Radiative-convective models of the atmospheres of Uranus and Neptune: Heating sources and seasonal effects

Open Access

Fig. 19

Uranus: comparison of the temperature retrieved (blue line) from the Voyager 2/IRIS experiment (Orton et al. 2015) and the simulated temperature (orange line) at 100 hPa (solid line) and 400 hPa (dashed line). Uncertainties from the spectral inversion of IRIS data are lower than 1 K.

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