Computer Science – Information Theory
Scientist
Computer Science
Information Theory
Scientist
Shitz
Giessen U
Department of Physics and Astronomy, University of Victoria, PO Box 3055 STN CSC, Victoria, B.C., V8W 3P6, Canada of Physics and Astronomy, University of Victoria, P.O. Box 3055 STN CSC, Victoria B.C. V8W 3P6, Canada, ; Visiting Astronomer at the Dominion Astrophysical Observatory, operated by the National Research Council of Canada Bear Solar Observatory, New Jersey Institute of Technology, Big Bear City, CA 92314, USA
Geomagnetism Laboratory, the University of Liverpool, Oxford Street, Liverpool, L69 7ZE, UK. Columbia University, Vancouver, Canada
Physics and Astronomy Department, University of Victoria, PO Box 3055 STN CSC, Victoria, BC, V8W 3P6, Canada
British Columbia, University, Vancouver, Canada
Electrical Engineering, Imperial College London, London, United Kingdom; Metallurgical Institute, Kunming, Communist China
Victoria, University, Canada
National Astronomical Observatoires, Chinese Academy of Sciences, 100012 Beijing, PR China ; Max-Planck Institute for Solar System Research, 37191 Katlenburg-Lindau, Germany and Astronomy Department, University of Victoria, Victoria, Canada
Cornell University, Ithaca, N.Y.
University of Victoria
Department of Physics and Astronomy, University of Victoria, P.O. Box 3055, Victoria, B.C., V8W 3P6, Canada
Department of Physics and Astronomy, University of Victoria
Department of Physics and Astronomy, University of Victoria, PO Box 3055, Victoria BC V8W 3P6, Canada
Department of Physics and Astronomy, University of Victoria, PO Box 3055 STN CSC, Victoria, B.C. V8W 3P6, Canada
Dept. of Physics and Astronomy, University of Victoria, PO Box 3055, Victoria BC, V8W 3P6, Canada
University of Victoria, Canada
Department of Physics and Astronomy, University of Victoria, Victoria, BCV8W 3P6, Canada
Department of Phy
4ω Thomson scattering probe for high-density plasma characterization at Titan
A 200 GHz Near Field Measurement System
A comparison of archaeointensity results from Chinese ceramics using microwave and conventional Thellier's and Shaw's methods
A comparison of archaeointensity results from Chinese ceramics using Thellier's and Shaw's palaeointensity methods
A definitive period for the Be star LQ And.
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