Changeset 8cc9048 in sasview for src/sas/sasgui/perspectives/calculator/media/resolution_calculator_help.rst
- Timestamp:
- Jan 12, 2018 12:24:18 PM (7 years ago)
- Branches:
- master, magnetic_scatt, release-4.2.2, ticket-1009, ticket-1094-headless, ticket-1242-2d-resolution, ticket-1243, ticket-1249, ticket885, unittest-saveload
- Children:
- 4b4b746
- Parents:
- a40e913
- File:
-
- 1 edited
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src/sas/sasgui/perspectives/calculator/media/resolution_calculator_help.rst
r5ed76f8 r8cc9048 29 29 careful to note that distances are specified in cm! 30 30 31 4) Enter values for the source wavelength(s), $\lambda$, and its spread (= $\ text{FWHM}/\lambda$).31 4) Enter values for the source wavelength(s), $\lambda$, and its spread (= $\mathrm{FWHM}/\lambda$). 32 32 33 33 For monochromatic sources, the inputs are just one value. For TOF sources, … … 58 58 region near the beam block/stop 59 59 60 [i.e., $Q < (2 \pi \cdot \ text{beam block diameter}) / (\text{sample-to-detector distance} \cdot \lambda_\text{min})$]60 [i.e., $Q < (2 \pi \cdot \mathrm{beam block diameter}) / (\mathrm{sample-to-detector distance} \cdot \lambda_\mathrm{min})$] 61 61 62 62 the variance is slightly under estimated.
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