New section of the HITRAN database: Collision-induced absorption (CIA)

By C. Richard, I. Gordon, L. Rothman, M. Abel, L. Frommhold, M. Gustafsson, J. Hartmann, C. Hermans, W. J. Lafferty, G. Orton and 2 more. 2012

305 citations recorded by the source corpus.

Subfields: Atmospheric Science, Atomic and Molecular Physics, and Optics, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/7ba52892eec1af5b9f8b392dcb2ade948bda3949

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Atmospheric Science

1. M. Marley
2. Jon Fortney
3. R. Freedman
4. D. Saumon
5. T. Robinson
6. C. Morley
7. K. Lodders
8. C. Visscher

In Atomic and Molecular Physics, and Optics

1. M. Marley
2. Jon Fortney
3. R. Freedman
4. D. Saumon
5. C. Visscher
6. T. Robinson
7. C. Morley
8. K. Zahnle

In Spectroscopy

1. N. Madhusudhan
2. M. Marley
3. D. Saumon
4. Arazi Pinhas
5. J. Lustig-Yaeger
6. Jon Fortney
7. S. Leggett
8. R. Lupu

Citations in the corpus

• Update of the HITRAN collision-induced absorption section (2019, unknown): “Remaining de fi ciencies described in the Richard et al. (2012) paper have inspired many new laboratory measurements and theoretical calculations.”
• Transient reducing greenhouse warming on early Mars (2016, unknown): “H 2 and N 2 – CH 4 CIA data [ Borysow and Frommhold , 1986; Borysow and Tang , 1993; Richard et al. , 2012].”
• HD 209458b in new light: evidence of nitrogen chemistry, patchy clouds and sub-solar water (2017, methodology): “For collisionally-induced absorption, we consider H2 −H2 and H2 −He absorption from the HITRAN database (Richard et al. 2012).”
• Modeling climate diversity, tidal dynamics and the fate of volatiles on TRAPPIST-1 planets (2017, background): “…& Hartmann 1989; Campargue et al. 2012), Collision Induced Absorptions (Gruszka & Borysow 1997; Baranov et al. 2004; Wordsworth et al. 2010a; Richard et al. 2012) and various other continua (Gruszka & Borysow 1997; Clough et al. 2005; Richard et al. 2012) were properly included in the…”
• NEGLECTED CLOUDS IN T AND Y DWARF ATMOSPHERES (2012, background): “Recent work by Saumon et al. (2012) has modeled a range of brown dwarfs using improved line lists for ammonia from Yurchenko et al. (2011) and an improved treatment of the pressure-induced opacity of H2 collisions from Richard et al. (2012).”
• Observing the Atmospheres of Known Temperate Earth-sized Planets with JWST (2017, background): “…molecule pairs including N2–N2, O2–O2, CO2–CO2, and N2–CH4 (Bezard et al. 1990; Borysow & Tang 1993; Lafferty et al. 1996; Gruszka & Borysow 1997; Baranov et al. 2004; Wordsworth et al. 2010; Lee et al. 2016; Hartmann et al. 2017), as well as hydrogen and helium CIA opacities (Richard et al. 2012).”
• Exoplanetary Atmospheres: Key Insights, Challenges, and Prospects (2019, background): “For example, recent line lists are now available for various species including H2O (10, 221), CO (221, 147), CO2 (221, 108, 109), CH4 (284, 285), NH3 (283), HCN (100, 11), collisioninduced-absorption (215) and AlO (203).”
• GASEOUS MEAN OPACITIES FOR GIANT PLANET AND ULTRACOOL DWARF ATMOSPHERES OVER A RANGE OF METALLICITIES AND TEMPERATURES (2014, methodology): “For H2 CIA we use Richard et al. (2012) in place of previous work by Borysow (2002).”
• H2O abundances and cloud properties in ten hot giant exoplanets (2018, methodology): “The CIA data are sourced from the HITRAN archive (Richard et al. 2012).”
• The habitability of Proxima Centauri b II. Possible climates and Observability (2016, methodology): “The GCM includes an up-to-date generalized radiative transfer (Rothman et al. 2009; Wordsworth et al. 2010; Richard et al. 2012) for variable gaseous atmospheric compositions made of various cocktails of CO2, N2 and H2O, using the correlated-k method (Fu & Liou 1992; Eymet et al. 2016).”
• QUANTITATIVELY ASSESSING THE ROLE OF CLOUDS IN THE TRANSMISSION SPECTRUM OF GJ 1214b (2013, background): “This opacity database includes two significant updates since Freedman et al. (2008), which are described in Saumon et al. (2012): a new molecular line list for ammonia (Yurchenko et al. 2011) and an improved treatment of collision induced H2 absorption (Richard et al. 2012).”
• On the Cool Side: Modeling the Atmospheres of Brown Dwarfs and Giant Planets (2014, background): “A recent compendium can be found in Richard et al. (2012).”
• Mass–Metallicity Trends in Transiting Exoplanets from Atmospheric Abundances of H2O, Na, and K (2019, background): “…consider absorption due to H2O (Rothman et al. 2010), Na (Allard et al. 2019), K (Allard et al. 2016), CH4 (Yurchenko & Tennyson 2014), NH3 (Yurchenko et al. 2011), HCN (Barber et al. 2014), CO (Rothman et al. 2010), and H2-H2 and H2-He collision induced absorption (CIA; Richard et al. 2012).”
• Exoplanet Biosignatures: A Review of Remotely Detectable Signs of Life (2017, background): “At very high O2 concentrations, O2-O2 CIA (also referred to as O4) absorption occurs at 0.445, 0.475, 0.53, 0.57, and 0.63 mm (Hermans et al., 1999; Richard et al., 2012; Schwieterman et al., 2016).”