Radar investigations of the solar system objects at extremely low frequencies

Details Radar investigations of the solar system objects at extremely low frequencies Radar investigations of the solar system objects at extremely low frequencies

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3..286a&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 286-289

Physics

Scientific paper

The first discussion on the use of a radar to study the Solar System has been introduced by F. J. Keer [14], and F. G. Bass and S. Ya. Braude [3]. The research of the Sun with a radar technique became to be of particularly king interest. The next step in this trend was made in Massachusetts Institute of Technology by El Campo array [1, 2, 4], [10]--[13]. The first results with reflected signal from the Sun were obtained on El Campo array in 1961. This program was prolonged up to 1969 and the sequence of the successful events were analyzed and interpret by I. M. Gordon and N. N. Gerasimova [5]--[8].

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