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The Penetrating particle ANalyzer (PAN) instrument for measurements of low energy cosmic rays

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21670%2F19%3A00342136" target="_blank" >RIV/68407700:21670/19:00342136 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1109/NSS/MIC42101.2019.9059946" target="_blank" >https://doi.org/10.1109/NSS/MIC42101.2019.9059946</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1109/NSS/MIC42101.2019.9059946" target="_blank" >10.1109/NSS/MIC42101.2019.9059946</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    The Penetrating particle ANalyzer (PAN) instrument for measurements of low energy cosmic rays

  • Original language description

    PAN is an instrument designed to precisely measure and monitor the flux, composition, and direction of highly penetrating particles (>100MeV/nucleon) in deep space and interplanetary missions with an energy resolution better than 10% for nuclei from H to Fe at 1GeV/n. The detector, limited to about 20kg in mass and 20W in power consumption, is based on the well-known magnetic spectrometer detection principle, and exploits the advantages provided by the integration of ultra-thin microstrip silicon detectors, hybrid silicon pixel detectors and silicon photomultipliers. This novel layout and detection concept facilitates the flexibility of the PAN instrument for a variegate spectrum of space missions and applications, and opens the possibility to deploy PAN instruments over a distributed array monitoring the radiation environment in different positions of the heliosphere. PAN will measure the properties of cosmic rays in the 100MeV/n - 20GeV/n energy range in deep space with unprecedented accuracy, providing novel results to investigate the mechanisms of origin, acceleration and propagation of galactic cosmic rays and of solar energetic particles, and producing unique information for solar system exploration missions.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2019

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    2019 IEEE Nuclear Science Symposium and Medical Imaging Conference (NSS/MIC)

  • ISBN

    978-1-7281-4164-0

  • ISSN

  • e-ISSN

    1095-7863

  • Number of pages

    8

  • Pages from-to

  • Publisher name

    IEEE Industrial Electronic Society

  • Place of publication

    Vienna

  • Event location

    Manchester Convention Centre, Manchester

  • Event date

    Oct 26, 2019

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article

    000569982800338