English: This graph shows temperature profile in the en:troposphere and in the lower en:stratosphere of en:Uranus. Heights are also indicated. *The blue curve is from Lindal et al.^[1].

• The green curve is from Bishop et al.^[2]

• The dashed blue curve is an extrapolation of the 1987 Lindal et al. data^[1] (solid blue) using a constant lapse rate of 0.82 K/km.

• The filled pink circles with error bars are temperatures from West et al.^[3]

• The graph also shows locations of the main cloud and haze layers according to 1990 Bishop et al.^[2], Atreya et al.^[4] and dePater et al. ^[5]

References

1. ↑ ^{a b} Lindal, G.F., Lyons, J.R., Sweetnam, D.N., Eshleman, V.R., Hinson, D.P., Tyler, G.L., 1987. The atmosphere of Uranus: Results of radio occultation measurements with Voyager 2. J. Geophys. Res. 92, 14987–€“15001 (Table 1);
2. ↑ ^{a b} Bishop, J.; Atreya, S.K.; Herbert, F.; and Romani, P. (1990). "Reanalysis of Voyager 2 UVS Occultations at Uranus: Hydrocarbon Mixing Ratios in the Equatorial Stratosphere", Icarus 88: 448–463 (Table 1).
3. ↑ West, R. A.; Lane, A. L.; Nelson, R. M.; Wallis, B. D.; Hord, C. W.; Esposito, L. W.; Simmons, K. E. (1987). "Temperature and Aerosol Structure of the Nightside Uranian Stratosphere from Voyager 2 Photopolarimeter Stellar Occultation Measurements", JOURNAL OF GEOPHYSICAL RESEARCH 92: 15,030–€“36.
4. ↑ Atreya, S.; Egeler, P.; Baines, K. (2006). "Water-ammonia ionic ocean on Uranus and Neptune?", Geophysical Research Abstracts 8: 05179
5. ↑ dePater, Imke; Romani, Paul N.; Atreya, Sushil K. (1991). "Possible Microwave Absorbtion in by H2S gas Uranus’ and Neptune’s Atmospheres", Icarus 91: 220–233.