Comet Level Slot Machine
Comet User Guide Last update: September 23, 2020 Trial Accounts give potential users rapid access to Comet for the purpose of evaluating Comet for their research. This can be a useful step in accessing the usefulness of the system by allowing them to compile, run, and do initial benchmarking of their application prior to submitting a larger Startup or Research allocation. Trial Accounts are for 1000 CPU, or 100 GPU, core-hours. Requests are fulfilled within 1 working day. Comet Technical SummaryComet is a dedicated XSEDE cluster designed by Dell and SDSC delivering ~2.0 petaflops, featuring Intel next-gen processors with AVX2, Mellanox FDR InfiniBand interconnects and Aeon storage. The standard compute nodes consist of Intel Xeon E5-2680v3 (formerly codenamed Haswell) processors, 128 GB DDR4 DRAM (64 GB per socket), and 320 GB of SSD local scratch memory. The GPU nodes contain four NVIDIA GPUs each. The large memory nodes contain 1.5 TB of DRAM and four Haswell processors each. The network topology is 56 Gbps FDR InfiniBand with rack-level full bisection bandwidth and 4:1 oversubscription cross-rack bandwidth. Comet has 7 petabytes of 200 GB/second performance storage and 6 petabytes of 100 GB/second durable storage. It also has dedicated gateway hosting nodes and a Virtual Machine repository. External connectivity to Internet2 and ESNet is 100 Gbps. NEW! The Comet User Portal is a gateway for launching interactive applications such as MATLAB, and an integrated web-based environment for file management and job submission. All Comet users with XSEDE accounts have access via their XSEDE credentials. Serving the Long TailComet was designed and is operated on the principle that the majority of computational research is performed at modest scale. Comet also supports science gateways, which are web-based applications that simplify access to HPC resources on behalf of a diverse range of research communities and domains, typically with hundreds to thousands of users. Comet is an NSF-funded system operated by the San Diego Supercomputer Center at UC San Diego. Comet is available through the Extreme Science and Discovery Environment (XSEDE) program.
Resource allocation policies are designed to serve more users than traditional HPC systems
Job scheduling policies are designed for user productivity
Comet's system architecture is designed for user productivity
Comet Technical Details
Comet supports the XSEDE core software stack, which includes remote login, remote computation, data movement, science workflow support, and science gateway support toolkits. Systems Software Environment
Supported Application Softwareby Domain of Science
As an XSEDE computing resource, Comet is accessible to XSEDE users who are given time on the system. To obtain an account, users may submit a proposal through the XSEDE Allocation Request System (XRAS) or request a Trial Account. Interested parties may contact XSEDE User Support for help with a Comet proposal. Logging in to CometComet supports several access methods:
To login to Comet from the command line, use the hostname: The following are examples of Secure Shell ( Notes and hints
Do NOT use the login nodes for computationally intensive processes. These nodes are meant for compilation, file editing, simple data analysis, and other tasks that use minimal compute resources. All computationally demanding jobs should be submitted and run through the batch queuing system. The Environment Modules package provides for dynamic modification of your shell environment. Module commands set, change, or delete environment variables, typically in support of a particular application. They also let the user choose between different versions of the same software or different combinations of related codes. ModulesFor example, if the Intel module and mvapich2_ib module are loaded and the user compiles with mpif90, the generated code is compiled with the Intel Fortran 90 compiler and linked with the mvapich2_ib MPI libraries. Several modules that determine the default Comet environment are loaded at login time. /stardew-valley-pc-no-free-slots.html. These include the MVAPICH implementation of the MPI library and the Intel compilers. We strongly suggest that you use this combination whenever possible to get the best performance.
