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Autor(en): 
  • Guy C. Burdiak
  • Cylindrical Liner Z-pinches as Drivers for Converging Strong Shock Experiments 
     

    (Buch)
    Dieser Artikel gilt, aufgrund seiner Grösse, beim Versand als 3 Artikel!


    Übersicht

    Auf mobile öffnen
     
    Lieferstatus:   Auf Bestellung (Lieferzeit unbekannt)
    Veröffentlichung:  Juni 2014  
    Genre:  Naturwissensch., Medizin, Technik 
     
    Astrophysics / Astrophysics and Astroparticles / B / Electrical Power Engineering / energy systems / Energy technology & engineering / Energy technology and engineering / Mechanical Power Engineering / Nuclear Fusion / Nuclear physics / Physics and Astronomy / Plasma (Ionized gases) / Plasma Physics
    ISBN:  9783319069616 
    EAN-Code: 
    9783319069616 
    Verlag:  Springer Nature EN 
    Einband:  Gebunden  
    Sprache:  English  
    Serie:  Springer Theses  
    Dimensionen:  H 235 mm / B 155 mm / D  
    Gewicht:  3731 gr 
    Seiten:  144 
    Illustration:  XV, 144 p. 106 illus., 38 illus. in color., schwarz-weiss Illustrationen, farbige Illustrationen 
    Bewertung: Titel bewerten / Meinung schreiben
    Inhalt:
    The thesis represents the development of an entirely new experimental platform for generating and studying converging radiative shock waves. It was discovered that the application of large magnetic pressures to gas-filled cylindrical metallic tubes could sequentially produce three shocks within the gas. A comprehensive set of instrumentation was devised to explore this system in detail and an exceptionally thorough experimental and theoretical study was carried out in order to understand the source of the shock waves and their dynamics. The research is directed towards some of the most interesting topics in high energy density physics (HEDP) today, namely the interaction of HED material with radiation and magnetic fields, with broad applications to inertial confinement fusion (ICF) and laboratory plasma astrophysics. The work has already generated significant international interest in these two distinct research areas and the results could have significant importance for magnetic ICF concepts being explored at Sandia National Laboratories in the US and for our understanding of the very strong shock waves that are ubiquitous in astrophysics.
      
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