Atmospheric Turbulence in the Clouds of Venus

Main Authors: Peralta, Javier, Hueso, Ricardo, Sánchez-Lavega, Agustín
Format: Proceeding
Terbitan: Springer Netherlands , 2007
Subjects:
Online Access: https://zenodo.org/record/4532748
Daftar Isi:
  • Power spectra obtained from cloud brightness distribution in Galileo violet images are used as a proxy of the kinetic energy power spectra in order to study the atmospheric turbulence in Venus. Interpretation based on a review of predicted regimes from classical laws is made, in addition to comparing Venus results with the ones obtained in Earth.