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Statements

Subject Item
n2:RIV%2F68378289%3A_____%2F02%3A04033540%21RIV%2F2004%2FAV0%2FA04004%2FN
rdf:type
n18:Vysledek skos:Concept
dcterms:description
Simulations of the response of the neutral and ionized composition in the D-region to the October 1989 solar proton event (SPE) are used to find the day to night differences in this response. There is a natural difference between day and night conditions - the incoming solar electromagnetic radiation. This is responsible for the day to night difference in both undisturbed and (likely) also in disturbed condition. At the same time changes of the neutral minor compounds from day to night during SPE affect the ionized component chemistry. Two photochemical models (for neutral and ionized species) connected via ionisation rates caused by Solar protons, and via neutral component variability are used for study. Simulations of the response of the neutral and ionized composition in the D-region to the October 1989 solar proton event (SPE) are used to find the day to night differences in this response. There is a natural difference between day and night conditions - the incoming solar electromagnetic radiation. This is responsible for the day to night difference in both undisturbed and (likely) also in disturbed condition. At the same time changes of the neutral minor compounds from day to night during SPE affect the ionized component chemistry. Two photochemical models (for neutral and ionized species) connected via ionisation rates caused by Solar protons, and via neutral component variability are used for study.
dcterms:title
Day to night differences in neutral component and electron density response during Solar proton event (model calcula tions. Day to night differences in neutral component and electron density response during Solar proton event (model calcula tions.
skos:prefLabel
Day to night differences in neutral component and electron density response during Solar proton event (model calcula tions. Day to night differences in neutral component and electron density response during Solar proton event (model calcula tions.
skos:notation
RIV/68378289:_____/02:04033540!RIV/2004/AV0/A04004/N
n5:strany
39;48
n5:aktivita
n7:Z n7:P
n5:aktivity
P(IAA3042804), Z(AV0Z3042911)
n5:cisloPeriodika
N/A
n5:dodaniDat
n8:2004
n5:domaciTvurceVysledku
n15:7020139
n5:druhVysledku
n12:J
n5:duvernostUdaju
n9:S
n5:entitaPredkladatele
n13:predkladatel
n5:idSjednocenehoVysledku
642254
n5:idVysledku
RIV/68378289:_____/02:04033540
n5:jazykVysledku
n17:eng
n5:klicovaSlova
ionosphere; Solar proton event; neutral and ion chemistry and composition
n5:klicoveSlovo
n6:ionosphere n6:neutral%20and%20ion%20chemistry%20and%20composition n6:Solar%20proton%20event
n5:kodStatuVydavatele
SK - Slovenská republika
n5:kontrolniKodProRIV
[0D5A545FFF41]
n5:nazevZdroje
Acta astronomica et geophysica Universitatis Comenianae
n5:obor
n14:DG
n5:pocetDomacichTvurcuVysledku
1
n5:pocetTvurcuVysledku
4
n5:pocetUcastnikuAkce
0
n5:pocetZahranicnichUcastnikuAkce
0
n5:projekt
n11:IAA3042804
n5:rokUplatneniVysledku
n8:2002
n5:svazekPeriodika
24
n5:tvurceVysledku
Kuminov, A. Krivolutsky, A. Laštovička, Jan Ondrášková, A.
n5:zamer
n10:AV0Z3042911
s:issn
0004-6248
s:numberOfPages
10