remote sesning Archives - Astrobiology

Left: Assumed temperature/pressure structure of the Venus atmosphere. Centre: The concentrations of condensed units ncond/n that deposit and are removed from the model when advancing to the next atmospheric height. Right: Element abundances with respect to oxygen ϵk/ϵO remaining in the gas phase. -- astro-ph.EP

Astrogeology, Atmospheres, Climate, Weather, Biogeochemical Cycles & Geobiology, Biosignatures & Paleobiology, Exoplanets, -moons, -comets, Imaging & Spectroscopy, Status Report, Venus

Prediction Of Sulphate Hazes In The Lower Venus Atmosphere

by Keith CowingAugust 30, 2025August 30, 2025

We study the amount, size distribution and material composition of (sub-)mic aerosol particles in the lower Venus atmosphere < 50 km.