Research
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Fossil fuels are headed for extinction. Projected timetables for when this will happen vary, but the ultimate exhaustion of fossil fuel supplies is a certainty. Alternative energy sources must be found. Arguably, the most promising alternative is fusion, the energy source that lights up the sun and every other star. And two U.S.
Department of Energy laboratories are combining forces to solve the
technological challenges that might bring this stellar energy down to
earth.
Fusion takes place when lighter atomic nuclei are combined to form heavier nuclei. It is a reaction that releases roughly one million times the energy released by the burning of oil. A fusion power plant would use the nuclei of the two hydrogen isotopes--deuterium, which can be directly extracted from water, and tritium, which is produced by adding neutrons to lithium atoms. Enough fusion water to supply a year’s worth of electrical power to a metropolitan city could be delivered in a pickup truck. Unlike the burning of oil or other fossil fuels, a fusion reaction does not contribute to global warming. Unlike nuclear fission, fusion cannot sustain an uncontrolled chain reaction and does not produce high-level radioactive by-products that must be carefully stored for thousands of years. One approach to harnessing fusion as a power source is a technique called inertial fusion energy. In an IFE reactor, pea-sized capsules of fusion fuel are heated so quickly and uniformly, they burn while confined by their own inertia. IFE fuel capsules can be heated either with a beam of laser light or with a beam of heavy ions (positively charged atoms with more than three protons). To determine whether or not a beam of heavy ions could be used to cost-effectively heat an IFE target, researchers at Lawrence Berkeley and Lawrence Livermore National Laboratories have agreed to collaborate as a Heavy-Ion Fusion Virtual National Laboratory. They are proposing to design and construct a unique particle accelerator -ˆ of a type known as an induction linac—that will address all of the critical heavy ion IFE technological issues. This proposal is being called the “Integrated Research Experiment.” Submitted by Lawrence Berkeley
National
Laboratory
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David Cooper, associate director for
Computations
at DOE’s Lawrence Livermore National
Laboratory,
joined DOE Assistant Secretary Vic Reis and Deputy Assistant Secretary
Gil Weigand recently to kick off a program aimed at increasing the number
of university students in computer science, engineering and other academic
disciplines related to DOE’s Accelerated
Strategic Computer Initiative. The program benefits the two
participating
universities—Northern Arizona University
and the University of Utah—as well as
the Livermore Lab, DOE and the nation’s security.
The 10-year, billion-dollar ASCI program should deliver 100-trillion calculations-per-second computing capabilities by the year 2004. Highly skilled people who can operate the hardware and develop software and peripherals are an essential component. “To be truly successful, ASCI must develop the hardware, software, infrastructure and people to produce 100-trillion-operations-per-second computer simulations by 2004,” explained Cooper. “This pilot project addresses that last vital element: people. By working with universities like Northern Arizona University, we can introduce students at the undergraduate level to the ASCI program and facilities. By serving as interns or spending summers working at the DOE Labs, these students will become familiar with large scale simulations. “Hopefully, some of them will choose their
career to assist us in programming and administering these very
complicated
systems.”
The program will provide opportunities for students to learn about career-paths in government, industry, the national laboratories, and academia. More specifically, the partnership should increase student awareness of ASCI opportunities at DOE labs. For further information contact David Schwoegler, 925/422-6900. Submitted by Lawrence Livermore National Laboratory |
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Volume 24, February 22,
1999
Rev:
-