Low-frequency instabilities driven by oxygen ion beams in plasma sheet region

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dc.contributor.author Kakad, Amar
dc.contributor.author Lakhina, G.S.
dc.contributor.author Singh, S.V.
dc.date.accessioned 2015-09-03T09:01:54Z
dc.date.accessioned 2021-02-12T10:20:20Z
dc.date.available 2015-09-03T09:01:54Z
dc.date.available 2021-02-12T10:20:20Z
dc.date.issued 2005
dc.identifier.citation Advances in Space Research, v.36/10, p.1890-1894, 2005, doi: 10.1016/j.asr.2004.01.029 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/318
dc.description.abstract Low-frequency instabilities driven by ionospheric oxygen ion beam are studied in the plasma sheet region. In three component cold and uniform plasma consisting of electrons, protons and oxygen ions, the linear dispersion relation is derived with velocity shear in each component. The dispersion relation is solved for the case of uniform as well as nonuniform oxygen ion beam with shear flow passing through stationary electron–ion plasma. It is found that uniform oxygen ion beam can excite the low-frequency instabilities provided the Mach number exceeds a critical value. For the case of nonuniform oxygen ion beam it is found that the velocity shear can give rise to Kelvin–Helmholtz type instabilities. These low-frequency waves may be responsible for the low-frequency turbulence observed in the plasma sheet region. en_US
dc.language.iso en en_US
dc.subject Low-frequency instabilities en_US
dc.subject Magnetosphere en_US
dc.subject Plasma sheet region en_US
dc.subject Oxygen ion beams en_US
dc.title Low-frequency instabilities driven by oxygen ion beams in plasma sheet region en_US
dc.type Article en_US
dcterms.source doi: 10.1016/j.asr.2004.01.029
dc.identifier.accession 090810


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