[da5536f] | 1 | .. _orientation: |
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| 2 | |
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| 3 | Oriented particles |
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| 4 | ================== |
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| 5 | |
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| 6 | With two dimensional small angle diffraction data SasView will calculate scattering from |
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| 7 | oriented particles, applicable for example to shear flow or orientation in a magnetic field. |
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| 8 | |
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| 9 | In general we first need to define the mean, or a reference orientation of the particles with respect |
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| 10 | to the incoming neutron or X-ray beam. This is done using three angles: $\theta$ and $\phi$ define the |
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| 11 | orientation of the axis of the particle, angle $\Psi$ is defined as the orientation of the major |
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| 12 | axis of the particle cross section with respect to its starting position along the beam direction. |
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| 13 | The figures below are for an elliptical cross section cylinder, |
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| 14 | but may be applied analogously to other shapes of particle. |
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| 15 | |
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| 16 | .. note:: |
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| 17 | It is very important to note that these angles, in particular $\theta$ and $\phi$, are NOT in general |
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| 18 | the same as the $\theta$ and $\phi$ appearing in equations for the scattering form factor which gives |
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| 19 | the scattered intensity or indeed in the equation for scattering vector $Q$. |
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| 20 | The $\theta$ rotation must be applied before the $\phi$ rotation, else there is an ambiguity. |
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| 21 | |
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| 22 | .. figure:: |
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| 23 | orient_img/elliptical_cylinder_angle_definition.png |
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| 24 | |
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| 25 | Definition of angles for oriented elliptical cylinder, where axis_ratio b/a is shown >1, |
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| 26 | Note that rotation $\theta$, initially in the $xz$ plane, is carried out first, then |
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| 27 | rotation $\phi$ about the $z$ axis, finally rotation $\Psi$ is around the axis of the cylinder. |
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| 28 | The neutron or X-ray beam is along the $z$ axis. |
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| 29 | |
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| 30 | .. figure:: |
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| 31 | orient_img/elliptical_cylinder_angle_projection.png |
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| 32 | |
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| 33 | Some examples of the orientation angles for an elliptical cylinder, with $\Psi$ = 0. |
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| 34 | |
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| 35 | Having established the mean direction of the particle we can then apply angular orientation distributions. |
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| 36 | This is done by a numerical integration over a range of angles in a similar way to polydispersity for particle size. |
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| 37 | In the current version of sasview the orientational dispersity is defined with respect to the axes of the particle. |
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| 38 | |
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| 39 | The $\theta$ and $\phi$ parameters to orient the cylinder only appear in the model when fitting 2d data. |
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| 40 | On introducing "Orientational Distribution" in the angles, "distribution of theta" and "distribution of phi" parameters will |
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| 41 | appear. These are actually rotations about the axes $\delta_1$ and $\delta_2$ of the cylinder, the $b$ and $a$ axes of the |
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| 42 | cylinder cross section. (When $\theta = \phi = 0$ these are parallel to the $Y$ and $X$ axes of the instrument.) |
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| 43 | The third orientation distribution, in $\psi$, is about the $c$ axis of the particle. Some experimentation may be required to |
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| 44 | understand the 2d patterns fully. A number of different shapes of distribution are available, as described for polydispersity. |
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| 45 | |
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| 46 | Earlier versions of SasView had numerical integration issues in some circumstances when |
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| 47 | distributions passed through 90 degrees. The distributions in particle coordinates are more robust, but should still be approached |
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| 48 | with care for large ranges of angle. |
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| 49 | |
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| 50 | Note that the form factors for asymmetric particles are also performing numerical integrations over one or more variables, so |
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| 51 | care should be taken, especially with very large particles or more extreme aspect ratios. Users can experiment with the |
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| 52 | values of Npts and Nsigs, the number of steps used in the integration and the range spanned in number of standard deviations. |
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| 53 | The standard deviation is entered in units of degrees. For a rectangular (uniform) distribution the full width |
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| 54 | should be $\pm\sqrt(3)$ ~ 1.73 standard deviations. |
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| 55 | |
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| 56 | Where appropriate, for best numerical results, keep $a < b < c$ and the $\theta$ distribution narrower than the $\phi$ distribution. |
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| 57 | |
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| 58 | Some more detailed technical notes are provided in the Developer section of this manual. |
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| 59 | |
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| 60 | *Document History* |
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| 61 | |
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| 62 | | 2017-10-27 Richard Heenan |
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