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Propagation of Waves in Weakly Ionized Two-fluid Plasmas. II. Nonlinear Alfvénic Waves

  • Authors: David Martínez-Gómez

David Martínez-Gómez 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 4.

Time-averaged energy densities (top panels) and heating rates (bottom panels) computed from simulations of Alfvén waves (left column), ion-cyclotron waves (center column), and whistler waves (right column) with a period of τ = 0.02 s and amplitude of the driver given by Ac = 0.01cA,T. Case of a plasma with np = 1.4 × 1015 m−3, χ = 100, B0 = 10 G, and νnc = 100ω. Diamonds, asterisks, and crosses in the top panels represent the total energy density ﹩\langle { \mathcal U }\rangle ﹩, the magnetic energy density ﹩\langle { \mathcal M }\rangle ﹩, and the total kinetic energy density ﹩\langle { \mathcal K }\rangle ﹩. The solid lines in the bottom panels represent the heating rates computed using Equation (39).

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