Meridional Variations of C 2 H 2 in Jupiter's Stratosphere From Juno UVS Observations

@inproceedings{Giles2021MeridionalVO,
  title={Meridional Variations of C
 2
 H
 2
 in Jupiter's Stratosphere From Juno UVS Observations},
  author={Rohini S. Giles and Thomas K. Greathouse and Vincent Hue and G. Randall Gladstone and Henrik Melin and Leigh N. Fletcher and Patrick G. J. Irwin and Joshua A. Kammer and Maarten H. Versteeg and Bertrand Bonfond and Denis C. Grodent and Scott J. Bolton and Steven M. Levin},
  year={2021}
}
The UVS instrument on the Juno mission records far-ultraviolet reflected sunlight from Jupiter. These spectra are sensitive to the abundances of chemical species in the upper atmosphere and to the distribution of the stratospheric haze layer. We combine observations from the first 30 perijoves of the mission in order to study the meridional distribution of acetylene (C2H2) in Jupiter’s stratosphere. We find that the abundance of C2H2 decreases towards the poles by a factor of 2–4, in agreement… Expand

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References

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