peacock-data-public-datasets-idc-cronscript
/
venv
/lib
/python3.10
/site-packages
/scipy
/constants
/_constants.py
""" | |
Collection of physical constants and conversion factors. | |
Most constants are in SI units, so you can do | |
print '10 mile per minute is', 10*mile/minute, 'm/s or', 10*mile/(minute*knot), 'knots' | |
The list is not meant to be comprehensive, but just convenient for everyday use. | |
""" | |
from __future__ import annotations | |
import math as _math | |
from typing import TYPE_CHECKING, Any | |
from ._codata import value as _cd | |
import numpy as _np | |
if TYPE_CHECKING: | |
import numpy.typing as npt | |
""" | |
BasSw 2006 | |
physical constants: imported from CODATA | |
unit conversion: see e.g., NIST special publication 811 | |
Use at own risk: double-check values before calculating your Mars orbit-insertion burn. | |
Some constants exist in a few variants, which are marked with suffixes. | |
The ones without any suffix should be the most common ones. | |
""" | |
__all__ = [ | |
'Avogadro', 'Boltzmann', 'Btu', 'Btu_IT', 'Btu_th', 'G', | |
'Julian_year', 'N_A', 'Planck', 'R', 'Rydberg', | |
'Stefan_Boltzmann', 'Wien', 'acre', 'alpha', | |
'angstrom', 'arcmin', 'arcminute', 'arcsec', | |
'arcsecond', 'astronomical_unit', 'atm', | |
'atmosphere', 'atomic_mass', 'atto', 'au', 'bar', | |
'barrel', 'bbl', 'blob', 'c', 'calorie', | |
'calorie_IT', 'calorie_th', 'carat', 'centi', | |
'convert_temperature', 'day', 'deci', 'degree', | |
'degree_Fahrenheit', 'deka', 'dyn', 'dyne', 'e', | |
'eV', 'electron_mass', 'electron_volt', | |
'elementary_charge', 'epsilon_0', 'erg', | |
'exa', 'exbi', 'femto', 'fermi', 'fine_structure', | |
'fluid_ounce', 'fluid_ounce_US', 'fluid_ounce_imp', | |
'foot', 'g', 'gallon', 'gallon_US', 'gallon_imp', | |
'gas_constant', 'gibi', 'giga', 'golden', 'golden_ratio', | |
'grain', 'gram', 'gravitational_constant', 'h', 'hbar', | |
'hectare', 'hecto', 'horsepower', 'hour', 'hp', | |
'inch', 'k', 'kgf', 'kibi', 'kilo', 'kilogram_force', | |
'kmh', 'knot', 'lambda2nu', 'lb', 'lbf', | |
'light_year', 'liter', 'litre', 'long_ton', 'm_e', | |
'm_n', 'm_p', 'm_u', 'mach', 'mebi', 'mega', | |
'metric_ton', 'micro', 'micron', 'mil', 'mile', | |
'milli', 'minute', 'mmHg', 'mph', 'mu_0', 'nano', | |
'nautical_mile', 'neutron_mass', 'nu2lambda', | |
'ounce', 'oz', 'parsec', 'pebi', 'peta', | |
'pi', 'pico', 'point', 'pound', 'pound_force', | |
'proton_mass', 'psi', 'pt', 'quecto', 'quetta', 'ronna', 'ronto', | |
'short_ton', 'sigma', 'slinch', 'slug', 'speed_of_light', | |
'speed_of_sound', 'stone', 'survey_foot', | |
'survey_mile', 'tebi', 'tera', 'ton_TNT', | |
'torr', 'troy_ounce', 'troy_pound', 'u', | |
'week', 'yard', 'year', 'yobi', 'yocto', | |
'yotta', 'zebi', 'zepto', 'zero_Celsius', 'zetta' | |
] | |
# mathematical constants | |
pi = _math.pi | |
golden = golden_ratio = (1 + _math.sqrt(5)) / 2 | |
# SI prefixes | |
quetta = 1e30 | |
ronna = 1e27 | |
yotta = 1e24 | |
zetta = 1e21 | |
exa = 1e18 | |
peta = 1e15 | |
tera = 1e12 | |
giga = 1e9 | |
mega = 1e6 | |
kilo = 1e3 | |
hecto = 1e2 | |
deka = 1e1 | |
deci = 1e-1 | |
centi = 1e-2 | |
milli = 1e-3 | |
micro = 1e-6 | |
nano = 1e-9 | |
pico = 1e-12 | |
femto = 1e-15 | |
atto = 1e-18 | |
zepto = 1e-21 | |
yocto = 1e-24 | |
ronto = 1e-27 | |
quecto = 1e-30 | |
# binary prefixes | |
kibi = 2**10 | |
mebi = 2**20 | |
gibi = 2**30 | |
tebi = 2**40 | |
pebi = 2**50 | |
exbi = 2**60 | |
zebi = 2**70 | |
yobi = 2**80 | |
# physical constants | |
c = speed_of_light = _cd('speed of light in vacuum') | |
mu_0 = _cd('vacuum mag. permeability') | |
