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Spatial and temporal variability of whistler mode emissions in the Earth’s inner magnetosphere

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    0497709 - ÚFA 2019 BE eng A - Abstract
    Santolík, Ondřej
    Spatial and temporal variability of whistler mode emissions in the Earth’s inner magnetosphere.
    2 nd URSI AT-RASC Proceedings. Gent: URSI, 2018.
    [URSI Atlantic Radio Science Meeting (AT-RASC) /2./. 28.05.2018-01.06.2018, Gran Canaria]
    Institutional support: RVO:68378289
    Keywords : magnetosphere * plasmasphere * Van Allen radiation belt * whistler mode waves
    OECD category: Fluids and plasma physics (including surface physics)
    http://www.ursi.org/proceedings/procAT18/papers/SH0114.pdf

    Electromagnetic whistler-mode emissions are important components of the puzzle of the dynamic behavior of
    the outer Van Allen radiation belt and the slot region. Survey data of the Waves instrument from the Electric
    and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) onboard the Van Allen Probes are
    recorded with a nearly 100 % coverage. We use more than 5 years of these measurements to investigate
    statistical properties of wave power which directly influences results of quasilinear diffusion models.
    Previous results have shown that average wave power inside the plasmasphere has a flat peak at a MLT between
    8 h and 17 h and L values between 2 and 4 and that it increases with geomagnetic activity. Our results indicate
    that random variations of wave power are still larger or comparable to the effects of these systematic trends.
    Power variations from simultaneous spatially separated measurements are dominated by separations in MLT at
    scales below 30 min, with a weaker influence of separations in L or magnetic latitude. Measurements which
    were done at close points in space show temporal variations at time scales of tens of minutes.
    Permanent Link: http://hdl.handle.net/11104/0290218

     
     
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