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Added installation functionality and renamed the package
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#!/usr/bin/env Python3
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import numpy as np
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'''
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@ Author: Joost van den Born
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@ Contact: born@astron.nl
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@ Description: A comparison of various atmospheric refraction models.
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Also these are used to calculate the difference in
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atmospheric dispersion, given a set of conditions.
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'''
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def BarrellAndSears(l, T=288.15, p=101325, H=0):
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'''
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From Barrell & Sears, 1939
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Equation 7.7, page 52
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For atmospheric air (i.e. CO2 = 300 ppm)
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This equation is applicable for the ranges T=10-30C and p=720-800 mmHg.
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Input:
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l - Wavelength in microns
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T - Temperature in Kelvin
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p - Atmospheric pressure in Pa
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H - fractional humidity (0=<H=<1)
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Returns:
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n - Refractive index of atmospheric air at the given conditions
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'''
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T = K2C(T)
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P = hPA2mmHg(p/100)
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R = (0.378125 + 0.0021414 / l**2 + 0.00001793 / l**4) * (P*(1 + (1.049 - 0.0157*T) * P * 1e-6)/(1 + 0.003661*T)) - (0.0624 - 0.000680 / l**2) * H / (1 + 0.003661*T)
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n = R/1e6 + 1
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return n
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def Ciddor(l):
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'''
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From Ciddor, 1996
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Equations 1
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At default conditions only. For more flexibility use
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Observatory.n_tph()
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Input:
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l - Wavelength in microns
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Returns:
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n - Refractive index of atmospheric air at the given conditions
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'''
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s = 1 / l
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R = 5792105 / (238.0185 - s**2) + 167917 / (57.362 - s**2)
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n = R/1e8 + 1
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return n
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def Edlen1953(l):
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'''
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From Edlen, 1953
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Equation 2
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At standard conditions only
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Input:
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l - Wavelength in microns
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Returns:
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n - Refractive index of atmospheric air at the given conditions
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'''
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s = 1 / l
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R = 6432.8 + 2949810 / (146 - s**2) + 25540/(41-s**2)
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n = R/1e8 + 1
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return n
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def Edlen1966(l):
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'''
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From Edlen, 1966
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Equation 1
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At standard conditions only
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Input:
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l - Wavelength in microns
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Returns:
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n - Refractive index of atmospheric air at the given conditions
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'''
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s = 1 / l
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R = 8342.13 + 2406030 / (130 - s**2) + 15997 / (38.9 - s**2)
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n = R/1e8 + 1
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return n
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def Owens(l, T=288.15, p=101325, H=0):
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'''
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From Owens, 1967
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Equation 32
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Note that the pressure P and H are in torricelli (Torr),
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however, this is almost precisely 1 Torr = 1 mmHg
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Input:
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l - wavelength in micron