epsilon_0 = _cd('vacuum electric permittivity') | |
h = Planck = _cd('Planck constant') | |
hbar = h / (2 * pi) | |
G = gravitational_constant = _cd('Newtonian constant of gravitation') | |
g = _cd('standard acceleration of gravity') | |
e = elementary_charge = _cd('elementary charge') | |
R = gas_constant = _cd('molar gas constant') | |
alpha = fine_structure = _cd('fine-structure constant') | |
N_A = Avogadro = _cd('Avogadro constant') | |
k = Boltzmann = _cd('Boltzmann constant') | |
sigma = Stefan_Boltzmann = _cd('Stefan-Boltzmann constant') | |
Wien = _cd('Wien wavelength displacement law constant') | |
Rydberg = _cd('Rydberg constant') | |
# mass in kg | |
gram = 1e-3 | |
metric_ton = 1e3 | |
grain = 64.79891e-6 | |
lb = pound = 7000 * grain # avoirdupois | |
blob = slinch = pound * g / 0.0254 # lbf*s**2/in (added in 1.0.0) | |
slug = blob / 12 # lbf*s**2/foot (added in 1.0.0) | |
oz = ounce = pound / 16 | |
stone = 14 * pound | |
long_ton = 2240 * pound | |
short_ton = 2000 * pound | |
troy_ounce = 480 * grain # only for metals / gems | |
troy_pound = 12 * troy_ounce | |
carat = 200e-6 | |
m_e = electron_mass = _cd('electron mass') | |
m_p = proton_mass = _cd('proton mass') | |
m_n = neutron_mass = _cd('neutron mass') | |
m_u = u = atomic_mass = _cd('atomic mass constant') | |
# angle in rad | |
degree = pi / 180 | |
arcmin = arcminute = degree / 60 | |
arcsec = arcsecond = arcmin / 60 | |
# time in second | |
minute = 60.0 | |
hour = 60 * minute | |
day = 24 * hour | |
week = 7 * day | |
year = 365 * day | |
Julian_year = 365.25 * day | |
# length in meter | |
inch = 0.0254 | |
foot = 12 * inch | |
yard = 3 * foot | |
mile = 1760 * yard | |
mil = inch / 1000 | |
pt = point = inch / 72 # typography | |
survey_foot = 1200.0 / 3937 | |
survey_mile = 5280 * survey_foot | |
nautical_mile = 1852.0 | |
fermi = 1e-15 | |
angstrom = 1e-10 | |
micron = 1e-6 | |
au = astronomical_unit = 149597870700.0 | |
light_year = Julian_year * c | |
parsec = au / arcsec | |
# pressure in pascal | |
atm = atmosphere = _cd('standard atmosphere') | |
bar = 1e5 | |
torr = mmHg = atm / 760 | |
psi = pound * g / (inch * inch) | |
# area in meter**2 | |
hectare = 1e4 | |
acre = 43560 * foot**2 | |
# volume in meter**3 | |
litre = liter = 1e-3 | |
gallon = gallon_US = 231 * inch**3 # US | |
# pint = gallon_US / 8 | |
fluid_ounce = fluid_ounce_US = gallon_US / 128 | |
bbl = barrel = 42 * gallon_US # for oil | |
gallon_imp = 4.54609e-3 # UK | |
fluid_ounce_imp = gallon_imp / 160 | |
# speed in meter per second | |
kmh = 1e3 / hour | |
mph = mile / hour | |
# approx value of mach at 15 degrees in 1 atm. Is this a common value? | |
mach = speed_of_sound = 340.5 | |
knot = nautical_mile / hour | |
# temperature in kelvin | |
zero_Celsius = 273.15 | |
degree_Fahrenheit = 1/1.8 # only for differences | |
# energy in joule | |
eV = electron_volt = elementary_charge # * 1 Volt | |
calorie = calorie_th = 4.184 | |
calorie_IT = 4.1868 | |
erg = 1e-7 | |
Btu_th = pound * degree_Fahrenheit * calorie_th / gram | |
Btu = Btu_IT = pound * degree_Fahrenheit * calorie_IT / gram | |
ton_TNT = 1e9 * calorie_th | |
# Wh = watt_hour | |
# power in watt | |
hp = horsepower = 550 * foot * pound * g | |
# force in newton | |
dyn = dyne = 1e-5 | |
lbf = pound_force = pound * g | |
kgf = kilogram_force = g # * 1 kg | |
# functions for conversions that are not linear | |
def convert_temperature( | |
val: npt.ArrayLike, | |
old_scale: str, | |
new_scale: str, | |
) -> Any: | |
""" | |
Convert from a temperature scale to another one among Celsius, Kelvin, | |
Fahrenheit, and Rankine scales. | |
Parameters | |
---------- | |
