Nonresonant instability of kinetic Alfvén waves with κ-electrons

Show simple item record

dc.rights.license CC BY 4.0
dc.contributor.author Barik, K.C.
dc.contributor.author Singh, S.V.
dc.contributor.author Lakhina, G.S.
dc.date.accessioned 2022-05-27T05:38:12Z
dc.date.available 2022-05-27T05:38:12Z
dc.date.issued 2020
dc.identifier.citation Astronomical Journal, v,897, https://doi.org/10.3847/1538-4357/ab962a en_US
dc.identifier.uri http://library.iigm.res.in:8080/xmlui/handle/123456798/133
dc.description.abstract A 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.iso en en_US
dc.subject Solar wind en_US
dc.subject Space plasmas en_US
dc.title Nonresonant instability of kinetic Alfvén waves with κ-electrons en_US
dc.type Article en_US
dcterms.source https://doi.org/10.3847/1538-4357/ab962a


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search DSpace


Advanced Search

Browse

My Account