L. Wang

发表

Elsevier Editorial System(tm) for Journal of Quantitative Spectroscopy and Radiative Transfer Manuscript Draft the 1.58 m Transparency Window of Methane (6165-6750 Cm -1 ): Empirical Line List and Temperature Dependence between 80 K and 296 K

V. Boudon, S. Kassi, An-wen Liu, 2010 .

Methane line parameters in the HITRAN2012 database

V. M. Devi, T. Carrington, I. Gordon, 2013 .

Water vapor line parameters from 6450 to 9400 cm -1

S. Mikhailenko, L. Wang, L. Régalia, 2014 .

The WKLMC empirical line lists (5852–7919 cm−1) for methane between 80 K and 296 K: “Final” lists for atmospheric and planetary applications

D. Mondelain, S. Kassi, A. Campargue, 2013 .

Refinements of the WKMC empirical line lists (5852–7919 cm−1) for methane between 80 K and 296 K

A. Nikitin, D. Mondelain, S. Kassi, 2012 .

The absorption spectrum of methane at 80 and 294 K in the icosad (6717–7589 cm−1): Improved empirical line lists, isotopologue identification and temperature dependence

D. Mondelain, S. Kassi, A. Campargue, 2012 .

The absorption spectrum of water in the 1.25 μm transparency window (7408–7920 cm−1)

S. Mikhailenko, S. Kassi, A. Campargue, 2011 .

The 1.28 μm transparency window of methane (7541-7919 cm⁻¹): empirical line lists and temperature dependence (80 K-300 K).

D. Mondelain, S. Kassi, A. Campargue, 2011, Physical chemistry chemical physics : PCCP.

Acetylene, 12C2H2: new CRDS data and global vibration-rotation analysis up to 8600 cm−1

A. Fayt, M. Herman, S. Kassi, 2008 .

Applications of a new set of methane line parameters to the modeling of Titan’s spectrum in the 1.58 μm window

P. Drossart, V. Boudon, A. Nikitin, 2012 .

An empirical line list for methane in the 1.26–1.71 μm region for planetary investigations (T = 80–300 K). Application to Titan

P. Drossart, E. Lellouch, A. Coustenis, 2012 .