Loading and Unloading ModulesYou must remove some modules before loading others. Some modules depend on others, so they may be loaded or unloaded as a consequence of another module command. For example, if intel and mvapich are both loaded, running the command module unload intel will automatically unload mvapich. Subsequently issuing the module load intel command does not automatically reload mvapich. If you find yourself regularly using a set of module commands, you may want to add these to your configuration files (' module: command not foundThe error message 'module: command not found' is sometimes encountered when switching from one shell to another or attempting to run the module command from within a shell script or batch job. The reason that the module command may not be inherited as expected is that it is defined as a function for your login shell. If you encounter this error execute the following from the command line (interactive shells) or add to your shell script (including Slurm batch scripts) Useful CommandsThe Adding Users to an AccountProject PIs and co-PIs can add or remove users from an account. To do this, log in to your XSEDE portal account and go to the Add User page. ChargingThe charge unit for all SDSC machines, including Comet, is the Service Unit (SU). This corresponds to the use of one compute core for one hour. Keep in mind that your charges are based on the resources that are tied up by your job and don't necessarily reflect how the resources are used. Charges are based on either the number of cores or the fraction of the memory requested, whichever is larger. The minimum charge for any job longer than 10 seconds is 1 SU. Job Charge Considerations
CompilingComet provides the Intel, Portland Group (PGI), and GNU compilers along with multiple MPI implementations (MVAPICH2, MPICH2, OpenMPI). Most applications will achieve the best performance on Comet using the Intel compilers and MVAPICH2 and the majority of libraries installed on Gordon have been built using this combination. Although other compilers and MPI implementations are available, we suggest using these only for compatibility purposes. All three compilers now support the Advanced Vector Extensions 2 (AVX2). Using AVX2, up to eight floating point operations can be executed per cycle per core, potentially doubling the performance relative to non-AVX2 processors running at the same clock speed. Note that AVX2 support is not enabled by default and compiler flags must be set as described below. Using the Intel Compilers (Default/Suggested)The Intel compilers and the MVAPICH2 MPI implementation will be loaded by default. If you have modified your environment, you can reload by executing the following commands at the Linux prompt or placing in your startup file (' For AVX2 support, compile with the ' Intel MKL libraries are available as part of the 'intel' modules on Comet. Once this module is loaded, the environment variable MKL_ROOT points to the location of the mkl libraries. The MKL link advisor can be used to ascertain the link line (change the MKL_ROOT aspect appropriately). For example to compile a C program statically linking 64 bit scalapack libraries on Comet: For more information on the Intel compilers:
Note for C/C++ users: compiler warning - Using the PGI CompilersThe PGI compilers can be loaded by executing the following commands at the Linux prompt or placing in your startup file (~/.cshrc or ~/.bashrc) For AVX support, compile with '`-fast`' For more information on the PGI compilers:
Using the GNU CompilersThe GNU compilers can be loaded by executing the following commands at the Linux prompt or placing in your startup files (~/.cshrc or ~/.bashrc) For AVX support, compile with '`-mavx`'. Note that AVX support is only available in version 4.7 or later, so it is necessary to explicitly load the gnu/4.9.2 module until such time that it becomes the default. For more information on the GNU compilers:
MVAPICH2-GDR on Comet GPU NodesThe GPU nodes on Comet have MVAPICH2-GDR available. MVAPICH2-GDR is based on the standard MVAPICH2 software stack. It incorporates designs that take advantage of the new GPUDirect RDMA technology for inter-node data movement on NVIDIA GPUs clusters with Mellanox InfiniBand interconnect. The ' Notes and hints
Running Jobs on Regular Compute NodesComet uses the Simple Linux Utility for Resource Management (SLURM) batch environment. When you run in batch mode, you submit jobs to be run on the compute nodes using the Comet places limits on the number of jobs queued and running on a per group (allocation) and partition basis. Please note that submitting a large number of jobs (especially very short ones) can impact the overall scheduler response for all users. If you are anticipating submitting a lot of jobs, please contact the XSEDE Help Desk before you submit them. We can work to check if there are bundling options that make your workflow more efficient and reduce the impact on the scheduler. The limits for each partition are given in the below table:
Requesting interactive resources using |
Option | Result |
---|---|
-i interval | Repeatedly report at intervals (in seconds) |
-i job_list | Displays information for specified job(s) |
-i part_list | Displays information for specified partitions (queues) |
-i state_list | Shows jobs in the specified state(s) |
Users can cancel their own jobs using the 'scancel
' command as follows:
Help with ibrun
The options and arguments for ibrun are as follows:
Using Globus Endpoints, Data Movers and Mount Points
All of Comet's NFS and Lustre filesystems are acccessible via the Globus endpoint 'xsede#comet
'. The servers also mount Gordon's filesystems, so the mount points are different for each system. The following table shows the mount points on the data mover nodes (that are the backend for 'xsede#comet
' and 'xsede#gordon
').
