Graphical resources / Defined Functions

Graphical resources

Guest

Rus | Eng

..Up

Graphics resource statistics

Функции и аргументы

Перевод единиц измерения

Defined Functions

Статистика по интервалам волновых чисел

Defined Functions

The title of the composite plot	(Axis Y, X) Physical Quantity (Unit)	Reference
1. The generalized absorption coefficient for the 15 μ band of CO₂ - Solid curve, Elsasser and King; broken curve, Kaplan. Defined Function = ln(l/2), generalized absorption coefficient l=(2παS/d²), S is the line strength, α the half-width at half-maximum k_ν. [7] Elsasser W.M. and J.I.F.King, Rept. No.9, Contract AF 19(122)-392, University of Utah, (September 1,1953). [9] Kaplan L.D. J Chem Phys 18,186 (1950); see also, J Meteorol 9,1 (1952).	Y. Defined Function X. Wavenumber (cm⁻¹)	Howard J. N., Burch D. E., Williams D., Infrared transmission of synthetic atmospheres. IV. Application of Theoretical Band Models, Journal of Optical Society of America, 1956, Volume 46, no. 5, Pages 334-338, DOI: 10.1364/JOSA.46.000334, https://doi.org/10.1364/JOSA.46.000334.
2. Logarithmic plot of absorption coefficient vs. wave number for pure CO₂. Defined Function = Log₁₀α + 10	Y. Defined Function X. Wavenumber (cm⁻¹)	B.H. Winters, S. Silverman, W.S. Benedict, Line shape in the wing beyond the band head of the 4·3 μ band of CO₂, Journal of Quantitative Spectroscopy and Radiation Transfer, 1964, Volume 4, Issue 4, Pages 527-537, DOI: 10.1016/0022-4073(64)90014-7.

