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
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