original_docstring: 
      Return the scattered intensity in a plane normal to the incident light.
  
      This is the scattered intensity in a plane that is perpendicular to the
      field of the incident plane wave. The intensity is normalized such
      that the integral of the unpolarized intensity over 4pi steradians
      is equal to the single scattering albedo.
  
      Args:
         m: the complex index of refraction of the sphere
         x: the size parameter of the sphere
         mu: the angles, cos(theta), to calculate intensities
  
      Returns
         The intensity at each angle in the array mu.  Units [1/sr]
      
docstring: Return the scattered intensity in a plane normal to the incident light.
  This is the scattered intensity in a plane that is perpendicular to the
  field of the incident plane wave. The intensity is normalized such
  that the integral of the unpolarized intensity over 4pi steradians
  is equal to the single scattering albedo.
docstring_tokens: Return the scattered intensity in a plane normal to the incident light . This is the scattered intensity in a plane that is perpendicular to the field of the incident plane wave . The intensity is normalized such that the integral of the unpolarized intensity over 4pi steradians is equal to the single scattering albedo .
code: def i_per(m, x, mu):
      """
      Return the scattered intensity in a plane normal to the incident light.
  
      This is the scattered intensity in a plane that is perpendicular to the
      field of the incident plane wave. The intensity is normalized such
      that the integral of the unpolarized intensity over 4pi steradians
      is equal to the single scattering albedo.
  
      Args:
         m: the complex index of refraction of the sphere
         x: the size parameter of the sphere
         mu: the angles, cos(theta), to calculate intensities
  
      Returns
         The intensity at each angle in the array mu.  Units [1/sr]
      """
      s1, _ = mie_S1_S2(m, x, mu)
      intensity = abs(s1)**2
      return intensity.astype('float')
code_tokens: def i_per ( m , x , mu ) : s1 , _ = mie_S1_S2 ( m , x , mu ) intensity = abs ( s1 ) ** 2 return intensity . astype ( 'float' )
short_docstring: Return the scattered intensity in a plane normal to the incident light.
short_docstring_tokens: Return the scattered intensity in a plane normal to the incident light .
comment: """
      Return the scattered intensity in a plane normal to the incident light.
  
      This is the scattered intensity in a plane that is perpendicular to the
      field of the incident plane wave. The intensity is normalized such
      that the integral of the unpolarized intensity over 4pi steradians
      is equal to the single scattering albedo.
  
      Args:
         m: the complex index of refraction of the sphere
         x: the size parameter of the sphere
         mu: the angles, cos(theta), to calculate intensities
  
      Returns
         The intensity at each angle in the array mu.  Units [1/sr]
      """