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Searching for "Making Scheduling "Cool" Temperature-Aware Workload Placement in Data Centers." – sorted by Relevance.

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  • An Overview of COOL and COOL-IDL  
  • by C. Jacquemot, F. Herrmann, P. S. Jensen, P. Gautron, J. Mukerji, H. G. Baumgarten, H. Hartlage — 1994 — Multi-threaded Processes in Chorus/MIX. In Proc. of EUUG Spring'90 Conference
  • …OU/TR-94-3 Esprit Project N 0 6603 OUVERTURE An Overview of COOL and COOL--IDL date: March 1994…
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  • A COOL Language Report  
  • by Gordon O'Connell, Mantis H. M. Cheng — 2000
  • …A COOL Language Report Gordon O'Connell and Mantis H.M. Cheng Department of Computer Science…
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  • Cooling of Superuid Neutron Stars  
  • by D. G. Yakovlev, O.Y. Gnedin, A.D. Kaminker — 2002
  • … temperature T 10 11 K, but gradually cool down. In about 30 s after the birth a star becomes fully…
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  • Cooling Limits on Galaxy Formation  
  • by Gas Dynamical Simulations, Daniel Kall, John Hultman
  • … to cool. If a substantial fraction of the gas is still heated to virial temperatures, these models still…
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  • Cool Star Chromospheres and the Sun  
  • by Cool Star Chromospheres, Seth Redfield, The Sun, Jeffrey L. Linsky, Seth Red Eld, Tom Ayres, Alex Brown, Graham Harper
  • …, indicating that the wind has a low ionization temperature. Cool Star Chromospheres and the Sun 11 Figure 8…
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  • Electron Cooling Possibilities for HERA  
  • by Brinkmann Derbenev, M. Gentner, D. Husmann, C. Steier
  • …. This implies that cooling protons in HERA only makes sense when they are already injected near the equilibrium…
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  • Project S'COOL  
  • by Carolyn Green Scientific, Carolyn J. Green, Lin H. Chambers — 1998
  • … their curriculum into the classroom schedule. S'COOL fits in very naturally with the meteorology units found in a…
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  • On Cooling of Magnetized Neutron Stars  
  • by Shibanov And, Y. A. Shibanov, D. G. Yakovlev
  • … on the NS cooling are more sophisticated than anticipated previously. 2. Surface temperature distribution…
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