MOSIR Project

Dynamical and thermodynamical structure in cloud layer simulated by a GCM with correlated-k distribution radiative transfer model

Chemical species in the Venus atmosphere calculated by a GCM with chemistry and cloud microphysics

Characteristics of Venusian gravity waves and thermal tides inferred from thermal infrared cloud images

A new dynamical core using radial basis functions

Hydraulic jumps and cloud formation on Mars

Mesoscale modelling of the Venus atmosphere: From the surface to the clouds

Evolution of small-scale cloud morphology

Variations of tropopause height and gravity waves in the Venusian polar atmosphere

One-dimensional Microphysics Model of Venusian Clouds from 40 to 100 km

Planetary-scale wave simulated in high-resolution Venus PCM

Kelvin wave at the top of cloud layer observed by AKATSUKI

Long-term monitoring of Venusian atmosphere by Akatsuki LIR - Focusing on thermal-tides: Periodic variation in diurnal-tide?

A study on the climatology of the Martian atmospheric general circulation and the role of unresolved waves using a reanalysis data

Cloud trains associated with mountain lee waves on Mars, 11 Mars Years observations

The VenSpec-U instrument onboard EnVision

The Venus Climate Database VCD version 2.3 (and 3.0)

Summary of AKATSUKI data and ALEDAS-V data

Long-term variations of temperature and H2SO4 gas mixing ratio by the Venus Express and Akatsuki radio occultation measurements

Intercomparison between Venus Thermospheric Models

Wave-driven cloud formation on Venus