• 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