Computer Science – Social and Information Networks
Scientist
Computer Science
Social and Information Networks
Scientist
Department of Physics, Shaanxi University of Technology, Hanzhong 723001
Key Laboratory for Atmospheric Chemistry, Centre for Atmosphere Watch and Services, Chinese Academy of Meteorological Sciences, Beijing, China
Department of Physics, Shaanxi University of Technology, Hanzhong, Shaanxi Province, 723001; College of Physics, Electronics and Information, Yunnan Normal University, Kunming 650092
Key Laboratory for Atmospheric Chemistry, Chinese Academy of Meteorological Sciences, Beijing, China
Advanced Materials Research Institute, University of New Orleans
MIT
Chicago, University, Chicago, IL
Chicago Univ., IL.
Massachusetts Institute of Technology, Cambridge, MA, USA
Electrical and Computer Engineering, University of Illinois, Urbana, Illinois 61801, USA Institute of Technology, Cambridge, USA
Shanghai Astronomical Observatory, China
University of Illinois at Urbana-Champaign, 1308 W. Main St, Urbana, IL 61801, USA
Department of Electrical and Computer Engineering, University of Illinois at Urbana-Champaign, 1406 W Green St, Urbana, IL 61801, USA
Department of Electrical and Computer Engineering, University of Illinois at Urbana-Champaign, Urbana, Illinois, USA
Chinese Academy of Meteorological Sciences, Beijing, China
Department of Physics, University of Utah, Salt Lake City, Utah 84112
Electro-Optic Systems Laboratory University of Illinois at Urbana-Champaign, 1308 W. Main St., Urbana, IL 61801, USA
Department of Electrical and Computer Engineering, University of Illinois at Urbana-Champaign, CSL, 1308 West Main Street
A search for dark matter in events with one jet and missing transverse energy in pp-bar collisions at sqrt(s) = 1.96 TeV
A Study of High Frequency AGWs Observed in OH Airglow: Seasonal Trend in Momentum Flux
A study of the chemical composition of cosmic rays around 1018eV.
An Analysis of Periodic Components in BL Lac Object S5 0716 +714 with MUSIC Method
An observation of cosmic ray positrons from 10-20 GeV
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