# Tutorial:Visualization

In this tutorial we will explain how to visualize outputs from Octopus. Several different file formats are available in Octopus that are suitable for a variety of visualization software. We will not cover all of them here. See Manual:Visualization for more information.

## Benzene molecule

As an example, we will use the benzene molecule. At this point, the input should be quite familiar to you:

`CalculationMode`

= gs`UnitsOutput`

= eV_Angstrom`Radius`

= 5*angstrom`Spacing`

= 0.15*angstrom`Output`

= wfs + density + elf + potential`OutputFormat`

= cube + xcrysden + dx + axis_x + plane_z`XYZCoordinates`

= "benzene.xyz"

Coordinates are in this case given in the ** benzene.xyz** file. This file should look like:

12 Geometry of benzene (in Angstrom) C 0.000 1.396 0.000 C 1.209 0.698 0.000 C 1.209 -0.698 0.000 C 0.000 -1.396 0.000 C -1.209 -0.698 0.000 C -1.209 0.698 0.000 H 0.000 2.479 0.000 H 2.147 1.240 0.000 H 2.147 -1.240 0.000 H 0.000 -2.479 0.000 H -2.147 -1.240 0.000 H -2.147 1.240 0.000

Here we have used two new input variables:

`Output`

: this tells Octopus what quantities to output.`OutputFormat`

: specifies the format of the output files.

In this case we ask Octopus to output the wavefunctions (`wfs`), the density, the electron localization function (`elf`) and the Kohn-Sham potential. We ask Octopus to generate this output in several formats, that are required for the different visualization tools that we mention below. If you want to save some disk space you can just keep the option that corresponds to the program you will use. Take a look at the documentation on variables `Output`

and `OutputFormat`

for the full list of possible quantities to output and formats to visualize them in.

If you now run Octopus with this input file, you should get the following files in the ** static** directory:

%ls static convergence forces vh.z=0 wf-st0001.cube wf-st0003.dx wf-st0005.xsf wf-st0007.y=0,z=0 wf-st0009.z=0 wf-st0012.cube wf-st0014.dx density.cube info vks.cube wf-st0001.dx wf-st0003.xsf wf-st0005.y=0,z=0 wf-st0007.z=0 wf-st0010.cube wf-st0012.dx wf-st0014.xsf density.dx v0.cube vks.dx wf-st0001.xsf wf-st0003.y=0,z=0 wf-st0005.z=0 wf-st0008.cube wf-st0010.dx wf-st0012.xsf wf-st0014.y=0,z=0 density.xsf v0.dx vks.xsf wf-st0001.y=0,z=0 wf-st0003.z=0 wf-st0006.cube wf-st0008.dx wf-st0010.xsf wf-st0012.y=0,z=0 wf-st0014.z=0 density.y=0,z=0 v0.xsf vks.y=0,z=0 wf-st0001.z=0 wf-st0004.cube wf-st0006.dx wf-st0008.xsf wf-st0010.y=0,z=0 wf-st0012.z=0 wf-st0015.cube density.z=0 v0.y=0,z=0 vks.z=0 wf-st0002.cube wf-st0004.dx wf-st0006.xsf wf-st0008.y=0,z=0 wf-st0010.z=0 wf-st0013.cube wf-st0015.dx elf_rs.cube v0.z=0 vxc.cube wf-st0002.dx wf-st0004.xsf wf-st0006.y=0,z=0 wf-st0008.z=0 wf-st0011.cube wf-st0013.dx wf-st0015.xsf elf_rs.dx vh.cube vxc.dx wf-st0002.xsf wf-st0004.y=0,z=0 wf-st0006.z=0 wf-st0009.cube wf-st0011.dx wf-st0013.xsf wf-st0015.y=0,z=0 elf_rs.xsf vh.dx vxc.xsf wf-st0002.y=0,z=0 wf-st0004.z=0 wf-st0007.cube wf-st0009.dx wf-st0011.xsf wf-st0013.y=0,z=0 wf-st0015.z=0 elf_rs.y=0,z=0 vh.xsf vxc.y=0,z=0 wf-st0002.z=0 wf-st0005.cube wf-st0007.dx wf-st0009.xsf wf-st0011.y=0,z=0 wf-st0013.z=0 elf_rs.z=0 vh.y=0,z=0 vxc.z=0 wf-st0003.cube wf-st0005.dx wf-st0007.xsf wf-st0009.y=0,z=0 wf-st0011.z=0 wf-st0014.cube

## Visualization

### Gnuplot

Visualization of the fields in 3-dimensions is complicated. In many cases it is more useful to plot part of the data, for example the values of a scalar field along a line of plane that can be displayed as a 1D or 2D plot.

The `gnuplot` program is very useful for making these types of plots (and many more) and can directly read Octopus output. First type `gnuplot` to enter the program's command line. Now to plot a the density along a line (the X axis in this case) type

plot "static/density.y=0,z=0" w l

To plot a 2D field, for example the density in the plane z=0, you can use the command

splot "static/density.z=0" w l

If you want to get a color scale for the values of the field use "`w pm3d`" instead of "`w l`".

### VisIt

The program VisIt is an open-source data visualizer developed by Lawrence Livermore National Laborartory. It supports multiple platforms including Linux, OS X and Windows, most likely you can download a precompiled version for your platform here.

For this tutorial you need to have Visit installed and running. VisIt can read several formats, the most convenient for Octopus data is the `cube` format: `OutputFormat`

= `cube`. This is a common format that can be read by several visualization and analysis programs, it has the advantage that includes both the requested scalar field and the geometry in the same file. Visit can also read other formats that Octopus can generate like `xyz`, `XSF` (partial support), and `VTK`.

The following video contains the instruction on how to open a `cube` file in VisIt. Note that the video has subtitles in case you don't have audio in your current location, you can enable them by clicking the "CC" button.

### XCrySDen

Atomic coordinates (finite or periodic), forces, and functions on a grid can be plotted with the free program XCrySDen. Its XSF format also can be read by V_Sim and Vesta. Beware, these all probably assume that your output is in Angstrom units (according to the specification), so use `UnitsOutput`

= eV_Angstrom, or your data will be misinterpreted by the visualization software.

### UCSF Chimera

Those ** .dx** files can be also be opened by UCSF Chimera.

Once having UCSF Chimera installed and opened, open the benzene.xyz file from **File > Open**.

To open the ** .dx** file, go to

**Tools > Volume Data > Volume Viewer**. A new window opens. There go to

**File > Open**and select

**.**

`static/density.dx`To "color" the density go to **Tools > Surface Color**. A new dialog opens and there choose **Browse** to open the vh.dx file. Then click **Color** and you should have an image similar to the below one.