ON THE ORIGIN OF LOW- AND MIDDLER-LATITUDE IONOSPHERIC TURBULENCE

dc.contributor.authorMolchanov O.A.
dc.date.accessioned2022-11-03T10:21:05Z
dc.date.available2022-11-03T10:21:05Z
dc.date.issued2004
dc.description.abstractThe paper is motivated by our recent results of observation on the satellites Cosmos-900, Aureol-3 and Intercosmos-24, which are presented in this issue (Molchanov et al.). We try to show that a drift mode leading to the ionospheric turbulence (IT) is sustained by wind of the neutral particles, that a source of the IT is energy flux from the atmospheric gravity waves (AGW) to the long scales of IT, and that IT develops to smaller scales as in the classic Kolmogorov's turbulence. Then the earthquake influence observed can be explained by redistribution of the AGW pumping during periods of seismic activity.
dc.identifierhttps://www.elibrary.ru/item.asp?id=13453716
dc.identifier.citationPhysics and Chemistry of the Earth, Parts A/B/C, 2004, 29, 4-9, 559-567
dc.identifier.issn1474-7065
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/39350
dc.titleON THE ORIGIN OF LOW- AND MIDDLER-LATITUDE IONOSPHERIC TURBULENCE
dc.typeСтатья

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