Zobrazeno 1 - 10
of 11
pro vyhledávání: '"Candice L. Renaud"'
Publikováno v:
Icarus. 326:186-196
In a recent work on line shape parameters for the H2O-H2 [Renaud et al., Icarus, 306,275, 2018] it was shown that this far off-resonance collision system displays strong vibrational dependence. In Renaud et al., calculations were made for bands with
Autor:
V. Malathy Devi, Candice L. Renaud, D. Chris Benner, Mary Ann H. Smith, Bastien Vispoel, Robert L. Sams, Robert R. Gamache, Thomas A. Blake
Publikováno v:
Journal of Molecular Spectroscopy. 348:13-36
A Bruker IFS-120HR Fourier transform spectrometer located at the Pacific Northwest National Laboratory (PNNL) in Richland, Washington was used to record a series of spectra of pure H2O and air-broadened H2O in the regions of the ν1 and ν3 bands (34
Publikováno v:
Icarus. 306:275-284
Water can be detected throughout the universe: in comets, asteroids, dwarf planets, the inner and outer planets in our solar system, cool stars, brown dwarfs, and on many exoplanets. Here the focus is on locations rich in hydrogen gas. To properly st
Autor:
V. Malathy Devi, D. Chris Benner, Keeyoon Sung, Timothy J. Crawford, Robert R. Gamache, Candice L. Renaud, Mary Ann H. Smith, Arlan W. Mantz, Geronimo L. Villanueva
Publikováno v:
Journal of Quantitative Spectroscopy and Radiative Transfer. 203:158-174
Autor:
Arlan W. Mantz, Geronimo L. Villanueva, Keeyoon Sung, Robert R. Gamache, Mary Ann H. Smith, Timothy J. Crawford, V. Malathy Devi, D. Chris Benner, Candice L. Renaud
Publikováno v:
Journal of Quantitative Spectroscopy and Radiative Transfer. 203:133-157
Lorentz half-width coefficients and their temperature dependence exponents for CO2 broadening in the fundamental bands of HDO are important for reliable and accurate interpretation of Mars and Venus atmospheric data and to determine D/H. Uncertaintie
Autor:
Arlan W. Mantz, Keeyoon Sung, Robert R. Gamache, D. Chris Benner, Geronimo L. Villanueva, Candice L. Renaud, Mary Ann H. Smith, V. Malathy Devi, Timothy J. Crawford
Publikováno v:
Journal of Quantitative Spectroscopy and Radiative Transfer. 187:472-488
CO 2 -rich planetary atmospheres such as those of Mars and Venus require accurate knowledge of CO 2 broadened HDO half-width coefficients and their temperature dependence exponents for reliable abundance determination. Although a few calculated line
Publikováno v:
Journal of Molecular Spectroscopy. 326:144-150
A line list of transitions for seven isotopologues of water vapor in the 1100–4100 wavenumber range has been constructed for application to atmospheres rich in CO 2 . The quantum transitions for H 2 16 O, H 2 18 O, H 2 17 O, HD 16 O, HD 18 O, and H
Autor:
V. Malathy Devi, Candice L. Renaud, Robert R. Gamache, Mary Ann H. Smith, Bastien Vispoel, D. Chris Benner, Robert L. Sams, Thomas A. Blake
Publikováno v:
Proceedings of the 72nd International Symposium on Molecular Spectroscopy.
Autor:
Arlan W. Mantz, Candice L. Renaud, Timothy J. Crawford, Keeyoon Sung, V. Malathy Devi, Mary Ann H. Smith, Geronimo L. Villanueva, D. Chris Benner, Robert R. Gamache
Publikováno v:
Proceedings of the 71st International Symposium on Molecular Spectroscopy.
RRG and CLR were supported by the National Science Foundation through Grant \# AGS-1156862.
Autor:
Candice L. Renaud, Robert R. Gamache
Publikováno v:
Journal of Physics: Conference Series. 810:012032
Line shape parameters for hydrogen broadening of water vapor are needed to understand remote sensing measurements of planetary and exoplanet atmospheres. In order to address these needs, semiclassical calculations based on the Modified Complex Robert