Some requirements for the future giant low frequency ground based radio telescopes

Details Some requirements for the future giant low frequency ground based radio telescopes Some requirements for the future giant low frequency ground based radio telescopes

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja....14149k&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #14149

Astronomy and Astrophysics

Astronomy

Scientific paper

During last years the interest to the low frequency radio astronomy is growing considerably. The projects of space-borne and ground-based new generation giant radio telescope (i.e. LOFAR) are discussed actively. The largest existing low frequency systems, at first, UTR-2 and URAN Ukraine) and NDA (France) are useful for the probing of new astrophysical ideas as well as of new technical approaches and requirements including future giant radio telescopes and solar system radio astronomy purposes. The 30 elements array with active dipoles was created on UTR-2 observatory for the test of some principal requirements. The investigations of the array confirmed the sensitivity, frequency range, interference immunity and low cost what need for the future instruments.

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