waves for the considered plasma parameters. It is also observed that the combined sources of ion beam and velocity shear can excite the KAWs in nonresonant instability with finite wave frequency (the mode is not a purely growing mode). Also note that κ-electrons restrict the wave propagation very close to 90°, whereas the Maxwellian electrons permit the wave to propagate a few degrees away from 90°. It is inferred that the presence of κ-electrons shrinks the wave-unstable region of a KAW’s nonresonant instability. The coupling between KAWs and ion-acoustic waves occurs at a lower value of βi for Maxwellian electrons as compared to κ-electrons.en_US
dc.language.isoenen_US
dc.subjectSolar winden_US
dc.subjectSpace plasmasen_US
dc.titleNonresonant instability of kinetic Alfvén waves with κ-electronsen_US
dc.typeArticleen_US
dcterms.sourcehttps://doi.org/10.3847/1538-4357/ab962a
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