3. Logarithmic plot of absorption coefficient vs. wave number for CO₂ broadened with N₂. Defined Function = Log₁₀α + 10	Y. Defined Function X. Wavenumber (cm⁻¹)
4. Logarithmic plot of absorption coefficient vs. wave number for CO₂ broadened with O₂.	Y. Defined Function X. Wavenumber (cm⁻¹)
5. Observations of induced absorption in carbon dioxide. The absorption coefficient/density [2], which at low densities is given by α/ρ²=2πνA in the notation of Eq. (3), is plotted instead of the dielectric loss to allow better comparison with the infrared observations. GS, Gebbie and Stone [7]; FW, Frenkel and Woods [8]; MB, Maryott and Birnbaum [9]; HKT, this work. 7. H. A. Gebbie and N. W. B. Stone, Proc. Phys. Soc. (London) 82,543 (1963) 8. L. Frenkel and D. Woods, J. Chern. Phys. 44, 2219 (1966). 9. G. Birnbaum and A. A. Maryott, J. Chern. Iihys. 36, 2032 (1962) Defined Function = absorption coefficient / density²	Y. Defined Function X. Wavenumber (cm⁻¹)	W. Ho, I. A. Kaufman, and P. Thaddeus, Microwave Absorption in Compressed CO₂, Journal of Chemical Physics, 1966, Volume 45, Issue 3, Pages 877, DOI: 10.1063/1.1727698, http://link.aip.org/link/doi/10.1063/1.1727698.
4. Observed and calculated profiles for the ν₁ band at 297°K. Defined function = (1/(l ν) ln(I₀/I), l -length, v- spectral interval, I₀, I - intensities.	Y. Defined Function X. Wavenumber (cm⁻¹)	L. Mannik, J. C. Stryland, The ν₁ Band of Carbon Dioxide in Pressure-Induced Absorption. II. Density and Temperature Dependence of the Intensity; Critical Phenomena, Canadian Journal of Physics, 1972, Volume 50, Issue 12, Pages 1355-1362, DOI: 10.1139/p72-186.
1. Temperature dependence of the N₂ continuum (taken from BURCH et al. [11]). 11. D. E. Burch, D. A. Gryvnak, R. R. Patn, and C. E. Bartky, J. Opt. Soc. Am. 59, 267 (1969). Defined function = lnT/(P²L) (atm^-2 km^-1)	Y. Defined Function X. Wavenumber (cm⁻¹)	Susskind J., Searl J.E. , Atmospheric absorption near 2400 cm^-1, Journal of Quantitative Spectroscopy and Radiative Transfer, 1977, Volume 18, no. 6, Pages 581-587, DOI: 10.1016/0022-4073(77)90082-6, https://doi.org/10.1016/0022-4073(77)90082-6.
1. Comparison of experimental α(ν) and calculated spectrum α_L(ν) of the high frequency wing of the ν₃ band of CO₂ at room temperature. The computed curve is from (6.3) with Δν = 36.3 cm^-1, A = 0.25. WSB is obtained from Fig. 2. Ref. (4) by dividing the experimental absorption.by the calculated Lorentz absorption. Winters B.H., S. Silverman, W.S. Benedict, Line shape in the wing beyond the band head of the 4.3 µ band of CO₂, Journal of Quantitative Spectroscopy and Radiative Transfer, Volume 4, Issue 4, July-August 1964, Pages 527-537 https://doi.org/10.1016/0022-4073(64)90014-7 Defined function = α(ν)/α_L(ν).	Y. Defined Function X. Wavenumber (cm⁻¹)	George Birnbaum, The shape of collision broadened lines from resonance to the far wings, Journal of Quantitative Spectroscopy and Radiation Transfer, 1979, Volume 21, Issue 6, Pages 597-607, DOI: 10.1016/0022-4073(79)90099-2.
5. Коэффициент поглощения за кантом полосы 4.3 мкм. 1 – результаты расчета авторов, 2 – данные работы [11], 3- данные работы [5]. The absorption coefficient behind the 4.3 µm band edge. 1 - the results of the authors' calculations, 2 - data from [11], 3 - data from [5]. Defined Function=-ln(K(ν)) [5] Буланин М.О., Булычев В.П., Гранский П.В., Коузов А.П., Тонков М.В. Исследование функций пропускания СО₂ в области полос 4.3 и 15 мкм. В кн.: Проблемы физики атмосферы. Вып. 13, Л., Изд. ЛГУ, 1976, с.14-24. [11] Burch D.E., Gryvnak D.A., Patty R.R., Bartky Ch.E. Absorption of infrared radiant energy by CO₂ and H₂O. IV. Shapes of collision -broadened CO₂ lines. J.Opt.Soc Amer. 1969, 59, No.3, 267-280.	Y. Defined Function X. Wavenumber (cm⁻¹)	Гальцев А.П., Цуканов В.В., Расчет формы колебательно-вращательных поплос поглощения углекислого газа методом статистического моделирования, Оптика и спектроскопия, 1979, Volume 46, Issue 3, Pages 467-473.
1. Спектр поглощения за кантом полосы 3ν₃ СО₂. а – эксперимент, б – расчет с дисперсионным контуром, в – расчет по формуле (1). 1 - для СО₂+СО₂, 2 – для СО₂+Ar, 3 – для СО₂+Не. Absorption spectrum behind the edge of the 3ν₃ CO₂ band. a - experiment, b - calculation with a dispersion contour, c - calculation by formula (1). 1 - for CO₂+CO₂, 2 - for CO₂+Ar, 3 - for CO₂+He. Defined Function=-lg(K)	Y. Defined Function X. Wavenumber (cm⁻¹)	Баранов Ю.И., Буланин М.О., Тонков М.В., Исследование крыльев линий колебательно-вращательной полосы 3ν₃ СО₂, Оптика и спектроскопия, 1981, Volume 50, no. 3, Pages 613-615.
2. Ход коэффициента поглощения за кантом полосы ν3. Сплошная линия – результаты расчета с потенциалом (11), штриховая - с потенциалом (12), точки и кружки – данные работ [25] и [26], соответственно. Defined Function = - ln(k(v)) [25] Буланин М.О., Булычев В.П., Гранский П.В., Коузов А.П., Тонков М.В. Исследование функций пропускания СО₂ в области полос 4.3 и 15 мкм. В кн.: Проблемы физики атмосферы. Вып. 13, Л., Изд. ЛГУ, 1976, с.14-24. [26] Burch D.E., Gryvnak D.A., Patty R.R., Bartky Ch.E. Absorption of infrared radiant energy by CO2 and H2O. IV. Shapes of collision -broadened CO₂ lines. J.Opt.Soc Amer. 1969, 59, No.3, 267-280.	Y. Defined Function X. Wavenumber (cm⁻¹)	Гальцев А.П., Цуканов В.В., Температурная зависимость коэффициента поглощения за кантом полос углекислого газа., Оптика и спектроскопия, 1983, Т. 55, Выпуск 2, Страницы 273-279.
1. Спектральная зависимость бинарных коэффициентов поглощения в крыле полосы ν₃ СО₂. Spectral dependence of binary absorption coefficients in the wing of the ν₃ СО₂ band. Defined Function=ln(B_ab) 1 – CO₂+CO₂, 2 – CO₂+N₂, 3 – CO₂+Ar, 4 – CO₂+D₂, 5 – CO₂+H₂, 6 – CO₂+He. B_ab=(ρ_a ρ_b l)^-1 ln(I₀/I) (unit cm^-1 Amagat^-2), ρ_a and ρ_bare the densities of the absorbing and disturbing gases, l is the thickness of the optical layer.	Y. Defined Function X. Wavenumber (cm⁻¹)	Sattarov, K., Tonkov, M.V., Infrared absorption in the wing of the ν₃ vibrational-rotational band of CO₂, Optics and Spectroscopy, 1983, Volume 54, Pages 562.
2. Зависимость коэффициентов поглощения от частоты в области крыла полосы ν₃ СО₂. Точки – эксперимент, кривые – расчет по формуле (9). Frequency dependence of absorption coefficients in the region of the wing of the ν₃ СО₂ band. Points - experiment, curves - calculation by formula (9). Defined Function = lgK_ab	Y. Defined Function X. Wavenumber (cm⁻¹)	Cаттаров Х., Исследование инфракрасных спектров углекислого газа и фреонов в условиях, близких к атмосферным, Ленинград, Автореферат канд ф.-м. н., 1983, 18 С..

