1996
DOI: 10.1002/asna.2113170508
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Some ideas concerning the problem of anomalous polar E region heating due to Farley‐Buneman turbulence

Abstract: The energetics of the excitation of the Farley-Buneman instability is considered, which is recently observed in the auroral and equatorial E regions of the Earth's ionosphere at altitudes between 100 km and 120 km. In the magnetic field of the Earth the Farley-Buneman instability is excited under the condition of a strong enough external electric field in the case of ion-neutral collisions with frequencies much larger than the ion gyrofrequency and electron-neutral collisions with frequencies much below the el… Show more

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Cited by 3 publications
(1 citation statement)
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“…Through this interaction a mechanism for the saturation of the turbulence in the electrojet is created which is not locally controlled as is usually assumed [St.-Maurice, 1990;Janhunen, 1994;Oppenheim et al, 1996], but which depends on the complete current circuit, including the electrojet part and the field aligned magnetospheric currents and their sources. This view has also been convincingly advocated by Liperovsky et al [1996]. The external power input to the turbulent plasma per unit volume in the ionosphere, E 0 Á hji, is dissipated by normal collisional damping of the marginally stable modes making up the turbulent density and velocity fluctuations.…”
Section: Introductionmentioning
confidence: 75%
“…Through this interaction a mechanism for the saturation of the turbulence in the electrojet is created which is not locally controlled as is usually assumed [St.-Maurice, 1990;Janhunen, 1994;Oppenheim et al, 1996], but which depends on the complete current circuit, including the electrojet part and the field aligned magnetospheric currents and their sources. This view has also been convincingly advocated by Liperovsky et al [1996]. The external power input to the turbulent plasma per unit volume in the ionosphere, E 0 Á hji, is dissipated by normal collisional damping of the marginally stable modes making up the turbulent density and velocity fluctuations.…”
Section: Introductionmentioning
confidence: 75%