Line radiation effects in laboratory and astrophysical plasmas
Journal of Quantitative Spectroscopy and Radiative Transfer Elsevier 99:1-3 (2006) 363-369
Radiation transfer effects on the spectra of laser-generated plasmas.
Physical review letters 96:18 (2006) 185002
Abstract:
Experimental x-ray spectra of the H-like 2p --> 1s (Lyman-alpha) doublet have been obtained using time-integrated high-resolution spectroscopy of a constrained-flow, laser-generated aluminum plasma. These spectra show monotonic alteration of the relative intensities of the doublet components with distance from the target surface. Excellent agreement between experiment and theory is found only if the modeling includes both ion collisional rates between the fine-structure components of the level and, more importantly, the radiative pumping of one Lyman-alpha component by the other component along the direction of the major velocity gradient (i.e., perpendicular to the direction of spectra observation). Understanding radiation transfer in plasmas with high velocity gradients is important in modeling many astrophysical objects, and this experiment acts as a benchmark for such complex calculations.Study of X-ray photoionized Fe plasma and comparisons with astrophysical modeling codes
Journal of Quantitative Spectroscopy and Radiative Transfer Elsevier 99:1-3 (2006) 712-729
Production of dense plasmas with sub-10-fs laser pulses.
Physical review letters 96:8 (2006) 085002
Abstract:
Close to solid state density plasmas with peak electron temperatures of about 190 eV have been generated with sub-10-fs laser pulses incident on solid targets. Extreme ultraviolet (XUV) spectroscopy is used to investigate the K shell emission from the plasma. In the spectra, a series limit for the H- and He-like resonance lines becomes evident which is explained by pressure ionization in the dense plasma. The spectra are consistent with computer simulations calculating the XUV emission and the expansion of the plasma.New experimental possibilities for measuring radiative opacity under conditions in the Sun's interior
Plasma Physics and Controlled Fusion IOP Publishing 47:12B (2005) b735