no code implementations • 21 Jan 2021 • Paul B. Rimmer, Sean Jordan, Tereza Constantinou, Peter Woitke, Oliver Shorttle, Richard Hobbs, Alessia Paschodimas
The depletion of SO$_2$ and H$_2$O in and above the clouds of Venus (45 -- 65 km) cannot be explained by known gas-phase chemistry and the observed composition of the atmosphere.
Earth and Planetary Astrophysics
no code implementations • 22 Dec 2020 • Patrick Barth, Christiane Helling, Eva E. Stüeken, Vincent Bourrier, Nathan Mayne, Paul B. Rimmer, Moira Jardine, Aline A. Vidotto, Peter J. Wheatley, Rim Fares
Hot Jupiters provide valuable natural laboratories for studying potential contributions of high-energy radiation to prebiotic synthesis in the atmospheres of exoplanets.
Earth and Planetary Astrophysics High Energy Astrophysical Phenomena Solar and Stellar Astrophysics Chemical Physics
no code implementations • 10 Dec 2020 • Jane S. Greaves, William Bains, Janusz J. Petkowski, Sara Seager, Clara Sousa-Silva, Sukrit Ranjan, David L. Clements, Paul B. Rimmer, Helen J. Fraser, Steve Mairs, Malcolm J. Currie
Using the JCMT PH3-discovery data, we show that mathematically-correct polynomial fitting of periodic ripples does not lead to "fake lines" (probability < ~1%).
Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics
2 code implementations • 1 Jul 2016 • Shang-Min Tsai, James R. Lyons, Luc Grosheintz, Paul B. Rimmer, Daniel Kitzmann, Kevin Heng
It is constructed for gaseous chemistry from 500 to 2500 K using a reduced C-H-O chemical network with about 300 reactions.
Earth and Planetary Astrophysics
