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ARENA 2014

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

ARENA 2014 conference secretariat

Session

Weds PM II

11 Jun 2014, 15:55

Presentation materials

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  1. 47. From the earth to the moon.
    Prof. Olaf Scholten (KVI-CART, Univ. of Groningen)
    11/06/2014, 15:55
    Weds PM II - Lunar
    TBD
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  2. 24. The effects of surface roughness on lunar Askaryan pulses
    Dr Clancy James (University of Erlangen-Nuernberg)
    11/06/2014, 16:35
    Weds PM II - Lunar
    The effects of lunar surface roughness, on both small and large scales, on Askaryan radio pulses generated by particle cascades beneath the lunar surface has never been fully estimated. Surface roughness affects the chances of a pulse escaping the lunar surface, its coherency, and the characteristic detection geometry. It will affect the expected signal shape, the relative utility of different...
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  3. 8. PRIDE – Passive Radio Ice Depth Experiment - An Instrument to Measure Outer Planet Lunar Ice Depths from Orbit using EHE Neutrinos
    Dr Timothy Miller (Johns Hopkins University Applied Physics Lab)
    11/06/2014, 16:55
    Weds PM II - Lunar
    We describe a potential confluence between EeV neutrino detection and planetary science: a concept for an instrument to measure the thickness of the ice shell on a planetary body, such as Jupiter’s moon Europa or Saturn’s moon Enceladus, by making use of the Askaryan Effect RF signal from EHE neutrinos observed from an orbiting spacecraft. Unlike a large high powered active device, i.e., an...
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  4. 34. On the feasibility of RADAR detection of high-energy cosmic neutrinos in ice
    Krijn de Vries (VUB)
    11/06/2014, 17:15
    Weds PM II - Lunar
    We discuss the radar detection technique for the detection of high-energy neutrino-induced particle cascades in ice. A high-energy neutrino interacting in ice will induce a particle cascade. When propagating through the ice, this cascade will ionize the medium producing a plasma. The different properties of this ionization plasma, such as its size and lifetime, will be discussed to determine...
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  5. 37. A Station For The Detection Of Ultra High Energy Cosmic Ray Induced Extensive Air Showers At The Telescope Array Radar (TARA)
    Mr Samridha Kunwar (The University of Kansas)
    11/06/2014, 17:35
    Weds PM II - Lunar
    The detection of high – energy cosmic rays is currently limited by the rarity of the most interesting rays striking Earth. We describe the development of an observatory based on a remote sensing technique known as bi-static radar, that aims to achieve remote coverage over large portions of the Earth's surface. The radar project's receiver and transmitter stations have already been functional...
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