Methods of Generation and Detailed Characterization of Millimeter-Scale Plasmas Using a Gasbag Target
Gasbag targets are useful for the research of laser-plasma interactions in inertial confinement fusion, especially in the laser overlapping regime. We report that on the Shenggnang-II laser facility, millimeter-scale plasmas are successfully generated by four 0.35 mu m laser beams using a gasbag tar...
        Saved in:
      
    
          | Published in | Chinese physics letters Vol. 28; no. 12; pp. 125202 - 1-125202-4 | 
|---|---|
| Main Authors | , , , , , , , , , , , , , , | 
| Format | Journal Article | 
| Language | English | 
| Published | 
            IOP Publishing
    
        01.12.2011
     | 
| Subjects | |
| Online Access | Get full text | 
| ISSN | 0256-307X 1741-3540  | 
| DOI | 10.1088/0256-307X/28/12/125202 | 
Cover
| Summary: | Gasbag targets are useful for the research of laser-plasma interactions in inertial confinement fusion, especially in the laser overlapping regime. We report that on the Shenggnang-II laser facility, millimeter-scale plasmas are successfully generated by four 0.35 mu m laser beams using a gasbag target. Multiple diagnostics are applied to characterize the millimeter-scale plasmas in detail. The images from the x-ray pinhole cameras confirm that millimeter-scale plasmas are indeed created. An optical Thomson scattering system diagnoses the electron temperature of the CH filling plasmas by probing the thermal ion-acoustic fluctuations, which indicates that the electron temperature has a 600 eV flat roof in 0.7-1.3 ns. Another key parameter, i.e. the electron density of the millimeter-scale plasmas, is inferred by the spectrum of the back stimulated Raman scattering of an additional 0.53 mu m laser beam. The inferred electron density keeps stable at 0.1n sub(c)in early time consistent with the controlled filling pressure and splits into a higher density in late time, which is attributed to the blast wave entering into the SRS interaction region | 
|---|---|
| Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23  | 
| ISSN: | 0256-307X 1741-3540  | 
| DOI: | 10.1088/0256-307X/28/12/125202 |