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The risky characteristics of the exposition by ionospheric and geomagnetic parameters

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    SYSNO ASEP0458082
    Document TypeE - Electronic Document
    R&D Document TypeThe record was not marked in the RIV
    TitleThe risky characteristics of the exposition by ionospheric and geomagnetic parameters
    Author(s) Podolská, Kateřina (UFA-U) RID, ORCID
    Number of authors1
    Issue dataPraha: Department od Demography and Geodemography, Charles University in Prague, Faculty of Science, 2016
    Publication formOnline - E
    Languageeng - English
    CountryCZ - Czech Republic
    Keywordsmortality ; causes of death ; civilization and degenerative diseases ; solar cycle ; geomagnetic activity
    Subject RIVDN - Health Impact of the Environment Quality
    Institutional supportUFA-U - RVO:68378289
    AnnotationThe influence of extraterrestrial phenomena is expected to have an impact on human health, and therefore on mortality in particular
    civilization and degenerative diseases. The main aim of this contribution is to assemble descriptive characteristics that represent the
    impact of the solar and geomagnetic activity on mortality by cause of death from groups VI. Diseases of the nervous system and IX.
    Diseases of the circulatory system. We study the daily number of deaths separately for both sexes at the age groups under 39 and
    40+. Differences are found for maximum solar activity and during the ascending and descending epoch of the solar cycles.
    We have constructed the characteristics that represent the risk of the solar activity on human health on the basis of the previous
    analysis of association between the daily numbers of death on diseases of the nervous system and diseases of the circulatory system
    and the solar and geomagnetic parameters in the Czech Republic during the years 1994 – 2013. These characteristics were
    constructed using the method of graphical models of conditional dependencies (CIG) in time series according to the phases of the
    solar cycle and the seasonal insolation at mid-latitudes.
    The computation was implemented in the SAS environment and the Mathematica 7.
    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 Publishing2017
    Electronic addresshttp://www.demografove.estranky.cz/en/articles/online_poster_session_2016/
Number of the records: 1  

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