Impulsively generated waves in two-fluid plasma in the solar chromosphere: Heating and generation of plasma outflows

Open Access

Fig. 7.

Time-distance plots for V_ix (a), V_iy (b), and V_iz correspond to coupled Alfvén and MAWs for B = [0, 10, 2] Gs. These plots correspond to the slices taken at x = 0 Mm in Fig. 4. The blue and red bands indicate the propagation of the waves.

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