52nd Annual Meeting of the APS Division of Plasma Physics
Volume 55, Number 15
Monday–Friday, November 8–12, 2010;
Chicago, Illinois
Session BI2: National Ignition Facility Design, Energetics, Symmetry and Mix
9:30 AM–12:30 PM,
Monday, November 8, 2010
Room: Grand Ballroom CD
Chair: Sean Regan, University of Rochester
Abstract ID: BAPS.2010.DPP.BI2.2
Abstract: BI2.00002 : Stimulated Raman scatter analyses of experiments conducted at the National Ignition Facility*
10:00 AM–10:30 AM
Preview Abstract
Abstract
Author:
D.E. Hinkel
(Lawrence Livermore National Laboratory)
The recent energetics campaign\footnote{N. B. Meezan {\it et
al.}, Phys. Plasmas {\bf 17}, 056304 (2010).} conducted at the
National Ignition Facility in Fall, 2009 achieved its two main
goals: providing radiation drive and symmetry suitable
for subsequent ignition experiments. Many diagnostics were
fielded during this campaign, one of which provided a
time-resolved wavelength spectrum of light reflected from the
target by stimulated Raman scatter (SRS). SRS occurs when
incident light reflects off self-generated electron plasma waves.
The SRS spectrum of an inner cone quad has provided insight into
these experiments. Analyses indicate that synthetic SRS
diagnostics better match those of experiments when an atomic
physics model with greater emissivity is utilized, along with
less inhibited electron transport (higher flux, with, ideally,
nonlocal electron transport). With these models,\footnote{M. D.
Rosen, this conference.} SRS primarily occurs in a region of the
target where nearest-neighbor 23$^{\circ}$ quads significantly
overlap the diagnosed 30$^{\circ}$ quad. This increases the gain
at lower density (lower wavelength), a feature consistent with
experimental results. Other predicted features, such as the
direction and spreading of the SRS as well as its intensity, are
also in better agreement with experiment.
Inclusion of this effect of multiple beams sharing a reflected
SRS light wave has resulted in modifications to our laser-plasma
interaction codes.\footnote{C. H. Still, this
conference.}$^,$\footnote{D. J. Strozzi, E. A. Williams, D. E.
Hinkel {\it et al.}, Phys. Plasmas {\bf 15}, 102703
(2008).}$^,$\footnote{R. L. Berger, C. H. Still, E. A. Williams,
and A. B. Langdon, Phys. Plasmas {\bf 5}, 4337 (1998); C. H.
Still, R. L. Berger, A. B. Langdon, D. E. Hinkel, L. J. Suter,
and E. A. Williams, Phys. Plasmas {\bf}, 2023 (2000); D. E.
Hinkel, D. A. Callahan, A. B. Langdon, S. H. Langer, C. H. Still,
and E. A. Williams, Phys. Plasmas {\bf 15}, 056314 (2008).}
These improved capabilities are being
tested by making predictions for upcoming National Ignition
Campaign experiments. Synthetic SRS spectra, reflectivity levels,
and the angular distribution of SRS light will be compared to
experimental results.
*This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2010.DPP.BI2.2