2019
DOI: 10.1029/2018gl081124
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Atmospheric Waves and Their Possible Effect on the Thermal Structure of Saturn's Thermosphere

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 … Show more

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Cited by 35 publications
(51 citation statements)
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“…1a). The profiles marked "model" are the Pedersen conductivities based on the GCM 24 and are shown for reference. www.nature.com/scientificreports www.nature.com/scientificreports/ time between orbits is nearly constant, ≈6.5 days).…”
Section: Resultsmentioning
confidence: 99%
“…1a). The profiles marked "model" are the Pedersen conductivities based on the GCM 24 and are shown for reference. www.nature.com/scientificreports www.nature.com/scientificreports/ time between orbits is nearly constant, ≈6.5 days).…”
Section: Resultsmentioning
confidence: 99%
“…In actuality, Jupiter's magnetic field is tilted with respect to its rotation axis and has very complex structure (e.g., Connerney et al, 2018). The next step in the development of the presented model is to include a more realistic magnetic field model (e.g., Connerney et al, 2018) including realistic mapping from the magnetosphere to the ionosphere and LT variation, a more detailed ionosphere model (e.g., Blelly et al, 2019), and parameterizations allowing for the incorporation of atmospheric waves (e.g., Tao et al, 2009;Müller-Wodarg et al, 2019). Such a complex asymmetric interaction region would lead to different neutral flow and heating structures which cannot be simulated with the current model setup.…”
Section: Discussionmentioning
confidence: 99%
“…The JIM and JTGCM models, while not self-consistently coupling the atmosphere and magnetosphere, do employ more realistic magnetic field models at the planet, which is one of the main reasons that their findings are different from those presented above. The next step in the development of the presented model is to include a more realistic magnetic field model (e.g., Connerney et al, 2018) including realistic mapping from the magnetosphere to the ionosphere and LT variation, a more detailed ionosphere model (e.g., Blelly et al, 2019), and parameterizations allowing for the incorporation of atmospheric waves (e.g., Tao et al, 2009;Müller-Wodarg et al, 2019). This model will be the most realistic three-dimensional representation of Jupiter's coupled magnetosphere-atmosphere system.…”
Section: Discussionmentioning
confidence: 99%
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