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albertmena authored Jan 9, 2024
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Showing 1 changed file with 10 additions and 7 deletions.
17 changes: 10 additions & 7 deletions docs/Utils/Conventions/index.rst
Original file line number Diff line number Diff line change
Expand Up @@ -84,16 +84,19 @@ Now we have to project the volume on the projection plane. As an example I have
:width: 200
:align: right



But as we know that our projection plane always has got its reference with X axis facing to the right and the Y axis looking down, we should rotate the projection obtained until it is well-referenced

+----------------------------------+----------------------------------+
| .. figure:: ../../../_static/images/Euler/Euler9.gif | ../../../_static/images/Euler/Euler10.gif |
| :width: 200 | :width: 200 |
| :align: center | :align: center |
| | |
| Descripción de la imagen 1 | Descripción de la imagen 2 |
+----------------------------------+----------------------------------+
.. figure:: ../../../_static/images/Euler/Euler9.gif
:alt: Euler9
:width: 200
:align: left

.. figure:: ../../../_static/images/Euler/Euler10.gif
:alt: Euler10
:width: 200
:align: right


In the las figures we can check the consistency of this reasoning. The projection with tilt=90, rot=90, psi=90 has been taken with SPIDER. As we can see the results are identical.
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