Number of the records: 1  

Capillary pinching discharge as water window radiation source

  1. 1.
    SYSNO ASEP0328421
    Document TypeC - Proceedings Paper (int. conf.)
    R&D Document TypeConference Paper
    TitleCapillary pinching discharge as water window radiation source
    TitleKapilární pinčující výboj jakožto zdroj záření ve vodním okně
    Author(s) Vrba, Pavel (UFP-V) RID
    Vrbová, M. (CZ)
    Jančárek, A. (CZ)
    Nevrkla, M. (CZ)
    Tamáš, M. (CZ)
    Stefanovic, M. (CZ)
    Source TitleProceeding of the 29th International Conference on Phenomena in Ionized Gases, 15. Plasma lamps and radiation sources. - Cancún : Institute of Physics(IOP), 2009 / Juárez Reyes A.M. - ISBN N
    Pagespb15-5-pb15-5
    Number of pages6 s.
    Publication formweb - web
    ActionThe 29th International Conference on Phenomena in Ionized Gases 2009
    Event date12.07.2009-17.07.2009
    VEvent locationCancún
    CountryMX - Mexico
    Event typeWRD
    Languageeng - English
    CountryMX - Mexico
    KeywordsCapillary Z-pinch ; water window radiation source ; RHMD Z* engine
    Subject RIVBH - Optics, Masers, Lasers
    R&D ProjectsGA102/07/0275 GA ČR - Czech Science Foundation (CSF)
    CEZAV0Z20430508 - UFP-V (2005-2011)
    AnnotationFast capillary discharge in nitrogen is investigated as a source of incoherent radiation with wavelengths 2 - 4 nm. There are expected relatively strong spectral lines of helium- and hydrogenlike- nitrogen ions in this region, if the nitrogen plasma is heated up to 40-80 eV. Plasma heating by the capillary Z-pinch is presumed. Spatial and time evolutions of pinching plasma quantities are modeled by means of RHMD Z* engine code for our current experimental set up. Under selected experimental conditions the power of radiation estimated in the spectral range 2.1 – 3.1 nm is remarkably higher than that in the spectral range 13 - 14.3 nm. Detail kinetics of nitrogen ions in the plasma was further evaluated by FLY code used as a post -processor. Instantaneous spectra were evaluated and the spectral line with the wavelength 2.88 nm prevails under optimized experimental conditions.
    WorkplaceInstitute of Plasma Physics
    ContactVladimíra Kebza, kebza@ipp.cas.cz, Tel.: 266 052 975
    Year of Publishing2010
Number of the records: 1  

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