Observation of the far wing of Lyman α due to neutral atom and ion collisions in a laser-produced plasma

被引:21
作者
Kielkopf, JF [1 ]
Allard, NF
机构
[1] Univ Louisville, Dept Phys, Louisville, KY 40292 USA
[2] Observ Paris, Dept Atomes & Mol Astrophys, F-92195 Meudon, France
[3] Inst Astrophys, CNRS, F-75014 Paris, France
来源
PHYSICAL REVIEW A | 1998年 / 58卷 / 06期
关键词
D O I
10.1103/PhysRevA.58.4416
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
The time-resolved spectrum of a laser-produced plasma in H-2 exhibits a continuum that we attribute to radiative collisions of H atoms in a 2p state with ground-state neutral atoms and protons. This binary collision Lyman-cu line wing observed from 1150 Angstrom to 1700 Angstrom is emitted by the shock dissociated gas that surrounds the focal region. The observed temperature, electron density, and shock front speed confirm models of the shock that predict that Lyman cu arises from a shell of atomic hydrogen in which the neutral atom and ion densities are sufficient to create the observed line broadening. The experimental far wing spectrum agrees with unified theory calculations of the Lyman-cu line, which allow for the dependence of the radiative dipole moment on internuclear separation during a radiative collision. Broad neutral atom effects become evident at 1180 Angstrom, 1260 Angstrom, and 1600 Angstrom when the density of neutral perturbers is of the order of 10(20) atoms/cm(3), while features at 1230 Angstrom, 1240 Angstrom, and 1400 Angstrom appear when the plasma is highly ionized. These satellites result from free-foe transitions of a H atom during collisions with other neutral atoms and protons and are correlated with potential curves and radiative dipole moments of H-2 and H-2(+). [S1050-2947(98)02811-X].
引用
收藏
页码:4416 / 4425
页数:10
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