#!/usr/bin/env python
# -*- coding: utf-8 -*-
"""
Rayleigh Optical Depth - Scattering in the Atmosphere
=====================================================
Implements rayleigh scattering / optical depth in the atmosphere computation:
- :func:`scattering_cross_section`
- :func:`rayleigh_optical_depth`
- :func:`rayleigh_scattering`
See Also
--------
`Rayleigh Optical Depth - Scattering in the Atmosphere IPython Notebook
<http://nbviewer.ipython.org/github/colour-science/colour-ipython/blob/master/notebooks/phenomenons/rayleigh.ipynb>`_ # noqa
References
----------
.. [1] Bodhaine, B. A., Wood, N. B., Dutton, E. G., & Slusser, J. R. (1999).
On Rayleigh optical depth calculations. Journal of Atmospheric …,
16(11 PART 2), 1854–1861.
doi:10.1175/1520-0426(1999)016%3C1854:ORODC%3E2.0.CO;2
.. [2] Wikipedia. (n.d.). Rayleigh scattering. Retrieved September 23, 2014,
from http://en.wikipedia.org/wiki/Rayleigh_scattering
"""
from __future__ import division, unicode_literals
import numpy as np
from colour.colorimetry import (
DEFAULT_SPECTRAL_SHAPE,
SpectralPowerDistribution)
from colour.constants import AVOGADRO_CONSTANT
__author__ = 'Colour Developers'
__copyright__ = 'Copyright (C) 2013 - 2015 - Colour Developers'
__license__ = 'New BSD License - http://opensource.org/licenses/BSD-3-Clause'
__maintainer__ = 'Colour Developers'
__email__ = 'colour-science@googlegroups.com'
__status__ = 'Production'
__all__ = ['STANDARD_AIR_TEMPERATURE',
'STANDARD_CO2_CONCENTRATION',
'AVERAGE_PRESSURE_MEAN_SEA_LEVEL',
'DEFAULT_LATITUDE',
'DEFAULT_ALTITUDE',
'air_refraction_index_Penndorf1957',
'air_refraction_index_Edlen1966',
'air_refraction_index_Peck1972',
'air_refraction_index_Bodhaine1999',
'N2_depolarisation',
'O2_depolarisation',
'F_air_Penndorf1957',
'F_air_Young1981',
'F_air_Bates1984',
'F_air_Bodhaine1999',
'molecular_density',
'mean_molecular_weights',
'gravity_List1968',
'scattering_cross_section',
'rayleigh_optical_depth',
'rayleigh_scattering']
STANDARD_AIR_TEMPERATURE = 288.15
"""
*Standard air* temperature :math:`T[K]` in kelvin degrees (:math:`15\circ C`).
STANDARD_AIR_TEMPERATURE : numeric
"""
STANDARD_CO2_CONCENTRATION = 300
"""
*Standard air* :math:`CO_2` concentration in parts per million (ppm).
STANDARD_CO2_CONCENTRATION : numeric
"""
AVERAGE_PRESSURE_MEAN_SEA_LEVEL = 101325
"""
*Standard air* average pressure :math:`Hg` at mean sea-level in pascal (Pa).
AVERAGE_PRESSURE_MEAN_SEA_LEVEL : numeric
"""
DEFAULT_LATITUDE = 0
"""
Default latitude in degrees (equator).
DEFAULT_LATITUDE : numeric
"""
DEFAULT_ALTITUDE = 0
"""
Default altitude in meters (sea level).
DEFAULT_ALTITUDE : numeric
"""
[docs]def air_refraction_index_Penndorf1957(wavelength, *args):
"""
Returns the air refraction index :math:`n_s` from given wavelength
:math:`\lambda` in micrometers (:math:`\mu m`) using Penndorf (1957)
method.
Parameters
----------
wavelength : numeric
Wavelength :math:`\lambda` in micrometers (:math:`\mu m`).
\*args : \*
Arguments.
Returns
-------
numeric
Air refraction index :math:`n_s`.
See Also
--------
air_refraction_index_Edlen1966, air_refraction_index_Peck1972,
air_refraction_index_Bodhaine1999
Examples
--------
>>> air_refraction_index_Penndorf1957(0.555) # doctest: +ELLIPSIS
1.0002777...
"""
wl = wavelength
n = 6432.8 + 2949810 / (146 - wl ** (-2)) + 25540 / (41 - wl ** (-2))
n = n / 1.0e8 + 1
return n
[docs]def air_refraction_index_Edlen1966(wavelength, *args):
"""
Returns the air refraction index :math:`n_s` from given wavelength
:math:`\lambda` in micrometers (:math:`\mu m`) using Edlen (1966) method.
