Changes in / [e110cb0:c99e717] in sasview
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docs/sphinx-docs/source/conf.py
r3ca67dcf r8cc9048 224 224 \newcommand{\lt}{<} % HTML needs \lt rather than < 225 225 \newcommand{\gt}{>} % HTML needs \gt rather than > 226 \renewcommand{\AA}{\ text{\r{A}}} % Allow \AA in math mode226 \renewcommand{\AA}{\mathrm{\r{A}}} % Allow \AA in math mode 227 227 \DeclareUnicodeCharacter {212B} {\AA} % Angstrom 228 228 \DeclareUnicodeCharacter {00B7} {\ensuremath{\cdot}} % cdot -
src/sas/sasgui/perspectives/calculator/media/resolution_calculator_help.rst
r5ed76f8 r3bd58f0 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., $Q < (2 \pi \cdot w) / (d_s \cdot \lambda_\mathrm{min})$, where $w$ is the beam block diameter, $d_s$ is the sample-to-detector distance, and $\lambda_\mathrm{min}$ is the minimum wavelength.] 61 61 62 62 the variance is slightly under estimated. -
src/sas/sasgui/perspectives/calculator/media/sas_calculator_help.rst
r1b67f3e r55abe4f 88 88 89 89 Now let us assume that the angles of the $\vec Q$ vector and the spin-axis ($x'$) 90 to the $x$-axis are $\phi$ and $\theta_\ text{up}$ respectively (see above). Then,90 to the $x$-axis are $\phi$ and $\theta_\mathrm{up}$ respectively (see above). Then, 91 91 depending upon the polarization (spin) state of neutrons, the scattering 92 92 length densities, including the nuclear scattering length density ($\beta_N$) … … 107 107 .. math:: 108 108 109 M_{\perp x'} &= M_{0q_x}\cos\theta_\ text{up} + M_{0q_y}\sin\theta_\text{up} \\110 M_{\perp y'} &= M_{0q_y}\cos\theta_\ text{up} - M_{0q_x}\sin\theta_\text{up} \\109 M_{\perp x'} &= M_{0q_x}\cos\theta_\mathrm{up} + M_{0q_y}\sin\theta_\mathrm{up} \\ 110 M_{\perp y'} &= M_{0q_y}\cos\theta_\mathrm{up} - M_{0q_x}\sin\theta_\mathrm{up} \\ 111 111 M_{\perp z'} &= M_{0z} \\ 112 112 M_{0q_x} &= (M_{0x}\cos\phi - M_{0y}\sin\phi)\cos\phi \\ -
src/sas/sasgui/perspectives/corfunc/media/corfunc_help.rst
rad476d1 r501712f 188 188 * Average Hard Block Thickness :math:`= L_c` 189 189 * Average Core Thickness :math:`= D_0` 190 * Average Interface Thickness :math:` \text{}= D_{tr}`191 * Polydispersity :math:`= \Gamma_{\ text{min}}/\Gamma_{\text{max}}`190 * Average Interface Thickness :math:`= D_{tr}` 191 * Polydispersity :math:`= \Gamma_{\mathrm{min}}/\Gamma_{\mathrm{max}}` 192 192 * Local Crystallinity :math:`= L_c/L_p` 193 193 … … 203 203 * Bound Fraction :math:`= <p>` 204 204 * Second Moment :math:`= \sigma` 205 * Maximum Extent :math:`= \delta_{\ text{h}}`205 * Maximum Extent :math:`= \delta_{\mathrm{h}}` 206 206 * Adsorbed Amount :math:`= \Gamma` 207 207
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