Scintillations on the Small Diameter Radio Sources

Details Scintillations on the Small Diameter Radio Sources Scintillations on the Small Diameter Radio Sources

Oct 1965

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1965natur.208..277c&link_type=abstract

Nature, Volume 208, Issue 5007, pp. 277 (1965).

Physics

10

Scientific paper

IRREGULARITIES in the solar wind appear to be responsible for the rapid scintillations on the radiation from small diameter radio sources1, and for some of the fine structure on Jovian decametric bursts2. At the Arecibo Ionospheric Observatory the irregularities as well as the sources are being examined by their scintillations. Early results of this programme have been reported by Cohen and Drake3. The purpose of this communication is merely to report that the scintillation phenomenon has been seen over an extended range of frequencies and positions, and that it is very strong and persistent.

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