Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-25T05:00:30.142Z Has data issue: false hasContentIssue false

MIMOZA-ND calculations of the influence of large-scale shell asymmetry on indirect drive target compression

Published online by Cambridge University Press:  07 March 2001

L.S. MKHITARIAN
Affiliation:
The Russian Federal Nuclear Center—All-Russia Scientific Research, Institute of Experimental Physics, 607190, Sarov, Nizhniy Novgorod region
S.A. BEL'KOV
Affiliation:
The Russian Federal Nuclear Center—All-Russia Scientific Research, Institute of Experimental Physics, 607190, Sarov, Nizhniy Novgorod region
Y.N. EREMENKO
Affiliation:
The Russian Federal Nuclear Center—All-Russia Scientific Research, Institute of Experimental Physics, 607190, Sarov, Nizhniy Novgorod region
G.G. KOCHEMASOV
Affiliation:
The Russian Federal Nuclear Center—All-Russia Scientific Research, Institute of Experimental Physics, 607190, Sarov, Nizhniy Novgorod region
O.A. VINOKUROV
Affiliation:
The Russian Federal Nuclear Center—All-Russia Scientific Research, Institute of Experimental Physics, 607190, Sarov, Nizhniy Novgorod region

Abstract

Experiments carried out at the ISKRA-5 facility have demonstrated high (not worse than 3%) symmetry of the X-ray radiation flux inside a spherical case (hohlraum). This fact gave us an opportunity for investigating into compression of the targets with the initial nonspherical geometry. The asymmetry affects both the total neutron yield and the moment of neutrons generation. In this paper we present the simulation results of the asymmetric targets dynamics which were carried out by means of the 2D MIMOZA-ND code. This code allows to take into account effects of nonstationary, nonequilibrium, spectral transfer of X-ray radiation. Comparison between simulation results and experimental data was made. It was demonstrated that one could observe a satisfactory agreement between experimental data and the total neutron yield, as well as the time delay of the moment of neutrons generation.

Type
ZABABAKHIN SPECIAL PAPERS
Copyright
© 2000 Cambridge University Press

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)