|
""" |
|
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. |
|
""" |
|
|
|
import math as _math |
|
from typing import TYPE_CHECKING, Any |
|
|
|
from ._codata import value as _cd |
|
|
|
if TYPE_CHECKING: |
|
import numpy.typing as npt |
|
|
|
from scipy._lib._array_api import array_namespace, _asarray |
|
|
|
|
|
""" |
|
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' |
|
] |
|
|
|
|
|
|
|
pi = _math.pi |
|
golden = golden_ratio = (1 + _math.sqrt(5)) / 2 |
|
|
|
|
|
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 |
|
|
|
|
|
kibi = 2**10 |
|
mebi = 2**20 |
|
gibi = 2**30 |
|
tebi = 2**40 |
|
pebi = 2**50 |
|
exbi = 2**60 |
|
zebi = 2**70 |
|
yobi = 2**80 |
|
|
|
|
|
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 = _cd('reduced Planck constant') |
|
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') |
|
|
|
|
|
gram = 1e-3 |
|
metric_ton = 1e3 |
|
grain = 64.79891e-6 |
|
lb = pound = 7000 * grain |
|
blob = slinch = pound * g / 0.0254 |
|
slug = blob / 12 |
|
oz = ounce = pound / 16 |
|
stone = 14 * pound |
|
long_ton = 2240 * pound |
|
short_ton = 2000 * pound |
|
|
|
troy_ounce = 480 * grain |
|
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') |
|
|
|
|
|
degree = pi / 180 |
|
arcmin = arcminute = degree / 60 |
|
arcsec = arcsecond = arcmin / 60 |
|
|
|
|
|
minute = 60.0 |
|
hour = 60 * minute |
|
day = 24 * hour |
|
week = 7 * day |
|
year = 365 * day |
|
Julian_year = 365.25 * day |
|
|
|
|
|
inch = 0.0254 |
|
foot = 12 * inch |
|
yard = 3 * foot |
|
mile = 1760 * yard |
|
mil = inch / 1000 |
|
pt = point = inch / 72 |
|
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 |
|
|
|
|
|
atm = atmosphere = _cd('standard atmosphere') |
|
bar = 1e5 |
|
torr = mmHg = atm / 760 |
|
psi = pound * g / (inch * inch) |
|
|
|
|
|
hectare = 1e4 |
|
acre = 43560 * foot**2 |
|
|
|
|
|
litre = liter = 1e-3 |
|
gallon = gallon_US = 231 * inch**3 |
|
|
|
fluid_ounce = fluid_ounce_US = gallon_US / 128 |
|
bbl = barrel = 42 * gallon_US |
|
|
|
gallon_imp = 4.54609e-3 |
|
fluid_ounce_imp = gallon_imp / 160 |
|
|
|
|
|
kmh = 1e3 / hour |
|
mph = mile / hour |
|
|
|
mach = speed_of_sound = 340.5 |
|
knot = nautical_mile / hour |
|
|
|
|
|
zero_Celsius = 273.15 |
|
degree_Fahrenheit = 1/1.8 |
|
|
|
|
|
eV = electron_volt = elementary_charge |
|
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 |
|
|
|
|
|
|
|
hp = horsepower = 550 * foot * pound * g |
|
|
|
|
|
dyn = dyne = 1e-5 |
|
lbf = pound_force = pound * g |
|
kgf = kilogram_force = g |
|
|
|
|
|
|
|
|
|
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]) |
|
|
|
""" |
|
xp = array_namespace(val) |
|
_val = _asarray(val, xp=xp, subok=True) |
|
|
|
if old_scale.lower() in ['celsius', 'c']: |
|
tempo = _val + zero_Celsius |
|
elif old_scale.lower() in ['kelvin', 'k']: |
|
tempo = _val |
|
elif old_scale.lower() in ['fahrenheit', 'f']: |
|
tempo = (_val - 32) * 5 / 9 + zero_Celsius |
|
elif old_scale.lower() in ['rankine', 'r']: |
|
tempo = _val * 5 / 9 |
|
else: |
|
raise NotImplementedError(f"{old_scale=} is unsupported: supported scales " |
|
"are Celsius, Kelvin, Fahrenheit, and " |
|
"Rankine") |
|
|
|
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(f"{new_scale=} is unsupported: supported " |
|
"scales are 'Celsius', 'Kelvin', " |
|
"'Fahrenheit', and 'Rankine'") |
|
|
|
return res |
|
|
|
|
|
|
|
|
|
|
|
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]) |
|
|
|
""" |
|
xp = array_namespace(lambda_) |
|
return c / _asarray(lambda_, xp=xp, subok=True) |
|
|
|
|
|
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]) |
|
|
|
""" |
|
xp = array_namespace(nu) |
|
return c / _asarray(nu, xp=xp, subok=True) |
|
|