Number of the records: 1  

Drifting field-aligned density structures in the night-side polar cap

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    SYSNO ASEP0024213
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JOstatní články
    TitleDrifting field-aligned density structures in the night-side polar cap
    TitleDriftující hustotní struktury v polární oblasti na noční straně
    Author(s) Santolík, Ondřej (UFA-U) RID, ORCID
    Persoon, A. M. (US)
    Gurnett, D. A. (US)
    Décréau, P. M. E. (FR)
    Pickett, J. S. (US)
    Maršálek, O. (US)
    Maksimovic, M. (FR)
    Cornilleau-Wehrlin, N. (FR)
    Source TitleGeophysical Research Letters. - : Wiley - ISSN 0094-8276
    Roč. 32, - (2005), L06106-1
    Number of pages4 s.
    Languageeng - English
    CountryUS - United States
    KeywordsMagnetospheric Physics ; Plasma convection ; Plasma waves and instabilities ; Polar cap phenomena ; Magnetospheric configuration and dynamics
    Subject RIVBL - Plasma and Gas Discharge Physics
    R&D ProjectsGA202/03/0832 GA ČR - Czech Science Foundation (CSF)
    ME 650 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    1P05ME811 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    CEZAV0Z30420517 - UFA-U, BC-A (2005-2011)
    AnnotationSpatio-temporal properties of density irregularities in the night-side polar cap are inferred from multi-point observations of auroral hiss at a radial distance of 5 Earth radii. In this case study, we use high resolution data of the wave instruments onboard the four Cluster spacecraft to estimate the local plasma density, obtaining values close to 1 cm−3 with density depletions decreasing down to 0.15 cm−3. Combined analysis in different points in space conclusively shows for the first time that these density structures are field-aligned and that they predominantly drift in the anti-sunward direction at speeds of a few km/s. This corresponds to a dawn-to-dusk convection electric field of approximately 1 mV/m. The transverse dimension of the observed density depletions, mapped down to the ionospheric heights, is of the order of a few tens of km. Their lifetime is probably longer than tens of seconds.
    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 Publishing2006
Number of the records: 1  

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