Astrophysically Relevant Turbulent Magnetic Fields in Table-Top Intense-Laser Experiments

ORAL

Abstract

We present experiments on the spatio-temporal dynamics of megagauss magnetic fields created in solid-density plasmas by intense femtosecond laser pulses. Our results display distinctive signatures of the Kolmogorov -5/3 scaling in the k-spectra of the turbulent magnetic fields. About 50 picoseconds after the incidence of the main interaction laser pulse, the spectrum displays two distinct turbulent regimes, characterized by a -5/3 scaling (for smaller values of k) and a -7/3 scaling (for larger values of k), separated by a spectral ``kink.'' Similar spectral ``knees'' have been observed previously in Alfven ion cyclotron waves in the turbulent magnetosheath of the earth as well as in turbulent processes in the solar photosphere.

Authors

  • G. Ravindra Kumar

    • Tata Institute of Fundamental Research, Mumbai, India
  • Gourab Chatterjee

    • Tata Institute of Fundamental Research, Mumbai, India
  • Amit D. Lad

    • Tata Institute of Fundamental Research, Mumbai, India
  • Prashant K. Singh

    • Tata Institute of Fundamental Research, Mumbai, India
  • Amitava Adak

    • Tata Institute of Fundamental Research, Mumbai, India
  • P. Brijesh

    • Tata Institute of Fundamental Research, Mumbai, India
  • Z.M. Sheng

    • Shanghai Jiao Tong University, Shanghai, China
  • Amita Das

    • Institute for Plasma Research, Gandhinagar, India
  • Sudip Sengupta

    • Institute for Plasma Research, Gandhinagar, India
  • Predhiman K. Kaw

    • Institute for Plasma Research, Gandhinagar, India