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Brillouin backscatter dependence upon pulse amplitudes, timing, target material, and geometry
1.B. H. Ripin, J. M. McMahon, E. A. McLean, W. M. Manheimer, and J. A. Stamper, Phys. Rev. Lett. 33, 634 (1974).
2.“Direct backscatter” or “backscatter” is defined here as the laser energy scattered back through the focusing lens only.
3.B. H. Ripin, F. C. Young, J. A. Stamper, C. M. Armstrong, R. Decoste, E. A. McLean, and S. E. Bodner, Phys. Rev. Lett. 39, 611 (1977).
4.B. H. Ripin, NRL Memo Report No. 3684, 1977 (unpublished).
5.D. W. Phillion, W. L. Kruer, and V. C. Rupert, Phys. Rev. Lett. 39, 1529 (1977).
6.J. L. Nuckolls, L. Wood, A. Thiessen, and G. Zimmerman, Nature (London) 239, 139 (1972).
7.B. H. Ripin, J. A. Stamper, and E. A. McLean, Proc. of 1978 IEEE Int’l Conf. on Plasma Science, Monterey, Calif. (IEEE, New York, 1978).
8.K. Eidmann and R. Sigel, Laser Interaction and Related Plasma Phenomena, edited by H. Schwarz and H. Hora (Plenum, New York, 1973), Vol. 3, p. 667.
9.R. H. Lehmberg, Phys. Rev. Lett. 41, 863 (1978).
10.D. G. Colombant and W. M. Manheimer Proc. of 1979 Int’l Conf. on Plasma Science, Montreal, 1979 (unpublished).
10.The work utilizes the saturation mechanism used in W. M. Manheimer and R. W. Flynn, Phys. Fluids 17, 409 (1974).
11.When the heat source (incident laser energy) is still on during the relevant expansion, as in a continuous pulse, an isothermal expansion model is appropriate and the density scale length at a given density is [F. Felber and R. Decoste, Phys. Fluids 21, 520 (1978)]. The plasma expansion following a prepulse, however, is slower (adiabatic) due to the lack of a heat source to maintain the plasma temperature.
12.F. Amiranoff, R. Benattar, R. Fabbro, E. Fabre, C. Garban, C. Popovics, A. Poquerusse, R. Sigel, C. Stenz, J. Virmont, and M. Weinfield, 7th Int’l Conf. on Plasma Physics and Controlled Nuclear Fusion Research, Innsbruck, Austria, 1978, paper IAEA‐CN‐37‐D4 (unpublished).
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