Počet záznamů: 1  

Solar eclipses and their effects in the ionospheric plasma

  1. 1.
    SYSNO ASEP0465441
    Druh ASEPA - Abstrakt
    Zařazení RIVO - Ostatní
    NázevSolar eclipses and their effects in the ionospheric plasma
    Tvůrce(i) Koucká Knížová, Petra (UFA-U) RID, ORCID
    Celkový počet autorů1
    Zdroj.dok.6th IAGA/ICMA/SCOSTEP Vertical Coupling Workshop: Abstracts. - Taipei : International Association of Geomagnetism and Aeronomy (IAGA), 2016
    S. 32
    Poč.str.1 s.
    Forma vydáníOnline - E
    AkceIAGA/ICMA/SCOSTEP Workshop on Vertical Coupling in the Atmosphere-Ionosphere System /6./
    Datum konání25.07.2016 - 29.07.2016
    Místo konáníTaipei
    ZeměTW - Taiwan - Čína
    Typ akceWRD
    Jazyk dok.eng - angličtina
    Země vyd.TW - Taiwan - Čína
    Klíč. slovaacoustic-gravity waves ; ionosphere ; solar eclipse
    Vědní obor RIVDG - Vědy o atmosféře, meteorologie
    CEPGA15-24688S GA ČR - Grantová agentura ČR
    Institucionální podporaUFA-U - RVO:68378289
    AnotaceTerrestrial atmosphere shows a high variability over a broad range of periodicities, which mostly consists
    of wave-like perturbations characterized by various spatial and temporal scales. The interest for short
    time variability in ionospheric attributes is related to the role that ionosphere plays in the Earth's
    environment and space weather. Acoustic-gravity waves (AGWs), waves in the period range from subseconds
    to several hours, are sources of most of the short-time ionospheric variability and play an
    important role in the dynamics and energetics of atmosphere and ionosphere systems.

    During solar eclipse, the lunar shadow creates a cool spot in the atmosphere that sweeps at supersonic
    speed across the Earth’s atmosphere. The atmosphere strongly responds to the decrease in ionization
    flux and heating. The very sharp border between sunlit and eclipsed region, characterized by strong
    gradients in temperature and ionization flux, moves throughout the atmosphere and drives it into a nonequilibrium
    state. Acoustic-gravity waves contribute to the return to equilibrium. At thermospheric
    heights, the reduction in temperature causes a decrease in pressure over the totality footprint to which
    the neutral winds respond. Thermal cooling and downward transport of gases lead to neutral composition
    changes in the thermosphere that have significant influence on the resulting electron density distribution.
    Although the mechanisms are not well understood, experimental studies show direct evidence that solar
    eclipses induce wave-like oscillations in the acoustic-gravity wave domain.
    PracovištěÚstav fyziky atmosféry
    KontaktKateřina Adamovičová, adamovicova@ufa.cas.cz, Tel.: 272 016 012 ; Kateřina Potužníková, kaca@ufa.cas.cz, Tel.: 272 016 019
    Rok sběru2017
Počet záznamů: 1  

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