Note to: Titan's Atmosphere in Late Southern Spring Observed with Adaptive Optics on the W.M. Keck II 10-meter Telescope
Using adaptive optics on the W.M. Keck II telescope we imaged Titan several times during 1999 to 2001 in narrowband near-infrared filters selected to probe Titan's stratosphere and upper troposphere. We observed a bright feature around the south pole, possibly a collar of haze or clouds. Furthe...
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ftcern:oai:cds.cern.ch:534655 2023-05-15T18:22:07+02:00 Note to: Titan's Atmosphere in Late Southern Spring Observed with Adaptive Optics on the W.M. Keck II 10-meter Telescope Roe, H G De Pater, I MacIntosh, B A Gibbard, S G Max, C E McKay, C P 2002-01-15 http://cds.cern.ch/record/534655 eng eng http://cds.cern.ch/record/534655 astro-ph/0201231 oai:cds.cern.ch:534655 Astrophysics and Astronomy 2002 ftcern 2018-07-28T05:18:35Z Using adaptive optics on the W.M. Keck II telescope we imaged Titan several times during 1999 to 2001 in narrowband near-infrared filters selected to probe Titan's stratosphere and upper troposphere. We observed a bright feature around the south pole, possibly a collar of haze or clouds. Further, we find that solar phase angle explains most of the observed east-west brightness asymmetry of Titan's atmosphere, although the data do not preclude the presence of a `morning fog' effect at small solar phase angle. Other/Unknown Material South pole CERN Document Server (CDS) South Pole |
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CERN Document Server (CDS) |
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English |
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Astrophysics and Astronomy |
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Astrophysics and Astronomy Roe, H G De Pater, I MacIntosh, B A Gibbard, S G Max, C E McKay, C P Note to: Titan's Atmosphere in Late Southern Spring Observed with Adaptive Optics on the W.M. Keck II 10-meter Telescope |
topic_facet |
Astrophysics and Astronomy |
description |
Using adaptive optics on the W.M. Keck II telescope we imaged Titan several times during 1999 to 2001 in narrowband near-infrared filters selected to probe Titan's stratosphere and upper troposphere. We observed a bright feature around the south pole, possibly a collar of haze or clouds. Further, we find that solar phase angle explains most of the observed east-west brightness asymmetry of Titan's atmosphere, although the data do not preclude the presence of a `morning fog' effect at small solar phase angle. |
author |
Roe, H G De Pater, I MacIntosh, B A Gibbard, S G Max, C E McKay, C P |
author_facet |
Roe, H G De Pater, I MacIntosh, B A Gibbard, S G Max, C E McKay, C P |
author_sort |
Roe, H G |
title |
Note to: Titan's Atmosphere in Late Southern Spring Observed with Adaptive Optics on the W.M. Keck II 10-meter Telescope |
title_short |
Note to: Titan's Atmosphere in Late Southern Spring Observed with Adaptive Optics on the W.M. Keck II 10-meter Telescope |
title_full |
Note to: Titan's Atmosphere in Late Southern Spring Observed with Adaptive Optics on the W.M. Keck II 10-meter Telescope |
title_fullStr |
Note to: Titan's Atmosphere in Late Southern Spring Observed with Adaptive Optics on the W.M. Keck II 10-meter Telescope |
title_full_unstemmed |
Note to: Titan's Atmosphere in Late Southern Spring Observed with Adaptive Optics on the W.M. Keck II 10-meter Telescope |
title_sort |
note to: titan's atmosphere in late southern spring observed with adaptive optics on the w.m. keck ii 10-meter telescope |
publishDate |
2002 |
url |
http://cds.cern.ch/record/534655 |
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South Pole |
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South Pole |
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South pole |
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South pole |
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http://cds.cern.ch/record/534655 astro-ph/0201231 oai:cds.cern.ch:534655 |
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1766201476128964608 |