- Planetary and gravity wave signatures in the F region ionosphere with…
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Planetary and gravity wave signatures in the F region ionosphere with impact on radio propagation predictions and variability

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    SYSNO ASEP0104043
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JOstatní články
    TitlePlanetary and gravity wave signatures in the F region ionosphere with impact on radio propagation predictions and variability
    TitlePlanetární a gravitační vlny v F oblasti ionosféry s dopadem na variabilitu a předpovídání šíření radiových vln
    Author(s) Altadill, D. (ES)
    Apostolov, E. M. (BG)
    Boška, Josef (GFU-E)
    Laštovička, Jan (GFU-E)
    Šauli, Petra (UFA-U) RID, ORCID
    Source TitleAnnals of Geophysics - ISSN 1593-5213
    Roč. 47, 2/3 (2004), s. 1109-1119
    Number of pages11 s.
    ActionFinal Meeting COST271 Action. Effects of the upper atmosphere on terrestrial and Earth-space communications (EACOS).
    Event date26.08.2004-27.08.2004
    VEvent locationAbingdon
    CountryGB - United Kingdom
    Event typeWRD
    Languageeng - English
    CountryIT - Italy
    Keywordsionosphere ; planetary waves ; gravity waves
    Subject RIVDG - Athmosphere Sciences, Meteorology
    R&D ProjectsOC 271.10 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    GA205/01/1071 GA ČR - Czech Science Foundation (CSF)
    GP205/02/P077 GA ČR - Czech Science Foundation (CSF)
    CEZAV0Z3042911 - UFA-U, BC-A
    AnnotationThe aim of the work within the WP3.1 of the COST 271 Action is the characterization of the variability introduced in the F region ionosphere by "Planetary Wave Signatures" (PWS) and "Gravity Wave Signatures" (GWS). Typical patterns of percentage of time occurence and time duration of PWS, their climatology and main drivers, as well as their vertical and longitudinal structure have been obtained. Despite of above characterization, the spectral distribution of event duration is too broad to allow for a reasonable prediction of PWS from ionospheric measurements themselves. GWS with a regular morning/evening wave bursts and specific GWS event whose arising can be predicted have been evaluated. As above, their typical pattern of occurance and time duration, and their vertical structure have been obtained. The latter events remain in the ionospheric variability during disturbed days while additional wave enhancements of auroral origin occur. However, both types of disturbances can be distinguished
    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 Publishing2005
Number of the records: 1  

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