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Franklin, NERSC's Cray XT4, is among the largest machines on the list of Top 500 supercomputers in the world.
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Now ComputingA small sample of massively parallel scientific computing jobs running right now at NERSC. CMB Analysis: A NERSC Tradition
One of the first images from the Planck spacecraft shown as a strip superimposed over a two-dimensional projection of the whole sky as seen in visible light. Image credit: ESA, LFI & HFI Consortia; background optical image: Axel Mellinger State-of-the-art computing resources located at NERSC are aiding in the long and complicated process of understanding data from the Planck spacecraft that is attempting to illuminate the nature and origin of dark matter in the universe. Scientists are creating high-resolution maps of extremely subtle variations in temperature and polarization of the Cosmic Microwave Background (CMB), which is leftover light from the Big Bang that permeates the universe. The work relies on a team of NERSC experts that knows how to optimize and maintain well-balanced high performance computing systems as well as supercomputers with sufficient I/O (input/output) capability. [ MORE...] |
News Center25 million hours of Cray XT4 time available via NISENERSC's Initiative for Scientific Exploration is providing 25 million Franklin hours to groups exploring new scientific research areas, programming models, or algorithms. [MORE] 30 million hours of Cray XT4 time to be allocated via ALCC30 million hours of NERSC time will be allocated via the ASCR Leadership Computing Challenge (ALCC) program. The deadline to apply is February 15. [MORE] Cloud Computing at NERSCNERSC will be exploring ways in which cloud computing can be used to advance scientific discovery. Users are invited to indicate their interest in cloud computing at NERSC. [MORE] Science News
Validating Fundamental Forces of Nature
William & Mary Professor of Physics William Detmold and his colleagues have achieved the
first quantum chromodynamics (QCD) calculations of the three-body
force between hadrons. A better understanding of these interactions
could ultimately improve models of nuclei, as well as provide valuable
insights into the life and death of stars.
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