All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

Dynamical position and orientation calibration of the KM3NeT telescope

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21670%2F24%3A00389342" target="_blank" >RIV/68407700:21670/24:00389342 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.22323/1.444.1033" target="_blank" >https://doi.org/10.22323/1.444.1033</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.22323/1.444.1033" target="_blank" >10.22323/1.444.1033</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Dynamical position and orientation calibration of the KM3NeT telescope

  • Original language description

    KM3NeT is an underwater neutrino telescope which detects the Cherenkov radiation created by the products of neutrino interactions. To accurately reconstruct neutrino events, a precise determination of the position and orientation of the optical modules, which detect the Cherenkov radiation, is required. As the detector elements sway with the deep sea currents, a continuous tracking of the positions and orientations is necessary. A network of acoustic emitters and receivers is used to position the optical modules. Their orientation is determined by compasses placed in each optical module. This contribution presents the methods to perform the position and orientation calibration of the KM3NeT telescope. The positions of the optical modules need to be resolved with an accuracy of better than 20 cm in order to achieve the envisaged angular resolution of the KM3NeT/ARCA telescope of 0.05 degrees. The orientations of the optical modules need to be resolved with an accuracy of about 3 degrees in order to not compromise the quality of the event reconstruction.

  • 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)

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 (ICRC2023)

  • ISBN

  • ISSN

    1824-8039

  • e-ISSN

    1824-8039

  • Number of pages

    10

  • Pages from-to

    1-10

  • Publisher name

    PoS - Proceedings of Science, Sissa Medialab srl

  • 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