Spectroscopic database of CO2 line parameters: 4300–7000 cm−1
By R. Toth, L. Brown, C. Miller, V. Devi, D. Benner. 2008
165 citations recorded by the source corpus.
Subfields: Atmospheric Science, Global and Planetary Change, Spectroscopy
View Paper: https://www.semanticscholar.org/paper/7396aefd2a526d0a9a52cd534679b25b411bbe0a
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
- Jonathan Tennyson
- S. Tashkun
- A. Nikitin
- Y. Bénilan
- H. S. P. Müller
- Paul I. Palmer
- Liang Feng
- Paul O. Wennberg
In Global and Planetary Change
In Spectroscopy
- Jonathan Tennyson
- A. Nikitin
- S. Tashkun
- A. Campargue
- L. Brown
- Sergei N. Yurchenko
- H. S. P. Müller
- N. Madhusudhan
Citations in the corpus
- The 2009 edition of the GEISA spectroscopic database (2011, methodology): “Using Fourier transform spectroscopy experiments the first team has performed very precise measurements of both line positions and line intensities of nine isotopologues of carbon dioxide in the 4300–7000 cm 1 region [33,38,48,52,57].”
- Methane observations from the Greenhouse Gases Observing SATellite: Comparison to ground‐based TCCON data and model calculations (2011, methodology): “2 of the OCO linelists which include line‐ mixing, whilst CH4 and H2O are taken from the TCCON linelists based on HITRAN08 [Rothman et al., 2009] with updates to CO2 [Toth et al., 2008], H2O [Toth, 2005; Jenouvrier et al., 2007] and CH4 [Frankenberg et al., 2008].”