Experimental studies of inertial Alfvén-wave propagation through an Alfvén-speed gradient

POSTER

Abstract

Alfvén waves are ubiquitous in space, laboratory, and astrophysical plasmas. Understanding the reflection and transmission of these waves as they travel through plasma inhomogeneities is important for understanding wave propagation, turbulence, and heating of plasmas in general. Alfvén waves are predicted to reflect when encountering a gradient in the Alfvén speed. However, our recent studies using the Large Area Plasma Device (LAPD) at the University of California, Los Angeles, observed no reflection for kinetic Alfvén waves propagating through an Alfvén-speed gradient. In the present work, we have conducted LAPD experiments to study inertial Alfvén-wave propagation through an Alfvén-speed gradient. The gradients were created by varying the magnetic field in the direction of the propagation of the Alfvén wave. Here, we will present our results for the transmission and reflection of Alfvén waves along the Alfvén-speed gradient.

*This work is supported by grants from the NSF Solar-Terrestrial Program under grant AGS-1834822 and the U.S. Department of Energy, Office of Science, Office of Fusion Energy Science under Award Numbers DE-SC0016602 and DE-SC0021261. The experiments were performed at the Basic Plasma Science Facility (BaPSF), which is supported by the DOE and NSF, with major facility instrumentation developed via an NSF award AGS–9724366.

Presenters

  • Garima Joshi

    • Columbia University

Authors

  • Garima Joshi

    • Columbia University
  • Troy Carter

    • University of California, Los Angeles
  • Daniel W Savin

    • Columbia University
  • Shreekrishna Tripathi

    • University of California, Los Angeles
  • Steve T Vincena

    • University of California, Los Angeles
    • UCLA
  • Michael Hahn

    • Columbia University