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- W2019490028 abstract "The range-azimuth distribution of auroral backscatter echoes received at Essoyla at frequencies of 93 and 45 MHz is predicted for a model which includes the effects of electron density, magnetic aspect angle, and the azimuth of current flow and also takes into account ionospheric refraction. The distribution is in the form of an arc with maxima of backscatter in both eastern and western wings. As the electron density increases, the intensity of the backscatter increases more rapidly and the azimuths of maximum backscatter separate even further. For currents flowing along the L-shells, the backscatter is strongest in the eastward wing. This asymmetry is intensified if the current flow is rotated anti-clockwise but if the current flow is rotated sufficiently in a clockwise direction the backscatter is stronger in the westward wing. These predictions are supported by observations made at Essoyla." @default.
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- W2019490028 date "1989-11-01" @default.
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- W2019490028 title "The amplitude of auroral backscatter: II. Topology of the backscatter range-azimuth distribution" @default.
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- W2019490028 doi "https://doi.org/10.1016/0021-9169(89)90008-1" @default.
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