
[c           @` s  d  Z  d d l m Z m Z m Z m Z d d l Z d d l m	 Z	 m
 Z
 d e	 f d     YZ d e e
 f d	     YZ e d
 d d d d d d Z e d d d d d d d Z e d d d d d d d Z e d d d d d d d Z e d d  d! d" d# d d Z e d$ d% d& d' d d d Z e d( d) d* d+ d, d d Z e d- d. d/ d+ d, d d Z e d0 d1 d2 d+ d3 d d Z e d4 d5 d6 d+ d7 d d Z e d8 d9 d: d; d< d d Z e d= d> d? d@ dA d d Z e dB dC dD dE d d d Z e dF dG dH dI dJ d d Z e dK dL dM dN dO d d Z e dP dQ dR dS dT d d Z e dU dV dW dX dY d d Z e dZ d[ d\ d] d^ d d Z e d_ d` da db dc d d Z e dd de df dg d d d Z  e dh di dj e j! dk d d d Z" e dl dm dn do dp d d Z# e dq dr ds dt du d d Z$ e e j% e j& e j' e j' dv dw e j( e j' dv d dx Z) e e j% e j& e j' dy dz e j( dy d d{ Z* e e j% e j& e j' e j' dv d| e j( e j' dv d d} Z+ d S(~   u   
Astronomical and physics constants in SI units.  See :mod:`astropy.constants`
for a complete listing of constants defined in Astropy.
i    (   t   absolute_importt   divisiont   print_functiont   unicode_literalsNi   (   t   Constantt
   EMConstantt
   CODATA2014c           B` s   e  Z d  Z i  Z e   Z RS(   u   CODATA 2014(   t   __name__t
   __module__t   default_referencet	   _registryt   sett   _has_incompatible_units(    (    (    s;   lib/python2.7/site-packages/astropy/constants/codata2014.pyR      s   t   EMCODATA2014c           B` s   e  Z e j Z RS(    (   R   R   R   R
   (    (    (    s;   lib/python2.7/site-packages/astropy/constants/codata2014.pyR      s   u   hu   Planck constantgW9u   J sgfkehZf7t   systemu   siu   hbaru   Reduced Planck constantgx# 8g}Z <7u   k_Bu   Boltzmann constantg^t0;u   J / (K)gUd9u   cu   Speed of light in vacuumg   JxޱAu   m / (s)g        u   Gu   Gravitational constantg7^wX=u   m3 / (kg s2)gn<u   g0u    Standard acceleration of gravityg:#@u   m / s2u   m_pu   Proton massgq祭`:u   kggL+8u   m_nu   Neutron massgr`:u   m_eu   Electron massgay9gՓ8u   uu   Atomic massgUtq`:gz8u   sigma_sbu   Stefan-Boltzmann constantgB*Kqn>u   W / (K4 m2)gnb]KB=u   eu   Electron chargegp%ڤ<u   CgC0iS:u   eps0u   Electric constantg.Hvx=u   F/mu   N_Au   Avogadro's numberggK҅Du	   1 / (mol)g VBJ:Cu   Ru   Gas constantg;  @u   J / (K mol)gv!>u   Rydu   Rydberg constantg71rDdAu   1 / (m)gC8
?u   a0u   Bohr radiusgRԁ=u   mgU;u   muBu   Bohr magnetongͻUl&;u   J/Tghe99u   alphau   Fine-structure constantg,)}?u    gΎ}=u   atmu   Standard atmospherei͋ u   Pau   mu0u   Magnetic constantgHך>u   N/A2u   sigma_Tu    Thomson scattering cross-sectiong@:u   m2g%7>8u   b_wienu)   Wien wavelength displacement law constantgg?u   m Kg9u׭4>g      $@u   statCu   esui
   u   abCu   emuu   Fru   gauss(,   t   __doc__t
   __future__R    R   R   R   t   numpyt   npt   constantR   R   R   R   t   ht   hbart   k_Bt   ct   Gt   g0t   m_pt   m_nt   m_et   ut   sigma_sbt   et   eps0t   N_At   Rt   Rydt   a0t   muBt   alphat   atmt   pit   mu0t   sigma_Tt   b_wient   abbrevt   namet   valuet   uncertaintyt   e_esut   e_emut   e_gauss(    (    (    s;   lib/python2.7/site-packages/astropy/constants/codata2014.pyt   <module>   st   "				   