61st Annual Meeting of the APS Division of Plasma Physics
Volume 64, Number 11
Monday–Friday, October 21–25, 2019;
Fort Lauderdale, Florida
Session GI3: Invited: ICF II
9:30 AM–12:30 PM,
Tuesday, October 22, 2019
Room: Floridian Ballroom CD
Chair: David Ampleford
Abstract ID: BAPS.2019.DPP.GI3.3
Abstract: GI3.00003 : Gamma measured ablator areal density observations, trends and time shifts on the National Ignition Facility*
10:30 AM–11:00 AM
Preview Abstract
Abstract
Author:
Kevin Meaney
(Los Alamos National Laboratory)
In inertial confinement fusion, few diagnostics are able to look at the
final state of the ablator in integrated, cyro-layered implosions. The Gamma
Reaction History diagnostic measures fusion gammas as well as the neutron
induced 4.4 MeV carbon ablator. Recently, a new analysis routine was
developed to isolate this carbon gamma line from other neutron induced
background, giving the areal density ($\rho $R) of the ablator as well as
the time shift between the carbon gammas and the DT fusion. Now carbon $\rho
$R values have been generated for a database across many National Ignition
Facility (NIF) shots. The values can be compared and contrasted across the
NIF campaigns. They reveal that the ablator is surprisingly not set by
velocity, DT cold fuel radius or picket intensity, as one might expect. But
instead is sensitive to the coast time, mass remaining and dopants. This
verifies that coast time is a vital metric that continues to apply pressure
onto the capsule late time, improving performance, as well as the
effectiveness of dopants to reduce mix and preheat and increase compression.
The data is also suggestive that fill tube jets increase the effective
carbon $\rho $R but the signal is within the uncertainty level. Future
improvements could use carbon $\rho $R in combination with x-ray diagnostics
to constrain the mass and density of all mixed material -- cold or hot. The
carbon gammas are observed to systematically arrive \textasciitilde 15ps
later than the DT fusion peak, implying the ablator areal density is
increasing across the burnwidth of the reaction. This shift allows
estimation of the amount of kinetic energy and velocity in the ablator at
bangtime and may reflect a slower final ablator speed than what is predicted
by simulations, consistent with a slower implosion and observed longer
burnwidth. Simulations predict that an igniting capsule has the carbon gamma
signal arrive before the DT fusion peak, suggesting the carbon gamma timing
could be a metric that could be used to quantify future ignition.
*This work was performed under the auspices of the U.S. Department of Energy by LANL under Contract No. DE-AC52–06NA25396
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2019.DPP.GI3.3