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ARENA 2014

9–12 Jun 2014
US/Eastern timezone
Proceedings are due October 1st, 2014.

ARENA 2014 conference secretariat

Session

Th AM I

12 Jun 2014, 08:30

Presentation materials

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  1. 42. Askaryan Radio Array (ARA): Status and Performance
    Dr Carl Pfendner (Ohio State University)
    12/06/2014, 08:30
    Thurs AM I - In-Ice Neutrino Main
    The Askaryan Radio Array (ARA) is an ultra-high energy (UHE) cosmic neutrino detector located at the South Pole. The cosmic ray flux cut off above primary energies of 10^19.5 eV leads us to expect a UHE neutrino flux due to the GZK effect. The detection of these UHE cosmic neutrinos will add to the understanding of the sources and physics of UHE cosmic rays. ARA uses the radio Cherenkov...
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  2. 48. GNO - Greenland Neutrino Observatory
    Keith Bechtol (KICP, University of Chicago)
    12/06/2014, 09:00
    Thurs AM I - In-Ice Neutrino Main
    The goal of the proposed Greenland Neutrino Observatory (GNO) is to discover and study ultra-high energy neutrinos by looking for radio emission from particle cascades induced by these neutrinos in the Greenland ice sheet. GNO will consist of an array of radio antenna stations deployed near Summit Station in central Greenland, sitting atop a 3 km deep ice sheet. Preliminary analysis of field...
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  3. 39. Performance of the ARIANNA Neutrino Telescope
    Dr Corey Reed (UC Irvine)
    12/06/2014, 09:30
    Thurs AM I - In-Ice Neutrino Main
    The ARIANNA experiment uses low noise, low power and inexpensive technology to search for radio pulses emitted by extremely high energy cosmic neutrino interactions. Three detector stations have been deployed in the Ross Ice Shelf of Antarctica, taking both environmental as well as radio pulse data. The stations are powered by solar and wind generators and transfer data north via...
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  4. 52. ANITA: analysis and program status
    David Seckel (University of Delaware)
    12/06/2014, 10:00
    Thurs AM I - In-Ice Neutrino Main
    A review of the instrument and science program is given, including the status of reanalysis of the cosmic ray events detected by the ANITA-I payload, and plans for ANITA-III.
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