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T - Temperature in Kelvin
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p - Atmospheric pressure in Pa
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H - Humdity (0<=H<=1)
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Returns:
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n - Refractive index of atmospheric air at the given conditions
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'''
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P = hPA2mmHg(p/100)
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T = K2C(T)
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s = 1 / l
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R = 8342.13 + 2406030 / (130 - s**2) + 15997 / (38.9 - s**2) * (P/720.775) * ((1 + P * (0.817 - 0.0133) * 1e-6)/(1 + 0.0036610*T)) - H * (5.722 - 0.0457*s**2)
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n = R/1e8 + 1
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return n
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def BonschPotulski(l, T=288.15, p=101325, CO2=450):
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'''
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From Bonsch & Potulski, 1998
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Equations 6, 7, 8
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Input:
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l - Wavelength in microns
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T - Temperature in Kelvin
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p - Atmospheric pressure in Pa
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CO2 - Particles per million of CO2
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Returns:
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n - Refractive index of atmospheric air at the given conditions
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'''
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x = CO2 / 1e6
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T = K2C(T)
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s = 1 / l
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# Rs = 8092.33 + 2333983 / (130 - s**2) + 15518 / (38.9 - s**2)
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Rs = 8091.37 + 2333983 / (130 - s**2) + 15518 / (38.9 - s**2)
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Rs = Rs / 1e8
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Rx = Rs * (1 + 0.5327 * (x - 0.0004))
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Rtp = Rx * p / 93214.60 * (1 + 1e-8 * (0.5953 - 0.009876 * T)*p) / (1 + 0.0036610 * T)
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n = Rtp + 1
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return n
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def BirchDowns(l):
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'''
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From Birch & Downs, 1993 and 1994 (correction)
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Equations 1 and 2
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Only at standard conditions
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Input:
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l - wavelength in micron
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Returns:
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n - Refractive index of atmospheric air at the given conditions
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'''
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s = 1 / l
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R = 8342.54 + 2406147 / (130 - s**2) + 15998 / (38.9-s**2)
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n = R/1e8 + 1
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return n
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def PeckReeder(l):
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'''
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From Peck & Reeder, 1972
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Equation 3
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Only at standard conditions
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Input:
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l - wavelength in micron
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Returns:
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n - Refractive index of atmospheric air at the given conditions
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'''
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s = 1 / l
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R = 8060.51 + 2480990 / (132.274 - s**2) + 17455.7 / (39.32957 - s**2)
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n = R/1e8 + 1
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return n
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def slalib(l, T=288.15, p=101325, H=0, h=0, lat=-24, tlr=0.0065, eps=1e-10):
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'''
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SLALIB uses the same atmospheric model as ZEMAX
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based on the works of Hohenkerk & Sinclair and Seidelmann.
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They take the B&S refraction formula as a basis.
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Requires the pySLALIB package to work.
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Input:
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l - Wavelength in microns
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T - Temperature in Kelvin
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p - Atmospheric pressure in Pa
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H - fractional humidity (0=<H=<1)
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h - Altitude of the observer (default=0 m)
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lat - Latitude of the observer (default=-24)
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tlr - temperature lapse rate (default=0.0065)
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eps - precision at which the calculation is aborted (default=1e-10)
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Returns:
