Cite this as (APA format)
Vandaele, A. C., Mahieux, A., Wilquet, V., Chamberlain, S., & Trompet, L. (2024). Venus atmospheric profiles - From SPICAV-SOIR on board VEx version w24.00 (Version w24.00) [Dataset]. Royal Belgian Institute for Space Aeronomy. https://doi.org/10.18758/71021090
Technical info
| Resource format | GZIP |
|---|---|
| Resource size | 47.7 MB |
Additional info
| Data last updated | April 25, 2024 |
|---|---|
| Metadata last updated | June 19, 2024 |
| Created | April 25, 2024 |
SOIR Data in VOtable format
VOtables (.xml files) for each molecule detected by SOIR and for each orbit where SOIR was operating.
The density "n_", logarithm of the density "log_n_" and volume mixing ratio "vmr_" are provided for different smoothing by a moving average with windows varying from +/-0.1 to +/- 1 scale height (by step of 0.1).
For species with only upper limits (H2S, HOCl, H2CO, O3, NH3, HCN, N2O, NO2, NO, HO2): the files contains three fields: altitude, upper limit and error.
The corresponding uncertainties on the vertical profiles are the variables starting with "err_"
The files also contains the vertical profile of pressure "p" and temperature "t". For aerosols, see the older version w23.00.
The data concerning the geometry of the measurements: solar longitude, and local time, latitude, longitude, and Julian date corresponding to the profile are also provided in the same files.