Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session NP11: Poster Session V: Laser-plasma Particle Acceleration; HEDP; Turbulence and Transport; DIII-D Tokamak; Machine Learning, Data Science (9:30am-12:30pm)
Wednesday, November 7, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.NP11.40
Abstract: NP11.00040 : Plasma mirror reflectivity and focal spot quality for glass and aluminum mirrors for laser pulses up to 30 picoseconds*
Presenter:
Brandon Christian Edghill
(Univ of California - San Diego)
Authors:
Brandon Christian Edghill
(Univ of California - San Diego)
Pierre Forestier-Colleoni
(Univ of California - San Diego)
Jaebum Park
(Lawrence Livermore Natl Lab)
Sasha Rubenchik
(Lawrence Livermore Natl Lab)
Farhat N Beg
(Univ of California - San Diego)
Tammy Yee Wing Ma
(Lawrence Livermore Natl Lab)
The Advanced Radiographic Capability (ARC) short pulse laser at the National Ignition Facility (NIF) at the Lawrence Livermore National Laboratory is capable of producing a high energy,∼4kJ , laser pulse of 30 ps in a ∼100μm focal spot, leading to an intensity of 1018 W/cm2. For many applications, including radiography and warm dense matter creation, higher laser intensities are desirable to produce the necessary x-ray and particle fluxes. Due to the complexity of the NIF target chamber, changing the location of the final focusing parabola in order to improve the focal spot size is not an option. This leads to the possible use of disposable ellipsoidal plasma mirrors placed within the chamber, close to the target in an attempt to focus the four ARC beams. The behavior of plasma mirrors at these relatively long pulse durations (>10 ps) is not well characterized. The results from the COMET laser at the Jupiter Laser Facility (JLF) carried out at similar pulse durations show the deterioration of glass plasma mirrors’ focal spots at longer pulse durations and less degradation when using aluminum plasma mirrors.
**This work performed under the auspices of the U.S. DOE by LLNL under Contract DE-AC52-07NA27344 and funded by the LLNL LDRD program under tracking code 17-ERD-039.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.NP11.40
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