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New model of Raman spectra in laser produced plasma

Conference ·
OSTI ID:7044792
Some experimental observations of Raman scattering in laser produced plasma have been previously attributed to the onset of the convective Stimulated Raman Instability (SRS-C). This interpretation has had a number of difficulties, associated with the calculated threshold for onset of the SRS-C, the existence of gaps in the frequency spectrum near the incident frequency ..omega../sub 0/ and near ..omega../sub 0//2, and with the angular distribution. We now propose a new explanation based on ordinary incoherent Thompson scattering, with a greatly enhanced plasma line. Transient local reversed-slope velocity distributions in the underdense region can be produced by pulses of hot electrons arising from the two-plasmon (2..omega../sub p/) or absolute stimulated Raman instabilities (SRS-A) occurring near the quarter critical surface. A simple model yields the observed spectral gaps near ..omega../sub 0/ and near ..omega../sub 0//2. It also explains the correlation of onset of this scattering with onset of the SRS-A, its transient localization in frequency and time, and the weak azimuthal angular variation. The existence of upscattered light is also predicted.
Research Organization:
Rochester Univ., NY (USA). Lab. for Laser Energetics
DOE Contract Number:
AC08-80DP40124
OSTI ID:
7044792
Report Number(s):
DOE/DP/40124-34; CONF-8405163-5; ON: DE84012487
Country of Publication:
United States
Language:
English