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Statements

Subject Item
n2:RIV%2F00216208%3A11320%2F12%3A10130874%21RIV13-MSM-11320___
rdf:type
skos:Concept n17:Vysledek
rdfs:seeAlso
http://dx.doi.org/10.1016/j.asr.2012.06.010
dcterms:description
We use the CORSIKA package (Heck et al., 1998) and AMS-01 flight data (Alcaraz et al., 2000) to evaluate the distribution of secondary particles in the Earth atmosphere. Distribution covers all longitudes and latitudes of STS-91 Space Shuttle flight trajectory to Mir Space Station. Moreover distribution covers all depth in the atmosphere in the evaluated area. We show distributions for e-, e+, mu+, mu-, gammas, hadrons and Cherenkov light from primary protons and helium component of cosmic rays flux. Our results compare favorably with other estimates made by different techniques. We also estimate an UV light production (300-400 nm) by electron component of secondaries at the top of the atmosphere and at ISS orbit. We use the CORSIKA package (Heck et al., 1998) and AMS-01 flight data (Alcaraz et al., 2000) to evaluate the distribution of secondary particles in the Earth atmosphere. Distribution covers all longitudes and latitudes of STS-91 Space Shuttle flight trajectory to Mir Space Station. Moreover distribution covers all depth in the atmosphere in the evaluated area. We show distributions for e-, e+, mu+, mu-, gammas, hadrons and Cherenkov light from primary protons and helium component of cosmic rays flux. Our results compare favorably with other estimates made by different techniques. We also estimate an UV light production (300-400 nm) by electron component of secondaries at the top of the atmosphere and at ISS orbit.
dcterms:title
Distribution of secondary particles intensities over Earth's surface: Effect of the geomagnetic field Distribution of secondary particles intensities over Earth's surface: Effect of the geomagnetic field
skos:prefLabel
Distribution of secondary particles intensities over Earth's surface: Effect of the geomagnetic field Distribution of secondary particles intensities over Earth's surface: Effect of the geomagnetic field
skos:notation
RIV/00216208:11320/12:10130874!RIV13-MSM-11320___
n17:predkladatel
n18:orjk%3A11320
n3:aktivita
n7:S n7:P n7:Z
n3:aktivity
P(ME09056), S, Z(MSM0021620860)
n3:cisloPeriodika
7
n3:dodaniDat
n10:2013
n3:domaciTvurceVysledku
n9:9732675
n3:druhVysledku
n4:J
n3:duvernostUdaju
n15:S
n3:entitaPredkladatele
n13:predkladatel
n3:idSjednocenehoVysledku
131615
n3:idVysledku
RIV/00216208:11320/12:10130874
n3:jazykVysledku
n21:eng
n3:klicovaSlova
AMS; CORSIKA; Extensive air showers; Magnetosphere; Cosmic rays
n3:klicoveSlovo
n5:CORSIKA n5:Cosmic%20rays n5:Extensive%20air%20showers n5:AMS n5:Magnetosphere
n3:kodStatuVydavatele
GB - Spojené království Velké Británie a Severního Irska
n3:kontrolniKodProRIV
[A7F6B5DCD569]
n3:nazevZdroje
Advances in Space Research
n3:obor
n19:BL
n3:pocetDomacichTvurcuVysledku
1
n3:pocetTvurcuVysledku
9
n3:projekt
n11:ME09056
n3:rokUplatneniVysledku
n10:2012
n3:svazekPeriodika
50
n3:tvurceVysledku
Santangelo, A. Szabelski, J. Fenu, F. Shinozaki, K. Pastircak, B. Urbář, Jaroslav Bobik, P. Bertaina, M. Kudela, K.
n3:wos
000307919400012
n3:zamer
n20:MSM0021620860
s:issn
0273-1177
s:numberOfPages
11
n8:doi
10.1016/j.asr.2012.06.010
n12:organizacniJednotka
11320