Published May 8, 2020
| Version v1
Dataset
Open
Dataset S1 of "A long-lived sharp disruption on the lower clouds of Venus"
Authors/Creators
-
Peralta, J.1
- Navarro, T.2
- Vun, C. W.1
- Sánchez-Lavega, A.3
- McGouldrick, K.4
- Horinouchi, T.5
- Imamura, T.6
- Hueso, R.3
- Boyd, J. P.7
- Schubert, G.2
- Kouyama, T.8
- Satoh, T.1
- Iwagami, N.9
- Young, E. F.10
- Bullock, M. A.10
- Machado, P.11
- Lee, Y. J.12
- Limaye, S. S.13
- Nakamura, M.1
- Tellmann, S.14
- Wesley, A.15
- Miles, P.16
- 1. ISAS (JAXA)
- 2. University of California
- 3. UPV/EHU
- 4. University of Colorado Boulder
- 5. Hokkaido University
- 6. The University of Tokyo
- 7. University of Michigan College of Engineering
- 8. National Institute of Advanced Industrial Science and Technology
- 9. Tokyo, Japan
- 10. Southwest Research Institute, Boulder
- 11. Institute of Astrophysics and Space Sciences, Portugal
- 12. Technische Universität Berlin,
- 13. University of Wisconsin
- 14. Universität zu Köln
- 15. Astronomical Society of Australia
- 16. Gemeye Observatory
Description
Simulation with the IPSL Venus GCM. This compressed zip file accompanying the article "A long-lived sharp disruption on the lower clouds of Venus" (DOI: 10.1029/2020GL087221) holds a NetCDF file with a README file describing its structure. The NetCDF file contains the IPSL GCM simulation of the Venus atmosphere for the case of a relaxed zonal wind profile (see subsection 2.4 in main article). Computations were performed on a grid of \(altitude\times latitude\times longitude\) with \(50\times 97\times 96\) elements and along 40 time steps covering 23 Earth days.
Calculated physical parameters include:
- Atmospheric pressure (Pa).
- Vertical Wind (m s-1) [positive downward].
- Air Temperature (K).
- Zonal Wind (m s-1) [positive westward].
- Solar radiance at top of the atmosphere (W m-2).
Notes
Files
IPSL_Venus_GCM_output.zip
Files
(220.6 MB)
| Name | Size | Download all |
|---|---|---|
|
md5:173c8752dadc1d2be2fe9b0036bef477
|
220.6 MB | Preview Download |