Generation of electron-acoustic waves in the magnetosphere

dc.contributor.authorSingh, S.V.
dc.contributor.authorLakhina, G.S.
dc.date.accessioned2015-09-15T06:53:41Z
dc.date.accessioned2021-02-12T09:29:03Z
dc.date.available2015-09-15T06:53:41Z
dc.date.available2021-02-12T09:29:03Z
dc.date.issued2001
dc.description.abstractGeneration of electron-acoustic waves (EAWs) is examined in an unmagnetized, four-component plasma consisting of stationary cold and hot Maxwellian electrons, drifting electron beam and ions. The addition of hot background electrons to the previously existing three-component model reduces the excited EAW frequencies and growth rates. Electrostatic linear dispersion equation is solved analytically for the growth rate and real frequency. The linear theory of EAWs is applied to the dayside auroral zone and other regions of the magnetosphere. The mechanism can generate frequencies over a wide range of Full-size image (<1 K)–Full-size image (<1 K), Full-size image (<1 K)–Full-size image (<1 K) and Full-size image (<1 K)–Full-size image (<1 K) in the dayside auroral zone, plasma sheet boundary layer and polar cusp, respectively. The e-folding time of the instability is of the order of a few milliseconds, and the waves are expected to grow nonlinearly to large amplitudes. Our four-component model can explain the broadband electrostatic noise (BEN) observations below the total electron plasma frequencies in these regions fairly well.en_US
dc.identifier.accession090909
dc.identifier.citationPlanetary and Space Science, v.49/1, p.107-114, 2001, doi: 10.1016/S0032-0633(00)00126-4en_US
dc.identifier.urihttp://library.iigm.res.in:4000/handle/123456789/412
dc.language.isoenen_US
dc.subjectElectron-acoustic wavesen_US
dc.subjectMagnetosphereen_US
dc.subjectEarth's magnetosphereen_US
dc.subjectBroadband electrostatic noise (BEN)en_US
dc.subjectEAWen_US
dc.titleGeneration of electron-acoustic waves in the magnetosphereen_US
dc.typeArticleen_US

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