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Showing 1 to 6 of 6 for “"Ultra-High energy cosmic ray"”.

  1. Using power spectra to look for anisotropies in ultra-high energy cosmic ray distributions

    The origins and compositions of ultra-high energy cosmic rays (UHECR) remains a mystery to this day. The Pierre Auger Observatory (PAO) is being constructed now in the hopes that it will help solve this mystery by detecting more UHECR than any previous experiment. In this dissertation, I will …

    lsu-thes Repository record for Using power spectra to look for anisotropies in ultra-high energy cosmic ray distributions (opens in a new tab)

  2. Measurement of the ultra high energy cosmic ray flux from data of very inclined showers at the Pierre Auger Observatory

    This work describes the derivation of the energy dependent flux of ultra-high energy cosmic rays from data of very inclined air showers observed with the Pierre Auger Observatory. The Pierre Auger Observatory measures extensive air showers initiated by interactions of ultra-high energy cosmic rays …

    aachen Repository record for Measurement of the ultra high energy cosmic ray flux from data of very inclined showers at the Pierre Auger Observatory (opens in a new tab)

  3. INVESTIGATING THE ORIGINS OF UHECRS USING THE PIERRE AUGER OBSERVATORY AND PALEO-DETECTORS

    … region for investigating the origins of cosmic rays is the toe of the ultra-high energy cosmic ray (UHECR) spectrum, above ≈ 50 EeV. The potential for small magnetic deflections at these energies is coupled with the presence of flux suppression, which may be a sign of the sources’ maximum …

    milano Repository record for INVESTIGATING THE ORIGINS OF UHECRS USING THE PIERRE AUGER OBSERVATORY AND PALEO-DETECTORS (opens in a new tab)

  4. Design, Implementation and First Results of the ANITA-HiCal Experiment

    … goal of the ANITA experiment is to detect UHE (Ultra-High Energy) neutrinos $(10^9$ to $10^{13}$ GeV) and cosmic rays through the RF (Radio-Frequency) emission of in-ice and atmospheric particle showers initiated, respectively, by these two types of particles. Radio detection of ultra-high

    ku Repository record for Design, Implementation and First Results of the ANITA-HiCal Experiment (opens in a new tab)

  5. Extreme universe space observatory on a super pressure balloon II fluorescence telescope on the ground and (briefly) in the air, The

    … signatures for such observations as well as high energy cosmic rays above the limb. The fluorescence telescope (FT) utilizing multi-anode photomultiplier tubes capable of discriminating single photons, aimed to measure ultra-high energy cosmic ray (UHECR) induced extensive air showers (EAS) …

    colo-mines Repository record for Extreme universe space observatory on a super pressure balloon II fluorescence telescope on the ground and (briefly) in the air, The (opens in a new tab)