MOSIR Project

IVC2019_07-2: Climate control on Venus: Connections among clouds, UV absorber, surface chemical reaction, and atmospheric circulation

IVC2019_07-3: Maintenances of Venusian Sulfuric Acid Clouds due to Chemistry and Dynamics Simulated by a General Circulation Model

IVC2019_07-4: Modeling the Distribution of Sulfur Species in the Atmosphere of Venus

IVC2019_07-5: Puzzling Cloud Cover of Venus

IVC2019_07-6: Spectral Properties of Unusual Nightside Cloud Features on Venus

IVC2019_09-1: A fully coupled photochemical-condensation model of the Venus atmosphere from the ground to 110 km

IVC2019_09-2: The Dust Cycle on Venus

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.