Insensitivity of a turbulent laser-plasma dynamo to initial conditions

Bott, A. F. A. and Chen, L. and Tzeferacos, P. and Palmer, C. A. J. and Bell, A. R. and Bingham, R. and Birkel, A. and Froula, D. H. and Katz, J. and Kunz, M. W. and Li, C.-K. and Park, H-S. and Petrasso, R. and Ross, J. S. and Reville, B. and Ryu, D. and Séguin, F. H. and White, T. G. and Schekochihin, A. A. and Lamb, D. Q. and Gregori, G. (2022) Insensitivity of a turbulent laser-plasma dynamo to initial conditions. Matter and Radiation at Extremes, 7 (4). 046901. ISSN 2468-2047 (https://doi.org/10.1063/5.0084345)

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Abstract

It has recently been demonstrated experimentally that a turbulent plasma created by the collision of two inhomogeneous, asymmetric, weakly magnetized, laser-produced plasma jets can generate strong stochastic magnetic fields via the small-scale turbulent dynamo mechanism, provided the magnetic Reynolds number of the plasma is sufficiently large. In this paper, we compare such a plasma with one arising from two pre-magnetized plasma jets whose creation is identical save for the addition of a strong external magnetic field imposed by a pulsed magnetic field generator. We investigate the differences between the two turbulent systems using a Thomson-scattering diagnostic, x-ray self-emission imaging, and proton radiography. The Thomson-scattering spectra and x-ray images suggest that the external magnetic field has a limited effect on the plasma dynamics in the experiment. Although the external magnetic field induces collimation of the flows in the colliding plasma jets and although the initial strengths of the magnetic fields arising from the interaction between the colliding jets are significantly larger as a result of the external field, the energies and morphologies of the stochastic magnetic fields post-amplification are indistinguishable. We conclude that, for turbulent laser-plasmas with supercritical magnetic Reynolds numbers, the dynamo-amplified magnetic fields are determined by the turbulent dynamics rather than the seed fields or modest changes in the initial flow dynamics of the plasma, a finding consistent with theoretical expectations and simulations of turbulent dynamos.

ORCID iDs

Bott, A. F. A., Chen, L., Tzeferacos, P., Palmer, C. A. J., Bell, A. R., Bingham, R. ORCID logoORCID: https://orcid.org/0000-0002-9843-7635, Birkel, A., Froula, D. H., Katz, J., Kunz, M. W., Li, C.-K., Park, H-S., Petrasso, R., Ross, J. S., Reville, B., Ryu, D., Séguin, F. H., White, T. G., Schekochihin, A. A., Lamb, D. Q. and Gregori, G.;
  • Item type:Article
    ID code:81629
    Dates:
    Date
    Event
    27 July 2022
    Published
    19 May 2022
    Accepted
    Subjects:Science > Physics
    Department:Faculty of Science > Physics
    Depositing user: Pure Administrator
    Date deposited:29 Jul 2022 11:35
    Last modified:14 Nov 2024 13:41
    URI:https://strathprints.strath.ac.uk/id/eprint/81629
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