During the International Geophysical Year, under the joint auspices of the United States National Committee for the IGY, the Voice of America, and the National Bureau of Standards, we operated a chain of 50 Mc/s VHF forward scatter circuits near the magnetic equator in South America [Bowles and Cohen, 1957]. An intense mode of VHF propagation associated with equatorial sporadic E was found to occur and was demonstrated to be closely identifiable in time‐variation and height with the equatorial electrojet. (A brief account of these findings was published by Gates [1959] and a more comprehensive report will be submitted shortly for publication.) As a result of Stanford University IGY backscatter studies at Huancayo, Egan (Stanford University Radio Propagation Laboratory Tech. Rept. 1, December 30, 1959, unpublished) confirmed our expectation [Bowles and Cohen, 1957] that the radio echoes from irregularities in the vicinity of the equatorial E region exhibit a magnetic‐field related aspect sensitivity similar to that of radio echoes from auroral ionization.