In this page, we list all available modules which can be shown by using the command module avail on Chalawan cluster.
Message Passing Interface (MPI)
| Module Name | Description | Package | Detail |
| openmpi-1.10.2_GNU (Default module)/ openmpi-1.10.2_intel2013 | Open MPI is a Message Passing Interface (MPI) library project combining technologies and resources from several other projects (FT-MPI, LA-MPI, LAM/MPI, and PACX-MPI). | Open MPI 1.10.2 + GCC 4.4.7 / Open MPI 1.10.2 + Intel Compiler 14.0.3 | Open MPI compile with GNU / Intel compiler |
| openmpi-2.0.2_GNU | Open MPI 1.10.2 + GCC | Open MPI compile with GNU |
| rocks-openmpi | Open MPI 1.6.2 + GCC 4.4.7 | Rocks-compiled Open MPI with tcp,self transport |
| rocks-openmpi_ib | Open MPI 1.6.2 + GCC 4.4.7 | Rocks-compiled Open MPI with openib,dapl transports |
| mvapich2-2.2b_GNU / mvapich2-2.2b_intel2013 | MVAPICH, also known as MVAPICH2, is a BSD-licensed implementation of the MPI standard developed by Ohio State University. | MVAPICH 2.2b + GCC 4.4.7 / MVAPICH 2.2b + Intel Compiler 14.0.3 | MVAPICH compile with GNU / Intel compiler |
| mvapich2-2.3b_intel2013 | MVAPICH 2.3b + Intel Compiler 14.0.3 | MVAPICH compile with Intel compiler |
| mpich2-gnu | MPICH is a high performance and widely portable implementation of the Message Passing Interface (MPI) standard. | | |
| mpich-x86_64 | | | |
Compiler
| Module Name | Description | Version |
| Gnu Compiler Collection (GCC) | The GNU Compiler Collection includes front ends for C, C++, Objective-C, FORTRAN, Ada, and Go, as well as libraries for these languages. | 4.4.7 (default) |
| GCC | 4.8.2 |
| GCC | 7.2.0 |
| go | Go is an open source programming language that makes it easy to build simple, reliable, and efficient software. | 1.9.2 |
| Intel® Composer XE 2013 SP1 | Intel® Composer XE 2013 SP1 is C++/FORTRAN performance suite for technical computing, enterprise and HPC on Windows, Linux and OS X. | SP1.3.174 |
| python | Python is an interpreted high-level programming language for general-purpose programming. Python features a dynamic type system and automatic memory management. It supports multiple programming paradigms, including object-oriented, imperative, functional and procedural, and has a large and comprehensive standard library. | 2.6.6 (default) |
| python | 2.7.13 |
| python | 3.6.0 |
Packages
| Module Name | Description | Version |
| astrometry.net | If you have astronomical imaging of the sky with celestial coordinates you do not know—or do not trust—then Astrometry.net is for you. Input an image and we'll give you back astrometric calibration meta-data, plus lists of known objects falling inside the field of view. | 0.67 |
| casa-4.7.2 | CASA, the Common Astronomy Software Applications package, is being developed with the primary goal of supporting the data post-processing needs of the next generation of radio astronomical telescopes such as ALMA and VLA. The package can process both interferometric and single dish data. | 4.7.2 |
| dftbplus-17.1 | DFTB+ is a fast and efficient versatile quantum mechanical simulation software package. It is based on the Density Functional Tight Binding (DFTB) method, containing almost all of the useful extensions which have been developed for the DFTB framework so far. | 17.1 |
| ffmpeg | FFmpeg is a complete, cross-platform solution to record, convert and stream audio and video. | 3.2 |
| gadgetviewer | Gadget File Viewer is a program for interactive visualization of Gadget N-body simulation snapshots. | 1.0.6 |
| MUSIC | MUlti-Scale Initial Condition (MUSIC), a program to generate zoom initial conditions for cosmological simulations. | 1.53 |
| nco-4.7.1 | The netCDF Operators (NCO) comprise about a dozen standalone, command-line programs that take netCDF, HDF, and/or DAP files as input, then operate (e.g., derive new fields, compute statistics, print, hyperslab, manipulate metadata, regrid) and output the results to screen or files in text, binary, or netCDF formats. NCO aids analysis of gridded and unstructured scientific data. The shell-command style of NCO allows users to manipulate and analyze files interactively, or with expressive scripts that avoid some overhead of higher-level programming environments. | 4.7.1 |
| OptiFDTD | Finite-Difference Time-Domain (FDTD) is a powerful, highly integrated and user-friendly software application that enables the computer-aided design and simulation of advanced passive and non-linear photonic components. | |
| orca-4.0.1 | The program ORCA is a modern electronic structure program package written by F. Neese, with contributions from many current and former coworkers and several collaborating groups. The binaries of ORCA are available free of charge for academic users for a variety of platforms. | 4.0.1 |
| psrsoft | PSRSoft is a system for easily installing and using various pulsar related software packages, without having to worry about strange dependencies and the typical unusual installation scripts. | 1.5 with all up-to-date packages |
| QuantumEspresso6.0 | Quantun Espresso an integrated suite of Open-Source computer codes for electronic-structure calculations and materials modeling at the nanoscale. It is based on density-functional theory, plane waves, and pseudopotentials | 6.0 |
| QUIP | The QUIP package is a collection of software tools to carry out molecular dynamics simulations. | |
| ROOT | A modular scientific software framework, developed by CERN. ROOT provides all the functionalities needed to deal with big data processing, statistical analysis, visualization and storage. | 6.06/02 |
| Starlink-2016A | The Starlink Software Collection is belonged to the Starlink Project which was a long running UK Project supporting astronomical data processing. This project was shut down in 2005 but the software continued to be developed at the Joint Astronomy Center until March 2015, and is now maintained by the East Asian Observatory. The code is open source. | 2016A |
| rockstar | The Rockstar Halo Finder | 0.99.9-RC3+ |
| WD2003 | The Wilson-Devinney Program is the light curve modelling tools. | 2003 |
| wimpsim-4.01 | This code calculates neutrinos from annihilation of WIMPs inside the Sun or the Earth, or from cosmic ray interactions in the solar atmosphere (using MCEq data tables), collects all the neutrinos that emerge and let these propagate out of the Sun/Earth to the detector including neutrino interactions and neutrino oscillations in a fully consistent three-flavour way. | 4.0.1 |
| WRF3.7.1_mvapich | The Weather Research and Forecasting (WRF) Model is a next-generation mesoscale numerical weather prediction system designed for both atmospheric research and operational forecasting applications. It features two dynamical cores, a data assimilation system, and a software architecture supporting parallel computation and system extensibility. | 3.7.1 |
| WRF3.8.1_mvapich | 3.8.1 |
