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Effect of Various EFIT NSTX Equilibria on EBW Simulations

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    SYSNO ASEP0043589
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JOstatní články
    TitleEffect of Various EFIT NSTX Equilibria on EBW Simulations
    TitleVliv různých rovnovách získaných z modifikovaných EFITů na NSTX na EBW simulace
    Author(s) Urban, Jakub (UFP-V) RID
    Preinhaelter, Josef (UFP-V) RID
    Sabbagh, S. (US)
    Pavlo, Pavol (UFP-V) RID
    Vahala, L. (US)
    Vahala, G. (US)
    Source TitleBulletin of the American Physical Society - ISSN 0003-0503
    Roč. 51, č. 7 (2006), QPI.00027
    Number of pages2 KB
    ActionAnnual Meeting of the Division of Plasma Physics/48th./
    Event date30.10.2006-3.11.2006
    VEvent locationPhiladelphia, Pennsylvania
    CountryUS - United States
    Event typeWRD
    Languageeng - English
    CountryUS - United States
    KeywordsConversion ; Emission ; Tokamaks ; Electron Bernstein waves ; Simulation ; MAST ; NSTX
    Subject RIVBL - Plasma and Gas Discharge Physics
    CEZAV0Z20430508 - UFP-V (2005-2011)
    AnnotationIn overdense NSTX plasmas the standard O and X mode radiation emitted from the first several electron cyclotron (EC) harmonics cannot be observed. An explanation for any such measured EC emission is the mode conversion of Electron Bernstein Waves (EBW) near the upper hybrid resonance region near the plasma edge. However EBW emission is strongly coupled to the equilibrium fields in NSTX as reconstructed from EFIT. We examine some models of EFIT ranging from the basic model that uses only the external magnetic measurements with simple models for plasma current and pressure, to those models that include effects of edge currents, MSE measurements and their effect on EBW simulations. The frequency dependence of EBWE provides optimization parameters for proposed EBW heating and current drive.
    WorkplaceInstitute of Plasma Physics
    ContactVladimíra Kebza, kebza@ipp.cas.cz, Tel.: 266 052 975
    Year of Publishing2007
Number of the records: 1  

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