Changeset 3b349ee in sasview for src/sas/qtgui/Calculators/media/resolution_calculator_help.rst
- Timestamp:
- May 18, 2018 8:02:02 AM (7 years ago)
- Branches:
- ESS_GUI, ESS_GUI_batch_fitting, ESS_GUI_bumps_abstraction, ESS_GUI_iss1116, ESS_GUI_iss879, ESS_GUI_iss959, ESS_GUI_opencl, ESS_GUI_ordering, ESS_GUI_sync_sascalc
- Children:
- 0459591
- Parents:
- dbba134 (diff), 3aa3351 (diff)
Note: this is a merge changeset, the changes displayed below correspond to the merge itself.
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src/sas/qtgui/Calculators/media/resolution_calculator_help.rst
r417c03f r3aa3351 10 10 ----------- 11 11 12 This tool isapproximately estimates the resolution of $Q$ from SAS instrumental12 This tool approximately estimates the resolution of $Q$ from SAS instrumental 13 13 parameter values assuming that the detector is flat and normal to the 14 14 incident beam. … … 19 19 -------------- 20 20 21 1) Select * SASResolution Estimator* from the *Tool* menu on the SasView toolbar.21 1) Select *Q Resolution Estimator* from the *Tool* menu on the SasView toolbar. 22 22 23 2) Select the source (Neutron or Photon)and source type (Monochromatic or TOF).23 2) Select the source and source type (Monochromatic or TOF). 24 24 25 25 *NOTE! The computational difference between the sources is only the … … 35 35 range. 36 36 37 Optionally, the wavelength (BUT NOT ofthe wavelength spread) can be extended37 Optionally, the wavelength (BUT NOT the wavelength spread) can be extended 38 38 by adding '; nn' where the 'nn' specifies the number of the bins for the 39 39 numerical integration. The default value is nn = 10. The same number of bins … … 49 49 7) 1D and 2D $dQ$ values will be displayed at the bottom of the panel, and a 2D 50 50 resolution weight distribution (a 2D elliptical Gaussian function) will also 51 be displayed in the plot panel even if the $Q$ inputs are outside of the 52 detector limit (the red lines indicate the limits of the detector). 51 be displayed in the plot panel. 53 52 54 53 TOF only: green lines indicate the limits of the maximum $Q$ range accessible 55 54 for the longest wavelength due to the size of the detector. 56 55 57 Note that the effect from the beam block/stop is ignored , soin the small $Q$56 Note that the effect from the beam block/stop is ignored. So, in the small $Q$ 58 57 region near the beam block/stop 59 58 … … 63 62 64 63 8) A summary of the calculation is written to the SasView *Console* at the 65 bottom of the main SasView window .64 bottom of the main SasView window, below the plot. 66 65 67 .. image:: resolution_tutor.png 66 .. figure:: resolution_tutor.png 67 68 .. 69 70 1) Define the source. Select *Photon* for X-ray. This selection only affects 71 the gravitational contribution of the resolution 72 2) Select between *Monochromatic* or *TOF* 73 3) For *TOF*, there is the option 74 of loading a custom spectral distribution using *Add New* in the combo 75 box 76 4) *Wavelength* and *wavelength spread*: one value for *Monochromatic*, 77 minimum and maximum of range for *TOF* 78 5) For *Source* and *Sample Size Aperture*, one value for a circular 79 aperture (diameter) and two values separated by a comma (,) for a 80 rectangular slit (side lengths) 81 6) One value for one ($Qx$, $Qy$) location or more values separated by a 82 comma (,) for more locations. *Note: the $Qx$, $Qy$ input boxes should 83 have the same number of values.* 84 7) Click on *Compute* button to start the calculation 85 8) *Sigma_x* and *Sigma_y* are the components of the 2D $dQ$ at the last 86 ($Qx$, $Qy$) point of inputs 87 9) *Sigma_lamd* is the 2D $dQ_{\lambda}$ at the last point of inputs. 88 *Note: $dQ_{\lambda}$ has only the Qr directional component* 89 10) *(1D Sigma)* is the 1D $dQ$ at the last ($Qx$, $Qy$) point of inputs 90 11) Plot of the result. For *TOF*, a green rectangle marks the limits of 91 maximum $Q$ range accessible for the longest wavelength due to the 92 size of the detector. 68 93 69 94 .. ZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZ
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