Parameters
----------
wavelength : numeric
Wavelength :math:`\lambda` in micrometers (:math:`\mu m`).
\*args : \*
Arguments.
Returns
-------
numeric
Air refraction index :math:`n_s`.
See Also
--------
air_refraction_index_Penndorf1957, air_refraction_index_Peck1972,
air_refraction_index_Bodhaine1999
Examples
--------
>>> air_refraction_index_Edlen1966(0.555) # doctest: +ELLIPSIS
1.0002777...
"""
wl = wavelength
n = 8342.13 + 2406030 / (130 - wl ** (-2)) + 15997 / (38.9 - wl ** (-2))
n = n / 1.0e8 + 1
return n
[docs]def air_refraction_index_Peck1972(wavelength, *args):
"""
Returns the air refraction index :math:`n_s` from given wavelength
:math:`\lambda` in micrometers (:math:`\mu m`) using
Peck and Reeder (1972) method.
Parameters
----------
wavelength : numeric
Wavelength :math:`\lambda` in micrometers (:math:`\mu m`).
\*args : \*
Arguments.
Returns
-------
numeric
Air refraction index :math:`n_s`.
See Also
--------
air_refraction_index_Penndorf1957, air_refraction_index_Edlen1966,
air_refraction_index_Bodhaine1999
Examples
--------
>>> air_refraction_index_Peck1972(0.555) # doctest: +ELLIPSIS
1.0002777...
"""
wl = wavelength
n = (8060.51 + 2480990 / (132.274 - wl ** (-2)) + 17455.7 /
(39.32957 - wl ** (-2)))
n = n / 1.0e8 + 1
return n
[docs]def air_refraction_index_Bodhaine1999(
wavelength,
CO2_concentration=STANDARD_CO2_CONCENTRATION):
"""
Returns the air refraction index :math:`n_s` from given wavelength
:math:`\lambda` in micrometers (:math:`\mu m`) using
Bodhaine, Wood, Dutton and Slusser (1999) method.
Parameters
----------
wavelength : numeric
Wavelength :math:`\lambda` in micrometers (:math:`\mu m`).
CO2_concentration : numeric
:math:`CO_2` concentration in parts per million (ppm).
Returns
-------
numeric
Air refraction index :math:`n_s`.
See Also
--------
air_refraction_index_Penndorf1957, air_refraction_index_Edlen1966,
air_refraction_index_Peck1972
Examples
--------
>>> air_refraction_index_Bodhaine1999(0.555) # doctest: +ELLIPSIS
1.0002777...
"""
wl = wavelength
CCO2 = CO2_concentration
n = ((1 + 0.54 * ((CCO2 * 1e-6) - 300e-6)) *
(air_refraction_index_Peck1972(wl) - 1) + 1)
return n
[docs]def N2_depolarisation(wavelength):
"""
Returns the depolarisation of nitrogen :math:`N_2` as function of
wavelength :math:`\lambda` in micrometers (:math:`\mu m`).
Parameters
----------
wavelength : numeric
Wavelength :math:`\lambda` in micrometers (:math:`\mu m`).
Returns
-------
numeric
Nitrogen :math:`N_2` depolarisation.
Examples
--------
>>> N2_depolarisation(0.555) # doctest: +ELLIPSIS
1.0350291...
"""
wl = wavelength
N2 = 1.034 + 3.17 * 1.0e-4 * (1 / wl ** 2)
return N2
[docs]def O2_depolarisation(wavelength):
"""
Returns the depolarisation of oxygen :math:`O_2` as function of
wavelength :math:`\lambda` in micrometers (:math:`\mu m`).
Parameters
----------
wavelength : numeric
Wavelength :math:`\lambda` in micrometers (:math:`\mu m`).
Returns
-------
numeric
Oxygen :math:`O_2` depolarisation.
Examples
--------
>>> O2_depolarisation(0.555) # doctest: +ELLIPSIS
1.1020225...
"""
wl = wavelength
O2 = (1.096 + 1.385 * 1.0e-3 * (1 / wl ** 2) +
1.448 * 1.0e-4 * (1 / wl ** 4))
return O2
[docs]def F_air_Penndorf1957(*args):
"""
Returns :math:`(6+3_p)/(6-7_p)`, the depolarisation term :math:`F(air)` or
*King Factor* using Penndorf (1957) method.
