Generation of electron-acoustic waves in the magnetosphere

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dc.contributor.author Singh, S.V.
dc.contributor.author Lakhina, G.S.
dc.date.accessioned 2015-09-15T06:53:41Z
dc.date.accessioned 2021-02-12T09:29:03Z
dc.date.available 2015-09-15T06:53:41Z
dc.date.available 2021-02-12T09:29:03Z
dc.date.issued 2001
dc.identifier.citation Planetary and Space Science, v.49/1, p.107-114, 2001, doi: 10.1016/S0032-0633(00)00126-4 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/412
dc.description.abstract Generation 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.language.iso en en_US
dc.subject Electron-acoustic waves en_US
dc.subject Magnetosphere en_US
dc.subject Earth's magnetosphere en_US
dc.subject Broadband electrostatic noise (BEN) en_US
dc.subject EAW en_US
dc.title Generation of electron-acoustic waves in the magnetosphere en_US
dc.type Article en_US
dc.identifier.accession 090909


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