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Fig. 2

image

Planetary atmospheric profiles adopting the XUV spectra of SF11 (solid) and L14 (dashed). Shown are the number densities (total, atomic H, and protons), outflow velocity, ionization fraction, and temperature. In the velocity plot, crosses indicate the sonic points and plus signs denote the locations where the outflow velocity exceeds the escape velocity. The vertical dotted line indicates the location of the L1 point.

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