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. Author manuscript; available in PMC: 2020 May 5.
Published in final edited form as: Astrophys J Lett. 2018 Feb 20;854(2):L30. doi: 10.3847/2041-8213/aaadbd

Figure 2:

Figure 2:

: Sample of fits in the 1200–1400 cm−1 part of the FP4 Titan spectrum containing the CH4 emission band which gives access to the temperature profile. The blue curves are the observations by CIRS at different dates and the red curves are the model simulations that best fit the data: (top) December 2013 near 70°S; (middle) December 2013 near 70°N; (bottom) August 2016 near 70°N.