Parameters
----------
\*args : \*
Arguments.
Returns
-------
numeric
Air depolarisation.
See Also
--------
F_air_Young1981, F_air_Bates1984, F_air_Bodhaine1999
Notes
-----
- The argument *wavelength* is only provided for consistency with the
other air depolarisation methods but is actually not used as this
definition is essentially a constant in its current implementation.
Examples
--------
>>> F_air_Penndorf1957(0.555)
1.0608
"""
return 1.0608
[docs]def F_air_Young1981(*args):
"""
Returns :math:`(6+3_p)/(6-7_p)`, the depolarisation term :math:`F(air)` or
*King Factor* using Young (1981) method.
Parameters
----------
\*args : \*
Arguments.
Returns
-------
numeric
Air depolarisation.
See Also
--------
F_air_Penndorf1957, F_air_Bates1984, F_air_Bodhaine1999
Notes
-----
- The argument *wavelength* is only provided for consistency with the
other air depolarisation methods but is actually not used as this
definition is essentially a constant in its current implementation.
Examples
--------
>>> F_air_Young1981(0.555)
1.048
"""
return 1.0480
[docs]def F_air_Bates1984(wavelength):
"""
Returns :math:`(6+3_p)/(6-7_p)`, the depolarisation term :math:`F(air)` or
*King Factor* as function of wavelength :math:`\lambda` in micrometers
(:math:`\mu m`) using Bates (1984) method.
Parameters
----------
wavelength : numeric
Wavelength :math:`\lambda` in micrometers (:math:`\mu m`).
Returns
-------
numeric
Air depolarisation.
See Also
--------
F_air_Penndorf1957, F_air_Young1981, F_air_Bodhaine1999
Examples
--------
>>> F_air_Bates1984(0.555) # doctest: +ELLIPSIS
1.0481535...
"""
wl = wavelength
O2 = O2_depolarisation(wl)
N2 = N2_depolarisation(wl)
Ar = 1.00
CO2 = 1.15
F_air = ((78.084 * N2 + 20.946 * O2 + CO2 + Ar) /
(78.084 + 20.946 + Ar + CO2))
return F_air
[docs]def F_air_Bodhaine1999(wavelength,
CO2_concentration=STANDARD_CO2_CONCENTRATION):
"""
Returns :math:`(6+3_p)/(6-7_p)`, the depolarisation term :math:`F(air)` or
*King Factor* as function of wavelength :math:`\lambda` in micrometers
(:math:`\mu m`) and :math:`CO_2` concentration in parts per million (ppm)
using Bodhaine, Wood, Dutton and Slusser (1999) method.
Parameters
----------
wavelength : numeric
Wavelength :math:`\lambda` in micrometers (:math:`\mu m`).
CO2_concentration : numeric, optional
:math:`CO_2` concentration in parts per million (ppm).
Returns
-------
numeric
Air depolarisation.
See Also
--------
F_air_Penndorf1957, F_air_Young1981, F_air_Bates1984
Examples
--------
>>> F_air_Bodhaine1999(0.555) # doctest: +ELLIPSIS
1.1246916...
"""
wl = wavelength
O2 = O2_depolarisation(wl)
N2 = N2_depolarisation(wl)
CO2_c = CO2_concentration
F_air = ((78.084 * N2 + 20.946 * O2 + 0.934 * 1 + CO2_c * 1.15) /
(78.084 + 20.946 + 0.934 + CO2_c))
return F_air
[docs]def molecular_density(temperature=STANDARD_AIR_TEMPERATURE,
avogadro_constant=AVOGADRO_CONSTANT):
"""
Returns the molecular density :math:`N_s` (molecules :math:`cm^{-3}`)
as function of air temperature :math:`T[K]` in kelvin degrees.
Parameters
----------
temperature : numeric, optional
Air temperature :math:`T[K]` in kelvin degrees.
avogadro_constant : numeric, optional
*Avogadro*'s number (molecules :math:`mol^{-1}`).
Returns
-------
numeric
Molecular density :math:`N_s` (molecules :math:`cm^{-3}`).
Notes
-----
- The *Avogadro*'s number used in this implementation is the one given by
by the Committee on Data for Science and Technology (CODATA):
:math:`6.02214179x10^{23}`, which is different from the reference [1]_
value :math:`6.0221367x10^{23}`.
