Computer Science – Performance
Scientific paper
Dec 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmin41b1362m&link_type=abstract
American Geophysical Union, Fall Meeting 2010, abstract #IN41B-1362
Computer Science
Performance
[1932] Informatics / High-Performance Computing, [1998] Informatics / Workflow, [7200] Seismology, [9820] General Or Miscellaneous / Techniques Applicable In Three Or More Fields
Scientific paper
Pegasus WMS is a Workflow Management System that can manage large-scale scientific workflows across Grid, local and Cloud resources simultaneously. Pegasus WMS provides a means for representing the workflow of an application in an abstract XML form, agnostic of the resources available to run it and the location of data and executables. It then compiles these workflows into concrete plans by querying catalogs and farming computations across local and distributed computing resources, as well as emerging commercial and community cloud environments in an easy and reliable manner. Pegasus WMS optimizes the execution as well as data movement by leveraging existing Grid and cloud technologies via a flexible pluggable interface and provides advanced features like reusing existing data, automatic cleanup of generated data, and recursive workflows with deferred planning. It also captures all the provenance of the workflow from the planning stage to the execution of the generated data, helping scientists to accurately measure performance metrics of their workflow as well as data reproducibility issues. Pegasus WMS was initially developed as part of the GriPhyN project to support large-scale high-energy physics and astrophysics experiments. Direct funding from the NSF enabled support for a wide variety of applications from diverse domains including earthquake simulation, bacterial RNA studies, helioseismology and ocean modeling. Earthquake Simulation: Pegasus WMS was recently used in a large scale production run in 2009 by the Southern California Earthquake Centre to run 192 million loosely coupled tasks and about 2000 tightly coupled MPI style tasks on National Cyber infrastructure for generating a probabilistic seismic hazard map of the Southern California region. SCEC ran 223 workflows over a period of eight weeks, using on average 4,420 cores, with a peak of 14,540 cores. A total of 192 million files were produced totaling about 165TB out of which 11TB of data was saved. Astrophysics: The Laser Interferometer Gravitational-Wave Observatory (LIGO) uses Pegasus WMS to search for binary inspiral gravitational waves. A month of LIGO data requires many thousands of jobs, running for days on hundreds of CPUs on the LIGO Data Grid (LDG) and Open Science Grid (OSG). Ocean Temperature Forecast: Researchers at the Jet Propulsion Laboratory are exploring Pegasus WMS to run ocean forecast ensembles of the California coastal region. These models produce a number of daily forecasts for water temperature, salinity, and other measures. Helioseismology: The Solar Dynamics Observatory (SDO) is NASA's most important solar physics mission of this coming decade. Pegasus WMS is being used to analyze the data from SDO, which will be predominantly used to learn about solar magnetic activity and to probe the internal structure and dynamics of the Sun with helioseismology. Bacterial RNA studies: SIPHT is an application in bacterial genomics, which predicts sRNA (small non-coding RNAs)-encoding genes in bacteria. This project currently provides a web-based interface using Pegasus WMS at the backend to facilitate large-scale execution of the workflows on varied resources and provide better notifications of task/workflow completion.
Deelman Ewa
Mehta Gaurang
Silva Fernando
Vahi Karan
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