Ignore:
Timestamp:
Jan 12, 2018 12:24:18 PM (7 years ago)
Author:
Adam Washington <adam.washington@…>
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
Message:

Remove all instances of \text from the repo

File:
1 edited

Legend:

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  • src/sas/sasgui/perspectives/calculator/media/resolution_calculator_help.rst

    r5ed76f8 r8cc9048  
    2929   careful to note that distances are specified in cm! 
    3030 
    31 4) Enter values for the source wavelength(s), $\lambda$, and its spread (= $\text{FWHM}/\lambda$). 
     314) Enter values for the source wavelength(s), $\lambda$, and its spread (= $\mathrm{FWHM}/\lambda$). 
    3232 
    3333   For monochromatic sources, the inputs are just one value. For TOF sources, 
     
    5858   region near the beam block/stop 
    5959 
    60    [i.e., $Q < (2 \pi \cdot \text{beam block diameter}) / (\text{sample-to-detector distance} \cdot \lambda_\text{min})$] 
     60   [i.e., $Q < (2 \pi \cdot \mathrm{beam block diameter}) / (\mathrm{sample-to-detector distance} \cdot \lambda_\mathrm{min})$] 
    6161 
    6262   the variance is slightly under estimated. 
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