Regions of the Ionosphere responsible for Radio Star Scintillations

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Scientific paper

THERE is at present conflicting evidence as to the region of the ionosphere which is responsible for the scintillation of radio stars. Thus workers in the northern hemisphere1,2 observing sources at fairly high angles of elevation, and also Mills and Thomas3 in the southern hemisphere observing the Cygnus source at an altitude of 15°, have found a marked correlation between the occurrence of scintillations and of spread F echoes. On the other hand, Bolton et al.4 at the same southern location as Mills, but observing sources within 10° of the horizon, found an equally marked correlation with sporadic E, but not with spread F.

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