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Rapid self-magnetization of laser speckles in plasmas by nonlinear anisotropic instability

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Rapid self-magnetization of laser speckles in plasmas by nonlinear anisotropic instability. / Thomas, A. G. R.; Kingham, R. J.; Ridgers, C. P.
In: New Journal of Physics, Vol. 11, 033001, 03.03.2009.

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Thomas AGR, Kingham RJ, Ridgers CP. Rapid self-magnetization of laser speckles in plasmas by nonlinear anisotropic instability. New Journal of Physics. 2009 Mar 3;11:033001. doi: 10.1088/1367-2630/11/3/033001

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Thomas, A. G. R. ; Kingham, R. J. ; Ridgers, C. P. / Rapid self-magnetization of laser speckles in plasmas by nonlinear anisotropic instability. In: New Journal of Physics. 2009 ; Vol. 11.

Bibtex

@article{1637a02b7f764b70b52bb7c224555f57,
title = "Rapid self-magnetization of laser speckles in plasmas by nonlinear anisotropic instability",
abstract = "Presented here are the first kinetic two-dimensional Vlasov-Fokker-Planck calculations of inertial confinement fusion-related laser-plasma interactions, to include self-consistent magnetic fields, hydrodynamic plasma expansion and anisotropic electron pressure. An underdense plasma, reminiscent of the gas fill of a hohlraum, is heated by a laser speckle with I lambda(2) = 1.0 x 10(15) W cm(-2) mu m(2) and radius omega(0) = 5 mu m. Inverse bremsstrahlung absorption of the laser and non-local electron transport lead to the development of a collisional analogue of the Weibel electromagnetic instability. The instability is seeded by magnetic fields, generated in an initial period of linear growth due to the anisotropic electron distribution arising in a laser speckle. Using the circular polarization does not generate significant fields. For linear polarization, the field generally saturates when the magnetization is omega tau(ei) > 1, and the effective growth rate is similar to the coherence time of typical laser speckles. The presence of these magnetic fluctuations significantly affects the heat fluxes and hydrodynamics in the plasma.",
keywords = "NONLOCAL ELECTRON-TRANSPORT, FIELD GENERATION, INVERSE BREMSSTRAHLUNG, WEIBEL INSTABILITY, HEATED PLASMAS, FUSION",
author = "Thomas, {A. G. R.} and Kingham, {R. J.} and Ridgers, {C. P.}",
year = "2009",
month = mar,
day = "3",
doi = "10.1088/1367-2630/11/3/033001",
language = "English",
volume = "11",
journal = "New Journal of Physics",
issn = "1367-2630",
publisher = "IOP Publishing Ltd",

}

RIS

TY - JOUR

T1 - Rapid self-magnetization of laser speckles in plasmas by nonlinear anisotropic instability

AU - Thomas, A. G. R.

AU - Kingham, R. J.

AU - Ridgers, C. P.

PY - 2009/3/3

Y1 - 2009/3/3

N2 - Presented here are the first kinetic two-dimensional Vlasov-Fokker-Planck calculations of inertial confinement fusion-related laser-plasma interactions, to include self-consistent magnetic fields, hydrodynamic plasma expansion and anisotropic electron pressure. An underdense plasma, reminiscent of the gas fill of a hohlraum, is heated by a laser speckle with I lambda(2) = 1.0 x 10(15) W cm(-2) mu m(2) and radius omega(0) = 5 mu m. Inverse bremsstrahlung absorption of the laser and non-local electron transport lead to the development of a collisional analogue of the Weibel electromagnetic instability. The instability is seeded by magnetic fields, generated in an initial period of linear growth due to the anisotropic electron distribution arising in a laser speckle. Using the circular polarization does not generate significant fields. For linear polarization, the field generally saturates when the magnetization is omega tau(ei) > 1, and the effective growth rate is similar to the coherence time of typical laser speckles. The presence of these magnetic fluctuations significantly affects the heat fluxes and hydrodynamics in the plasma.

AB - Presented here are the first kinetic two-dimensional Vlasov-Fokker-Planck calculations of inertial confinement fusion-related laser-plasma interactions, to include self-consistent magnetic fields, hydrodynamic plasma expansion and anisotropic electron pressure. An underdense plasma, reminiscent of the gas fill of a hohlraum, is heated by a laser speckle with I lambda(2) = 1.0 x 10(15) W cm(-2) mu m(2) and radius omega(0) = 5 mu m. Inverse bremsstrahlung absorption of the laser and non-local electron transport lead to the development of a collisional analogue of the Weibel electromagnetic instability. The instability is seeded by magnetic fields, generated in an initial period of linear growth due to the anisotropic electron distribution arising in a laser speckle. Using the circular polarization does not generate significant fields. For linear polarization, the field generally saturates when the magnetization is omega tau(ei) > 1, and the effective growth rate is similar to the coherence time of typical laser speckles. The presence of these magnetic fluctuations significantly affects the heat fluxes and hydrodynamics in the plasma.

KW - NONLOCAL ELECTRON-TRANSPORT

KW - FIELD GENERATION

KW - INVERSE BREMSSTRAHLUNG

KW - WEIBEL INSTABILITY

KW - HEATED PLASMAS

KW - FUSION

U2 - 10.1088/1367-2630/11/3/033001

DO - 10.1088/1367-2630/11/3/033001

M3 - Journal article

VL - 11

JO - New Journal of Physics

JF - New Journal of Physics

SN - 1367-2630

M1 - 033001

ER -