Examples
--------
>>> molecular_density(288.15) # doctest: +ELLIPSIS
2.5469021...e+19
>>> molecular_density(288.15, 6.0221367e23) # doctest: +ELLIPSIS
2.5468999...e+19
"""
T = temperature
N_s = (avogadro_constant / 22.4141) * (273.15 / T) * (1 / 1000)
return N_s
[docs]def mean_molecular_weights(CO2_concentration=STANDARD_CO2_CONCENTRATION):
"""
Returns the mean molecular weights :math:`m_a` for dry air as function of
:math:`CO_2` concentration in parts per million (ppm).
Parameters
----------
CO2_concentration : numeric, optional
:math:`CO_2` concentration in parts per million (ppm).
Returns
-------
numeric
Mean molecular weights :math:`m_a` for dry air.
Examples
--------
>>> mean_molecular_weights() # doctest: +ELLIPSIS
28.9640166...
"""
CO2_c = CO2_concentration * 1.0e-6
m_a = 15.0556 * CO2_c + 28.9595
return m_a
[docs]def gravity_List1968(latitude=DEFAULT_LATITUDE, altitude=DEFAULT_ALTITUDE):
"""
Returns the gravity :math:`g` in :math:`cm/s_2` (gal) representative of the
mass-weighted column of air molecules above the site of given latitude and
altitude using List (1968) method.
Parameters
----------
latitude : numeric, optional
Latitude of the site in degrees.
altitude : numeric, optional
Altitude of the site in meters.
Returns
-------
numeric
Gravity :math:`g` in :math:`cm/s_2` (gal).
Examples
--------
>>> gravity_List1968() # doctest: +ELLIPSIS
978.0356070...
>>> gravity_List1968(0, 1500) # doctest: +ELLIPSIS
977.5726106...
Gravity :math:`g` for Paris:
>>> gravity_List1968(48.8567, 35) # doctest: +ELLIPSIS
980.9524178...
"""
cos2phi = np.cos(2 * np.radians(latitude))
# Sea level acceleration of gravity.
g0 = 980.6160 * (1 - 0.0026373 * cos2phi + 0.0000059 * cos2phi ** 2)
g = (g0 - (3.085462e-4 + 2.27e-7 * cos2phi) * altitude +
(7.254e-11 + 1.0e-13 * cos2phi) * altitude ** 2 -
(1.517e-17 + 6e-20 * cos2phi) * altitude ** 3)
return g
[docs]def scattering_cross_section(wavelength,
CO2_concentration=STANDARD_CO2_CONCENTRATION,
temperature=STANDARD_AIR_TEMPERATURE,
avogadro_constant=AVOGADRO_CONSTANT,
n_s=air_refraction_index_Bodhaine1999,
F_air=F_air_Bodhaine1999):
"""
Returns the scattering cross section per molecule :math:`\sigma` of dry air
as function of wavelength :math:`\lambda` in centimeters (cm) using given
:math:`CO_2` concentration in parts per million (ppm) and temperature
:math:`T[K]` in kelvin degrees following Van de Hulst (1957) method.
Parameters
----------
wavelength : numeric
Wavelength :math:`\lambda` in centimeters (cm).
CO2_concentration : numeric, optional
:math:`CO_2` concentration in parts per million (ppm).
temperature : numeric, optional
Air temperature :math:`T[K]` in kelvin degrees.
avogadro_constant : numeric, optional
*Avogadro*'s number (molecules :math:`mol^{-1}`).
n_s : object
Air refraction index :math:`n_s` computation method.
F_air : object
:math:`(6+3_p)/(6-7_p)`, the depolarisation term :math:`F(air)` or
*King Factor* computation method.
Returns
-------
numeric
Scattering cross section per molecule :math:`\sigma` of dry air.
Warning
-------
Unlike most objects of :mod:`colour.phenomenons.rayleigh` module,
:func:`colour.phenomenons.rayleigh.scattering_cross_section` expects
wavelength :math:`\lambda` to be expressed in centimeters (cm).
Examples
--------
>>> scattering_cross_section(555 * 10e-8) # doctest: +ELLIPSIS
4.6613309...e-27
"""
wl = wavelength
wl_micrometers = wl * 10e3
n_s = n_s(wl_micrometers)
N_s = molecular_density(temperature, avogadro_constant)
F_air = F_air(wl_micrometers, CO2_concentration)
sigma = (24 * np.pi ** 3 * (n_s ** 2 - 1) ** 2 /
(wl ** 4 * N_s ** 2 * (n_s ** 2 + 2) ** 2))
sigma *= F_air
return sigma
[docs]def rayleigh_optical_depth(wavelength,
CO2_concentration=STANDARD_CO2_CONCENTRATION,
temperature=STANDARD_AIR_TEMPERATURE,
pressure=AVERAGE_PRESSURE_MEAN_SEA_LEVEL,
latitude=DEFAULT_LATITUDE,
altitude=DEFAULT_ALTITUDE,
avogadro_constant=AVOGADRO_CONSTANT,
n_s=air_refraction_index_Bodhaine1999,
F_air=F_air_Bodhaine1999):
"""
Returns the rayleigh optical depth :math:`T_r(\lambda)` as function of
wavelength :math:`\lambda` in centimeters (cm).
