Atmospheric waves and their possible effect on the thermal structure of Saturn's thermosphere
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Accepted version
Author(s)
Type
Journal Article
Abstract
Atmospheric waves have been discovered for the first time in Saturn's neutral upper atmosphere (thermosphere). Waves may be generated from instabilities, convective storms or other atmospheric phenomena. The inferred wave amplitudes change little with height within the sampled region, raising the possibility of the waves being damped, which in turn may enhance the eddy friction within the thermosphere. Using our Saturn Thermosphere Ionosphere General Circulation Model, we explore the parameter space of how an enhanced Rayleigh drag in different latitude regimes would affect the global circulation pattern within the thermosphere and, in turn, its global thermal structure. We find that Rayleigh drag of sufficient magnitude at midlatitudes may reduce the otherwise dominant Coriolis forces and enhance equatorward winds to transport energy from poles toward the equator, raising the temperatures there to observed values. Without this Rayleigh drag, energy supplied into the polar upper atmosphere by magnetosphere‐atmosphere coupling processes remains trapped at high latitudes and causes low‐latitude thermosphere temperatures to remain well below the observed levels. Our simulations thus suggest that giant planet upper atmosphere global circulation models need to include additional Rayleigh drag in order to capture the effects of physical processes otherwise not resolved by the codes.
Date Issued
2019-03-16
Date Acceptance
2019-02-22
Citation
Geophysical Research Letters, 2019, 46 (5), pp.2372-2380
ISSN
0094-8276
Publisher
American Geophysical Union (AGU)
Start Page
2372
End Page
2380
Journal / Book Title
Geophysical Research Letters
Volume
46
Issue
5
Copyright Statement
© 2019 American Geophysical Union. This is the accepted version of the following article: Müller‐Wodarg, I. C. F., Koskinen, T. T., Moore, L., Serigano, J., Yelle, R. V., Hörst, S. M., et al. ( 2019). Atmospheric waves and their possible effect on the thermal structure of Saturn's thermosphere. Geophysical Research Letters, 46, 2372– 2380., which has been published in final form at https://dx.doi.org/10.1029/2018gl081124
Subjects
MD Multidisciplinary
Meteorology & Atmospheric Sciences
Publication Status
Published
Date Publish Online
2019-03-11