3. Зависимость функции k(n) в области крыла полосы ν₃ СО₂. Точки – эксперимент, кривые – расчет по модели интерференции линий. n – число интерферирующих линий. Dependence of the function k(n) in the wing region of the ν₃ СО₂ band. Points - experiment, curves - calculation by the line interference model. n is the number of interfering lines. Defined Function = ln(κ), k=K^exp(ν)/K^L(ν), k- поправочная функция (correction factor).	Y. Defined Function X. Wavenumber (cm⁻¹)
109. Comparison of experimental and calculated spectrum (A₀ in cm^-1 amagat^-2) T=296°K. observed, Lorentz absorption, best fit obtained with the two-parameter lineshape factor of Birnbaum [see Eq. (5)]. The optimized values of the parameters are given in Table IV. Defined function = log₁₀A₀ + 10	Y. Defined Function X. Wavenumber (cm⁻¹)	R. Le Doucen, C. Cousin, C. Boulet, and A. Henry, Temperature dependence of the absorption in the region beyond the 4.3-µm band head of CO₂. 1: Pure CO₂ case, Applied Optics, 1985, Volume 24, Pages 897-906, DOI: 10.1364/AO.24.000897, http://www.opticsinfobase.org/ao/abstract.cfm?URI=ao-24-6-897.

