About: Day to night differences in neutral component and electron density response during Solar proton event (model calcula tions.     Goto   Sponge   NotDistinct   Permalink

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  • 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. (en)
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. (en)
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. (en)
skos:notation
  • RIV/68378289:_____/02:04033540!RIV/2004/AV0/A04004/N
http://linked.open.../vavai/riv/strany
  • 39;48
http://linked.open...avai/riv/aktivita
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  • P(IAA3042804), Z(AV0Z3042911)
http://linked.open...iv/cisloPeriodika
  • N/A
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  • 642254
http://linked.open...ai/riv/idVysledku
  • RIV/68378289:_____/02:04033540
http://linked.open...riv/jazykVysledku
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  • ionosphere; Solar proton event; neutral and ion chemistry and composition (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • SK - Slovenská republika
http://linked.open...ontrolniKodProRIV
  • [0D5A545FFF41]
http://linked.open...i/riv/nazevZdroje
  • Acta astronomica et geophysica Universitatis Comenianae
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http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
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http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 24
http://linked.open...iv/tvurceVysledku
  • Laštovička, Jan
  • Ondrášková, A.
  • Krivolutsky, A.
  • Kuminov, A.
http://linked.open...n/vavai/riv/zamer
issn
  • 0004-6248
number of pages
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