Number of the records: 1  

Searching for anomalous longitudinal profiles with the FRAM telescope

  1. 1.
    SYSNO ASEP0518134
    Document TypeC - Proceedings Paper (int. conf.)
    R&D Document TypeConference Paper
    TitleSearching for anomalous longitudinal profiles with the FRAM telescope
    Author(s) Blažek, Jiří (FZU-D) ORCID, RID
    Article number01009
    Source TitleEPJ Web of Conferences, 144. - Les Ulis : EDP Sciences, 2017 / Trávníček P. ; Prouza M. ; Gaug M. ; Keilhauer B. - ISSN 2100-014X
    Pagess. 1-4
    Number of pages4 s.
    Publication formOnline - E
    ActionInternational Workshop on ATmospheric MOnitoring for High Energy Astroparticle Detectors (AtmoHEAD)
    Event date12.09.2016 - 14.09.2016
    VEvent locationOlomouc
    CountryCZ - Czech Republic
    Event typeWRD
    Languageeng - English
    CountryFR - France
    KeywordsFRAM ; anomalous showers ; hadronic interactions ; atmospheric monitoring
    Subject RIVBF - Elementary Particles and High Energy Physics
    OECD categoryParticles and field physics
    R&D ProjectsLM2015038 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    LG15014 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    GA14-17501S GA ČR - Czech Science Foundation (CSF)
    Institutional supportFZU-D - RVO:68378271
    UT WOS000407742000009
    EID SCOPUS85021657544
    DOI10.1051/epjconf/201714401009
    AnnotationThe study of anomalous longitudinal profiles of extensive air showers presents an interesting opportunity to gain additional insight about the character of hadronic interactions at the highest energies. Moreover, the presence of such profiles would represent direct evidence of a light component in the primary cosmic rays of a given energy, independently of hadronic interaction models. The ratio of profiles observed to have a “double bump” structure (with two clearly distinguishable atmospheric depths of maximum particle count) compared to the total number of events can moreover be used to test the predictions of interaction models. However, the majority of such profiles observed at the Pierre Auger Observatory are caused by clouds. Here we describe a method of rapid monitoring of particularly interesting cosmic ray events, using the F/Photometric Rapid At-mospheric Monitor (FRAM) telescope to identify events with clear, cloudless atmospheric background. Thefunction of FRAM is described in detail and the number of triggered events is presented.
    WorkplaceInstitute of Physics
    ContactKristina Potocká, potocka@fzu.cz, Tel.: 220 318 579
    Year of Publishing2020
Number of the records: 1  

  This site uses cookies to make them easier to browse. Learn more about how we use cookies.