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n - Refractive index of atmospheric air at the given conditions
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'''
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from pyslalib import slalib
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zObs = np.deg2rad(45.06563)
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p = p/100
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R = []
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if type(l) == float:
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l = [l]
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for wl in l:
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R.append(slalib.sla_refro(zObs, h, T, p, H, wl, lat, tlr, eps))
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if len(l) == 1:
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return R[0]+1
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else:
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return np.asarray(R)+1
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def Mathar(l, T=288.15, p=101325, H=0):
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'''
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Refractivity model by Mathar (2007), valid above 1.4 microns
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Code taken and modified from:
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https://github.com/polyanskiy/refractiveindex.info-scripts/blob/master/scripts/Mathar%202007%20-%20Air%201.3-2.5um.py
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Input:
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l - Wavelength in microns
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T - Temperature in Kelvin
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p - Atmospheric pressure in Pa
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H - fractional humidity (0=<H=<1)
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Returns:
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n - Refractive index of atmospheric air at the given conditions
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'''
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if l < 1.3 or l > 24:
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print('Using the Mathar model at this wavelength (l={:.3f}) is not recommended!'.format(l))
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if l <= 2.65:
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########################################################################
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# model parameters for wavelengths between 1.3 and 2.5 microns
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cref = [ 0.200192e-3, 0.113474e-9, -0.424595e-14, 0.100957e-16, -0.293315e-20, 0.307228e-24] # cm^j
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cT = [ 0.588625e-1, -0.385766e-7, 0.888019e-10, -0.567650e-13, 0.166615e-16, -0.174845e-20] # cm^j · K
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cTT = [-3.01513, 0.406167e-3, -0.514544e-6, 0.343161e-9, -0.101189e-12, 0.106749e-16] # cm^j · K^2
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cH = [-0.103945e-7, 0.136858e-11, -0.171039e-14, 0.112908e-17, -0.329925e-21, 0.344747e-25] # cm^j · %^-1
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cHH = [ 0.573256e-12, 0.186367e-16, -0.228150e-19, 0.150947e-22, -0.441214e-26, 0.461209e-30] # cm^j · %^-2
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cp = [ 0.267085e-8, 0.135941e-14, 0.135295e-18, 0.818218e-23, -0.222957e-26, 0.249964e-30] # cm^j · Pa^-1
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cpp = [ 0.609186e-17, 0.519024e-23, -0.419477e-27, 0.434120e-30, -0.122445e-33, 0.134816e-37] # cm^j · Pa^-2
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cTH = [ 0.497859e-4, -0.661752e-8, 0.832034e-11, -0.551793e-14, 0.161899e-17, -0.169901e-21] # cm^j · K · %^-1
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cTp = [ 0.779176e-6, 0.396499e-12, 0.395114e-16, 0.233587e-20, -0.636441e-24, 0.716868e-28] # cm^j · K · Pa^-1
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cHp = [-0.206567e-15, 0.106141e-20, -0.149982e-23, 0.984046e-27, -0.288266e-30, 0.299105e-34] # cm^j · %^-1 · Pa^-1
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sref = 1e4/2.25 # cm^−1, reference wavenumber
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Tref = 273.15+17.5 # K, reference temperature
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pref = 75000 # Pa, reference pressure
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Href = 10 #%, reference humdity in percent
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########################################################################
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if l > 2.65 and l <= 4.275:
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########################################################################
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# model parameters for wavelengths between 2.8 and 4.2 microns
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cref = [ 0.200049e-3, 0.145221e-9, 0.250951e-12, -0.745834e-15, -0.161432e-17, 0.352780e-20] # cm^j
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cT = [ 0.588432e-1, -0.825182e-7, 0.137982e-9, 0.352420e-13, -0.730651e-15, -0.167911e-18] # cm^j · K
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cTT = [-3.13579, 0.694124e-3, -0.500604e-6, -0.116668e-8, 0.209644e-11, 0.591037e-14] # cm^j · K^2
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cH = [-0.108142e-7, 0.230102e-11, -0.154652e-14, -0.323014e-17, 0.630616e-20, 0.173880e-22] # cm^j · %^-1
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cHH = [ 0.586812e-12, 0.312198e-16, -0.197792e-19, -0.461945e-22, 0.788398e-25, 0.245580e-27] # cm^j · %^-2
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cp = [ 0.266900e-8, 0.168162e-14, 0.353075e-17, -0.963455e-20, -0.223079e-22, 0.453166e-25] # cm^j · Pa^-1
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cpp = [ 0.608860e-17, 0.461560e-22, 0.184282e-24, -0.524471e-27, -0.121299e-29, 0.246512e-32] # cm^j · Pa^-2
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cTH = [ 0.517962e-4, -0.112149e-7, 0.776507e-11, 0.172569e-13, -0.320582e-16, -0.899435e-19] # cm^j · K · %^-1
