Using cyclone: Difference between revisions
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<code>cyclone.hpc.uib.no</code> shares home directories with the new hexagon cluster. These home directories are separate from your standard UiB home directory. The contents of your home directories will not be synced, so you will manually need to transfer your scripts to the new system. | <code>cyclone.hpc.uib.no</code> shares home directories with the new hexagon cluster. These home directories are separate from your standard UiB home directory. The contents of your home directories will not be synced, so you will manually need to transfer your scripts to the new system. | ||
Please be aware that your local home directory is not expected to exceed 30GB at any time - even in periods when sys.adms. do not practice quotas. If you need to store larger amount of data, please plan for using the GFI&SKD storage - also decribed in this wiki. | |||
To monitor your home directory size, you can use these commands from cyclone command shell: | |||
<code>du -sh ~/ </code> | |||
Or to include more details on both dot files/directories and non-hidden home directory subfolders: | |||
<code>cd; du -sh .[^.]* *</code> | |||
Monitoring your homefolder quota, you can run the following command: | |||
<code>lfs quota -hp $(id -u) /shared/ </code> | |||
or just | |||
<code>lfs quota -hp $(id -u) $HOME </code> | |||
=== How to access software === | === How to access software === | ||
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* proj | * proj | ||
*: <code>PROJ/5.0.0-foss-2018b</code> | *: <code>PROJ/5.0.0-foss-2018b</code> | ||
=== Jupyter & Jupyterhub === | |||
Here is a step by step guide to setup and use Jupyter based on the <code>dynpie3</code> environment. | |||
[[File:Get started cyclone.pdf|thumb|Step by step guide for Jupyter on cyclone]] | |||
== Accessing the data from your own machines == | == Accessing the data from your own machines == | ||
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On MacOS you can mount folders through <code>Finder > Go > Connect to Server ...</code>. In the dialogue window that pops up, enter | On MacOS you can mount folders through <code>Finder > Go > Connect to Server ...</code>. In the dialogue window that pops up, enter | ||
<pre>smb://<user name>@ | <pre>smb://uib.no;<user name>@klient.uib.no/FELLES/MATNAT/GFI</pre> | ||
as the '''Server Address'''. You might want to replace <code>gfi</code> by <code>skd</code> to access the skd disks if that is your primary affiliation. | as the '''Server Address'''. You might want to replace <code>gfi</code> by <code>skd</code> to access the skd disks if that is your primary affiliation. | ||
On Ubuntu this is very similar: <code>Files > Go > Enter Location ...</code>. Enter the address: <pre>smb://<user name>@ | On Ubuntu this is very similar: <code>Files > Go > Enter Location ...</code>. Enter the address: <pre>smb://uib.no;<user name>@klient.uib.no/FELLES/MATNAT/GFI</pre> and enter your password in the next pop-up window, while keeping "UiB" in the "Domain" field. | ||
Alternatively you can mount the network drive with sshfs to a dedicated directory using <code>sshfs</code> (install with <code>sudo apt install sshfs</code>): | Alternatively you can mount the network drive with sshfs to a dedicated directory using <code>sshfs</code> (install with <code>sudo apt install sshfs</code>): | ||
<pre>mkdir ~/cyclone_gfi | <pre>mkdir ~/cyclone_gfi | ||
sshfs -o follow_symlinks <user name>@cyclone.hpc.uib.no:/gfi ~/cyclone_gfi/</pre> | From UiB network: sshfs -o follow_symlinks <user name>@cyclone.hpc.uib.no:/gfi/ ~/cyclone_gfi/ | ||
On Windows you can mount by navigating to <code>File Explorer > Map network drive</code> and enter <code>\\leo.hpc.uib.no\gfi</code>. Make sure to enable <code>Connect using different credentials</code> and fill in <code><user name>@uib.no</code> and your PW. | From ext. networks: sshfs -o follow_symlinks <user name>@sync.uib.no:/gfi/ ~/cyclone_gfi/ | ||
Unmount with: fusermount -u ~/cyclone_gfi</pre> | |||
On Windows you can mount by navigating to <code>File Explorer > Map network drive</code> and enter <code>\\leo.hpc.uib.no\gfi</code>. Make sure to enable <code>Connect using different credentials</code> and fill in <code><user name>@uib.no</code> and your PW. | |||
== Displaying GUIs on your screen == | == Displaying GUIs on your screen == |
Latest revision as of 10:50, 6 November 2024
Connection and first steps
Use ssh to connect
ssh -Y <username>@cyclone.hpc.uib.no
or just simply:
ssh -Y cyclone.hpc.uib.no
if you're connecting from a computer where you are logged in under the same name. When you are connecting for the first time, you will be asked to verify a signature. Reply "yes" to this question.
