Skip to content
New issue

Have a question about this project? Sign up for a free GitHub account to open an issue and contact its maintainers and the community.

Sign up for GitHub

By clicking “Sign up for GitHub”, you agree to our terms of service and privacy statement. We’ll occasionally send you account related emails.

Already on GitHub? Sign in to your account

Add Cosmo docs for Euler #181

Merged
merged 3 commits into from
Jul 29, 2024
Merged

Add Cosmo docs for Euler #181

Changes from all commits
Commits
Show all changes
3 commits
Select commit Hold shift + click to select a range
5dff9e2
Update cosmo.md
jonasjucker Jul 29, 2024
e45ce37
GitHub Action: Apply external link format
jonasjucker Jul 29, 2024
4535d35
Update cosmo.md
jonasjucker Jul 29, 2024
File filter

Filter by extension

Filter by extension
Conversations
Failed to load comments.
Loading
Jump to
Jump to file
Failed to load files.
Loading
Diff view
Diff view
9 changes: 2 additions & 7 deletions docs/models/cosmo.md
View file
Open in desktop
Original file line number Diff line number Diff line change
Expand Up @@ -4,6 +4,7 @@ The COSMO model is a limited-area, non-hydrostatic model developed by a collabor

## Support status
C2SM currently facilitates the utilisation of COSMO on the [Piz Daint :material-open-in-new:](https://www.cscs.ch/computers/piz-daint){:target="_blank"} computing platform for CPU and GPU architectures. The `master` and `c2sm-features` branches are being continuously tested an Piz Daint.
On the ETHZ [Euler CLuster :material-open-in-new:](https://scicomp.ethz.ch/wiki/Euler){:target="_blank"} COSMO is supported for CPU architectures only.

The following table summarises the features ported to GPU and their correspoding namelist parameters.

Expand Down Expand Up @@ -103,7 +104,7 @@ git clone [email protected]:C2SM-RCM/cosmo.git
If you do not already have an SSH key set up for GitHub but would like to do so, follow the [instructions :material-open-in-new:](https://docs.github.com/en/authentication/connecting-to-github-with-ssh/generating-a-new-ssh-key-and-adding-it-to-the-ssh-agent){:target="_blank"}.

## Configure and compile
For configuring and building COSMO with Spack, please refer to the official spack-c2sm documentation, which provides instructions for [setting up a Spack instance :material-open-in-new:](https://c2sm.github.io/spack-c2sm/latest/QuickStart.html#at-cscs-daint-tsa-balfrin){:target="_blank"} and [installing COSMO :material-open-in-new:](https://c2sm.github.io/spack-c2sm/latest/QuickStart.html#cosmo){:target="_blank"} on Piz Daint.
For configuring and building COSMO with Spack, please refer to the official spack-c2sm documentation, which provides instructions for [setting up a Spack instance :material-open-in-new:](https://c2sm.github.io/spack-c2sm/latest/QuickStart.html#at-cscs-ethz-daint-tsa-balfrin-and-euler){:target="_blank"} and [installing COSMO :material-open-in-new:](https://c2sm.github.io/spack-c2sm/latest/QuickStart.html#cosmo){:target="_blank"} on Piz Daint and Euler Cluster.

## Related tools
In the [Tools](../tools/index.md) section, you will find relevant tools for working with COSMO:
Expand Down Expand Up @@ -162,9 +163,3 @@ Output 0.19 0.43 0.86 72.65
```
It provides information about how long all compute-PEs had to wait at the end of the simulation for all IO processors to finish writing data to disk.
This timer should be as small as possible.

### Zlib replacement for NetCDF compression
Online compression, enabled with the `lcompress_netcdf=.true.` parameter, uses the slower Zlib by default.
A speedup of a factor of two can be achieved by using Zlib_ng instead.
The `+zlib_ng` variant for building COSMO is required in combination with the command `spack load cosmo@master%pgi cosmo_target=gpu +zlib_ng` before execution.
Unfortunately, the convenient way of using RPATH for this feature is not possible.
Loading