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).

J.P. acknowledges JAXA's International Top Young Fellowship. T.N. and G.S. thank NASA's Grant NNX16AC84G. A.S.-L. and R.H. were supported by Spanish project AYA2015-65041-P (MINECO/FEDER, UE) and Grupos Gobierno Vasco IT-765-13. N.I. thanks partial support by JSPS KAKENHI Grant JP16H02225. Y.J.L. received funding from EU H2020 MSCA-IF No.841432. P.M. acknowledges FCT's project P-TUGA PTDC/FISAST/29942/2017. S.S.L. thanks NASA's Grant NNX16AC79G. All authors acknowledge the hard work done by the Akatsuki team.