Figure 6 from Detection of Dynamical Instability in Titan’s Thermospheric Jet

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Detection of Dynamical Instability in Titan’s Thermospheric Jet

Authors: M. A. Cordiner, E. Garcia-Berrios, R. G. Cosentino, N. A. Teanby, C. E. Newman, C. A. Nixon, A. E. Thelen, and S. B. Charnley

2020 The Astrophysical Journal Letters 904 L12.

Provider: AAS Journals

Caption: Figure 6.

Best-fitting synthetic (convolved) wind fields derived for each molecule in 2016 and 2017, assuming a Gaussian zonal wind velocity profile as a function of latitude. Velocity contours are labeled in units of m s⁻¹. Wire-frame sphere indicates Titan’s orientation with respect to the ALMA field of view.

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