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Seasonal variation of the atmospheric muon flux in the KM3NeT detectors

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21670%2F24%3A00381638" target="_blank" >RIV/68407700:21670/24:00381638 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.22323/1.444.0355" target="_blank" >https://doi.org/10.22323/1.444.0355</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.22323/1.444.0355" target="_blank" >10.22323/1.444.0355</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Seasonal variation of the atmospheric muon flux in the KM3NeT detectors

  • Original language description

    KM3NeT is constructing two large volume water Cherenkov detectors in the Mediterranean Sea. By instrumenting the water with photo-multipliers, neutrinos can be detected through the Cherenkov light from charged products of their interactions. The dominating signal, however, comes from muons created in extensive air-showers resulting from cosmic ray interactions in the top of the atmosphere. Despite the water column above, the highest-energy muons (> TeV) reach the detectors. Air-showers develop in a non-isotropic atmosphere where the vertical temperature profile, and thus the density, varies over time. The changing density of the atmosphere affects the balance between interaction and decay (to muons) of mesons in the air-showers. Therefore, the muon flux is expected to correlate with the seasons and short-term temperature fluctuations, as confirmed by other experiments. In this contribution, we present a first measurement of the correlation of the detected muon rate with the effective atmospheric temperature (weighted by muon production spectrum and detector response) for the KM3NeT ORCA telescope. The measured rate is compared with simulations, which model the time-dependent detector efficiency and environmental factors for a constant atmospheric muon flux.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/LM2023063" target="_blank" >LM2023063: Laboratoire Souterrain de Modane – participation of the Czech Republic</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2024

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Article name in the collection

    38th International Cosmic Ray Conference

  • ISBN

  • ISSN

    1824-8039

  • e-ISSN

    1824-8039

  • Number of pages

    10

  • Pages from-to

    1-10

  • Publisher name

    SISSA-The International School for Advanced Studies

  • Place of publication

    Trieste

  • Event location

    Nagoya

  • Event date

    Jul 26, 2023

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article