1. Design and initial performance of the Askaryan Radio Array prototype EeV neutrino detector at the South Pole
- Author
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M. A. Huang, Robert Bard, H. Landsman, Lisa Ritter, Sybille Böser, Andrew Wendorff, Patrick Allison, Carsten Rott, Berkeley Hill, E. Grashorn, Kenneth L. Ratzlaff, Thomas Meures, Daniel Kennedy, M.H.A. Huang, Min-Zu Wang, J. Davies, R. Nichol, Tsung-Che Liu, Chris Weaver, Kael Hanson, M. Richman, Sho Yoshida, J. J. Beatty, P. Sandstrom, M. Newcomb, R. Young, A. Ishihara, Robert Morse, Amy Connolly, Luca Macchiarulo, Christian Miki, D. Seckel, Peter Gorham, C. C. Chen, J. Auffenberg, Pisin Chen, G. S. Varner, R. Meyhandan, David Dzb Besson, K. Mase, J. Touart, B. D. Fox, Michael DuVernois, Kara Kdh Hoffman, E. Hong, Albrecht Karle, K. Helbing, B. Rotter, and James Haugen
- Subjects
Planetary body ,Physics ,business.industry ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy ,Astronomy and Astrophysics ,law.invention ,Askaryan effect ,Jupiter ,Orbiter ,Neutrino detector ,law ,Astrophysics::Earth and Planetary Astrophysics ,Aerospace engineering ,Antenna (radio) ,Radar ,Neutrino ,business - Abstract
We describe a concept for an instrument to measure the thickness of the ice shell on a planetary body such as Jupiter’s moon Europa. Unlike a high powered and massive device such as an ice-penetrating radar, the instrument would be a passive receiver of a naturally occurring signal generated by interactions of deep penetrating cosmic ray neutrinos. We discuss the basic concept and consider the instrument design requirements from the perspective of a NASA Outer Planet Orbiter Mission. We show results of simulations, compare signal-to-noise estimates, and examine possible components and configurations for the antenna, receiver, and electronics. We note some options that can be used to reduce mass and power. Finally, we present a list of issues that would need further study to produce a more concrete design.
- Published
- 2012