A linearized coupled model of acoustic-gravity waves and the lower ionosphere at Mars

Open Access

Fig. 27

Distributions of peak altitude and peak amplitude of perturbed magnetic field magnitude ratio, B₁ /B₀, driven by AWs and GWs and displayed in panels a-b and panels c–d, respectively. $k_{z}^{l}$ are 0.11, 0.32, and 0.99 km⁻¹ for AWs and −0.07, −0.19, and −0.5 km⁻¹ for GWs. Horizontal wavelengths of the selected wave modes range from 10 km to 300 km in intervals of 10 km.

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