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cTp = [ 0.778638e-6, 0.446396e-12, 0.784600e-15, -0.195151e-17, -0.542083e-20, 0.103530e-22] # cm^j · K · Pa^-1
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cHp = [-0.217243e-15, 0.104747e-20, -0.523689e-23, 0.817386e-26, 0.309913e-28, -0.363491e-31] # cm^j · %^-1 · Pa^-1
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sref = 1e4/3.4 # cm^−1, reference wavenumber
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Tref = 273.15+17.5 # K, reference temperature
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pref = 75000 # Pa, reference pressure
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Href = 10 #%, reference humdity in percent
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########################################################################
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if l > 4.275 and l <= 6.35:
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########################################################################
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# model parameters for wavelengths between 4.35 and 5.2 microns
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cref = [ 0.200020e-3, 0.275346e-9, 0.325702e-12, -0.693603e-14, 0.285610e-17, 0.338758e-18] # cm^j
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cT = [ 0.590035e-1, -0.375764e-6, 0.134585e-9, 0.124316e-11, 0.508510e-13, -0.189245e-15] # cm^j · K
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cTT = [-4.09830, 0.250037e-2, 0.275187e-6, -0.653398e-8, -0.310589e-9, 0.127747e-11] # cm^j · K^2
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cH = [-0.140463e-7, 0.839350e-11, -0.190929e-14, -0.121399e-16, -0.898863e-18, 0.364662e-20] # cm^j · %^-1
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cHH = [ 0.543605e-12, 0.112802e-15, -0.229979e-19, -0.191450e-21, -0.120352e-22, 0.500955e-25] # cm^j · %^-2
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cp = [ 0.266898e-8, 0.273629e-14, 0.463466e-17, -0.916894e-23, 0.136685e-21, 0.413687e-23] # cm^j · Pa^-1
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cpp = [ 0.610706e-17, 0.116620e-21, 0.244736e-24, -0.497682e-26, 0.742024e-29, 0.224625e-30] # cm^j · Pa^-2
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cTH = [ 0.674488e-4, -0.406775e-7, 0.289063e-11, 0.819898e-13, 0.468386e-14, -0.191182e-16] # cm^j · K · %^-1
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cTp = [ 0.778627e-6, 0.593296e-12, 0.145042e-14, 0.489815e-17, 0.327941e-19, 0.128020e-21] # cm^j · K · Pa^-1
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cHp = [-0.211676e-15, 0.487921e-20, -0.682545e-23, 0.942802e-25, -0.946422e-27, -0.153682e-29] # cm^j · %^-1 · Pa^-1
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σref = 1e4/4.8 # cm^−1, reference wavenumber
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Tref = 273.15+17.5 # K, reference temperature
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pref = 75000 # Pa, reference pressure
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Href = 10 #%, reference humdity in percent
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########################################################################
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if l > 6.35 and l <= 15.05:
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########################################################################
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# model parameters for wavelengths between 7.5 and 14.1 microns
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cref = [ 0.199885e-3, 0.344739e-9, -0.273714e-12, 0.393383e-15, -0.569488e-17, 0.164556e-19] # cm^j
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cT = [ 0.593900e-1, -0.172226e-5, 0.237654e-8, -0.381812e-11, 0.305050e-14, -0.157464e-16] # cm^j · K
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cTT = [-6.50355, 0.103830e-1, -0.139464e-4, 0.220077e-7, -0.272412e-10, 0.126364e-12] # cm^j · K^2
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cH = [-0.221938e-7, 0.347377e-10, -0.465991e-13, 0.735848e-16, -0.897119e-19, 0.380817e-21] # cm^j · %^-1
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cHH = [ 0.393524e-12, 0.464083e-15, -0.621764e-18, 0.981126e-21, -0.121384e-23, 0.515111e-26] # cm^j · %^-2
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cp = [ 0.266809e-8, 0.695247e-15, 0.159070e-17, -0.303451e-20, -0.661489e-22, 0.178226e-24] # cm^j · Pa^-1
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cpp = [ 0.610508e-17, 0.227694e-22, 0.786323e-25, -0.174448e-27, -0.359791e-29, 0.978307e-32] # cm^j · Pa^-2
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cTH = [ 0.106776e-3, -0.168516e-6, 0.226201e-9, -0.356457e-12, 0.437980e-15, -0.194545e-17] # cm^j · K · %^-1
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cTp = [ 0.77368e-6, 0.216404e-12, 0.581805e-15, -0.189618e-17, -0.198869e-19, 0.589381e-22] # cm^j · K · Pa^-1
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cHp = [-0.206365e-15, 0.300234e-19, -0.426519e-22, 0.684306e-25, -0.467320e-29, 0.126117e-30] # cm^j · %^-1 · Pa^-1
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σref = 1e4/10.1 # cm^−1, reference wavenumber
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Tref = 273.15+17.5 # K, reference temperature
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pref = 75000 # Pa, reference pressure
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Href = 10 #%, reference humdity in percent
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########################################################################
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if l > 15.05:
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########################################################################
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# model parameters for wavelengths between 16 and 24 microns
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cref = [ 0.199436e-3, 0.299123e-8, -0.214862e-10, 0.143338e-12, 0.122398e-14, -0.114628e-16] # cm^j
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# something seems to be wrong with cT...
