Dmitrij V. Titov

TL;DR: The JUpiter ICy moons Explorer (JUICE) mission as mentioned in this paper was selected by ESA in May 2012 to perform detailed investigations of Jupiter and its system in all their interrelations and complexity with particular emphasis on Ganymede as a planetary body and potential habitat.

TL;DR: A review of the current state of the art of the knowledge of the Venus cloud system can be found in this paper focusing mainly on the results acquired after the Venera, Pioneer Venus and Vega missions.

TL;DR: In this paper, the results of investigation of the cloud top morphology performed by the VMC during more than 3 years of the Venus Express mission are presented. But, the authors focus on the data from the ultraviolet channel, centered at the characteristic wavelength of the unknown UV absorber that yields the highest contrasts on the cloud-top.

TL;DR: A comprehensive review of the results of the atmospheric thermal structure and radiative balance since the earlier works published in Venus and Venus II books from recent spacecraft and Earth-based investigations can be found in this article.

TL;DR: In this article, the authors present the annual behavior of atmospheric water vapor on Mars, as observed by the OMEGA spectrometer on board Mars Express during its first martian year.