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Detailed Reference Information |
Foster, J.C., Tetenbaum, D., del Pozo, C.F., St-Maurice, J.-P. and Moorcroft, D.R. (1992). Aspect angle variations in intensity, phase velocity, and altitude for high-latitude 34-cm E region irregularities. Journal of Geophysical Research 97: doi: 10.1029/91JA03144. issn: 0148-0227. |
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The sensitivity of the Millstone 440-MHz radar system is such that coherent echoes from E region irregularities can be observed over a 90-dB dynamic range above the incoherent scatter background. At antenna elevation angles between 4¿ and 20¿, aspect angles between 0¿ and 10¿ (from perpendicularity with the magnetic field) are viewed at E region heights at invariant latitudes between 61¿ &Lgr; and 57¿&Lgr;. During distributed conditions, when convection electric fields in excess of 15 mV/m and E region irregularities span this range of latitudes, antenna scanning experiments have been performed to determine the aspect angle sensitivity with high precision. Our measurements are unique in that they provide a clear high-frequency description of the variation in both power and Doppler shifts as functions of aspect angle, all the way from a region where the waves are known to be linearly unstable, in a direction perpendicular to the geomagnetic field, to as much as 10¿ away from perpendicularity. We find that the 440-MHz aspect sensitivity is about -15 dB deg-1 for aspect angles between 0¿ and 3¿, -10 dB deg-1 for aspect angles between 3¿ and 6¿, and -7 dB deg-1 for aspect angles between 6¿ and 9¿. The magnitude of the phase velocity is at an approximate ion acoustic level (350 m/s) for aspect angle 3¿. For highly disturbed conditions the magnitude of the velocity can increase to >700 m/s for aspect angles <2¿. The tendency for the altitude of the most intense return to decrease by ~5 km as the aspect angle increases beyond 2¿ can be explained as a consequence of the variation of aspect angle with height. ¿American Geophysical Union 1992 |
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Abstract |
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Keywords
Ionosphere, Ionospheric irregularities, Ionosphere, Auroral ionosphere, Space Plasma Physics, Turbulence |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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