Visible and near-infrared O line intensity corrections for HITRAN-96
- 1 July 2000
- journal article
- research article
- Published by Elsevier in Journal of Quantitative Spectroscopy and Radiative Transfer
- Vol. 66 (1) , 101-105
- https://doi.org/10.1016/s0022-4073(99)00223-x
Abstract
No abstract availableKeywords
This publication has 11 references indexed in Scilit:
- The 1997 spectroscopic GEISA databankJournal of Quantitative Spectroscopy and Radiative Transfer, 1999
- THE HITRAN MOLECULAR SPECTROSCOPIC DATABASE AND HAWKS (HITRAN ATMOSPHERIC WORKSTATION): 1996 EDITIONPublished by Elsevier ,1999
- Observational constraints on non-Lorentzian continuum effects in the near-infrared solar spectrum using ARM ARESE dataJournal of Quantitative Spectroscopy and Radiative Transfer, 1998
- Direct Observations of Excess Solar Absorption by CloudsScience, 1995
- Absorption of Solar Radiation by Clouds: Observations Versus ModelsScience, 1995
- Measurements of H216O Line Positions and Strengths: 11 610 to 12 861 cm−1Journal of Molecular Spectroscopy, 1994
- : line positions and intensities between 9500 and 11500 cm−1. The interacting vibrational states (041), (220), (121), (022), (300), (201), (102), and (003)Canadian Journal of Physics, 1989
- H216O: Line positions and intensities between 8000 and 9500 cm−1: the second hexad of interacting vibrational states: {(050), (130), (031), (210), (111), (012)}Canadian Journal of Physics, 1988
- The high-resolution spectrum of water vapor between 13 200 and 16 500 cm−1Journal of Molecular Spectroscopy, 1986
- The high-resolution spectrum of water vapor between 16500 and 25250 cm−1Journal of Molecular Spectroscopy, 1985