Shalygina, O. S.; Petrova, E. V.; Markiewicz, W. J.; Ignatiev, N. I.; Shalygin, E. V.: Optical properties of the Venus upper clouds from the data obtained by Venus Monitoring Camera on-board the Venus Express. Planetary and Space Science 113, pp. 135 - 158 (2015)
Basilevsky, A. T.; Shalygin, E. V.; Titov, D. V.; Markiewicz, W. J.; Scholten, F.; Roatsch, T.; Kreslavsky, M. A.; Moroz, L. V.; Ignatiev, N. I.; Fietheh, B.et al.; Osterlohh, B.; Michalikh, H.: Geologic interpretation of the near-infrared images of the surface taken by the Venus Monitoring Camera, Venus Express. Icarus 217 (2), pp. 434 - 450 (2012)
Cottini, V.; Ignatiev, N. I.; Piccioni, G.; Drossart, P.; Grassi, D.; Markiewicz, W. J.: Water vapor near the cloud tops of Venus from Venus Express/VIRTIS dayside data. Icarus 217, pp. 561 - 569 (2012)
Ignatiev, N. I.; Titov, D. V.; Piccioni, G.; Drossart, P.; Markiewicz, W. J.; Cottini, V.; Roatsch, T.; Almeida, M.; Manoel, N.: Altimetry of the Venus cloud tops from the Venus Express observations. Journal Geophysical Research 114, E00B43 (2009)
Titov, D. V.; Taylor, F. W.; Svedhem, H.; Ignatiev, N. I.; Markiewicz, W. J.; Piccioni, G.; Drossart, P.: Atmospheric structure and dynamics as the cause of ultraviolet markings in the clouds of Venus. Nature 456 (7222), pp. 620 - 623 (2008)
Khatuntsev, I.; Limaye, S.; Ignatiev, N. I.; Markiewicz, W.; Patsaeva, M.; Turin, A.; Titov, D. V.: Upper cloud motions from the Venus Monitoring Camera imaging onboard Venus Express in period from 2006 to 2014. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Khatuntsev, I. V.; Patsaeva, M. V.; Ignatiev, N. I.; Titov, D. V.; Markiewicz, W. J.; Limaye, S. S.; Turin, A. V.: Variations of the zonal flow at Venus cloud tops from VMC/VEX UV images in period from 2006 to 2014. European Planetary Science Congress, Cascais, Portugal (2014)
Patsaeva, M.; Ignatiev, N. I.; Markiewicz, W. J.; Khatuntsev, I.; Titov, D. V.; Patsaev, D.: Mesoscale circulation at the upper cloud level at middle latitudes from the imaging by Venus Monitoring Camera onboard Venus Express. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Patsaeva, M.; Khatuntsev, I.; Patsaev, D.; Titov, D.; Ignatiev, N. I.; Markiewicz, W. J.; Rodin, A.: Correlation of the cloud top wind pattern with cloud morphology at the upper cloud level of Venus at 25S-75S from VMC/Venus Express. European Planetary Science Congress, Cascais, Portugal (2014)
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