r""" For information about polarised and magnetic scattering, see the :doc:`magnetic help <../sasgui/perspectives/fitting/mag_help>` documentation. Definition ---------- The 1D scattering intensity is calculated in the following way (Guinier, 1955) .. math:: I(q) = \frac{\text{scale}}{V} \cdot \left[ 3V(\Delta\rho) \cdot \frac{\sin(qr) - qr\cos(qr))}{(qr)^3} \right]^2 + \text{background} where *scale* is a volume fraction, $V$ is the volume of the scatterer, $r$ is the radius of the sphere, *background* is the background level and *sld* and *sld_solvent* are the scattering length densities (SLDs) of the scatterer and the solvent respectively. Note that if your data is in absolute scale, the *scale* should represent the volume fraction (which is unitless) if you have a good fit. If not, it should represent the volume fraction times a factor (by which your data might need to be rescaled). The 2D scattering intensity is the same as above, regardless of the orientation of $\vec q$. Validation ---------- Validation of our code was done by comparing the output of the 1D model to the output of the software provided by the NIST (Kline, 2006). References ---------- A Guinier and G. Fournet, *Small-Angle Scattering of X-Rays*, John Wiley and Sons, New York, (1955) *2013/09/09 and 2014/01/06 - Description reviewed by S King and P Parker.* """ import numpy as np from numpy import pi, inf, sin, cos, sqrt, log name = " _sphere (python)" title = "PAK testing ideas for Spheres with uniform scattering length density" description = """\ P(q)=(scale/V)*[3V(sld-sld_solvent)*(sin(qr)-qr cos(qr)) /(qr)^3]^2 + background r: radius of sphere V: The volume of the scatter sld: the SLD of the sphere sld_solvent: the SLD of the solvent """ category = "shape:sphere" # ["name", "units", default, [lower, upper], "type","description"], parameters = [["sld", "1e-6/Ang^2", 1, [-inf, inf], "", "Layer scattering length density"], ["sld_solvent", "1e-6/Ang^2", 6, [-inf, inf], "", "Solvent scattering length density"], ["radius", "Ang", 50, [0, inf], "volume", "Sphere radius"], ] def form_volume(radius): return 1.333333333333333 * pi * radius ** 3 def Iq(q, sld, sld_solvent, radius): #print "q",q #print "sld,r",sld,sld_solvent,radius qr = q * radius sn, cn = sin(qr), cos(qr) ## The natural expression for the bessel function is the following: ## bes = 3 * (sn-qr*cn)/qr**3 if qr>0 else 1 ## however, to support vector q values we need to handle the conditional ## as a vector, which we do by first evaluating the full expression ## everywhere, then fixing it up where it is broken. We should probably ## set numpy to ignore the 0/0 error before we do though... bes = 3 * (sn - qr * cn) / qr ** 3 # may be 0/0 but we fix that next line bes[qr == 0] = 1 fq = bes * (sld - sld_solvent) * form_volume(radius) return 1.0e-4 * fq ** 2 Iq.vectorized = True # Iq accepts an array of q values def Iqxy(qx, qy, sld, sld_solvent, radius): return Iq(sqrt(qx ** 2 + qy ** 2), sld, sld_solvent, radius) Iqxy.vectorized = True # Iqxy accepts arrays of qx, qy values def sesans(z, sld, sld_solvent, radius): """ Calculate SESANS-correlation function for a solid sphere. Wim Bouwman after formulae Timofei Kruglov J.Appl.Cryst. 2003 article """ d = z / radius g = np.zeros_like(z) g[d == 0] = 1. low = ((d > 0) & (d < 2)) dlow = d[low] dlow2 = dlow ** 2 g[low] = (sqrt(1 - dlow2/4.) * (1 + dlow2/8.) + dlow2/2.*(1 - dlow2/16.) * log(dlow / (2. + sqrt(4. - dlow2)))) return g sesans.vectorized = True # sesans accepts an array of z values def ER(radius): return radius # VR defaults to 1.0 demo = dict(scale=1, background=0, sld=6, sld_solvent=1, radius=120, radius_pd=.2, radius_pd_n=45)