Color and aerosol changes in Jupiter after a North Temperate Belt disturbance
Icarus Elsevier BV 352 (2020) 114031
The transit spectra of Earth and Jupiter
ICARUS 242 (2014) 172-187
Stormy water on Mars: the distribution and saturation of atmospheric water during the dusty season
Science American Association for the Advancement of Science (2020)
Abstract:
The loss of water from Mars to space is thought to result from the transport of water to the upper atmosphere, where it is dissociated to hydrogen and escapes the planet. Recent observations have suggested large, rapid seasonal intrusions of water into the upper atmosphere, boosting the hydrogen abundance. We use the Atmospheric Chemistry Suite on the ExoMars Trace Gas Orbiter to characterize the water distribution by altitude. Water profiles during the 2018–2019 southern spring and summer stormy seasons show that high-altitude water is preferentially supplied close to perihelion, and supersaturation occurs even when clouds are present. This implies that the potential for water to escape from Mars is higher than previously thought.Global Distribution and Seasonality of Martian Atmospheric HCl Explained Through Heterogeneous Chemistry
Geophysical Research Letters American Geophysical Union (AGU) 52:6 (2025)
LIRIS: demonstrating how small satellites can revolutionise lunar science data sets
Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 13546 (2025) 135460d-135460d-9