A Baseline Design for the Long Wavelength Array Stations

Details A Baseline Design for the Long Wavelength Array Stations A Baseline Design for the Long Wavelength Array Stations

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd..12e..58r&link_type=abstract

Long Wavelength Astrophysics, 26th meeting of the IAU, Joint Discussion 12, 21 August 2006, Prague, Czech Republic, JD12, #58

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Long Wavelength Array (LWA) is intended to be a radio astronomical and ionospheric interferometer operating in the 20-80 MHz band. The full LWA will consist of ~52 stations, each of which will consist of ~256 dipoles. In this paper, we present a baseline design for an LWA station. The goal is to provide a concrete design that satisfies the scientific requirements and can be used to support cost analysis and as a starting point for engineering optimizations. Basic research in radio astronomy at the Naval Research Laboratory is supported by NRL/ONR.

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