SO2, SO3, OCS, H2S, and other trace gases in the Venus mesosphere from SOIR on board Venus Express: Detection and upper limit profiles
- 1IASB - BIRA, Planetary Atmosphere, Brussels, Belgium (arnaud.mahieux@aeronomie.be)
- 2The University of Texas at Austin, Austin, Texas
- 3Université Catholique de Louvain, Louvain-la-Neuve, Belgium
- 4Space Science Institute, Boulder, Colorado
- 5The Australian National University, Canberra, ACT, Australia
- 6Japanese Space Agency, Tokyo, Japan
We report the detection of SO2, SO3, H2S, and OCS above the cloud deck using the SOIR instrument on-board Venus Express, and upper limit profiles of HOCl, CS, and CS2.
The SOIR instrument performs solar occultation measurements in the IR region (2.2 - 4.3 µm) at a resolution of 0.12 cm-1, the highest of all instruments on board Venus Express. It combines an echelle spectrometer and an AOTF (Acousto-Optical Tunable Filter) for the order selection. SOIR performed more than 1500 solar occultation measurements leading to about two millions spectra.
The wavelength range probed by SOIR allows a detailed chemical inventory of the Venus atmosphere at the terminator in the mesosphere, with an emphasis on vertical distribution of the gases.
In this work, we report detections in the mesosphere, between 60 and 100 km.
Implications for the mesospheric chemistry will also be addressed.
How to cite: Mahieux, A., Robert, S., Mills, F., Trompet, L., Aoki, S., Piccialli, A., Jessup, K. L., and Vandaele, A. C.: SO2, SO3, OCS, H2S, and other trace gases in the Venus mesosphere from SOIR on board Venus Express: Detection and upper limit profiles, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-2004, https://doi.org/10.5194/egusphere-egu22-2004, 2022.
