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Statements

Subject Item
n2:RIV%2F68378289%3A_____%2F03%3A04033543%21RIV%2F2004%2FAV0%2FA04004%2FN
rdf:type
n4:Vysledek skos:Concept
dcterms: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 and relatively 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 weak if any effec 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 and relatively 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 weak if any effec
dcterms:title
Cosmic rays and total ozone at higher middle latitudes. Cosmic rays and total ozone at higher middle latitudes.
skos:prefLabel
Cosmic rays and total ozone at higher middle latitudes. Cosmic rays and total ozone at higher middle latitudes.
skos:notation
RIV/68378289:_____/03:04033543!RIV/2004/AV0/A04004/N
n3:strany
2139;2144
n3:aktivita
n5:P
n3:aktivity
P(KSK3012103)
n3:cisloPeriodika
9
n3:dodaniDat
n9:2004
n3:domaciTvurceVysledku
n14:7020139 n14:9492933
n3:druhVysledku
n17:J
n3:duvernostUdaju
n15:S
n3:entitaPredkladatele
n16:predkladatel
n3:idSjednocenehoVysledku
602321
n3:idVysledku
RIV/68378289:_____/03:04033543
n3:jazykVysledku
n10:eng
n3:klicovaSlova
cosmic rays; ozone
n3:klicoveSlovo
n11:cosmic%20rays n11:ozone
n3:kodStatuVydavatele
GB - Spojené království Velké Británie a Severního Irska
n3:kontrolniKodProRIV
[A63664FD4B85]
n3:nazevZdroje
Advances in space research
n3:obor
n13:DG
n3:pocetDomacichTvurcuVysledku
2
n3:pocetTvurcuVysledku
3
n3:pocetUcastnikuAkce
0
n3:pocetZahranicnichUcastnikuAkce
0
n3:projekt
n12:KSK3012103
n3:rokUplatneniVysledku
n9:2003
n3:svazekPeriodika
31
n3:tvurceVysledku
Kudela, K. Laštovička, Jan Križan, Peter
s:issn
0273-1177
s:numberOfPages
6