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 BI01: Invited: Parker Solar Probe and Distribution Functions
9:30 AM–12:30 PM,
Monday, November 9, 2020
Chair: Amy Keesee, University of New Hampshire
Abstract: BI01.00005 : Measurements of Electron Distribution Functions in Laser-Produced Plasmas Using Angularly Resolved Thomson Scattering
11:30 AM–12:00 PM
Live
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Abstract
Author:
Avram Milder
(Lab for Laser Energetics)
Electron velocity distribution functions (EDF's) are the foundation of most
plasma physics. Here we present the first measurements of the complete EDF
without any assumptions on its shape or the underlying physics that
generated it. This first-principle measurement showed that during
significant inverse bremsstrahlung heating by laser beams, the bulk of the
distributions were measured to be super-Gaussian in shape, while the
electrons above 3\texttimes the thermal velocity were distributed according
to Maxwell--Boltzmann (Maxwellian) statistics. When the inverse
bremsstrahlung rates were negligible, Maxwell EDF's were measured. To enable
single-shot temporally and spatially resolved measurements, an optical
diagnostic was invented that uses the collective nature of plasmas and the
angular dependence of the scattering to enable the EDF to be determined over
several orders of magnitude without any assumptions on its form. This novel
Thomson-scattering technique encoded the electron motion to the frequency of
scattered light and used collective scattering to increase the signal at
velocities where the number of electrons are limited. The ability to measure
the EDF beyond 4\texttimes the thermal velocity with high precision allowed
the results to address long-standing physics questions regarding the
relaxation of high-velocity electrons toward a Maxwellian. These results are
in excellent agreement with pioneering computational work by J. P. Matte \textit{et al.}\footnote{
J. P. Matte \textit{et al.}, Plasma Phys. Control. Fusion \textbf{30}, 1665 (1988).} that
describe the evolution of the bulk electrons to a non-Maxwellian
distribution due to inverse bremsstrahlung heating. The response of
high-velocity (\textgreater 3$v_{\mathrm{th}})$ electrons was compared with
Fourkal \textit{et al.},\footnote{ E. Fourkal \textit{et al.}, Phys. Plasmas \textbf{8}, 550 (2001)} which
suggested electron--electron collisions dictate the shape of the tail while
the isotropy of the electric field dictates the amplitude of the tail. This
material is based upon work supported by the Department of Energy National
Nuclear Security Administration under Award Number DE-NA0003856.