Počet záznamů: 1  

Coincident Observations by the Kharkiv IS Radarand Ionosonde, DMSP and Arase (ERG) Satellites, and FLIP Model Simulations: Implicationsfor the NRLMSISE-00 Hydrogen Density, Plasmasphere, and Ionosphere

  1. 1.
    SYSNO ASEP0492721
    Druh ASEPJ - Článek v odborném periodiku
    Zařazení RIVJ - Článek v odborném periodiku
    Poddruh JČlánek ve WOS
    NázevCoincident Observations by the Kharkiv IS Radarand Ionosonde, DMSP and Arase (ERG) Satellites, and FLIP Model Simulations: Implicationsfor the NRLMSISE-00 Hydrogen Density, Plasmasphere, and Ionosphere
    Tvůrce(i) Kotov, D.V. (UA)
    Richards, P. G. (US)
    Truhlík, Vladimír (UFA-U) RID, ORCID
    Bogomaz, O. V. (UA)
    Shulha, M. (UA)
    Maruyama, N. (US)
    Hairston, M. (US)
    Miyoshi, Y. (JP)
    Kasahara, Y. (JP)
    Kumamoto, A. (JP)
    Tsuchiya, F. (JP)
    Matsuoka, A. (JP)
    Shinohara, I. (JP)
    Hernández-Pajares, M. (ES)
    Domnin, I. F. (UA)
    Zhivolup, T.G. (UA)
    Emelyanov, L. Ya. (UA)
    Chepurnyy, Ya. M. (UA)
    Celkový počet autorů18
    Zdroj.dok.Geophysical Research Letters. - : Wiley - ISSN 0094-8276
    Roč. 45, č. 16 (2018), s. 8062-8071
    Poč.str.10 s.
    Jazyk dok.eng - angličtina
    Země vyd.US - Spojené státy americké
    Klíč. slovathermospheric hydrogen ; 100% underestimation by NRLMSISE-00 model ; observations and simulations ; plasmasphere ; ionosphere ; prominent effects of weak magnetic storm
    Vědní obor RIVBL - Fyzika plazmatu a výboje v plynech
    Obor OECDFluids and plasma physics (including surface physics)
    CEPLTAUSA17100 GA MŠMT - Ministerstvo školství, mládeže a tělovýchovy
    Institucionální podporaUFA-U - RVO:68378289
    UT WOS000445612500021
    EID SCOPUS85053334140
    DOI10.1029/2018GL079206
    AnotaceThis paper reports the results of ionosphere and plasmasphere observations with the Kharkiv incoherent scatter radar and ionosonde, Defense Meteorological Satellite Program, and Arase (ERG) satellites and simulations with field line interhemispheric plasma model during the equinoxes and solstices of solar minimum 24. The results reveal the need to increase NRLMSISE-00 thermospheric hydrogen density by a factor of similar to 2. For the first time, it is shown that the measured plasmaspheric density can be reproduced with doubled NRLMSISE-00 hydrogen density only. A factor of similar to 2 decrease of plasmaspheric density in deep inner magnetosphere (L approximate to 2.1) caused by very weak magnetic disturbance (D-st > -22nT) of 24 December 2017 was observed in the morning of 25 December 2017. During the next night, prominent effects of partially depleted flux tube were observed in the topside ionosphere (similar to 50% reduced H+ ion density) and at the F2-layer peak (similar to 50% decreased electron density). The likely physical mechanisms are discussed.
    PracovištěÚstav fyziky atmosféry
    KontaktKateřina Adamovičová, adamovicova@ufa.cas.cz, Tel.: 272 016 012 ; Kateřina Potužníková, kaca@ufa.cas.cz, Tel.: 272 016 019
    Rok sběru2019
Počet záznamů: 1  

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