This HTML5 document contains 46 embedded RDF statements represented using HTML+Microdata notation.

The embedded RDF content will be recognized by any processor of HTML5 Microdata.

Namespace Prefixes

PrefixIRI
dctermshttp://purl.org/dc/terms/
n15http://localhost/temp/predkladatel/
n7http://linked.opendata.cz/resource/domain/vavai/projekt/
n5http://linked.opendata.cz/resource/domain/vavai/riv/tvurce/
n6http://linked.opendata.cz/ontology/domain/vavai/
n17http://linked.opendata.cz/resource/domain/vavai/zamer/
shttp://schema.org/
skoshttp://www.w3.org/2004/02/skos/core#
n3http://linked.opendata.cz/ontology/domain/vavai/riv/
n2http://linked.opendata.cz/resource/domain/vavai/vysledek/
rdfhttp://www.w3.org/1999/02/22-rdf-syntax-ns#
n14http://linked.opendata.cz/resource/domain/vavai/vysledek/RIV%2F68407700%3A21220%2F08%3A00149857%21RIV10-GA0-21220___/
n16http://linked.opendata.cz/ontology/domain/vavai/riv/klicoveSlovo/
n13http://linked.opendata.cz/ontology/domain/vavai/riv/duvernostUdaju/
xsdhhttp://www.w3.org/2001/XMLSchema#
n8http://linked.opendata.cz/ontology/domain/vavai/riv/aktivita/
n4http://linked.opendata.cz/ontology/domain/vavai/riv/jazykVysledku/
n12http://linked.opendata.cz/ontology/domain/vavai/riv/druhVysledku/
n9http://linked.opendata.cz/ontology/domain/vavai/riv/obor/
n19http://reference.data.gov.uk/id/gregorian-year/

Statements

Subject Item
n2:RIV%2F68407700%3A21220%2F08%3A00149857%21RIV10-GA0-21220___
rdf:type
n6:Vysledek skos:Concept
dcterms:description
In the fluorescence detection of ultra high energy cosmic rays, the number of emitted fluorescence photons is assumed to be proportional to the energy deposited in air by shower particles. We have performed measurements of the fluorescence yield in atmospheric gases excited by electrons over energies ranging from keV to hundreds of MeV in several accelerators. We found that within the measured energy ranges the proportionality holds at the level of few %. In the fluorescence detection of ultra high energy cosmic rays, the number of emitted fluorescence photons is assumed to be proportional to the energy deposited in air by shower particles. We have performed measurements of the fluorescence yield in atmospheric gases excited by electrons over energies ranging from keV to hundreds of MeV in several accelerators. We found that within the measured energy ranges the proportionality holds at the level of few %.
dcterms:title
Energy dependence of air fluorescence yield measured by AIRFLY Energy dependence of air fluorescence yield measured by AIRFLY
skos:prefLabel
Energy dependence of air fluorescence yield measured by AIRFLY Energy dependence of air fluorescence yield measured by AIRFLY
skos:notation
RIV/68407700:21220/08:00149857!RIV10-GA0-21220___
n3:aktivita
n8:P n8:Z
n3:aktivity
P(1M06002), P(GA202/05/2470), P(LA08016), P(LC527), Z(AV0Z10100502), Z(AV0Z10100522)
n3:cisloPeriodika
1
n3:dodaniDat
n19:2010
n3:domaciTvurceVysledku
n5:7574355 n5:6112137
n3:druhVysledku
n12:J
n3:duvernostUdaju
n13:S
n3:entitaPredkladatele
n14:predkladatel
n3:idSjednocenehoVysledku
366208
n3:idVysledku
RIV/68407700:21220/08:00149857
n3:jazykVysledku
n4:eng
n3:klicovaSlova
Energy deposit; air fluorescence detection; ultra high energy cosmic rays
n3:klicoveSlovo
n16:air%20fluorescence%20detection n16:ultra%20high%20energy%20cosmic%20rays n16:Energy%20deposit
n3:kodStatuVydavatele
NL - Nizozemsko
n3:kontrolniKodProRIV
[6FA1BFA9FC74]
n3:nazevZdroje
Nuclear Instruments and Methods in Physics Research, Section A, Accelerators, Spectrometers, Detectors and Associated Equipment
n3:obor
n9:BF
n3:pocetDomacichTvurcuVysledku
2
n3:pocetTvurcuVysledku
45
n3:projekt
n7:LA08016 n7:GA202%2F05%2F2470 n7:LC527 n7:1M06002
n3:rokUplatneniVysledku
n19:2008
n3:svazekPeriodika
597
n3:tvurceVysledku
Vacek, Václav Doubrava, Michal
n3:wos
000261700600006
n3:zamer
n17:AV0Z10100522 n17:AV0Z10100502
s:issn
0168-9002
s:numberOfPages
4
n15:organizacniJednotka
21220