High-power laser-produced plasmas and astrophysics
- 1 September 1991
- journal article
- research article
- Published by Cambridge University Press (CUP) in Laser and Particle Beams
- Vol. 9 (4) , 869-879
- https://doi.org/10.1017/s0263034600006613
Abstract
The temperatures and the densities of plasmas produced by high-power lasers vary widely but in certain cases are similar to those found in astrophysical plasmas. In recent years our understanding of intense laser–matter interaction and the evolution of the resultingplasma has increased to the point where experiments can be designed to produce plasmas that allow astrophysical models to be tested. In this paper I review experimental work on laser-produced plasmas that is relevant to astrophysics. In the fields of highlyionized ion line identification and radiative opacity, relevant measurements have already been performed. Other experiments that could be performed with current laser facilities, including studies of X-ray nebula plasmas and complex radiation line transport, are described. In addition, experiments to investigate plasmas under more extreme conditions, which may be achievable with more powerful lasers, are mentioned.Keywords
This publication has 35 references indexed in Scilit:
- Measurement and Analysis of Radiation Transport in Laser-Irradiated TargetsEurophysics Letters, 1990
- Conversion of laser light into x rays in thin foil targetsPhysical Review A, 1990
- Observations of High-Density Plasmas Produced with Picosecond High-Power KrF IrradiationEurophysics Letters, 1989
- Blue Shift of the K Absorption Edge in Laser-Shocked SolidsEurophysics Letters, 1989
- Bracketing the astrophysical opacities for the King IVa mixtureThe Astrophysical Journal, 1989
- Quasi-monochromatic, projection radiography of dense laser driven spherical targetsOptics Communications, 1985
- Is the metal contribution to the astrophysical opacity incorrect?The Astrophysical Journal, 1984
- Calculation of gain at X-ray wavelengths resulting from optical pumping of helium-like ionsJournal of Quantitative Spectroscopy and Radiative Transfer, 1982
- Efficiency of the Bowen fluorescence mechanism in static nebulaeThe Astrophysical Journal, 1980
- Transfer of X-rays through a spherically symmetric gas cloudThe Astrophysical Journal, 1976