Machine | Location on machine | Location on Globus/Data Movers |
---|---|---|
Comet, Gordon | /home/$USER | /home/$USER |
Comet, Gordon | /oasis/projects/nsf | /oasis/projects/nsf |
Comet | /oasis/scratch/comet | /oasis/scratch-comet |
Gordon | /oasis/scratch | /oasis/scratch |
SSD Scratch Space
The compute nodes on Comet have access to fast flash storage. There is 250GB of SSD space available for use on each compute node. The latency to the SSDs is several orders of magnitude lower than that for spinning disk (> 100 microseconds vs. milliseconds) making them ideal for user-level check pointing and applications that need fast random I/O to large scratch files. Users can access the SSDs only during job execution under the following directories local to each compute node:
Partition | Space Available |
---|---|
compute, shared | 212 GB |
gpu, gpu-shared | 286 GB |
large-shared | 286 GB |
A limited number of nodes in the 'compute' partition have larger SSDs with a total of 1464 GB available in local scratch. They can be accessed by adding the following to the Slurm script:
Parallel Lustre Filesystems
In addition to the local scratch storage, users will have access to global parallel filesystems on Comet. Overall, Comet has 7 petabytes of 200 GB/second performance storage and 6 petabytes of 100 GB/second durable storage.
Users can now access /oasis/projects
from Comet. The two Lustre filesystems available on Comet are:
Lustre Comet scratch filesystem: /oasis/scratch/comet/$USER/temp_project
Lustre NSF projects filesystem: /oasis/projects/nsf
VCs are not meant to replace the standard HPC batch queuing system, which is well suited for most scientific and technical workloads. In addition, a VC should not be simply thought of as a VM (virtual machine). Future XSEDE resources, such as Indiana University's Jetstream will address this need. VCs are primarily intended for those users who require both fine-grained control over their software stack and access to multiple nodes. With regards to the software stack, this may include access to operating systems different from the default version of CentOS available on Comet or to low-level libraries that are closely integrated with the Linux distribution. Science Gateways serving large research communities and that require a flexible software environment are encouraged to consider applying for a VC, as are current users of commercial clouds who want to make the transition for performance or cost reasons.
Maintaining and configuring a virtual cluster requires a certain level of technical expertise. We expect that each project will have at least one person possessing strong systems administration experience with the relevant OS since the owner of the VC will be provided with 'bare metal' root level access. SDSC staff will be available primarily to address performance issues that may be related to problems with the Comet hardware and not to help users build their system images.
All VC requests must include a brief justification that addresses the following:
- Why is a VC required for this project?
- What expertise does the PI's team have for building and maintaining the VC?
The GPU nodes can be accessed via either the 'gpu' or the 'gpu-shared' partitions.
or
In addition to the partition name (required), the type of GPU (optional) and the individual GPUs are scheduled as a resource.
GPUs will be allocated on a first-available, first-schedule basis, unless specified with the [type] option, where type can be K80 or P100 (type is case sensitive).
For example on the 'gpu' partition the following lines are needed to utilize 4 P100 GPUs:
Users should always set --ntasks-per-node
equal to 6 x [number of GPUs requested]
on all k80 'gpu-shared' jobs, and 7 x [number of GPUs requested]
on all p100 'gpu-shared' jobs, to ensure proper resource distribution by the scheduler. Additionally, when requesting the P100 nodes it is recommended to ask for 25GB per GPU (unless more is needed for the code). The following requests 2 p100 GPUs on a 'gpu-shared' partition:
(for a single GPU this would be --gres=gpu:p100:1, --mem=25G
)
Here is an example AMBER script using the gpu-shared queue, aimed at a K80 Node.
k80 gpu-shared job
Please see /share/apps/examples/GPU
for more examples.
