NSSDCA ID: 1967-042A-02
Mission Name: Ariel 3The purpose of this experiment was to map large-scale noise sources in the galaxy using loop antennas connected to a swept-frequency receiver covering 2 to 4.3 MHz. For a description of this experiment, see F. G. Smith and P. C. Gregory, "The Ariel III cosmic radio noise experiment," Proc. Roy. Soc. A, v. 311, pp. 517-525, 1969.
Questions and comments about this experiment can be directed to: Coordinated Request and User Support Office
Name | Role | Original Affiliation | |
---|---|---|---|
Prof. F. Graham Smith | Principal Investigator | University of Cambridge |