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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 15, issue 6
Ann. Geophys., 15, 760–766, 1997
https://doi.org/10.1007/s00585-997-0760-4
© European Geosciences Union 1997
Ann. Geophys., 15, 760–766, 1997
https://doi.org/10.1007/s00585-997-0760-4
© European Geosciences Union 1997

  30 Jun 1997

30 Jun 1997

Flow angle dependence for the asymmetry of broad 50-MHz coherent echoes at large magnetic aspect angles

A. V. Kustov1, G. J. Sofko1, J. A. Koehler1, and M. V. Uspensky2 A. V. Kustov et al.
  • 1Institute of Space and Atmospheric Studies, University of Saskatchewan, 116 Science Place, Saskatoon, Saskatchewan, S7N 5E2, Canada
  • 2Murmansk State Technical University, Murmansk, Sportivnaya, 1, 183023 Russia

Abstract. The skewness of broad Type 2-like spectra has been studied using data collected by two orthogonal CW 50-MHz radio links with co-located scattering volumes. Geometrical aspect angles of observations were about 10°. One short event was considered. For this event, the electron flow direction was changing periodically (period about 9 minutes) presumably due to the passage of a magnetospheric MHD wave through the ionosphere. It was found that for the radar observations along the electrojet flow, the skewness had the same sign as the mean Doppler shift with average absolute values in between 0.5-1.0. For observations perpendicular to the electrojet flow, spectra were more symmetrical (average skewness was around 0) and the sign of the skewness was sometimes opposite to the sign of the mean Doppler shift. These observations are interpreted in terms of contribution from both the Farley-Buneman and gradient-drift instabilities to the resultant spectrum. Differences with radar observations at small aspect angles are discussed.

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