Parameters sensitive to the mass composition of cosmic rays and their application at the Pierre Auger Observatory
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F12%3A00388748" target="_blank" >RIV/68378271:_____/12:00388748 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Parameters sensitive to the mass composition of cosmic rays and their application at the Pierre Auger Observatory
Original language description
The Pierre Auger Observatory studies extensive cosmic ray showers of energy above 1018 eV. The mass composition of the shower?inducing primary particles plays an important role in the search for an anisotropy of their arrival directions and in considerations about the possible mechanisms of their acceleration. Several air shower parameters carrying information about the mass of primary cosmic ray are introduced and their applications to data of the Pierre Auger Observatory are discussed.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BF - Elementary particle theory and high energy physics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/LA08016" target="_blank" >LA08016: Participation in the project of the Pierre Auger Observatory</a><br>
Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
WDS´12 - Proceedings of Contributed Papers, Part III
ISBN
978-80-7378-226-9
ISSN
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e-ISSN
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Number of pages
5
Pages from-to
137-141
Publisher name
Matfyzpress
Place of publication
Praha
Event location
Praha
Event date
May 29, 2012
Type of event by nationality
EUR - Evropská akce
UT code for WoS article
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