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cT = [ 0.621723e-1, -0.177074e-4, 0.152213e-6, -0.954584-9, -0.996706e-11, 0.921476e-13] # cm^j · K
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cTT = [-23.2409, 0.108557, -0.102439e-2, 0.634072e-5, 0.762517e-7, -0.675587e-9 ] # cm^j · K^2
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cH = [-0.772707e-7, 0.347237e-9, -0.272675e-11, 0.170858e-13, 0.156889e-15, -0.150004e-17] # cm^j · %^-1
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||||
cHH = [-0.326604e-12, 0.463606e-14, -0.364272e-16, 0.228756e-18, 0.209502e-20, -0.200547e-22] # cm^j · %^-2
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cp = [ 0.266827e-8, 0.120788e-14, 0.522646e-17, 0.783027e-19, 0.753235e-21, -0.228819e-24] # cm^j · Pa^-1
|
||||
cpp = [ 0.613675e-17, 0.585494e-22, 0.286055e-24, 0.425193e-26, 0.413455e-28, -0.812941e-32] # cm^j · Pa^-2
|
||||
cTH = [ 0.375974e-3, -0.171849e-5, 0.146704e-7, -0.917231e-10, -0.955922e-12, 0.880502e-14] # cm^j · K · %^-1
|
||||
cTp = [ 0.778436e-6, 0.461840e-12, 0.306229e-14, -0.623183e-16, -0.161119e-18, 0.800756e-20] # cm^j · K · Pa^-1
|
||||
cHp = [-0.272614e-15, 0.304662e-18, -0.239590e-20, 0.149285e-22, 0.136086e-24, -0.130999e-26] # cm^j · %^-1 · Pa^-1
|
||||
σref = 1e4/20 # cm^−1, reference wavenumber
|
||||
Tref = 273.15+17.5 # K, reference temperature
|
||||
pref = 75000 # Pa, reference pressure
|
||||
Href = 10 #%, reference humdity in percent
|
||||
########################################################################
|
||||
|
||||
s = 1e4/l # cm^-1
|
||||
n = 1
|
||||
H = H*100
|
||||
|
||||
for j in range(0, 6):
|
||||
n += ( cref[j] + cT[j]*(1/T-1/Tref) + cTT[j]*(1/T-1/Tref)**2
|
||||
+ cH[j]*(H-Href) + cHH[j]*(H-Href)**2
|
||||
+ cp[j]*(p-pref) + cpp[j]*(p-pref)**2
|
||||
+ cTH[j]*(1/T-1/Tref)*(H-Href)
|
||||
+ cTp[j]*(1/T-1/Tref)*(p-pref)
|
||||
+ cHp[j]*(H-Href)*(p-pref) ) * (s-sref)**j
|
||||
return n
|
||||
|
||||
|
||||
def K2C(K):
|
||||
'''
|
||||
Kelvin to Celsius conversion
|
||||
'''
|
||||
return K - 273.15
|
||||
|
||||
def hPA2mmHg(hPa):
|
||||
'''
|
||||
hPa to mmHg conversion
|
||||
'''
|
||||
return 0.7500616827 * hPa
|
||||
Reference in new issue
Block a user