DocumentCode :
1927538
Title :
The Long Wavelength Array: Results from the first station and future prospects
Author :
Taylor, Greg
Author_Institution :
Dept. of Phys. & Astron., Univ. of New Mexico, Albuquerque, NM, USA
fYear :
2011
fDate :
13-20 Aug. 2011
Firstpage :
1
Lastpage :
1
Abstract :
The Long Wavelength Array (LWA) will be a new multi-purpose radio telescope operating in the frequency range 10-88 MHz. Scientific programs include pulsars, supernova remnants, general transient searches, radio recombination lines, solar and Jupiter bursts, investigations into the “dark ages” using redshifted hydrogen, and ionospheric phenomena. The first LWA station, LWA1, has just come-on line demonstrating the success of the LWA design concept. Additional information about the LWA is online at http://lwa.unm.edu. Partners in the LWA project include LANL, JPL, NRAO, NRL, UNM, NMT, and Virginia Tech.
Keywords :
radioastronomical techniques; radioastronomy; radiotelescopes; Jupiter bursts; Long Wavelength Array; frequency 10 MHz to 88 MHz; general transient search; ionospheric phenomena; multipurpose radio telescope; pulsars; radio recombination line; redshifted hydrogen phenomena; solar bursts; supernova remnants; Arrays; Collaboration; Jupiter; Physics; Radio astronomy; Web pages;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
General Assembly and Scientific Symposium, 2011 XXXth URSI
Conference_Location :
Istanbul
Print_ISBN :
978-1-4244-5117-3
Type :
conf
DOI :
10.1109/URSIGASS.2011.6051194
Filename :
6051194
Link To Document :
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