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Feasibility study and CXRS synthetic diagnostic model for COMPASS upgrade based on Cherab and Raysect framework

  1. 1.
    SYSNO ASEP0544101
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleFeasibility study and CXRS synthetic diagnostic model for COMPASS upgrade based on Cherab and Raysect framework
    Author(s) Tomeš, Matěj (UFP-V)
    Carr, M. (GB)
    Meakins, A. (GB)
    Imríšek, Martin (UFP-V) RID
    Jaulmes, Fabien (UFP-V) ORCID
    Balner, Vojtěch (UFP-V)
    Bogár, Klára (UFP-V) ORCID
    Bílková, Petra (UFP-V) RID
    Weinzettl, Vladimír (UFP-V) RID, ORCID
    Hron, Martin (UFP-V) RID, ORCID
    Pánek, Radomír (UFP-V) RID
    Number of authors11
    Article number112498
    Source TitleFusion Engineering and Design. - : Elsevier - ISSN 0920-3796
    Roč. 170, September (2021)
    Number of pages8 s.
    Languageeng - English
    CountryCH - Switzerland
    KeywordsCharge exchange recombination spectroscopy ; Cherab ; cxrs ; Forward model ; Raysect ; Synthetic diagnostic
    Subject RIVBL - Plasma and Gas Discharge Physics
    OECD categoryFluids and plasma physics (including surface physics)
    Method of publishingLimited access
    Institutional supportUFP-V - RVO:61389021
    UT WOS000687337400004
    EID SCOPUS85103693727
    DOI10.1016/j.fusengdes.2021.112498
    AnnotationIn this article the forward model and feasibility study of the CXRS (Charge Exchange Recombination Spectroscopy) diagnostic for the COMPASS Upgrade tokamak [1] based on the Raysect and Cherab framework [2–4] is presented. The neutral beam model available in Cherab is expanded and based on individual acceleration grid beamlets. The spatial density distribution calculation takes into account 3D geometry of the port structure. Beam density profile calculated with the expanded model is used to estimate realistic radial resolution of measurement and to produce forward models of the spectra. Effects of background plasma and beam halo are not included. The spectra are used to reconstruct the plasma profiles and are compared with the simulation input to estimate measurement errors with respect to positions of collecting optics.
    WorkplaceInstitute of Plasma Physics
    ContactVladimíra Kebza, kebza@ipp.cas.cz, Tel.: 266 052 975
    Year of Publishing2022
    Electronic addresshttps://www.sciencedirect.com/science/article/pii/S092037962100274X?via%3Dihub
Number of the records: 1  

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