Recommended Isolated-Line Profile for Representing High-Resolution Spectroscoscopic Transitions

摘要: transitions Jonathan Tennyson1, Peter F. Bernath2, Alain Campargue3, Attila G. Csaszar4, Ludovic Daumont,5 Robert R. Gamache6, Joseph T. Hodges7, Daniel Lisak8, Olga V. Naumenko9, Laurence S. Rothman10, Ha Tran11, Jean-Michel Hartmann11, Nikolai Zobov12, Jeanna Buldyreva13, Chris D. Boone14, Maria De Vizia15, Livio Gianfrani15, McPheat16, Damien Weidmann16, Murray17, Ngoc Hoa Ngo18, Oleg L. Polyansky1,12 1Department of Physics and Astronomy, University College London, UK; 2Department Chemistry Biochemistry,Old Dominion University, USA; 3Universite Grenoble 1/CNRS, France; 4Institute Chemistry, Lorand Eotvos Hungary; 5GSMA, UMR CNRS 7331, Universite de Reims Champagne Ardenne, 6Department Environmental, Earth, Atmospheric Sciences Massachusetts Lowell, 7National Institute Standards Technology, Gaithersburg, U.S.A.; 8Institute Physics, Nicolaus Copernicus Torun, Poland; 9Institute Optics, Russian Academy Sciences, Tomsk, Russia; 10Harvard-Smithsonian Center for Astrophysics, Cambridge, 11Laboratoire Interuniversitaire des Systemes Atmospheriques, 7583, Paris Est Creteil, 12Institute Applied Nizhny Novgorod, 13Institut UTINAM 6213, Franche-Comte, Besancon, 14Department Waterloo, Canada; 15Department Mathematics Second Naples, Caserta, Italy; 16Rutherford Appleton Laboratory, Didcot, 17Space Imperial 18Faculty Hanoi National Education, Vietnam