On the relation of the 'slant E condition' in polar cap ionograms to the solar wind sector structure

Physics

Scientific paper

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E Region, Interplanetary Magnetic Fields, Ionograms, Ionospheric Disturbances, Polar Caps, Solar Wind, Histograms, Magnetic Field Configurations, Polarity, Satellite Observation

Scientific paper

The 'slant E condition' (SEC) in polar cap ionograms has been shown previously to indicate excitation of the Farley-Buneman instability in the E region. The SEC at Godhavn (Greenland) is shown here to correlate with the solar wind sector structure, the occurrence rate of SEC being large a few days after passage of a sector boundary and declining in the trailing part of the sector. Analysis of SEC occurrence in terms of the solar wind velocity measured on board Heos 2 indicates that no SEC occurs when solar wind velocity is less than 350-400 km/sec (in apparent agreement with the interpretation of SEC in terms of the Farley-Buneman instability).

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