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Table 1

Parameters of methane profiles shown in Fig. 5.

Kzz*$K_{zz}^*$ [cm2/s ] Lyα B [R] Raman B [R] z [km] (P [mbar]) for τabs1216=0.11$\tau _{{\rm{abs}}}^{1216} = 0.1 - 1$ at SZA=0 nCH4${n_{{\rm{C}}{{\rm{H}}_4}}}$ & NCH4${N_{{\rm{C}}{{\rm{H}}_4}}}$ at τabs1216=1$\eqalign{ & \tau _{{\rm{abs}}}^{1216} = 0.1 - 1 \cr & \tau _{{\rm{abs}}}^{1216} = 1 \cr} $ [cm−3 & cm2] z [km] (P [mbar]) where nCH4~1cm3${n_{{\rm{C}}{{\rm{H}}_4}}}\~1\,{\rm{c}}{{\rm{m}}^{ - 3}}$ Remark
2430 710 13.16 297–259 (7.45e-2–1.58e-1) 3.35e10 & 5.3e16 ∼520 (2.25e-3) a
2150 713 14 292–257 (8.2e-2–1.65e-1) 3.2e10 & 4.87e16 ∼515 (2.4e-3) b
1130 728 20 275–239 (1.14e-2–2.43e-1) 3.8e10 & 5.2e16 ∼480 (3.9e-3) b
1040 731 21 272–237 (1.21e-2–2.54e-1) 3.82e10 & 5.13e16 ∼478 (4e-3) b
170 138 20 223–192 (3.47e-1–7.3e-1) 5.21e10 & 5.13e16 ∼395 (1.37e-2) c

Notes. nCH4${N_{{\rm{C}}{{\rm{H}}_4}}}$ represents methane column density. Remarks: (a) reference profile; (b) fit to observation; (c) fit to observation without considering resonant scattering. For these simulations, we employed the model atmosphere used to explain the 2011 HST STIS Lyα observations by Joshi et al. (2025), with minor adjustments. Further details are provided in Sect. 4.

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