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Showing 1 to 9 of 9 for “"ultra high energy cosmic rays"”.

  1. Design And Development Of An Autonomous Radar Receiver For The Detection Of Ultra High Energy Cosmic Rays

    The detection of ultra-high energy cosmic rays is constrained by their flux, requiring detectors with apertures of hundreds or even thousands of square kilometers and close to one hundred percent duty cycle. The sheer scale that would be required of conventional detectors, to acquire sufficient …

    ku Repository record for Design And Development Of An Autonomous Radar Receiver For The Detection Of Ultra High Energy Cosmic Rays (opens in a new tab)

  2. Propagation of Ultra-High Energy Cosmic Rays and anisotropy studies with the Pierre Auger Observatory: the multiscale approach

    … the investigation of the arrival directions of ultra-high energy cosmic rays (UHECRs). The clustering of such events, collected by the Pierre Auger Observatory, is used to infer the nature of sources and their density, as well as other physical unknowns. Results are based on the comparison …

    catania Repository record for Propagation of Ultra-High Energy Cosmic Rays and anisotropy studies with the Pierre Auger Observatory: the multiscale approach (opens in a new tab)

  3. All-Sky Search for Neutrinos Correlated with Gamma-Ray Bursts in Extended Time Windows Using Eight Years of IceCube Data

    … as potential sources of hadronic acceleration of ultra-high energy cosmic rays and, more recently, as potential sources of the diffuse neutrino flux measured by IceCube. This thesis presents a search for neutrinos correlated with 2,091 gamma-ray bursts (GRBs) in prompt and extended time windows …

    maryland Repository record for All-Sky Search for Neutrinos Correlated with Gamma-Ray Bursts in Extended Time Windows Using Eight Years of IceCube Data (opens in a new tab)

  4. Stabilizing energy reconstructions of the surface detector at the Pierre Auger Observatory

    At the Pierre Auger Observatory, ultra-high energy cosmic rays are measured through indirect measurements of the extensive air showers they induce. Accordingly, an energy reconstruction process must be undertaken. For the surface detector, the models utilized for energy reconstruction are empirical …

    colo-mines Repository record for Stabilizing energy reconstructions of the surface detector at the Pierre Auger Observatory (opens in a new tab)

  5. FROM DATA PRODUCTION TO SEARCH FOR GALACTIC COSMICRAY SOURCES WITH THE PIERRE AUGER OBSERVATORY

    … astrophysics and particle physics, investigates ultra-high-energy cosmic rays (UHECRs), the most energetic particles known in the Universe. Despite decades of research, their origins remain elusive. These particles are detected through extensive air showers, cascades of secondary particles …

    milano Repository record for FROM DATA PRODUCTION TO SEARCH FOR GALACTIC COSMICRAY SOURCES WITH THE PIERRE AUGER OBSERVATORY (opens in a new tab)

  6. 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)

  7. Targets of opportunity source catalog, prioritization, scheduler and related mechanics for the EUSO-SPB2 mission, The

    … Balloon 2 (EUSO-SPB2) was developed to observe ultra high energy cosmic rays and very high energy (VHE) neutrinos from suborbital space. These earth-skimming VHE tau-neutrinos can interact with the Earth’s limb to produce tau leptons which can exit the Earth and decay to initiate extensive air …

    colo-mines Repository record for Targets of opportunity source catalog, prioritization, scheduler and related mechanics for the EUSO-SPB2 mission, The (opens in a new tab)