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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 2.

Normalized transverse perturbations of velocity of charges (top row), velocity of neutrals (middle row), and magnetic field (bottom row) at the time t = 40τ from simulations of waves generated by the linearly polarized driver given by Equations (18), but taking into account the effect of Hall’s term. The same plasma parameters as in Figure 1 have been used. The black dashed and dotted lines represent the damping associated with the ion-cyclotron and the whistler modes, respectively. Only the y-component of the perturbations is shown.

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