Collision-induced absorption coefficients of H2 pairs at temperatures from 60 K to 1000 K

By A. Borysow. 2002

211 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/415e2e1a46f5b0966881c8099208a2c40f8ff970

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Citations in the corpus

SPECTROSCOPIC EVIDENCE FOR A TEMPERATURE INVERSION IN THE DAYSIDE ATMOSPHERE OF HOT JUPITER WASP-33b (2015, background): “Our CIA opacities are obtained from Borysow et al. (1997) and Borysow (2002).”
HYDROGEN GREENHOUSE PLANETS BEYOND THE HABITABLE ZONE (2011, background): “Cooling from the escape of H at the exobase, the adiabatic upward motion of gas in the atmosphere to maintain steady-state, and the collision-induced opacity of H2 (Borysow et al. 1997; Borysow 2002) are included.”
C/O RATIO AS A DIMENSION FOR CHARACTERIZING EXOPLANETARY ATMOSPHERES (2012, methodology): “We obtain the H2-H2 collision-induced opacities from Borysow et al. (1997) and Borysow (2002).”
A CONSISTENT RETRIEVAL ANALYSIS OF 10 HOT JUPITERS OBSERVED IN TRANSMISSION (2016, background): “H2-H2 and H2-He collisioninduced absorption is taken from Borysow & Frommhold (1989); Borysow et al. (1989); Borysow & Frommhold (1990); Borysow et al. (1997) and Borysow (2002).”
TRANSMISSION SPECTRA OF THREE-DIMENSIONAL HOT JUPITER MODEL ATMOSPHERES (2009, background): “What limits the amplitude of these near IR features, which are predominantly due to water vapor absorption, is a strong contribution from H2 collision induced absorption (CIA) (e.g. Borysow 2002).”
The Evolution of L and T Dwarfs in Color-Magnitude Diagrams (2008, background): “…of the role of the K i and Na i resonance doublets at optical wavelengths (Burrows et al. 2000), (2) improved H2 CIA opacity (Borysow et al. 2001; Borysow 2002), (3) a new line list for TiO (Allard et al. 2000; Freedman et al. 2008), (4) improved modeling of the condensation chem- istry (Lodders…”
A Spitzer Infrared Spectrograph Spectral Sequence of M, L, and T Dwarfs (2004, background): “In particular, the suppression of the K-band is a result of collision-induced H2 1−0 dipole absorption (CIA H2) centered at 2.4 µm (Borysow 2002; Knapp et al. 2004) which is enhanced in such environments.”
ROTATION AND WINDS OF EXOPLANET HD 189733 b MEASURED WITH HIGH-DISPERSION TRANSMISSION SPECTROSCOPY (2015, methodology): “…spectrum of HD 189733 b was modeled by following the same prescriptions of Brogi et al. (2014) concerning the choice of line lists for CO and H 2 O (Rothman et al. 2010), CH 4 (Rothman et al. 2009), line profiles, and collisioninduced absorption by hydrogen (Borysow & Fu 2001; Borysow 2002).”
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).”
Detection of carbon monoxide in the high-resolution day-side spectrum of the exoplanet HD 189733b (2013, methodology): “The model spectra are the result of line-by-line calculations using a range of parameterised pressure-temperature structures (see below), H2-H2 collision-induced absorption (Borysow et al. 2001; Borysow 2002) and absorption from a single trace gas.”
A TEMPERATURE AND ABUNDANCE RETRIEVAL METHOD FOR EXOPLANET ATMOSPHERES (2009, background): “And, we obtain the H2-H2 collisioninduced opacities from Borysow et al. (1997), and Borysow (2002).”
A Possible Bifurcation in Atmospheres of Strongly Irradiated Stars and Planets (2003, background): “Opacity due to Collision–Induced Absorption (CIA) by H2 and helium is taken from Borysow and Frommhold (1990), Zheng and Borysow (1995), and Borysow, Jørgensen, and Zheng (1997), as updated in Borysow (2002).”
Low-Temperature Opacities (2005, background): “A detailed list of the references for the CIA opacities can be found in Allard et al. (2001) and Borysow (2002).”
Carbon monoxide and water vapor in the atmosphere of the non-transiting exoplanet HD 179949 b (2014, background): “The model spectra are the result of line-by-line calculations including H2H2 collision-induced absorption (Borysow & Fu 2001; Borysow 2002) and absorption from three trace gases, CO, H2O, and CH4, which are the dominant sources of opacities at these wavelengths (Madhusudhan 2012; Moses et al. 2013).”
An Infrared Spectroscopic Sequence of M, L, and T Dwarfs (2004, background): “The K-band flux in T dwarfs is further suppressed by collision-induced H2 absorption (Borysow 2002).”
Synthetic Spectra and Colors of Young Giant Planet Atmospheres: Effects of Initial Conditions and Atmospheric Metallicity (2008, background): “These include collisional induced absorption (CIA) by H2 molecules (Borysow 2002, where the opacity per unit volume is dependent on the square of the pressure), and Na and K, which have strongly pressure broadened optical absorption lines (Burrows et al. 2000; Allard et al. 2003).”
MID-INFRARED PHOTOMETRY OF COLD BROWN DWARFS: DIVERSITY IN AGE, MASS, AND METALLICITY (2010, background): “This may be due to the first overtone band of pressure-induced H2 becoming significant at J (Borysow 2002), or to the brightening of Y due to the weakening of the very broad 0.77 µm K I feature as K I condenses into KCl (Lodders 1999).”
Optimal estimation retrievals of the atmospheric structure and composition of HD 189733b from secondary eclipse spectroscopy (2011, background): “He and the coefficients are taken from Borysow et al. (1989), Borysow & Frommhold (1989), Borysow & Frommhold (1990), Zheng & Borysow (1995), Borysow et al. (1997), and Borysow (2002).”
Line and Mean Opacities for Ultracool Dwarfs and Extrasolar Planets (2007, methodology): “Our source for the subroutines to calculate the collision-induced absorption comes from the recent work of A. Borysow and her collaborators (Borysow 1991, 1992, 2002; Borysow et al. 1985, 1997, 2000; Birnbaum et al. 1996; Zheng & Borysow 1995; Borysow & Frommhold 1990).”