GPU modes can be controlled for jobs in the 'gpu' partition. By default, the GPUs are in non-exclusive mode and the persistence mode is 'on'. If a particular 'gpu' partion job needs exclusive access the folowing options should be set in your batch script:
#SBATCH --constraint=exclusive
To turn persistence off add the following line to your batch script:
#SBATCH --constraint=persistenceoff
Jobs run in the 'gpu-shared' partition are charged differently from other shared partitions on Comet to reflect fractions of a resource used, based on number of GPUs requested and the relative performance of the different GPU types. P100 GPUs are generally substantially faster than K80 nodes, achieving more than twice the performance for some applications. 1 GPU is equivalent to 1/4th of the node or 6 cores on k80 nodes and 7 cores on p100 nodes.
The charging equation is:
GPU SUs = (Number of K80 GPUs) + (Number of P100 GPUS)*1.5) x (wallclock time)
The large memory nodes can be accessed via the 'large-shared' partition. Charges are based on either the number of cores or the fraction of the memory requested, whichever is larger.
For example, on the 'large-shared' partition, the following job requesting 16 cores and 445 GB of memory (about 31.3% of 1455 GB of one node's available memory) for 1 hour will be charged 20 SUs:
455/1455(memory) * 64(cores) * 1(duration) ~= 20
While there is not a separate 'large' partition, a job can still explicitly request all of the resources on a large memory node. Please note that there is no premium for using Comet's large memory nodes, but the processors are slightly slower (2.2 GHz compared to 2.5 GHz on the standard nodes), Users are advised to request the large nodes only if they need the extra memory.
Software Packages
Comet supports the XSEDE core software stack, which includes remote login, remote computation, data movement, science workflow support, and science gateway support toolkits.
Software Package | Compiler Suites | Parallel Interface |
---|---|---|
AMBER: Assisted Model Building with Energy Refinement | intel | mvapich2_ib |
APBS: Adaptive Poisson-Boltzmann Solver | intel | mvapich2_ib |
Car-Parrinello 2000 (CP2K) | intel | mvapich2_ib |
DDT | ||
FFTW: Fastest Fourier Transform in the West | intel, pgi, gnu | mvapich2_ib |
GAMESS: General Atomic Molecular Electronic Structure System | intel | native: sockets, ip over ib vsmp: scalemp mpich2 |
GAUSSIAN | pgi | Single node, shared memory |
GROMACS: GROningen MAchine for Chemical Simulations | intel | mvapich2_ib |
HDF4/HDF5: Hierarchical Data Format | intel, pgi, gnu | mvapich2_ib for hdf5 |
LAMMPS:Large-scale Atomic/Molecular Massively Parallel Simulator | intel | mvapich2_ib |
NAMD: NAnoscale Molecular Dynamics | intel | mvapich2_ib |
NCO: NetCDF Operators | intel, pgi, gnu | none |
NetCDF: Network Common Data Format | Intel, pgi, gnu | none |
Python modules (scipy etc) | gnu:ipython, nose, pytz intel:matplotlib, numpy, scipy, pyfits | None |
RDMA-Hadoop | None | None |
RDMA-Spark | None | None |
Singularity: User Defined Images | None | None |
VisIt Visualization Package | intel | openmpi |
Software Package Descriptions
AMBER
AMBER is package of molecular simulation programs including SANDER (Simulated Annealing with NMR-Derived Energy Restraints) and a modified version of PMEME (Particle Mesh Ewald Molecular Dynamics) that is faster and more scalable.
APBS
APBS evaluates the electrostatic properties of solvated biomolecular systems. View the APBS documentation
Car-Parrinello 2000
CP2K is a program to perform simulations of molecular systems. It provides a general framework for different methods such as Density Functional Theory (DFT) using a mixed Gaussian and plane waves approach (GPW) and classical pair and many-body potentials. View the CP2K documentation
DDT
DDT is a debugging tool for scalar, multithreaded and parallel applications. DDT Debugging Guide from TACC
FFTW
FFTW is a library for computing the discrete Fourier transform in one or more dimensions, of arbitrary input size, and of both real and complex data. View the FFTW documentation
GAMESS
GAMESS is a program for ab initio quantum chemistry. GAMESS can compute SCF wavefunctions, and correlation corrections to these wavefunctions as well as Density Functional Theory. GAMESS documentation, examples, etc.
