We.P.P35 - 23rd International Conference on Spectral Line Shapes
Transkrypt
We.P.P35 - 23rd International Conference on Spectral Line Shapes
Multispectrum-fitting of phenomenological collisional line-shape models to a speed-dependent Blackmore profile for spectroscopic analysis and databases P Wcisło1, D Lisak1, R Ciuryło1, A S Pine2 1 Institute of Physics, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University, -Grudziadzka 5, 87-100 Toruń, Poland 2 Alpine Technologies, 14401 Poplar Hill Road, Germantown, Maryland 20874 USA A variety of phenomenological line-shape models [1-9] are compared with a speed-dependent Blackmore profile [10-12] describing an O2 spectral line measured earlier with a very high signal-to-noise ratio, S/N > 105 [13,14]. In this reference Blackmore profile (SDh B12 P), the speed-dependence of the selfbroadening and shifting is given by a hypergeometric function characterized by an isotropic long-range attractive r−5 interaction potential, and the velocity-changing collision operator is calculated from a corresponding short-range r−12 repulsion. Simultaneous fitting [15,16] of the phenomenological models to the Blackmore profile simulated at 15 pressures from 5 to 800 Torr provides model parameters, linear in pressure, with correlation reduced from single-spectrum fits. None of these fitting models are able to reproduce the reference spectra to within a S/N greater than 6 × 104 . The quality of fit [13], based on the peak intensity divided by the residuals, indicate which models are adequate for analysis of spectra measured with a given S/N . The model dependence or systematic deviations of the fitting parameters is seen to be much larger than their least-squares statistical standard deviations. The model differences of the common parameters, such as line position, intensity and broadening, usually are inversely related to the quality of fit, but not always. These differences indicate the possible magnitude of systemic errors caused by oversimplified treatment of velocity-changing collisions. The application of these results to spectral analysis, improved databases [17], atmospheric remote sensing [18], trace gas metrology [19], and Doppler thermometry is discussed [20]. References: [1] [2] [3] [4] [5] [6] [7] [8] [9] [10] [11] [12] [13] [14] [15] [16] [17] [18] [19] [20] Galatry L 1961 Phys. Rev. 122 1218 Nelkin M and Ghatak A 1964 Phys. Rev. 135 p A4 Rautian S G and Sobelman I I 1966 Usp. Fiz. Nauk. 90 209 [Rautian S G and Sobelman I I 1967 Sov. Phys. Usp. 9 701] Berman P R 1972 J. Quant. Spectrosc. Radiat. Transfer 12 1331 Pine A S 1999 J. Quant. Spectrosc. Radiat. Transf. 62 397 Robert D, Joubert P, Lance B 2000 J. Mol. Struct. 517-518 393 Priem D, Rohart F, Colmont J M, Wlodarczak G, Bouanich J P 2000 J. Mol. Struct. 517-518 435 Ciuryło R, Pine A S, Szudy J 2001 J. Quant. Spectrosc. Radiat. Transf. 68 257 Ngo N H, Lisak D, Tran H, Hartmann J-M 2013 J. Quant. Spectrosc. Radiat. Transf. 129 89 Blackmore R 1987 J. Chem. Phys. 87 791 Ciuryło R, Shapiro D A, Drummond J R, May A D 2002 Phys. Rev. A 65 012502 Wcisło P, Ciuryło R 2013 J. Quant. Spectrosc. Radiat. Transfer 120 36 Cygan A, Lisak D, Wójtewicz S, Domysławska J, Hodges J T, Trawiński R S, Ciuryło R 2012 Phys Rev A 85 022508 Wcisło P, Cygan A, Lisak D, Ciuryło R 2013 Phys. Rev. A 88 012517 Benner D C,R insland C P, Devi V M, Smith M A H, Atkins D 1995 J. Quant. Spectrosc. Radiat. Transf. 53 705 Pine A S, Ciuryło R 2001 J. Mol. Spectrosc. 208 180 Hill C, Gordon I E, Rothman L S, Tennyson J 2013 J. Quant. Spectrosc. Radiat. Transf. 130 51 Miller C E, Brown L R, Toth R A, Benner D C, Devi V M 2005 C.R. Phys 6 876 Hashiguchia K, Lisak D, Cygan A, Ciuryło R, Abe H 2013 Sens. Actuators A 241 152 Gianfrani L 2016 Phil. Trans. R. Soc. A 374 20150047