MOSIR Project

IVC2019_09-4: Modeling of Observations of the OH Nightglow in the Venusian Mesosphere

IVC2019_09-5: Studying the polarization in CO2 absorption bands of Venus atmosphere

IVC2019_09-6: Variations of lower clouds and water vapor amount in deep Venus atmosphere based on night windows observations by the SPICAV-IR/Venus-Express

IVC2019_09-7: Retrieval of upper haze aerosol properties from SPICAV-UV and -IR data

IVC2019_10-1: Organization of the convection in the Venusian cloud layer

IVC2019_10-2: Comparison of horizontal distributions of temperature and UV absorbers at the Venus cloud-tops

IVC2019_10-3: Towards a (GCM-based) Venus Climate Database

IVC2019_10-4: Numerical modeling of the Venus atmosphere

IVC2019_10-5: Investigations below the clouds of Venus with the IPSL Venus GCM

IVC2019_11-1: Detection of large stationary gravity waves over ten Venusian solar days seen in LIR images

IVC2019_11-2: A new mesoscale model for Venus' atmosphere and its application to the bow-shaped structures discovered by Akatsuki

IVC2019_11-3: Venus atmosphere dynamics revealed by cloud tracking using images from Akatsuki

IVC2019_11-4: Akatsuki (cloud-tracking) and TNG/HARPS-N (Doppler velocimetry) coordinated wind measurements of cloud top Venus atmosphere.

IVC2019_11-5: Meridional and Zonal winds at Venus atmosphere from Cloud tracking, Doppler techniques and comparison with modelling

IVC2019_12-2: Understanding the Impact of Waves on Venus' Upper Atmosphere through General Circulation Model Simulations

IVC2019_12-3: The Venus Ionosphere as seen by the Akatsuki Radio Science Experiment

IVC2019_12-4: Upper atmosphere of Venus and impact from solar wind plasma: What we have learned from Venus Express

IVC2019_12-5: Circulation of Venusian atmosphere at 90-110 km based on apparent motions of the O2 1.27 um nightglow from VIRTIS-M (Venus Express) data

IVC2019_12-6: An Investigation of the Solar Wind Influence on the Venus Upper Atmosphere Structure and Dynamics

IVC2019_12-7: H+/O+ escape rates in the Venusian magnetotail and their dependence on upstream conditions