
[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 e j d e j d e j d e j e j 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$ d% d& d d d Z e d' d( d) d* d+ d d Z e d, d- d. d* d+ d d Z e d/ d0 d1 d* d2 d d Z e d3 d4 d5 d* d6 d d Z e d7 d8 d9 d: d; d d Z e d< d= d> d? d@ d d Z e dA dB dC dD d d d Z e dE dF dG dH dI d d Z e dJ dK dL dM dN d d Z e dO dP dQ dR dS d d Z  e dT dU dV dW dX d d Z! e dY dZ d[ d\ d] d d Z" e d^ d_ d` da db d d Z# e dc dd de df d d d Z$ e dg dh di e j dj d d d Z% e dk dl dm dn do d d Z& e	 dp 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
   CODATA2010c           B` s,   e  Z d  Z i  Z e   Z e d d  Z RS(   u   CODATA 2010c      	   C` s+   t  t |   j |  | | | | | | |  S(   N(   t   superR   t   __new__(   t   clst   abbrevt   namet   valuet   unitt   uncertaintyt	   referencet   system(    (    s;   lib/python2.7/site-packages/astropy/constants/codata2010.pyR      s    N(   t   __name__t
   __module__t   default_referencet	   _registryt   sett   _has_incompatible_unitst   NoneR   (    (    (    s;   lib/python2.7/site-packages/astropy/constants/codata2010.pyR      s   	t   EMCODATA2010c           B` s   e  Z e j Z RS(    (   R   R   R   R   (    (    (    s;   lib/python2.7/site-packages/astropy/constants/codata2010.pyR      s   u   hu   Planck constantgY9u   J sgc[57R   u   siu   hbaru   Reduced Planck constantg      ?u   k_Bu   Boltzmann constantg~ͬ0;u   J / (K)g"z9u   cu   Speed of light in vacuumg   JxޱAu   m / (s)g        u   Gu   Gravitational constantg>,"LX=u   m3 / (kg s2)gV瞯=u   g0u    Standard acceleration of gravityg:#@u   m / s2u   m_pu   Proton massg"`:u   kgg=,J98u   m_nu   Neutron massg\ r`:u   m_eu   Electron massgǭy9gx8+8u   uu   Atomic massgG`q`:g7'B8u   sigma_sbu   Stefan-Boltzmann constantg@ט"Mqn>u   W / (K4 m2)g; M=u   eu   Electron chargegQڤ<u   CgTq:u   eps0u   Electric constantg.Hvx=u   F/mu   N_Au   Avogadro's numbergjDu	   1 / (mol)g ;WCu   Ru   Gas constantg&- @u   J / (K mol)giUMu>u   Rydu   Rydberg constantgx1rDdAu   1 / (m)gK8?u   a0u   Bohr radiusg:Zԁ=u   mgJ;u   muBu   Bohr magnetong}Ul&;u   J/Tghe99u   alphau   Fine-structure constantgi'*}?u    g7Q=u   atmu   Standard atmospherei͋ u   Pau   mu0u   Magnetic constantgHך>u   N/A2u   sigma_Tu    Thomson scattering cross-sectiong:u   m2g9pLF8u   b_wienu)   Wien wavelength displacement law constantg=	ӌg?u   m Kg(JuU&>u   CODATA 2010g      $@u   statCu   esui
   u   abCu   emuu   Fru   gauss(-   t   __doc__t
   __future__R    R   R   R   t   numpyt   npt   constantR   R   R   R   t   hR   t   piR   R   t   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   mu0t   sigma_Tt   b_wienR
   R   t   e_esut   e_emut   e_gauss(    (    (    s;   lib/python2.7/site-packages/astropy/constants/codata2010.pyt   <module>   sv   "																   