Cosmic rays and total ozone at higher middle latitudes.

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F03%3A04033543" target="_blank" >RIV/68378289:_____/03:04033543 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Cosmic rays and total ozone at higher middle latitudes.
Original language description
Various external factors of solar origin like solar activity (solar cycle, 27-day variation etc.), geomagnetic storms and other solar wind-related phenomena, and changes of fluxes of high-energy particles can potentially affect the ozone layer. Here we examine the effects of Forbush decreases and other decreases of the galactic cosmic ray (GCR) flux on the columnar ozone content (= total ozone) at higher middle latitudes near 50 N. The Forbush decreases usually occur together with geomagnetic storms andrelatively often together wiyh solar proton events (SPEs). Then it is difficult, if not impossible, to distinguish between the effects of geomagnetic storms, SPEs and Forbush decreases and other decreases of GCR flux. Therefore we present here the result of investigations of the effects Forbush decreases and other substantial decreases of the GCR flux on the total ozone for events when there was no geomagnetic storm. Due to dominance of summertime events in the selected data set, very w
Czech name
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Czech description
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Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
DG - Atmospheric sciences, meteorology
OECD FORD branch
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Project
<a href="/en/project/KSK3012103" target="_blank" >KSK3012103: Processes in the Earth and on its surface, in its gaseous and plasmatic cover and in outer space</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2003
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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