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Jim Fischer, Peter Lyster, and Bill Feiereisen peer to the right.

Left to right: ESS Project Manager Jim Fischer, ESS Principal Investigator Peter Lyster and NASA HPCC Program Manager Bill Feiereisen view recent computationl gains.


Galaxy visualization

Science Team I Principal Investigator George Lake and University of Washington colleagues discovered a phenomenon they call galaxy harassment through comparing supercomputer simulations and Hubble Space Telescope observations. This visualization depicts the smoothed surface brightness of the stellar tidal debris from a harassed galaxy after 4 billion years of evolution. Credits : George Lake, Thomas Quinn, Neal Datz, Joachim Stadel, Ben Moore, University of Washington.


Peter Lyster

Peter Lyster, University of Maryland, leads an ESS Grand Challenge team melding atmospheric observations and climate model prediction into a robust data analysis scheme for NASA's Earth Observing System.



Four photos of Peter Lyster

Peter Lyster

100 gigaflops Grand Challenge Applications, by Jarrett Cohen

Earth and space sciences project awards $25.8 million to advance Grand Challenge applications


NASA High Performance Computing and Communications (HPCC) Program's Earth and Space Sciences (ESS) project has entered its second phase with cooperative agreements totaling $25.8 million for the development of Grand Challenge applications 10 times faster than today. Resulting increases in complexity and resolution will provide a new understanding of fundamental problems in ESS disciplines.

A three-year collaboration among NASA scientists, nine Science Team II investigator teams, and Cray Research will achieve these advances (see illustration, page 22). The challenges being pursued include modeling changes in global climate and the Earth's interior, simulating the evolution and dynamics of stars, probing microgravity environments, and processing remote sensing imagery and signals. For broader benefit, the new computer programs and documentation will be made available to the research community on the World Wide Web's National HPCC Software Exchange.


"With 49 gigabytes of memory and 230 gigaflops peak performance, this system will be NASA's leading testbed for scalalble parallel computing, in which a program's speed increases proportionally with the number of processors."

-James Fischer, ESS project manager


"This effort will further the earth and space sciences by helping to overcome one of high-performance computing's greatest bottlenecks — the lack of usable software for parallel machines," said Lee Holcomb, director of the Aviation Systems Technology Division at NASA Headquarters. "Such computational studies strongly mesh with NASA's observational and theo-retical programs and contribute to our wider mission of scientific research and space exploration."

Scientific breakthroughs will be enabled by a 384-processor CRAY T3E supercomputer being placed at the Goddard Space Flight Center (GSFC) as part of a $13.2 million agreement with Cray Research. "With 49 gigabytes of memory and 230 gigaflops peak performance, this system will be NASA's leading testbed for scalable parallel computing, in which a program's speed increases proportionally with the number of processors," said James Fischer, ESS project manager. Cray Research subsequently will assemble a CRAY T3E as large as 1,024 processors to allow 100 gigaflops sustained on investigator applications.

Project Goals and History

Centering on scalable parallel machines' performance advantages, the ESS Project has sought to demonstrate the potential of balanced teraflops systems for meeting


The challenges being pursued include modeling changes in global climate and the Earth's interior, simulating the evolution and dynamics of stars, probing microgravity environments, and processing remote sensing imagery and signals.


Grand Challenge application requirements. "Without an accelerated development program, this level of improvement may not be available for 15 to 20 years," said Robert Ferraro, ESS/Jet Propulsion Laboratory (JPL) associate project manager.

A 1992 NASA Research Announcement was used to select Science Team I. Eight Principal Investigator (PI) teams addressed Grand Challenges, while a complementary set of 21 Guest Computational Investigators developed scalable algorithmic techniques.

Science Team I investigators achieved 10- to 20- fold speed gains over 3 years, with several surpassing 10 gigaflops sustained. Among these was an atmospheric data assimilation routine programmed by the Richard Rood (GSFC Data Assimilation Office) PI team and ESS Project/JPL researchers that attained 18.3 gigaflops on a 512-node Intel Paragon, at least 120 times faster than on a CRAY C90.

Accompanying such performance have been scientific discoveries that could not have been made without supercomputers. For instance, the George Lake (University of Washington) PI team's high-resolution cosmology simulations revealed that "galaxy harassment," a term they invented to describe continual mutual bombardment, can explain the rapid evolution of galaxies in clusters observed by the Hubble Space Telescope (see Nature, 2/15/96).

Science Team II

The selection process for Science Team II began in 1995 with the issuance of a Cooperative Agreement Notice soliciting proposals for PI teams and computing testbeds. Cooperative agreements are closely linked research efforts between NASA and the awardees in which all payments are triggered by meeting prenegotiated milestones. "Though evaluated independently, the investigators and testbed vendor ultimately are driven to collaborate to meet the milestones of 10, 50, and 100 gigaflops sustained performance on each team's application codes," said Lisa Hamet Bernard, ESS deputy project manager for testbeds.

Computing Testbed Upgrades

Their first milestone is being met on an interim CRAY T3D system (the CRAY T3E's predecessor) with 512 processors and 32 billion bytes of memory placed at GSFC this September. By June 1997, NASA and the investigators will complete transition to the 384-processor CRAY T3E. Access to larger CRAY T3E systems will occur before the program's conclusion in 1999. Time on the computers is being divided among the ESS Project and the CAS Project investigators and other NASA ESS researchers.


NASA Logo

ESS Project Science Team II

US Map graphic showing distribution of investigators
Principal Investigator Teams
Simulations of the Earth's Core and Mantle Dynamics—Peter Olson, Johns Hopkins University
Synthetic Aperture Radar Interferometry and Imaging Science—David Curkendall, JPL
Four Dimensional Data Assimilation—Peter Lyster, University of Maryland, College Park
An Earth System Model—Atmosphere/ Ocean Dynamics and Tracers Chemistry, Carlos R. Mechoso, UCLA
Rayleigh-Benard-Marangoni Problems in a Microgravity Environment—Graham Carey, University of Texas at Austin
Turbulent Convection and Dynamos in Stars—Andrea Malagoli, University of Chicago
Solar Activity and Heliosheric Dynamics—John Gardener, Naval Research Laboratory
Multiscale Modeling of the Helioshere—Tamas Gombosi, University of Michigan, Ann Arbor
Relativistic Astrophysics and Gravitational Wave Astronomy—Paul Saylor, University of Illinois at Urbana-Champaign

ESS Project Staff Scientists
Project Scientists: George Lake, University of Washington, Seattle
Chief Computational Scientist: Steven Zalesak, Goddard Space Flight Center
Director of Evaluation: Thomas Sterling, California Institute of Technology and JPL




For More Information

Additional information about the ESS project and Science Team II investigations is available on the World Wide Web (http://ess.gsfc.nasa.gov/).

INSIGHTS was published by the High Performance Computing and Communications Program office.

Program manager: Bill Feiereisen
Editor, photography, design: Judy Conlon
Color separations: TH Graphics
Web Page design: Brandon Bailey