62nd Annual Meeting of the APS Division of Plasma Physics
Volume 65, Number 11
Monday–Friday, November 9–13, 2020;
Remote; Time Zone: Central Standard Time, USA
Session ZI01: Invited: ICF and HEDP Diagnostics
9:30 AM–12:30 PM,
Friday, November 13, 2020
Chair: Johan Frenje, MIT
Abstract: ZI01.00005 : Measurement of mix at the fuel-ablator interface in indirectly-driven capsule implosions on the NIF
11:30 AM–12:00 PM
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Abstract
Author:
Gareth Hall
(Lawrence Livermore Natl Lab)
The interface between the capsule ablator and fuel ice layer is susceptible
to hydrodynamic instabilities. The subsequent mixing of hot ablator material
into the ice reduces fuel compression at stagnation and is a candidate for
reduced capsule performance. The ability to diagnose ice-ablator mix is
critical to understanding and improving stability at this interface.
Combining the Crystal Backlighter Imager with the Single Line of Sight
camera on the NIF provides multiple quasi-monochromatic 7.2keV radiographs
of layered capsule implosions per experiment, with high spatial and temporal
resolution. The narrow bandwidth of this diagnostic platform allows
radiography of the inner edge of the capsule limb close to stagnation
without capsule self-emission contaminating the data, providing a wealth of
information that can be used to assess the stability of the ice-ablator
interface. An important factor which affects the stability of the
ice-ablator interface is preheating of the ablator adjacent to the fuel by
energetic components of the x-ray drive, destabilizing the interface. Adding
a high-Z dopant layer to the ablator mitigates this effect. Results will be
presented from a campaign in which this radiographic technique was used to
measure the effect of tungsten dopant concentration on the ice-ablator
interface for a series of 3-shock High Density Carbon implosions. These
measurements reveal that while the addition of dopant provides an overall
stabilizing effect, there are significant differences between the equatorial
and polar regions of the capsule. It is hypothesized that this is due to the
anisotropy of the energetic components of the x-ray drive, suggesting that
this must be considered when addressing preheat. This work performed under
the auspices of the U.S. Department of Energy by Lawrence Livermore National
Laboratory under Contract DE-AC52-07NA27344.