Home directories
cyclone.hpc.uib.no
shares home directories with the new hexagon cluster. These home directories are separate from your standard UiB home directory. The contents of your home directories will not be synced, so you will manually need to transfer your scripts to the new system.
Please be aware that your local home directory is not expected to exceed 30GB at any time - even in periods when sys.adms. do not practice quotas. If you need to store larger amount of data, please plan for using the GFI&SKD storage - also decribed in this wiki.
To monitor your home directory size, you can use these commands from cyclone command shell:
du -sh ~/
Or to include more details on both dot files/directories and non-hidden home directory subfolders:
cd; du -sh .[^.]* *
Monitoring your homefolder quota, you can run the following command:
lfs quota -hp $(id -u) /shared/
or just
lfs quota -hp $(id -u) $HOME
How to access software
In contrast to the old skd-cyclone, most scientific software is only available through software modules. Modules need to be loaded manually before the respective software can be used. We use software modules, because they provide are a clean and handy way to offer conflicting software or software versions: Instead of updating software and potentially breaking user scripts and programs new software is then made available in parallel to those that require it.
Start-up scripts
It might be handy to automatically load modules for software that you use frequently every time you login to cyclone. To accomplish that for bash, there are two relevant files, $HOME/.bashrc
and $HOME/.bash_profile
. .bash_profile
should contain things that need to be defined at login time only, like PATH
and other environment variables, startup programs, etc. You just need things once, not in every shell you open. In most cases, you also need the things from .bashrc
in your login shell. That's why .bash_profile
sources .bashrc
as well, but .bashrc doesn't usually source .bash_profile
. In contrast, .bashrc
should typically contain things you want to set in every shell you open, like aliases, functions, etc. These are per shell session items that are not inherited from environment (source and detailed explanation).
An example .bash_profile
for inspiration
module load cdo/1.6.9 module load ncarg/6.3.0-login alias rm="rm -i" alias cp="cp -i" alias erai="cd /Data/skd/share/Reanalysis/ERA_INTERIM/6HOURLY/" if [ -f ~/.bashrc ]; then . ~/.bashrc fi
An example .bash_profile
for inspiration
alias rm="rm -i" alias cp="cp -i" alias erai="cd /Data/skd/share/Reanalysis/ERA_INTERIM/6HOURLY/"
Available software
Below is a list of frequently used software and which module to load on the new cyclone. Relevant module names are printed like for matlab/2015b
. Modules can be loaded by module load <module name>
, and unloaded module unload <module name>
. More details on the module system.
To list all available modules, use the command
module avail
Hexagon-specific modules are now no longer listed and available on cyclone. All packages listed with this command should work, so please report to support@hpc.uib.no
if they do not.
Data analysis and plotting
- CDO
CDO
,CDO/1.9.5-foss-2018b
- Dynlib
- See temporary solution for python. Requires in addition
OpenBLAS/0.3.1-GCC-7.3.0-2.30
andScaLAPACK/2.0.2-gompi-2018b-OpenBLAS-0.3.1
.
- See temporary solution for python. Requires in addition
- ghostview
- <no module required>
- grads
- <no module required>
- Matlab
Matlab
,Matlab/2018a
,Matlab/2012a
- ncdump and other netCDF utilities
netCDF
,netCDF/4.6.1-foss-2018b
- NCL
NCL
,NCL/6.5.0
- nco
NCO
,NCO/4.7.4-foss-2018b
- ncview
ncview
,ncview/2.1.7-foss-2018b
. Load only when needed! The package is currently known to break some GUI programs like gedit and gvim.
