More than three decades have passed since the publication of the last review of the Venus
clouds and hazes. The paper published in 1983 in the Venus book summarized the …

Both heliophysics and planetary physics seek to understand the complex nature of the solar
wind's interaction with solar system obstacles like Earth's magnetosphere, the ionospheres …

Venus Express is the first European mission to planet Venus. The mission aims at a
comprehensive investigation of Venus atmosphere and plasma environment and will …

The Venus Express mission is scheduled for launch in 2005. Among many other
instruments, it carries a magnetometer to investigate the Venus plasma environment …

Six years of continuous monitoring of Venus by European Space Agency's Venus Express
orbiter provides an opportunity to study dynamics of the atmosphere our neighbor planet …

The Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) on board the ESA/Venus
Express mission has technical specifications well suited for many science objectives of …

Simultaneous observations of Venus by Visible and Infrared Thermal Imaging Spectrometer
and Venus Monitoring Camera onboard the Venus Express spacecraft are used to map the …

Using over 6 years of magnetic field data (October 2014–December 2020) collected by the
Mars Atmosphere and Volatile EvolutioN, we conduct a statistical study on the three …

Vertical distributions of the molecular density and mixing ratios of H2O and HDO in the
Venus mesosphere have been obtained using Solar Occultation at Infrared (SOIR), a high …

Since the discovery of ultraviolet markings on Venus, their observations have been a
powerful tool to study the morphology, motions and dynamical state at the cloud top level …