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- W1993770848 abstract "Observations of the NW-SE component of F region convection obtained with a scintillation drift experiment have been compared with power and Doppler velocity measurements of auroral E region coherent backscatter at 50 MHz made with the Bistatic Auroral Radar System (BARS), which is able to observe only at large magnetic aspect angles. It was found that E region backscatter was observed only when the NW–SE component of the F region drift was in the SE direction. This and other observations are shown to be consistent with a recently proposed explanation for these large aspect angle VHF backscatter observations, based on refraction through auroral ionization structures in the E region. In most cases the vector velocity derived from BARS observations had a magnitude substantially below that inferred from the scintillation measurements. Observations during one period were noticeably different from the others, with unusually small Doppler velocities." @default.
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- W1993770848 date "1990-01-01" @default.
- W1993770848 modified "2023-09-25" @default.
- W1993770848 title "Bistatic auroral radar system and three-receiver-ionospheric-motions velocities: A comparison" @default.
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- W1993770848 doi "https://doi.org/10.1029/ja095ia09p15219" @default.
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