Temporal and spectral behavior of sub-picosecond laser-created X-ray sources from low- to moderate-Z elements

被引:7
作者
Bastiani-Ceccotti, S. [1 ]
Renaudin, P. [2 ]
Dorchies, F. [3 ]
Harmand, M. [3 ]
Peyrusse, O. [3 ]
Audebert, P. [1 ]
Jacquemot, S. [1 ,2 ]
Calisti, A. [4 ]
Benredjem, D. [5 ]
机构
[1] UPMC, CNRS, Ecole Polytech, LULI,CEA, F-91128 Palaiseau, France
[2] DIF, DAM, CEA, F-91297 Arpajon, France
[3] Univ Bordeaux, CNRS, CEA, CELIA, F-33405 Talence, France
[4] Univ Aix Marseille 1, PIIM, F-13397 Marseille 20, France
[5] Univ Paris 11, LAC, F-91405 Orsay, France
关键词
Plasma spectroscopy; Non-LTE plasmas; High-Z plasmas; K-shell spectra; L-shell spectra; SHELL SPECTRA; DENSE-PLASMAS; LINE-SHAPE; SPECTROSCOPY; EMISSION; PULSES; HOT; MODEL; IONS; TIME;
D O I
10.1016/j.hedp.2009.05.018
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
We report on a set of experiments in which solid targets of different atomic numbers (Z) were irradiated with laser pulses of time durations ranging from 300 fs to 33 ps, and energies up to 26 J. The time-resolved X-ray emission in the 7.6-8.1 angstrom spectral range was measured using an ultra-fast X-ray streak camera coupled with a conical Bragg crystal. In this way we were able to follow the dramatic modification of the spectral features as a function of the laser duration. The features evolve from a "ns-type" emission, characterized by narrow and well-defined spectral lines, to very broad spectral features, due not only to the Stark broadening but also to the proliferation of satellites lines. The measured spectra also show strong time dependence, which allows us to follow the time evolution of the hydrodynamic parameters. We then compare the derived parameter with the CHIVAS hydro-radiative simulations. The experimental results are also compared with the AVERROES/TRANSPEC collisional-radiative code, and with precise spectral line shape calculations (PPP and PrismSPECT). The results seem to indicate regimes of interaction where hot electrons play an important role on spectral line formation. (C) 2009 Elsevier B.V. All rights reserved.
引用
收藏
页码:99 / 104
页数:6
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