Assessment of the consistency of near‐infrared water vapor line intensities using high‐spectral‐resolution ground‐based Fourier transform measurements of solar radiation
暂无分享,去创建一个
[1] Gang Li,et al. The HITRAN 2008 molecular spectroscopic database , 2005 .
[2] Robert A. Toth,et al. Measurements of positions, strengths and self-broadened widths of H2O from 2900 to 8000 cm−1: line strength analysis of the 2nd triad bands , 2005 .
[3] D. Ehhalt. Vertical profiles of HDO/H 2 O in the troposphere , 2005 .
[4] R. Tolchenov,et al. Water line parameters for weak lines in the range 7400 – 9600 cm 1 , 2005 .
[5] Juergen Fischer,et al. Satellite- and ground-based observations of atmospheric water vapor absorption in the region , 2004 .
[6] K. Smith,et al. Absorption by water vapour in the 1 to region , 2004 .
[7] Laurence S. Rothman,et al. The HITRAN molecular spectroscopic database: edition of 2000 including updates through 2001 , 2003 .
[8] Stanley C. Solomon,et al. Field test of spectral line intensity parameters for tropospheric water vapor , 2003 .
[9] W. J. van der Zande,et al. Evaluation of spectroscopic databases of water vapor between 585 and 600 nm , 2002 .
[10] David Carlson,et al. Corrections of Humidity Measurement Errors from the Vaisala RS80 Radiosonde—Application to TOGA COARE Data , 2002 .
[11] Robert A. Toth,et al. Empirical Line Parameters of H216O near 0.94 μm: Positions, Intensities and Air-Broadening Coefficients , 2002 .
[12] U. Lohmann,et al. Impact of improved near infrared water vapor line data on absorption of solar radiation in GCMs , 2001 .
[13] David A. Newnham,et al. High‐resolution atmospheric absorption by water vapor in the 830–985 nm region: Evaluation of spectroscopic databases , 2001 .
[14] Effects of improvements in near‐infrared water vapour line intensities on short‐wave atmospheric absorption , 2001 .
[15] Jonathan Tennyson,et al. New studies of the visible and near‐infrared absorption by water vapour and some problems with the HITRAN database , 2000 .
[16] Harry Partridge,et al. Convergence testing of the analytic representation of an ab initio dipole moment function for water: Improved fitting yields improved intensities , 2000 .
[17] Lawrence P. Giver,et al. Visible and near-infrared H216O line intensity corrections for HITRAN-96 , 2000 .
[18] M. Chipperfield,et al. Ground-based FTIR Measurements with High Temporal Resolution , 1998 .
[19] J. Notholt,et al. An uncertainty budget for ground‐based Fourier transform infrared column measurements of HCl, HF, N2O, and HNO3 deduced from results of side‐by‐side instrument intercomparisons , 1997 .
[20] Harry Partridge,et al. The determination of an accurate isotope dependent potential energy surface for water from extensive ab initio calculations and experimental data , 1997 .
[21] K. Trenberth,et al. Earth's annual global mean energy budget , 1997 .
[22] Robert L. Kurucz,et al. The Solar Spectrum: Atlases and Line Identifications , 1995 .
[23] J. Flaud,et al. H216O: Line positions and intensities between 8000 and 9500 cm−1: the second hexad of interacting vibrational states: {(050), (130), (031), (210), (111), (012)} , 1988 .
[24] P. Griffiths. Fourier Transform Infrared Spectrometry , 2007 .