Image Details

Choose export citation format:

Temporal Variability of Titan’s Middle-atmospheric Zonal Winds from Southern Fall to Late Winter (2016–2023)

  • Authors: Martin A. Cordiner, Yuan Lian, Juan M. Lora, Nicholas A. Lombardo, Lucy Wright, Jonathon Nosowitz, Richard Cosentino, Nicholas A. Teanby, Conor A. Nixon, Alexander E. Thelen, Claire E. Newman, Steven B. Charnley, Eliot F. Young

Martin A. Cordiner et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 5.

Observed zonal wind velocity profiles (v(l)) and 1σ error envelopes retrieved from our ALMA CH3CN observations on seven epochs, using a continuously variable parameterization with latitudinal sampling of 30°. These wind profiles are primarily sensitive to zonal winds in the altitude range 200–490 km. Ls values for each observation date are also shown in the legend. Vertical dashed lines indicate latitudes l = −60°, 0°, and 60°; dotted lines indicate l = −45° and −5° to indicate the latitudes plotted in Figure 6.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse