Changeset e964ab1 in sasmodels for doc/developer


Ignore:
Timestamp:
Oct 28, 2017 9:11:13 PM (7 years ago)
Author:
Paul Kienzle <pkienzle@…>
Branches:
master, core_shell_microgels, magnetic_model, ticket-1257-vesicle-product, ticket_1156, ticket_1265_superball, ticket_822_more_unit_tests
Children:
3d40839
Parents:
5f8b72b
Message:

reformat orientation docs to 80 columns

File:
1 edited

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  • doc/developer/overview.rst

    reda8b30 re964ab1  
    171171------------------------------------- 
    172172 
    173 For 2d data from oriented anisotropic particles, the mean particle orientation is defined by angles $\theta$, $\phi$ and $\Psi$, which 
    174 are not in general the same as similarly named angles in many form factors. The wikipedia page on Euler angles  
    175 (https://en.wikipedia.org/wiki/Euler_angles) lists the different conventions available. To quote: "Different authors may use different  
    176 sets of rotation axes to define Euler angles, or different names for the same angles. Therefore, any discussion employing Euler angles 
     173For 2d data from oriented anisotropic particles, the mean particle 
     174orientation is defined by angles $\theta$, $\phi$ and $\Psi$, which are not 
     175in general the same as similarly named angles in many form factors. The 
     176wikipedia page on Euler angles (https://en.wikipedia.org/wiki/Euler_angles) 
     177lists the different conventions available. To quote: "Different authors may 
     178use different sets of rotation axes to define Euler angles, or different 
     179names for the same angles. Therefore, any discussion employing Euler angles 
    177180should always be preceded by their definition." 
    178181 
    179 We are using the z-y-z convention with extrinsic rotations $\Psi-\theta-\phi$ for the particle orientation and $x-y-z$ convention with  
    180 extrinsic rotations $\psi-\theta-\phi$ for jitter, with jitter applied before particle orientation. 
    181  
    182 For numerical integration within form factors etc. sasmodels is mostly using Gaussian quadrature with 20, 76 or 150 points depending on  
    183 the model.  It also makes use of symmetries such as calculating only over one quadrant rather than the whole sphere.  There is often a  
    184 U-substitution replacing $\theta$ with $cos(\theta)$ which changes the limits of integration from 0 to $\pi/2$ to 0 to 1 and also conveniently  
    185 absorbs the $sin(\theta)$ scale factor in the integration.  This can cause confusion if checking equations to say include in a paper or thesis! 
    186 Most models use the same core kernel code expressed in terms of the rotated view (qa, qb, qc) for both the 1D and the 2D models, but there  
    187 are also historical quirks such as the parallelepiped model, which has a useless transformation representing j0(a qa) as j0(b qa a/b). 
     182We are using the z-y-z convention with extrinsic rotations $\Psi-\theta-\phi$ 
     183for the particle orientation and $x-y-z$ convention with extrinsic rotations 
     184$\psi-\theta-\phi$ for jitter, with jitter applied before particle 
     185orientation. 
     186 
     187For numerical integration within form factors etc. sasmodels is mostly using 
     188Gaussian quadrature with 20, 76 or 150 points depending on the model. It also 
     189makes use of symmetries such as calculating only over one quadrant rather 
     190than the whole sphere. There is often a U-substitution replacing $\theta$ 
     191with $cos(\theta)$ which changes the limits of integration from 0 to $\pi/2$ 
     192to 0 to 1 and also conveniently absorbs the $sin(\theta)$ scale factor in the 
     193integration. This can cause confusion if checking equations to say include in 
     194a paper or thesis! Most models use the same core kernel code expressed in 
     195terms of the rotated view (qa, qb, qc) for both the 1D and the 2D models, but 
     196there are also historical quirks such as the parallelepiped model, which has 
     197a useless transformation representing j0(a qa) as j0(b qa a/b). 
    188198 
    189199Useful testing routines include - 
    190200 
    191 :mod:`asymint` a direct implementation of the surface integral for certain models to get a more trusted value for the 1D integral using a reimplementation of the 2D kernel in python and mpmath  
    192 (which computes math functions to arbitrary precision). It uses $\theta$ ranging from 0 to $\pi$ and $\phi$ ranging from 0 to $2\pi$.  It perhaps would benefit 
    193 from including the U-substitution for theta. 
    194  
    195 :mod:`check1d` uses sasmodels 1D integration and compares that with a rectangle distribution in $\theta$ and $\phi$, with $\theta$ limits set to 
    196 $\pm90/\sqrt(3)$ and $\phi$ limits set to $\pm180/\sqrt(3)$   
    197 [The rectangle weight function uses the fact that the distribution width column is labelled sigma to decide  
    198 that the 1-sigma width of a rectangular distribution needs to be multiplied by $\sqrt(3)$ to get the corresponding gaussian equivalent,  
    199 or similar reasoning.]  This should rotate the sample through the entire $\theta-\phi$  
    200 surface according to the pattern that you see in jitter.py when you modify it to use 'rectangle' rather than 'gaussian' for its distribution  
    201 without changing the viewing angle. When computing the dispersity integral, weights are scaled by abs(cos(dtheta)) to account for the points in  
    202 phi getting closer together as dtheta increases.  This integrated dispersion is computed at a set of $(qx, qy)$ points $(q cos(\alpha), q sin(\alpha))$  
    203 at some angle $\alpha$ (currently angle=0) for each q used in the 1-D integration.  The individual q points should be equivalent to asymint rect-n  
    204 when the viewing angle is set to (theta,phi,psi) = (90, 0, 0). Such tests can help to validate that 2d intensity is consistent with 1d models. 
    205   
    206 :mod:`sascomp -sphere=n` uses the identical rectangular distribution to compute the pattern of the qx-qy grid.  You can see from triaxial_ellipsoid 
    207 that there may be something wrong conceptually since the pattern is no longer circular when the view (theta,phi,psi) is not (90, phi, 0).   
    208 check1d shows that it is different from the sasmodels 1D integral even when at theta=0, psi=0. Cross checking the values with asymint,  
    209 the sasmodels 1D integral is better at low q, though for very large structures there are not enough points in the integration for sasmodels 1D  
    210 to compute the high q 1D integral correctly. [Some of that may now be fixed?] 
    211  
    212 The :mod:`sascomp` utility can be used for 2d as well as 1d calculations to compare results for two sets of parameters or processor types, for example 
     201:mod:`asymint` a direct implementation of the surface integral for certain 
     202models to get a more trusted value for the 1D integral using a 
     203reimplementation of the 2D kernel in python and mpmath (which computes math 
     204functions to arbitrary precision). It uses $\theta$ ranging from 0 to $\pi$ 
     205and $\phi$ ranging from 0 to $2\pi$. It perhaps would benefit from including 
     206the U-substitution for theta. 
     207 
     208:mod:`check1d` uses sasmodels 1D integration and compares that with a 
     209rectangle distribution in $\theta$ and $\phi$, with $\theta$ limits set to 
     210$\pm90/\sqrt(3)$ and $\phi$ limits set to $\pm180/\sqrt(3)$ [The rectangle 
     211weight function uses the fact that the distribution width column is labelled 
     212sigma to decide that the 1-sigma width of a rectangular distribution needs to 
     213be multiplied by $\sqrt(3)$ to get the corresponding gaussian equivalent, or 
     214similar reasoning.] This should rotate the sample through the entire 
     215$\theta-\phi$ surface according to the pattern that you see in jitter.py when 
     216you modify it to use 'rectangle' rather than 'gaussian' for its distribution 
     217without changing the viewing angle. When computing the dispersity integral, 
     218weights are scaled by abs(cos(dtheta)) to account for the points in phi 
     219getting closer together as dtheta increases. This integrated dispersion is 
     220computed at a set of $(qx, qy)$ points $(q cos(\alpha), q sin(\alpha))$ at 
     221some angle $\alpha$ (currently angle=0) for each q used in the 1-D 
     222integration. The individual q points should be equivalent to asymint rect-n 
     223when the viewing angle is set to (theta,phi,psi) = (90, 0, 0). Such tests can 
     224help to validate that 2d intensity is consistent with 1d models. 
     225 
     226:mod:`sascomp -sphere=n` uses the identical rectangular distribution to 
     227compute the pattern of the qx-qy grid. You can see from triaxial_ellipsoid 
     228that there may be something wrong conceptually since the pattern is no longer 
     229circular when the view (theta,phi,psi) is not (90, phi, 0). check1d shows 
     230that it is different from the sasmodels 1D integral even when at theta=0, 
     231psi=0. Cross checking the values with asymint, the sasmodels 1D integral is 
     232better at low q, though for very large structures there are not enough points 
     233in the integration for sasmodels 1D to compute the high q 1D integral 
     234correctly. [Some of that may now be fixed?] 
     235 
     236The :mod:`sascomp` utility can be used for 2d as well as 1d calculations to 
     237compare results for two sets of parameters or processor types, for example 
    213238these two oriented cylinders here should be equivalent. 
    214239 
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