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dc.contributor.authorSingh, S.V.
dc.contributor.authorReddy, R.V.
dc.contributor.authorLakhina, G.S.
dc.date.accessioned2015-10-05T10:06:56Z
dc.date.accessioned2021-02-12T09:31:17Z-
dc.date.available2015-10-05T10:06:56Z
dc.date.available2021-02-12T09:31:17Z-
dc.date.issued2009
dc.identifier.citationAdvances in Space Research, v.43/12, p.1940-1944, 2009, doi: 10.1016/j.asr.2009.02.015en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/529-
dc.description.abstractBroadband electrostatic noise (BEN) is commonly observed in different regions of the Earth’s magnetosphere, eg., auroral region, plasma sheet boundary layer, etc. The frequency of these BENs lies in the range from lower hybrid to the local electron plasma frequency and sometimes even higher. Spacecraft observations suggest that the high and low-frequency parts of BEN appear to be two different wave modes. There is a well established theory for the high-frequency part which can be explained by electrostatic solitary waves, however, low-frequency part is yet to be fully understood. The linear theory of low-frequency waves is developed in a four-component magnetized plasma consisting of three types of electrons, namely cold background electron, warm electrons, warm electron beam and ions. The electrostatic dispersion relation is solved, both analytically and numerically. For the parameters relevant to the auroral region, our analysis predict excitation of electron acoustic waves in the frequency range of 17 Hz to 2.6 kHz with transverse wavelengths in range of (1–70) km. The results from this model may be applied to explain some features of the low-frequency part of the broadband electrostatic noise observed in other regions of the magnetosphere.en_US
dc.language.isoenen_US
dc.subjectBroadband electrostatic noiseen_US
dc.subjectLow-frequency wavesen_US
dc.subjectMagnetosphereen_US
dc.subjectBENen_US
dc.titleBroadband electrostatic noise and low-frequency waves in the Earth’s magnetosphereen_US
dc.typeArticleen_US
dc.identifier.accession091042
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