Abstract
Theoretical calculations of a Thomson scattering cross section and dynamical form factors are presented for high-Z, laser-produced, inhomogeneous plasmas. Relevance of these results to astrophysical plasmas is pointed out. Comparisons with recent experimental observations are discussed with emphasis on the e †ects of plasma inhomogeneity, ion-ion collisions, and non-Maxwellian distribution functions.
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CITATION STYLE
Rozmus, W., Glenzer, S. H., Estabrook, K. G., Baldis, H. A., & MacGowan, B. J. (2000). Modeling of Thomson Scattering Spectra in High‐ z , Laser‐produced Plasmas. The Astrophysical Journal Supplement Series, 127(2), 459–463. https://doi.org/10.1086/313319
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