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Effects of the Geomagnetic Storm and the Solar Eclipse Observed During March 2015

  1. 1.
    0472421 - ÚFA 2017 RIV BG eng A - Abstract
    Boška, Josef - Koucká Knížová, Petra - Kouba, Daniel - Mošna, Zbyšek - Potužníková, Kateřina
    Effects of the Geomagnetic Storm and the Solar Eclipse Observed During March 2015.
    Book of Abstracts: Eighth Workshop "Solar Influences on the Magnetosphere, Ionosphere and Atmosphere". Sofia: Space Research and Technologies Institute, Bulgarian Academy of Sciences, 2016. s. 2.
    [Workshop "Solar Influences on the Magnetosphere, Ionosphere and Atmosphere" /8th/. 30.05.2016-03.06.2016, Sunny Beach]
    R&D Projects: GA ČR(CZ) GA15-24688S
    Institutional support: RVO:68378289
    Keywords : geomagnetic storm * ionospheric vertical sounding * ionospheric drift velocity * solar eclipse
    Subject RIV: DG - Athmosphere Sciences, Meteorology
    http://ws-sozopol.stil.bas.bg/

    During March 2015 two significant events strongly disturbed the state of the ionosphere
    over Central Europe. Strong geomagnetic storm with Kp - 8 and DST - 223 started 17.3.2015.
    During the recovery phase of this storm the second significant event Solar eclipse 20.3.2015
    strongly affected the state of the ionosphere above Europe.
    Paper presents changes of the state of the ionosphere observed during geomagnetic storm
    17.3.2015 and Solar eclipse 20.3.2015 as was observed at ionospheric observatory Pruhonice.
    Digisonde DPS4 D, installed at the Pruhonice observatory, allow standard ionospheric
    vertical sounding measurements. Digisonde DPS4 D is also working as Doppler radar and allow
    ionospheric drift measurements. Ionospheric vertical sounding and drift velocity was measured
    with standard delay time 15 minutes during geomagnetic storm. Solar eclipse 20.3.2015 above
    Pruhonice started 08:36 UT and finished 10:45 UT with magnitude 0.743.
    Ionospheric vertical sounding data and drift velocity measurements with delay time 3
    minutes was measured during eclipse event. Tis time resolution allow observation short time
    changes of the inosphere during eclipse event.
    Permanent Link: http://hdl.handle.net/11104/0269733

     
     
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