- python, plus selection of scientific packages
- First choose and load the python module for the python version that you want to use, either
Python/2.7.15-foss-2018b
for python 2.7.15, orPython/3.7.0-foss-2018b
for python 3.7.0. - Then, as a temporary solution, many scientific python packages are installed in the following virtual environments:
source /Data/gfi/users/local/share/virtualenv/dynpie2/bin/activate
for python 2.7.15.source /Data/gfi/users/local/share/virtualenv/dynpie3-2021a/bin/activate
for python 3.7.0.- For the pygrib module,
ecCodes/2.7.3-foss-2018b
is required in addition.
- First choose and load the python module for the python version that you want to use, either
- R
- <no module required>
Text editors
- emacs
- Is installed globally, but requires
util-linux/2.32-GCCcore-7.3.0
to work.
- Is installed globally, but requires
- gedit
- <no module required>
- gvim
- <no module required>
- vi(m)
- <no module required>
Compilers and libraries
- blas
OpenBLAS/0.3.1-GCC-7.3.0-2.30
. Note: The library is calledlibopenblas
, so you'll need to compile with-lopenblas
.
- eccodes (replacement for grib_api)
ecCodes/2.7.3-foss-2018b
- gcc, gfortran
GCC
,GCC/7.3.0-2.30
- grib_api
grib_api/1.24.0-foss-2018b
- HDF5 libraries
HDF5/1.10.2-foss-2018b
- lapack
ScaLAPACK/2.0.2-gompi-2018b-OpenBLAS-0.3.1
. Note: The library is calledlibscalapack
, so you'll need to compile with-lscalapack
.
- MPI
OpenMPI/3.1.1-GCC-7.3.0-2.30
- netcdf
- For C-libaries:
netCDF/4.6.1-foss-2018b
, - For Fortran-libraries
netCDF-Fortran/4.4.4-foss-2018b
, compile with option-I/shared/apps/netCDF-Fortran/4.4.4-foss-2018b/include
- For C-libaries:
- proj
PROJ/5.0.0-foss-2018b
Jupyter & Jupyterhub
Here is a step by step guide to setup and use Jupyter based on the dynpie3
environment.
Accessing the data from your own machines
Note: From your personal machines you will need to be connected to the UiB VPN to be able to mount the following network drives.
On MacOS you can mount folders through Finder > Go > Connect to Server ...
. In the dialogue window that pops up, enter
smb://uib.no;<user name>@klient.uib.no/FELLES/MATNAT/GFI
as the Server Address. You might want to replace gfi
by skd
to access the skd disks if that is your primary affiliation.
On Ubuntu this is very similar: Files > Go > Enter Location ...
. Enter the address:
smb://uib.no;<user name>@klient.uib.no/FELLES/MATNAT/GFI
and enter your password in the next pop-up window, while keeping "UiB" in the "Domain" field.
Alternatively you can mount the network drive with sshfs to a dedicated directory using sshfs
(install with sudo apt install sshfs
):
mkdir ~/cyclone_gfi From UiB network: sshfs -o follow_symlinks <user name>@cyclone.hpc.uib.no:/gfi/ ~/cyclone_gfi/ From ext. networks: sshfs -o follow_symlinks <user name>@sync.uib.no:/gfi/ ~/cyclone_gfi/ Unmount with: fusermount -u ~/cyclone_gfi
On Windows you can mount by navigating to File Explorer > Map network drive
and enter \\leo.hpc.uib.no\gfi
. Make sure to enable Connect using different credentials
and fill in <user name>@uib.no
and your PW.
Displaying GUIs on your screen
The ssh-login command at the top of this wiki enables trusted X11 forwarding (the -Y
option), which allows you to display Graphical User Interfaces (GUIs) on your screen. This way you may be able to run software on a high performance system in a more userfriendly way than by just operating via the terminal. To make this work properly you may have to edit the ssh configuration file (/etc/ssh/ssh_config
on linux systems) by adding or uncommenting the following two lines:
X11Forwarding yes ForwardX11Trusted yes
Editing this file requires superuser priviliges so you may have to ask the IT department for support. For Mac the solution should be pretty similar, windows requires additional software like PuTTY (for establishing an ssh-connection) and an XServer (e.g. VcXsrv).