GAUSSIAN
Gaussian 09 provides state-of-the-art capabilities for electronic structure modeling. Gaussian 09 User's Reference
GROMACS
GROMACS is a versatile molecular dynamics package, primarily designed for biochemical molecules like proteins, lipids and nucleic acids. GROMACS Online Manual
HDF4/HDF5
HDF is a collection of utilities, applications and libraries for manipulating, viewing, and analyzing data in HDF format. HDF 5 Resources
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LAMMPS
LAMMPS is a classical molecular dynamics simulation code. LAMMPS User Manual
NAMD
NAMD is a parallel, object-oriented molecular dynamics code designed for high-performance simulation of large biomolecular systems. NAMD User Guide
NCO
NCO operates on netCDF input files (e.g. derive new data, average, print, hyperslab, manipulate metadata) and outputs results to screen or text, binary, or netCDF file formats. NCO documentation on SourceForge
netCDF
netCDF is a set of libraries that support the creation, access, and sharing of array-oriented scientific data using machine-independent data formats. netCDF documentation on UCAR's Unidata Program Center
Python modules
The Python modules under /opt/scipy consist of: node, numpy, scipy, matplotlib, pyfits, ipython and pytz. Video tutorial from a TACC workshop on Python
RDMA-Hadoop
RDMA-based Apache Hadoop 2.x is a high performance derivative of Apache Hadoop developed as part of the High-Performance Big Data (HiBD) project at the Network-Based Computing Lab of The Ohio State University. The installed release on Comet (v0.9.7) is based on Apache Hadoop 2.6.0. The design uses Comet's InfiniBand network at the native level (verbs) for HDFS, MapReduce, and RPC components, and is optimized for use with Lustre.
The design features a hybrid RDMA-based HDFS design with in-memory and heterogenous storage including RAM Disk, SSD, HDD, and Lustre. In addition, optimized MapReduce over Lustre (with RDMA-based shuffle) is also available. The implementation is fully integrated with SLURM (and PBS) on Comet with scripts available to dynamically deploy hadoop clusters within the SLURM scheduling framework.
Examples for various modes of usage are available in /share/apps/examples/HADOOP/RDMA. Please email [email protected] (reference Comet as the machine, and SDSC as the site) if you have any further questions about usage and configuration. Read more about the RDMA Hadoop and HiBD project.
RDMA-Spark
RDMA-based Apache Spark is a high performance derivative of Apache Hadoop developed as part of the High-Performance Big Data (HiBD) project at the Network-Based Computing Lab of The Ohio State University. The installed release on Comet (v0.9.1) is based on Apache Spark 1.5.1. The design uses Comet's InfiniBand network at the native level (verbs) for RDMA-based data shuffle, SEDA-based shuffle architecture, efficient connection management, non-blocking and chunk-based data transfer, and off-JVM-heap buffer management.
The RDMA-Spark cluster setup and usage is managed via the myHadoop framework. An example script is provided in /share/apps/examples/SPARK/sparkgraphx_rdma. Please email [email protected] (reference Comet as the machine, and SDSC as the site) if you have any further questions about usage and configuration. See details on RDMA Spark.
Singularity
Singularity is a platform to support users that have different environmental needs than what is provided by the resource or service provider. While the high level perspective of other container solutions seems to fill this niche very well, the current implementations are focused on network service virtualization rather than application level virtualization focused on the HPC space. Because of this, Singularity leverages a workflow and security model that makes it a very reasonable candidate for shared or multi-tenant HPC resources like Comet without requiring any modifications to the scheduler or system architecture. Additionally, all typical HPC functions can be leveraged within a Singularity container (e.g. InfiniBand, high performance file systems, GPUs, etc.). While Singularity supports MPI running in a hybrid model where you invoke MPI outside the container and it runs the MPI programs inside the container, we have not yet tested this.
Examples for various modes of usage are available in /share/apps/examples/Singularity. Please email [email protected] (reference Comet as the machine, and SDSC as the site) if you have any further questions about usage and configuration. Read more about Singularity.
VisIt Visualization Package
The VisIt visualization package supports remote submission of parallel jobs and includes a Python interface that provides bindings to all of its plots and operators so they may be controlled by scripting. Watch the Getting Started With VisIt tutorial
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