Parameters
----------
wavelength : numeric
Wavelength :math:`\lambda` in centimeters (cm).
CO2_concentration : numeric, optional
:math:`CO_2` concentration in parts per million (ppm).
temperature : numeric, optional
Air temperature :math:`T[K]` in kelvin degrees.
pressure : numeric
Surface pressure :math:`P` of the measurement site.
latitude : numeric, optional
Latitude of the site in degrees.
altitude : numeric, optional
Altitude of the site in meters.
avogadro_constant : numeric, optional
*Avogadro*'s number (molecules :math:`mol^{-1}`).
n_s : object
Air refraction index :math:`n_s` computation method.
F_air : object
:math:`(6+3_p)/(6-7_p)`, the depolarisation term :math:`F(air)` or
*King Factor* computation method.
Returns
-------
numeric
Rayleigh optical depth :math:`T_r(\lambda)`.
Warning
-------
Unlike most objects of :mod:`colour.phenomenons.rayleigh` module,
:func:`colour.phenomenons.rayleigh.rayleigh_optical_depth` expects
wavelength :math:`\lambda` to be expressed in centimeters (cm).
Examples
--------
>>> rayleigh_optical_depth(555 * 10e-8) # doctest: +ELLIPSIS
0.1004070...
"""
CO2_c = CO2_concentration
sigma = scattering_cross_section(wavelength,
CO2_c,
temperature,
avogadro_constant,
n_s,
F_air)
# Conversion from pascal to dyne/cm2.
P = pressure * 10
m_a = mean_molecular_weights(CO2_c)
g = gravity_List1968(latitude, altitude)
T_R = sigma * (P * avogadro_constant) / (m_a * g)
return T_R
rayleigh_scattering = rayleigh_optical_depth
def rayleigh_scattering_spd(shape=DEFAULT_SPECTRAL_SHAPE,
CO2_concentration=STANDARD_CO2_CONCENTRATION,
temperature=STANDARD_AIR_TEMPERATURE,
pressure=AVERAGE_PRESSURE_MEAN_SEA_LEVEL,
latitude=DEFAULT_LATITUDE,
altitude=DEFAULT_ALTITUDE,
avogadro_constant=AVOGADRO_CONSTANT,
n_s=air_refraction_index_Bodhaine1999,
F_air=F_air_Bodhaine1999):
"""
Returns the rayleigh spectral power distribution for given spectral shape.
Parameters
----------
shape : SpectralShape, optional
Spectral shape used to create the rayleigh scattering spectral power
distribution.
CO2_concentration : numeric, optional
:math:`CO_2` concentration in parts per million (ppm).
temperature : numeric, optional
Air temperature :math:`T[K]` in kelvin degrees.
pressure : numeric
Surface pressure :math:`P` of the measurement site.
latitude : numeric, optional
Latitude of the site in degrees.
altitude : numeric, optional
Altitude of the site in meters.
avogadro_constant : numeric, optional
*Avogadro*'s number (molecules :math:`mol^{-1}`).
n_s : object
Air refraction index :math:`n_s` computation method.
F_air : object
:math:`(6+3_p)/(6-7_p)`, the depolarisation term :math:`F(air)` or
*King Factor* computation method.
Returns
-------
SpectralPowerDistribution
Rayleigh optical depth spectral power distribution.
Examples
--------
>>> rayleigh_scattering_spd() # doctest: +ELLIPSIS
<colour.colorimetry.spectrum.SpectralPowerDistribution object at 0x...>
"""
return SpectralPowerDistribution(
name=('Rayleigh Scattering - {0} ppm, {1} K, {2} Pa, {3} Degrees, '
'{4} m').format(CO2_concentration,
temperature,
pressure,
latitude,
altitude),
data=dict((wavelength, rayleigh_scattering(wavelength * 10e-8,
CO2_concentration,
temperature,
pressure,
latitude,
altitude,
avogadro_constant,
n_s,
F_air))
for wavelength in shape))
Colour 0.3