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On the origin of lower- and upper-frequency cutoffs on wedge-like spectrograms observed by DEMETER in the midlatitude ionosphere

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    SYSNO ASEP0343319
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleOn the origin of lower- and upper-frequency cutoffs on wedge-like spectrograms observed by DEMETER in the midlatitude ionosphere
    Author(s) Shklyar, D. R. (RU)
    Parrot, M. (FR)
    Chum, Jaroslav (UFA-U) RID, ORCID
    Santolík, Ondřej (UFA-U) RID, ORCID
    Titova, E. E. (RU)
    Source TitleJournal of Geophysical Research - ISSN 0148-0227
    Roč. 115, - (2010), A05203/1-A05203/12
    Number of pages12 s.
    Languageeng - English
    CountryUS - United States
    KeywordsDEMETER ; midlatitude ionosphere ; spectrograms
    Subject RIVBL - Plasma and Gas Discharge Physics
    R&D ProjectsME09107 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    GA205/09/1253 GA ČR - Czech Science Foundation (CSF)
    CEZAV0Z30420517 - UFA-U, BC-A (2005-2011)
    UT WOS000277480900002
    DOI10.1029/2009JA014672
    AnnotationWe report observations of unusual lower and upper cutoff frequencies on VLF spectrograms recorded by the DEMETER satellite orbiting at 700 km. The upper cutoff frequencies vary approximately in proportion to L-3. The lower cutoff frequencies in the spectrograms are almost constant. Between these cutoffs, which form a wedge, intense whistlers are observed, whereas only 0+ whistlers, and probably, ducted whistlers are present outside the cutoffs. We explain the observed spectrograms on the basis of the features of whistler-mode wave propagation in the inner magnetosphere. The upper cutoff frequency is determined by the limiting trajectories that confine the waves of a given frequency propagating obliquely from a source located in the opposite hemisphere. The lower frequency cutoff is determined by the LHR maximum, since quasiresonant waves with lower frequencies originating in the opposite hemisphere do not reach the satellite due to the LHR reflection above it.
    WorkplaceInstitute of Atmospheric Physics
    ContactKateřina Adamovičová, adamovicova@ufa.cas.cz, Tel.: 272 016 012 ; Kateřina Potužníková, kaca@ufa.cas.cz, Tel.: 272 016 019
    Year of Publishing2011
Number of the records: 1  

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