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mlz
BornAgain
Commits
8bda6c90
Commit
8bda6c90
authored
2 years ago
by
Wuttke, Joachim
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correct paths to galaxi figures
parent
f04812cd
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!1543
changes from r20.0
,
!1530
correct paths to drawings
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hugo/content/py/fitting/instrument-description/index.md
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hugo/content/py/fitting/instrument-description/index.md
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8bda6c90
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@@ -22,7 +22,7 @@ Our sample represents a 3-layer system (substrate, teflon and air)
with Ag nanoparticles sitting on top of the teflon layer.
The PILATUS 1M detector was placed at a distance of 1730 mm from the sample.
{{
<
figscg
src=
"
.
/setup_galaxi_experiment.png"
class=
"center"
>
}}
{{
<
figscg
src=
"
/img/draw
/setup_galaxi_experiment.png"
class=
"center"
>
}}
The results of the measurement are represented by the intensity image taken in certain conditions
(beam wavelength, inclination angle, detector position) and stored in a 32-bit tiff file. To be able to fit these data we have to
...
...
@@ -77,8 +77,8 @@ simulation.setRegionOfInterest(85.0, 70.0, 120.0, 92.)
```
{{
<
galleryscg
>
}}
{{
<
figscg
src=
"
.
/galaxi_imported_data.png"
width=
"350px"
class=
"center"
>
}}
{{
<
figscg
src=
"
.
/galaxi_cropped_data.png"
width=
"350px"
class=
"center"
>
}}
{{
<
figscg
src=
"
/img/draw
/galaxi_imported_data.png"
width=
"350px"
class=
"center"
>
}}
{{
<
figscg
src=
"
/img/draw
/galaxi_cropped_data.png"
width=
"350px"
class=
"center"
>
}}
{{
<
/
galleryscg
>
}}
The final simulation setup looks as follows:
...
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