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- W2048931966 abstract "Evidence is presented to show that active auroral forms that pass across the line of sight to a radio star can have a direct effect on the scintillations of the signal received on a frequency of 223 Mc. This effect is most pronounced if the level of scintillation activity is relatively low before the aurora crosses the star position. Two examples are presented: in the first, an intense auroral band between the radio source in Cassiopeia (angular diameter, 4′) and the receiver disrupts the characteristic sinusoidal trace produced by the radio star signal in the output of the phase switch interferometer. This long-duration fade lasted for a period of about 8 minutes. In the second example, the aurora is accompanied by strong angular scintillation coincident with strong absorption of 27.6 Mc galactic radio waves. In both examples the radio star was within 10° of the geomagnetic zenith." @default.
- W2048931966 created "2016-06-24" @default.
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- W2048931966 date "1960-07-01" @default.
- W2048931966 modified "2023-09-28" @default.
- W2048931966 title "Effect of line-of-sight aurora on radio star scintillations" @default.
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- W2048931966 doi "https://doi.org/10.1029/jz065i007p01981" @default.
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