Driven two-fluid Alfvén waves in a solar magnetic flux tube with a realistic ionization rate

Open Access

Fig. 6.

Damping length of Alfvén waves vs. the position of the driver with P_d = 2.5 s and V₀ = 1 km s⁻¹ in Eq. (16) (dots) for the solar chromosphere with B_v = 10 G and obtained from the dispersion relation of Eq. (17) (asterisks).

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