5 papers
A Model of UV-Blue Absorbance in Bulk Liquid of Venusian Cloud Aerosols Is Consistent with Efficient Organic Absorbers at High Concentrations
Jan Spacek, Yeon J. Lee, Paul B. Rimmer +1
At visible wavelengths, Venus appears serene and pale-yellow, but since the 1920s, observers have noted high-contrast features in the ultraviolet. These features track the about 4-…
A Full-Atmosphere Model of Jupiter
AntonÃn KnÞek, Paul B. Rimmer, Martin Ferus
This paper presents a combined 1D photochemical-thermochemical kinetics model of Jupiter's deeper atmosphere, troposphere and stratosphere. The model covers atmospheric pressure ra…
Nitrogen chemistry of hycean worlds on the example of K2-18b
Maja W. Radecka, Paul B. Rimmer
A recent observation of the exoplanet K2-18b sparked interest among scientists - large amounts of carbon dioxide and methane were detected in an H2-rich background atmosphere. If t…
Shedding a Light on the Kinetics of the Carboxysulfitic Scenario
S. B. White, P. B. Rimmer, Z. Liu
One way in which we can attempt to relate chemical pathways to geochemical environments is by studying the kinetics of a given sequence of reactions and identifying the conditions…
Impact sculpting of the early martian atmosphere
Oliver Shorttle, Homa Saeidfirozeh, Paul Rimmer +4
Intense bombardment of solar system planets in the immediate aftermath of protoplanetary disk dissipation has played a key role in their atmospheric evolution. During this epoch, e…