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26–29 Aug 2013
Beckman Center of the National Academies of Sciences and Engineering
US/Pacific timezone

Measuring Potential Noise Backgrounds for the Telescope Array Radar (TARA) near Long Ridge, UT

27 Aug 2013, 14:30
30m
Huntington (Beckman Center of the National Academies of Sciences and Engineering)

Huntington

Beckman Center of the National Academies of Sciences and Engineering

100 Academy Way, Irvine, CA 92617

Speaker

Jordan Hanson

Description

The main transmitter and receiver stations for the Telescope Array Radar bi-static cosmic ray detection system are now complete. To perform background-free coincidence studies, low-cost , sustainable power remote stations are being designed and built. A site survey was conducted in March 2013 with the goal of finding a remote site in the desert near the main TARA receiver at Long Ridge, UT. The two main goals were to locate a site with little or no radio backgrounds, and a site that was within range of the 40 kW TARA transmitter. A collection of possible future sites were located, and monte carlo simulations were performed which indicate that there is little cost to signal sensitivity by placing a detector at any of these sites. The remote station concept, noise data, and monte carlo analysis will all be presented.

Presentation materials