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Mid-latitude spread-F structure
Institution:1. Royal Meteorological Institute (RMI), Ringlaan 3, Brussels B-1180, Belgium;2. Observatori de l''Ebre (OE), Univ. Ramon Llull – CSIC, Horta Alta 38, 43520 Roquetes, Spain;3. Leibniz-Institute of Atmospheric Physics at the University Rostock, Schlossstr. 6, Kuehlungsborn 18225, Germany;4. Lowell Digisonde International, 175 Cabot Street, Lowell, MA 01854, USA;5. University of Massachusetts Lowell, Space Science Laboratory, Lowell, MA 01854, USA;6. National Observatory of Athens, IAASARS, Metaxa and Vas. Pavlou, Palaia Penteli 15236, Greece;7. Institute of Atmospheric Physics, Czech Academy of Sciences, Bocni II 1401, 141 31 Prague, Czech Republic
Abstract:Spread-F has been observed at frequencies of 1.98, 3.84 and 5.80 MHz and multiple angles of arrival have been resolved using an HF radar near Brisbane (27°S, 153°E). The spreading of the ionogram trace has been shown to be due to a spread in angles of arrival of echoes, rather than any ‘vertical’ spreading. The reflection process appears to involve total specular reflection rather than scattering. The previously reported very strong bias for angles of arrival from the north-west at Brisbane is supported. The direction of movement of the reflection points is not radial and therefore, the structure cannot be purely frontal with purely linear movement, as is often supposed. The velocities are much less than for coexisting travelling ionospheric disturbances. The variations of angle of arrival, range and rate of change of range with frequency do not fit previously proposed ideas of the plasma distribution and an alternative is suggested in which the distortions of the isoionic surfaces resemble small, elongated, asymmetrical ‘hills’ or ‘dips’.
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