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HDO and SO 2 thermal mapping on Venus. III. Short-term and long-term variations between 2012 and 2016
- Source :
- Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 595, pp.A74. ⟨10.1051/0004-6361/201628999⟩, Astronomy and Astrophysics-A&A, 2016, 595, pp.A74. ⟨10.1051/0004-6361/201628999⟩
- Publication Year :
- 2016
- Publisher :
- HAL CCSD, 2016.
-
Abstract
- International audience; We present the analysis of a four-year observational campaign using the TEXES high-resolution imaging spectrometer at the NASA Infrared Telescope Facility to map sulfur dioxide and deuterated water over the disk of Venus. Data have been recorded in two spectral ranges around 1345 cm −1 (7.4 µm) and 530 cm −1 (19 µm) in order to probe the cloudtop at an altitude of about 64 km (SO 2 and HDO at 7.4 µm) and a few kilometers below (SO 2 at 19 µm). Observations took place during six runs between January 2012 and January 2016. The diameter of Venus ranged between 12 and 33 arcsec. Data were recorded with a spectral resolving power up to 80 000 and a spatial resolution of about 1 arcsec (at 7.4 µm) and 2.5 arcsec (at 19 µm). Mixing ratios were estimated from HDO/CO 2 and SO 2 /CO 2 line depth ratios, using weak neighboring transitions of comparable depths. The whole dataset demonstrates that the two molecules behave very differently to each other. The HDO maps are uniform over the disk. The disk-integrated H 2 O mixing ratio (estimated assuming a D/H of 200 VSMOW in the mesosphere of Venus) show moderate variations (by less than a factor of 2) over the four-year period. A value of 1.0−1.5 ppmv is obtained in most of the cases. The SO 2 maps, in contrast, show strong variations over the disk of Venus, by a factor as high as 5. Long-term variations of SO 2 show that the disk-integrated SO 2 mixing ratio also varies between 2012 and 2016 by a factor as high as ten, with a minimum value of 30 +/−5 ppbv on February 26, 2014 an a maximum value of 300 +/−50 ppbv on January 14, 2016. The SO 2 maps also show a strong short-term variability. It can be seen that the SO 2 maximum feature usually follows the four-day rotation of the clouds over a timescale of two hours, which corresponds to a rotation of 7.5 deg over the planetary disk, but its morphology also changes, which suggests that the lifetime of this structure is not more than a few hours.
- Subjects :
- 010504 meteorology & atmospheric sciences
Infrared telescope
Imaging spectrometer
Venus
Astrophysics
Rotation
01 natural sciences
planets and satellites: terrestrial planets
Altitude
0103 physical sciences
Mixing ratio
010303 astronomy & astrophysics
0105 earth and related environmental sciences
Line (formation)
Physics
planets and satellites: atmospheres
biology
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
planets and satellites: composition
Astronomy
Astronomy and Astrophysics
biology.organism_classification
Deuterium
13. Climate action
Space and Planetary Science
techniques: imaging spectroscopy
[SDU]Sciences of the Universe [physics]
Subjects
Details
- Language :
- English
- ISSN :
- 00046361
- Database :
- OpenAIRE
- Journal :
- Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 595, pp.A74. ⟨10.1051/0004-6361/201628999⟩, Astronomy and Astrophysics-A&A, 2016, 595, pp.A74. ⟨10.1051/0004-6361/201628999⟩
- Accession number :
- edsair.doi.dedup.....c1516f71fa70d40f1d6f5ba16e6aa913