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Detection of Carbon Monoxide’s 4.6 Micron Fundamental Band Structure in WASP-39b’s Atmosphere with JWST NIRSpec G395H
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From Solar System to Exoplanets: What can we learn from Planetary Spectroscopy?
J. I. Moses, T. Cavalié, L. N. Fletcher and M. T. Roman Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 378(2187) 20190477 (2020) https://doi.org/10.1098/rsta.2019.0477
Radiolysis of Ices by Cosmic-Rays: CH4 and H2O Ices Mixtures Irradiated by 40 MeV 58Ni11+ Ions
Scientific rationale for Uranus and Neptune in situ explorations
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Room temperature self- and H2-broadened line parameters of carbon monoxide in the first overtone band: Theoretical and revised experimental results
Koorosh Esteki, Adriana Predoi-Cross, Chad Povey, et al. Journal of Quantitative Spectroscopy and Radiative Transfer 203 309 (2017) https://doi.org/10.1016/j.jqsrt.2017.04.008
The Delivery of Water to Protoplanets, Planets and Satellites
O. Grasset, J. Castillo-Rogez, T. Guillot, L. N. Fletcher and F. Tosi Space Sciences Series of ISSI, The Delivery of Water to Protoplanets, Planets and Satellites 64 191 (2017) https://doi.org/10.1007/978-94-024-1628-2_6
THE EFFECT OF CARBON MONOXIDE ON PLANETARY HAZE FORMATION
Mid-infrared spectroscopy of Uranus from the Spitzer infrared spectrometer: 2. Determination of the mean composition of the upper troposphere and stratosphere
Electrifying Atmospheres: Charging, Ionisation and Lightning in the Solar System and Beyond
Karen L. Aplin SpringerBriefs in Astronomy, Electrifying Atmospheres: Charging, Ionisation and Lightning in the Solar System and Beyond 45 (2013) https://doi.org/10.1007/978-94-007-6633-4_7
AN EXTERNAL ORIGIN FOR CARBON MONOXIDE ON URANUS FROM
HERSCHEL
/SPIRE?
Y. Yair, G. Fischer, F. Simões, N. Renno and P. Zarka Space Sciences Series of ISSI, Planetary Atmospheric Electricity 30 29 (2008) https://doi.org/10.1007/978-0-387-87664-1_4
Commission 16: Physical Study of Planets and Satellites
Guy J. Consolmagno, Régis Courtin, C. Blanco, et al. Proceedings of the International Astronomical Union 1(T26A) 143 (2005) https://doi.org/10.1017/S174392130600442X
Improved constraints on Neptune's atmosphere from
submillimetre-wavelength observations