[1] The winter polar vortex on Saturn’s largest moon Titan has profound effects on atmospheric circulation and chemistry and for the current northern midwinter season is the major dynamical feature of Titan’s stratosphere and mesosphere. We use 2 years of observations from Cassini’s composite infrar...

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113
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.659.8403
http://www.astro.umd.edu/%7Enixon/papers-pdf/teanby-08b-vortex.pdf
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spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.659.8403 2023-05-15T17:39:58+02:00 The Pennsylvania State University CiteSeerX Archives application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.659.8403 http://www.astro.umd.edu/%7Enixon/papers-pdf/teanby-08b-vortex.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.659.8403 http://www.astro.umd.edu/%7Enixon/papers-pdf/teanby-08b-vortex.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://www.astro.umd.edu/%7Enixon/papers-pdf/teanby-08b-vortex.pdf Citation Teanby N. A et al. (2008 Titan’s winter polar vortex structure revealed by chemical tracers J. Geophys. Res 113 text ftciteseerx 2016-01-08T16:47:22Z [1] The winter polar vortex on Saturn’s largest moon Titan has profound effects on atmospheric circulation and chemistry and for the current northern midwinter season is the major dynamical feature of Titan’s stratosphere and mesosphere. We use 2 years of observations from Cassini’s composite infrared spectrometer to determine cross sections of five independent chemical tracers (HCN, HC3N, C2H2, C3H4, and C4H2), which are then used to probe dynamical processes occurring within the vortex. Our results provide compelling evidence that the vortex acts as a strong mixing barrier in the stratosphere and mesosphere, effectively separating a tracer-enriched air mass in the north from air at lower latitudes. In the mesosphere, above the level of the vortex jet, a tracer-depleted zone extends away from the north pole toward the equator and enrichment is confined to high northern latitudes. However, below this level, mixing processes cause tongues of gas to extend away from the polar region toward the equator. These features are not reproduced by current general circulation models and suggest that a residual polar circulation is present and that waves and instabilities form a more important part of Titan’s atmospheric dynamics than previously thought. We also observe an unexpected enrichment of C4H2 in the northern stratosphere, which suggests photochemical polymerization of C2H2. Our observations provide stringent new constraints for dynamical and photochemical models and identify key polar processes for the first time. Some of the processes we see have analogues in Earth’s polar vortex, while others are unique to Titan. Text North Pole Unknown Midwinter ENVELOPE(139.931,139.931,-66.690,-66.690) North Pole
institution Open Polar
collection Unknown
op_collection_id ftciteseerx
language English
topic Citation
Teanby
N. A
et al. (2008
Titan’s winter polar vortex structure revealed by chemical tracers
J. Geophys. Res
113
spellingShingle Citation
Teanby
N. A
et al. (2008
Titan’s winter polar vortex structure revealed by chemical tracers
J. Geophys. Res
113
topic_facet Citation
Teanby
N. A
et al. (2008
Titan’s winter polar vortex structure revealed by chemical tracers
J. Geophys. Res
113
description [1] The winter polar vortex on Saturn’s largest moon Titan has profound effects on atmospheric circulation and chemistry and for the current northern midwinter season is the major dynamical feature of Titan’s stratosphere and mesosphere. We use 2 years of observations from Cassini’s composite infrared spectrometer to determine cross sections of five independent chemical tracers (HCN, HC3N, C2H2, C3H4, and C4H2), which are then used to probe dynamical processes occurring within the vortex. Our results provide compelling evidence that the vortex acts as a strong mixing barrier in the stratosphere and mesosphere, effectively separating a tracer-enriched air mass in the north from air at lower latitudes. In the mesosphere, above the level of the vortex jet, a tracer-depleted zone extends away from the north pole toward the equator and enrichment is confined to high northern latitudes. However, below this level, mixing processes cause tongues of gas to extend away from the polar region toward the equator. These features are not reproduced by current general circulation models and suggest that a residual polar circulation is present and that waves and instabilities form a more important part of Titan’s atmospheric dynamics than previously thought. We also observe an unexpected enrichment of C4H2 in the northern stratosphere, which suggests photochemical polymerization of C2H2. Our observations provide stringent new constraints for dynamical and photochemical models and identify key polar processes for the first time. Some of the processes we see have analogues in Earth’s polar vortex, while others are unique to Titan.
author2 The Pennsylvania State University CiteSeerX Archives
format Text
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.659.8403
http://www.astro.umd.edu/%7Enixon/papers-pdf/teanby-08b-vortex.pdf
long_lat ENVELOPE(139.931,139.931,-66.690,-66.690)
geographic Midwinter
North Pole
geographic_facet Midwinter
North Pole
genre North Pole
genre_facet North Pole
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