Search Results - "Clay, R. W."

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    Ultra High Energy Cosmic Rays by Protheroe, R. J., Clay, R. W.

    “…Cosmic rays with energies above 1018 eV are currently of considerable interest in astrophysics and are to be further studied in a number of projects which are…”
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    Journal Article
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    Muon Content of Extensive Air Showers: Comparison of the Energy Spectra Obtained by the Sydney University Giant Air-Shower Recorder and by the Pierre Auger Observatory by Karpikov, I. S., Bellido, J. A., Clay, R. W., Kalmykov, N. N., Rubtsov, G. I., Troitsky, S. V.

    Published in Physics of atomic nuclei (01-11-2019)
    “…The Sydney University Giant Air-shower Recorder(SUGAR) measured the energy spectrum of ultra-high-energy cosmic rays reconstructed from muon detector reading…”
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    In Search of the Origin of the Highest Energy Cosmic Rays by Clay, R W, Dawson, B R

    Published in Space science reviews (01-01-2003)
    “…The origin of the highest energy cosmic rays is a long-standing problem in astrophysics. We know such particles exist, but their rarity has hampered the…”
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    Journal Article
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    The Source Energy Spectrum of Cosmic Rays by Clay, R. W.

    “…An examination is made of the relationship between the observed energy spectrum of cosmic rays and the averaged spectrum of the cosmic rays at their sources…”
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    Journal Article
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    Timing analysis techniques at large core distances for multi-TeV gamma ray astronomy by Stamatescu, V., Rowell, G.P., Denman, J., Clay, R.W., Dawson, B.R., Smith, A.G.K., Sudholz, T., Thornton, G.J., Wild, N.

    Published in Astroparticle physics (01-07-2011)
    “…We present an analysis technique that uses the timing information of Cherenkov images from extensive air showers (EAS). Our emphasis is on distant, or large…”
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    New Results from an ATCA Study of Intraday Variable Radio Sources by Bignall, H. E., Jauncey, D. L., Kedziora-Chudczer, L. L., Lovell, J. E. J., Macquart, J.-P., Rayner, D. P., Tingay, S. J., Tzioumis, A. K., Clay, R. W., Dodson, R. G., McCulloch, P. M., Nicolson, G. D.

    “…We are undertaking an observational program using the ATCA to monitor the intraday variability (IDV) of a sample of sources at 4.8 and 8.6 GHz. The sources…”
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