Open Access
Fig. 17
Cumulative, height-integrated number density of He, ∫
, in the optically thin region of the atmosphere p < p(τs(λ) = 1) for thesub-stellar, anti-stellar and equatorial morning and evening terminator points for
λ = 0.1 μm, 1.0 μm, 10.5 μm and 107 μm.
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