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)
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
The MPS instruments on board ESA’s JUICE spacecraft have successfully completed their commissioning in space - and delivered their first observational data.
A collision nearly 30 years ago permanently changed Jupiter's atmospheric chemistry; the aftermath is still helping to better understand the gas giant.
The launch was successful; the ESA’s space probe JUICE is now on its way to the Jupiter system. There, it will primarily study the gas giant's icy moons.
ESA's space probe is on the move: First it heads for the launch site in Kourou - and in April it will begin its long journey to Jupiter and its icy moons.