Table 1
Parameters of methane profiles shown in Fig. 5.
[cm2/s ] |
Lyα B [R] | Raman B [R] | z [km] (P [mbar]) for at SZA=0◦ |
& at [cm−3 & cm2] |
z [km] (P [mbar]) where ![]() |
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.
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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