Winds and cloud morphology in the southern polar region of Venus
Spinning on average 60 times faster than the surface, the atmosphere of Venus is superrotational, a state in which the averaged angular momentum is much greater than that corresponding to co-rotation with the solid globe. The rapid mean flow, which is main- tained by momentum transports in the deep...
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ftunivevora:oai:dspace.uevora.pt:10174/6911 2023-09-05T13:21:50+02:00 Winds and cloud morphology in the southern polar region of Venus Luz, David Berry, David L. Peralta, Javier Piccioni, Giuseppe Drossart, Pierre VIRTIS-Venus Express Team 2010 http://hdl.handle.net/10174/6911 http://meetings.copernicus.org/epsc2010/abstracts/EPSC2010-670.pdf eng eng European Planetary Science Congress 2010 http://meetings.copernicus.org/epsc2010/abstracts/EPSC2010-670.pdf http://hdl.handle.net/10174/6911 sim nao nd dberry@uevora.pt 343 openAccess Venus Planetary Atmospheres Venus Express VIRTIS lecture 2010 ftunivevora 2023-08-14T17:30:25Z Spinning on average 60 times faster than the surface, the atmosphere of Venus is superrotational, a state in which the averaged angular momentum is much greater than that corresponding to co-rotation with the solid globe. The rapid mean flow, which is main- tained by momentum transports in the deep atmo- sphere, presents a puzzle to the atmospheric and plan- etary sciences[1]. After previous missions revealed a bright polar feature at the north pole[9, 10], the Venus Express spacecraft discovered a fast-rotating counter- part at the southern polar region[6], which has been identified as a vortex[2]. The southern polar vortex can be observed at 5.0 μm as a bright, highly vari- able structure which is ∼ 15 K warmer than the sur- rounding air[6]. Although the Venus superrotation has been measured by tracking cloud features at UV and infrared wavelengths[7, 4, 8, 5], the winds in the po- lar region remain poorly constrained. Characterizing the zonal and meridional circulation in this region, as well as their variability, is crucial for understanding the mechanisms that maintain superrotation. In partic- ular, mean zonal winds are necessary to understand the nature of the polar vortex, how it is connected with the general circulation of the atmosphere, and to diagnose momentum transports. Winds at 45 and 65 km can be detected from cloud motion monitoring by the VIRTIS-M subsection on- board the Venus Express (VEX) spacecraft. Our ob- jective is to provide direct wind measurements at cloud tops and in the lower cloud level, in order to help in- terpret the VEX observations concerning the meso- spheric wind regime and temperature fields. In par- ticular, we present direct measurements of the zonal and meridional winds at both altitudes. For this work we selected nadir-pointing, high- spatial resolution VIRTIS data cubes obtained from apocenter in order to minimize the geometric distortion of the polar region. On average these contain lat- itudes extending from the pole to 70S. Since the VIR- TIS field of view is ... Lecture North Pole Repositório Científico da Universidade de Évora North Pole Ular ENVELOPE(140.951,140.951,72.498,72.498) Venus ENVELOPE(-57.842,-57.842,-61.925,-61.925) |
institution |
Open Polar |
collection |
Repositório Científico da Universidade de Évora |
op_collection_id |
ftunivevora |
language |
English |
topic |
Venus Planetary Atmospheres Venus Express VIRTIS |
spellingShingle |
Venus Planetary Atmospheres Venus Express VIRTIS Luz, David Berry, David L. Peralta, Javier Piccioni, Giuseppe Drossart, Pierre VIRTIS-Venus Express Team Winds and cloud morphology in the southern polar region of Venus |
topic_facet |
Venus Planetary Atmospheres Venus Express VIRTIS |
description |
Spinning on average 60 times faster than the surface, the atmosphere of Venus is superrotational, a state in which the averaged angular momentum is much greater than that corresponding to co-rotation with the solid globe. The rapid mean flow, which is main- tained by momentum transports in the deep atmo- sphere, presents a puzzle to the atmospheric and plan- etary sciences[1]. After previous missions revealed a bright polar feature at the north pole[9, 10], the Venus Express spacecraft discovered a fast-rotating counter- part at the southern polar region[6], which has been identified as a vortex[2]. The southern polar vortex can be observed at 5.0 μm as a bright, highly vari- able structure which is ∼ 15 K warmer than the sur- rounding air[6]. Although the Venus superrotation has been measured by tracking cloud features at UV and infrared wavelengths[7, 4, 8, 5], the winds in the po- lar region remain poorly constrained. Characterizing the zonal and meridional circulation in this region, as well as their variability, is crucial for understanding the mechanisms that maintain superrotation. In partic- ular, mean zonal winds are necessary to understand the nature of the polar vortex, how it is connected with the general circulation of the atmosphere, and to diagnose momentum transports. Winds at 45 and 65 km can be detected from cloud motion monitoring by the VIRTIS-M subsection on- board the Venus Express (VEX) spacecraft. Our ob- jective is to provide direct wind measurements at cloud tops and in the lower cloud level, in order to help in- terpret the VEX observations concerning the meso- spheric wind regime and temperature fields. In par- ticular, we present direct measurements of the zonal and meridional winds at both altitudes. For this work we selected nadir-pointing, high- spatial resolution VIRTIS data cubes obtained from apocenter in order to minimize the geometric distortion of the polar region. On average these contain lat- itudes extending from the pole to 70S. Since the VIR- TIS field of view is ... |
format |
Lecture |
author |
Luz, David Berry, David L. Peralta, Javier Piccioni, Giuseppe Drossart, Pierre VIRTIS-Venus Express Team |
author_facet |
Luz, David Berry, David L. Peralta, Javier Piccioni, Giuseppe Drossart, Pierre VIRTIS-Venus Express Team |
author_sort |
Luz, David |
title |
Winds and cloud morphology in the southern polar region of Venus |
title_short |
Winds and cloud morphology in the southern polar region of Venus |
title_full |
Winds and cloud morphology in the southern polar region of Venus |
title_fullStr |
Winds and cloud morphology in the southern polar region of Venus |
title_full_unstemmed |
Winds and cloud morphology in the southern polar region of Venus |
title_sort |
winds and cloud morphology in the southern polar region of venus |
publisher |
European Planetary Science Congress 2010 |
publishDate |
2010 |
url |
http://hdl.handle.net/10174/6911 http://meetings.copernicus.org/epsc2010/abstracts/EPSC2010-670.pdf |
long_lat |
ENVELOPE(140.951,140.951,72.498,72.498) ENVELOPE(-57.842,-57.842,-61.925,-61.925) |
geographic |
North Pole Ular Venus |
geographic_facet |
North Pole Ular Venus |
genre |
North Pole |
genre_facet |
North Pole |
op_relation |
http://meetings.copernicus.org/epsc2010/abstracts/EPSC2010-670.pdf http://hdl.handle.net/10174/6911 sim nao nd dberry@uevora.pt 343 |
op_rights |
openAccess |
_version_ |
1776202407162675200 |