209. Comparison of experimental and calculated spectrum (A₀ in cm^-1 amagat^-2) T = 218°K: observed, Lorentz absorption, best fit obtained with the two-parameter lineshape factor of Birnbaum [see Eq. (5)]. The optimized values of the parameters are given in Table IV. Defined function = log₁₀A₀ + 10	Y. Defined Function X. Wavenumber (cm⁻¹)
7. Ratio of the experimental (from Refs. 20, 33, and 43) to calculated absorption coefficient for pure CO₂ at 296°K in the troughs between the R lines of the v₃ band. X Lorentzian model; 0 ECSA line-mixing model. Defined Function = K^exp(ν)/ K^th(ν). ESCA = The energy corrected sudden approximation 20. C. Cousin, R. Le Doucen, C. Bouiet, A. Henry, and D. Robert. 1. Quant. Spectrosc. Radiat. Transfer 36,521 (1986). 33. C. Cousin-Lucasseau, Thesis, Rennes, 1987. 43. C. Cousin, R. Le Doucen, J. P. Houdeau, C. Boulet, and A. Henry, Appl. Opt. 25, 2434 (1986).	Y. Defined Function X. Wavenumber (cm⁻¹)	J.-.M. Hartmann, Measurements and calculations of CO₂ room-temperature high-pressure spectra in the 4.3 μm region, Journal of Chemical Physics, 1989, Volume 90, Issue 6, Pages 2944–2950, DOI: 10.1063/1.455894.
5. Normalized absorption coefficient B₀(u) vs wave number u for CO₂-argon at room temperature; 0: experimental results, .: Lorentzian calculation, X: theoretical results B^RQS-EC₀ [cf. Eqs. (27) and (30) J obtained with the potential of Ref. 12 (A₂ = 0.266, R₂ = 1.09), b.: theoretical results B^RQS-EC₀ obtained with the optimized anisotropic potential V₂(R) given in Fig. 7. Defined function = ln(B₀(u)) 12. L. Berreby & E. Dayan, Mean square torque from linear molecule-rare gas atom systems at intermediate pressures, Molecular Physics, Volume 48, 1983 - Issue 3, Pages 581-592, https://doi.org/10.1080/00268978300100411	Y. Defined Function X. Wavenumber (cm⁻¹)	Boissoles J., Menoux V., Le Doucen R., Boulet C., Robert D., Collisionally induced population transfer effects in infrared absorption spectra. II. The wing of the Ar-broadened ν₃ band of CO₂, The Journal of Chemical Physics, 1989, Volume 91, Issue 4, Pages 2163-2171, DOI: 10.1063/1.457024, https://doi.org/10.1063/1.457024.
9. The ratios of the observed absorption (α_observed) in the wing region beyond the band head of CO₂ to the calculated ECS-P absorption (χ_ECS-P) at T = 300°K: ---, for CO₂+CO₂; • - for CO₂+N₂	Y. Defined Function X. Wavenumber (cm⁻¹)	J. Boissoles, C. Boulet, L. Bonamy and D. Robert, Calculation of absorption in the microwindows of the 4.3 μm CO₂ band from an ECS scaling analysis, Journal of Quantitative Spectroscopy and Radiative Transfer, 1989, Volume 42, Issue 6, Pages 509-520, DOI: 10.1016/0022-4073(89)90041-1.
1. CO₂-Ar absorption coefficient. o experiment [3], x, Δ – calculation with different potentials [3], •– calculation with dispersive line shape, ____ calculation according to the line wing theory Defined Function = ln(kappa) [3] Boulet C. in Spectral line shape, V.5, Proc 9th Int Conf, Torun, Poland, 1988, P.539	Y. Defined Function X. Wavenumber (cm⁻¹)	Tvorogov S.D., Nesmelova L.I., Rodimova O.B., Far wings of spectral lines: theory, interpretation and application in atmospheric optics, Proceedings of ASA Workshop, 1990. Tomsk, Tomsk, Издательство ИОА, 1990, Pages 14-18.