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rdf:type
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Description
| - One of the strongest solar proton events (SPE) occured in October 1989. The ionized layer in the atmosphere is a result of interaction between radiation (electromegnetic and particle) and the neutral atmosphere. Changes of the neutral and ionized composition due to this event are examined. The ionization rate, and ozone, NO and OH density temporal and spatial (vertical) devations induced by the SPE, calculated by a 1-D time dependent photochemical model separately for daytime and nighttime are used in a 1-D model of the lower ionosphere to calculate the response of ionized components and other parameters of the lower ionosphere. The results of model calculations are compared with the empirical model of high-latitude electron densities, with rocket measurements of O3 and n+ from Russian research vessel, with parameter f+ obtained for November 1969 SPE and with experimental aeff data for disturbed conditions.
- One of the strongest solar proton events (SPE) occured in October 1989. The ionized layer in the atmosphere is a result of interaction between radiation (electromegnetic and particle) and the neutral atmosphere. Changes of the neutral and ionized composition due to this event are examined. The ionization rate, and ozone, NO and OH density temporal and spatial (vertical) devations induced by the SPE, calculated by a 1-D time dependent photochemical model separately for daytime and nighttime are used in a 1-D model of the lower ionosphere to calculate the response of ionized components and other parameters of the lower ionosphere. The results of model calculations are compared with the empirical model of high-latitude electron densities, with rocket measurements of O3 and n+ from Russian research vessel, with parameter f+ obtained for November 1969 SPE and with experimental aeff data for disturbed conditions. (en)
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Title
| - Changes of the neutral and ionized composition in the D-region after solar proton event in october 1989 (model simulations).
- Changes of the neutral and ionized composition in the D-region after solar proton event in october 1989 (model simulations). (en)
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skos:prefLabel
| - Changes of the neutral and ionized composition in the D-region after solar proton event in october 1989 (model simulations).
- Changes of the neutral and ionized composition in the D-region after solar proton event in october 1989 (model simulations). (en)
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skos:notation
| - RIV/68378289:_____/03:04033539!RIV/2004/AV0/A04004/N
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http://linked.open.../vavai/riv/strany
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http://linked.open...avai/riv/aktivita
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http://linked.open...avai/riv/aktivity
| - P(IAA3042804), Z(AV0Z3042911)
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http://linked.open...iv/cisloPeriodika
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http://linked.open...vai/riv/dodaniDat
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http://linked.open...aciTvurceVysledku
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http://linked.open.../riv/druhVysledku
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http://linked.open...iv/duvernostUdaju
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http://linked.open...titaPredkladatele
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http://linked.open...dnocenehoVysledku
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http://linked.open...ai/riv/idVysledku
| - RIV/68378289:_____/03:04033539
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http://linked.open...riv/jazykVysledku
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http://linked.open.../riv/klicovaSlova
| - solar proton event; middle atmosphere (en)
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http://linked.open.../riv/klicoveSlovo
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http://linked.open...odStatuVydavatele
| - GB - Spojené království Velké Británie a Severního Irska
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http://linked.open...ontrolniKodProRIV
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http://linked.open...i/riv/nazevZdroje
| - Advances in space research
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http://linked.open...in/vavai/riv/obor
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http://linked.open...ichTvurcuVysledku
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http://linked.open...cetTvurcuVysledku
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http://linked.open...ocetUcastnikuAkce
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http://linked.open...nichUcastnikuAkce
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http://linked.open...vavai/riv/projekt
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http://linked.open...UplatneniVysledku
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http://linked.open...v/svazekPeriodika
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http://linked.open...iv/tvurceVysledku
| - Laštovička, Jan
- Ondrášková, A.
- Krivolutsky, A.
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http://linked.open...n/vavai/riv/zamer
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issn
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number of pages
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