Back to Search Start Over

In-flight observations of low-mode ρR asymmetries in NIF implosions.

Authors :
Zylstra, A. B.
Frenje, J. A.
Séguin, F. H.
Rygg, J. R.
Kritcher, A.
Rosenberg, M. J.
Rinderknecht, H. G.
Hicks, D. G.
Friedrich, S.
Bionta, R.
Meezan, N. B.
Olson, R.
Atherton, J.
Barrios, M.
Bell, P.
Benedetti, R.
Hopkins, L. Berzak
Betti, R.
Bradley, D.
Callahan, D.
Source :
Physics of Plasmas; 2015, Vol. 22 Issue 5, p1-9, 9p
Publication Year :
2015

Abstract

Charged-particle spectroscopy is used to assess implosion symmetry in ignition-scale indirect-drive implosions for the first time. Surrogate D³He gas-filled implosions at the National Ignition Facility produce energetic protons via D+³He fusion that are used to measure the implosion areal density (ρR) at the shock-bang time. By using protons produced several hundred ps before the main compression bang, the implosion is diagnosed in-flight at a convergence ratio of 3–5 just prior to peak velocity. This isolates acceleration-phase asymmetry growth. For many surrogate implosions, proton spectrometers placed at the north pole and equator reveal significant asymmetries with amplitudes routinely ≳10%, which are interpreted as ℓ=2 Legendre modes. With significant expected growth by stagnation, it is likely that these asymmetries would degrade the final implosion performance. X-ray self-emission images at stagnation show asymmetries that are positively correlated with the observed in-flight asymmetries and comparable in magnitude, contradicting growth models; this suggests that the hot-spot shape does not reflect the stagnated shell shape or that significant residual kinetic energy exists at stagnation. More prolate implosions are observed when the laser drive is sustained (“no-coast”), implying a significant time-dependent asymmetry in peak drive. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
1070664X
Volume :
22
Issue :
5
Database :
Complementary Index
Journal :
Physics of Plasmas
Publication Type :
Academic Journal
Accession number :
103031077
Full Text :
https://doi.org/10.1063/1.4918355