Astronomy and Astrophysics – Astrophysics – Instrumentation and Methods for Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Instrumentation and Methods for Astrophysics
Scientist
the University of Adelaide
HiRes-MIA Collaboration
University of Adelaide, Adelaide, Australia
The University of Adelaide
Adelaide, University, Adelaide, Australia
Adelaide Univ., Australia.
Department of Physics, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801
Utah, University, Salt Lake City
Department of Physics and Mathematical Physics, University of Adelaide, South Australia 5005, Australia
Adelaide, University, Australia
Department of Physics and Mathematical Physics, University-of-Adelaide, Adelaide, South Australia 5005 Australia
Department of Physics and Mathematical Physics, University of Adelaide, Adelaide 5005, Australia
Department of Physics, University of Utah, Salt Lake City, UT 84112, USA
Department of Physics, University of Utah, Salt Lake City, Utah 84112, USA
Department of Phys. & Math. Phys., Adelaide Univ., SA, Australia
Department of Physics and Mathematical Physics, The University ofAdelaide, S.A., 5005, Australia
Department of Physics and Mathematical Physics, University of Adelaide GPO Box 498, Adelaide 5001, Australia
Department of Phys., Utah Univ., Salt Lake City, UT, USA
School of Chemistry and Physics, University of Adelaide, Adelaide 5005, Australia.
Univ Adelaide
Department of Phys. & Math Phys., Adelaide Univ., SA, Australia
Department of Physics and Mathematical Physics, University of Adelaide, Adelaide, South Australia 5005, Australia
Department of Physics, University of Adelaide, Adelaide, SA 5005, Australia
School of Chemistry & Physics, University of Adelaide, Adelaide S.A. 5005, AustraliaObservatorio Pierre Auger, Av. San Martin Norte 304, 5613 Malargüe, Argentina
3 to 12 millimetre studies of dense gas towards the western rim of supernova remnant RX J1713.7-3946
A cloud monitoring system for remote sites
A coarse-grain search for anisotropy in the arrival directions of cosmic rays above 10 to the 17th eV
A Comparison of Cosmic Ray Composition Measurements at the Highest Energies
A Multi-Component Measurement of the Cosmic Ray Composition Between 10^{17} eV and 10^{18} eV
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