----- header of sync_f.pro extracted on: Fri May 31 15:31:07 2013

----- Documentation for /scisoft/xop2.3/src_idl/sources/sync_f.pro -----
 NAME:
       SYNC_F

 PURPOSE:
       Calculates the function used for calculating the angular 
	dependence of synchrotron radiation. 

 CATEGORY:
       Mathematics.

 CALLING SEQUENCE:
       Result = sync_f(rAngle [,rEnergy] )

 INPUTS:
       rAngle:  the reduced angle, i.e., angle[rads]*Gamma. It can be a
		scalar or a vector.
 OPTIONAL INPUTS:
       rEnergy:  a value for the reduced photon energy, i.e., 
		energy/critical_energy. It can be an scalar or a verctor. 
		If this input is present, the calculation is done for this 
		energy. Otherwise, the calculation results is the integration 
		over all photon energies.

 KEYWORD PARAMETERS:
	POLARIZATION: 0 Total 
		      1 Parallel       (l2=1, l3=0, in Sokolov&Ternov notation)
		      2 Perpendicular  (l2=0, l3=1)

	L2: The polarization value of L2
	L3: The polarization value of L3
		Note: If using L2 and L3, both L2 and L3 must be defined.
		      In this case, the Pol keyword is ignored.

	GAUSS: When this keyword is set, the "Gaussian" approximaxion 
		instead of the full calculation is used. 
		Only valid for integrated flux aver all photon energies.
 OUTPUTS:
       returns the value  of the sync_f function
		It is a scalar if both inputs are scalar. If one input
		is an array, the result is an array of the same dimension. 
		If both inputs are arrays, the resulting array has dimension
		NxM, N=Dim(rAngle) and M=Dim(rEnergy)

 PROCEDURE:
       The number of emitted photons versus vertical angle Psi is
	proportional to sync_f, which value is given by the formulas
	in the references.

	For angular distribution integrated over full photon energies (rEnergy 
	optional input not present) we use the Formula 9, pag 4 in Green. 
	For its gaussian approximation (in this case the polarization keyword 
	has no effect) we use for 87 in pag 32 in Green.

	For angular distribution at a given photon energy (rEnergy 
	optional input not present) we use the Formula 11, pag 6 in Green. 


	References: 
		G K Green, "Spectra and optics of synchrotron radiation" 
			BNL 50522 report (1976)
		A A Sokolov and I M Ternov, Synchrotron Radiation, 
			Akademik-Verlag, Berlin, 1968

 OUTPUTS:
       returns the value  of the sync_hi function

 PROCEDURE:
       Uses IDL's BeselK() function

 MODIFICATION HISTORY:
       Written by:     M. Sanchez del Rio, srio@esrf.fr, 2002-05-23
	2002-07-12 srio@esrf.fr adds circular polarization term for 
		wavelength integrated spectrum (S&T formula 5.25)