val : array_like | |
Value(s) of the temperature(s) to be converted expressed in the | |
original scale. | |
old_scale : str | |
Specifies as a string the original scale from which the temperature | |
value(s) will be converted. Supported scales are Celsius ('Celsius', | |
'celsius', 'C' or 'c'), Kelvin ('Kelvin', 'kelvin', 'K', 'k'), | |
Fahrenheit ('Fahrenheit', 'fahrenheit', 'F' or 'f'), and Rankine | |
('Rankine', 'rankine', 'R', 'r'). | |
new_scale : str | |
Specifies as a string the new scale to which the temperature | |
value(s) will be converted. Supported scales are Celsius ('Celsius', | |
'celsius', 'C' or 'c'), Kelvin ('Kelvin', 'kelvin', 'K', 'k'), | |
Fahrenheit ('Fahrenheit', 'fahrenheit', 'F' or 'f'), and Rankine | |
('Rankine', 'rankine', 'R', 'r'). | |
Returns | |
------- | |
res : float or array of floats | |
Value(s) of the converted temperature(s) expressed in the new scale. | |
Notes | |
----- | |
.. versionadded:: 0.18.0 | |
Examples | |
-------- | |
>>> from scipy.constants import convert_temperature | |
>>> import numpy as np | |
>>> convert_temperature(np.array([-40, 40]), 'Celsius', 'Kelvin') | |
array([ 233.15, 313.15]) | |
""" | |
# Convert from `old_scale` to Kelvin | |
if old_scale.lower() in ['celsius', 'c']: | |
tempo = _np.asanyarray(val) + zero_Celsius | |
elif old_scale.lower() in ['kelvin', 'k']: | |
tempo = _np.asanyarray(val) | |
elif old_scale.lower() in ['fahrenheit', 'f']: | |
tempo = (_np.asanyarray(val) - 32) * 5 / 9 + zero_Celsius | |
elif old_scale.lower() in ['rankine', 'r']: | |
tempo = _np.asanyarray(val) * 5 / 9 | |
else: | |
raise NotImplementedError("%s scale is unsupported: supported scales " | |
"are Celsius, Kelvin, Fahrenheit, and " | |
"Rankine" % old_scale) | |
# and from Kelvin to `new_scale`. | |
if new_scale.lower() in ['celsius', 'c']: | |
res = tempo - zero_Celsius | |
elif new_scale.lower() in ['kelvin', 'k']: | |
res = tempo | |
elif new_scale.lower() in ['fahrenheit', 'f']: | |
res = (tempo - zero_Celsius) * 9 / 5 + 32 | |
elif new_scale.lower() in ['rankine', 'r']: | |
res = tempo * 9 / 5 | |
else: | |
raise NotImplementedError("'%s' scale is unsupported: supported " | |
"scales are 'Celsius', 'Kelvin', " | |
"'Fahrenheit', and 'Rankine'" % new_scale) | |
return res | |
# optics | |
def lambda2nu(lambda_: npt.ArrayLike) -> Any: | |
""" | |
Convert wavelength to optical frequency | |
Parameters | |
---------- | |
lambda_ : array_like | |
Wavelength(s) to be converted. | |
Returns | |
------- | |
nu : float or array of floats | |
Equivalent optical frequency. | |
Notes | |
----- | |
Computes ``nu = c / lambda`` where c = 299792458.0, i.e., the | |
(vacuum) speed of light in meters/second. | |
Examples | |
-------- | |
>>> from scipy.constants import lambda2nu, speed_of_light | |
>>> import numpy as np | |
>>> lambda2nu(np.array((1, speed_of_light))) | |
array([ 2.99792458e+08, 1.00000000e+00]) | |
""" | |
return c / _np.asanyarray(lambda_) | |
def nu2lambda(nu: npt.ArrayLike) -> Any: | |
""" | |
Convert optical frequency to wavelength. | |
Parameters | |
---------- | |
nu : array_like | |
Optical frequency to be converted. | |
Returns | |
------- | |
lambda : float or array of floats | |
Equivalent wavelength(s). | |
Notes | |
----- | |
Computes ``lambda = c / nu`` where c = 299792458.0, i.e., the | |
(vacuum) speed of light in meters/second. | |
Examples | |
-------- | |
>>> from scipy.constants import nu2lambda, speed_of_light | |
>>> import numpy as np | |
>>> nu2lambda(np.array((1, speed_of_light))) | |
array([ 2.99792458e+08, 1.00000000e+00]) | |
""" | |
return c / _np.asanyarray(nu) | |