SummaryA technique of recording the elevation angle by a phase comparison method is described and applied to ground backscatter echoes at 16 MHz. It is shown that the results may be explained in terms of ionospheric tilts of 1 ° or 2° near sunset.
INTRODUOTIONSeveral methods are at present available to measure the angle of elevation of ionospheric radio waves at receiving stations (e.g. Friis, Feldman, and Sharpless 1934;Ross, Bramley, and Ashwell 1951;Miya 1954;Bain 1961). The present paper describes a phase comparison method and an electronically controlled phase changer. The aim of this project was to measure elevation angle of ground backscatter echoes and to test the extent to which the theory of Appleton and Beynon used by Shearman (1956) and later by Steele (1965a) is valid. The pre-sunset and post-sunset results are compared with the theory and the discrepancy is explained by involving a tilted ionosphere.II. EXPERIMENTAL TEOHNIQUE AND REOORDINGThe transmission was carried out at 16 MHz by a highly directive backscatter sounder (Thomas and McNicol 1960) from Brisbane (lat. 27 ·5° S., long. 152 ·9° E.). A pulse of 800 fLsec with a repetition frequency of 8 ·33 sec-1 was transmitted using an array of four three-element Yagi antennas. The Yagi array was aimed in a fixed direction, usually to the east or to the west. The calibration of the horizontal and vertical radiation pattern of the antenna system has been treated in detail elsewhere (Steele 1965b; McInnes 1966). The same antenna system is used for transmission and reception. The Brisbane receiver is used to record a range-amplitude display of the signal on a film moving continuously past the trace on an oscilloscope screen that is displayed by brightness or black-out modulation of the time-base trace. The gain of the receiver was decreased in 12 steps of 3 dB each over a period of 1 min.Two similar Yagi antennas, located 5'\ (,\ = 18·75 m) apart along an east-west direction on the ground, were used for the measurement of the elevation angle at Amberley (lat. 27 ·7° S., long. 152.7° E.) about 20 miles from Brisbane. The output of the two antennas was received as shown in the block diagram of Figure 1. In the signal path from one antenna was inserted a continuously-scanned phase changer, which changed its phase uniformly between 0° and 360° in 30 sec. The output of the other antenna and the output of the phase changer were added, amplified, and passed through a gated amplifier that selected a narrow slice (equivalent to 10 km) of the leading edge of the ground backscatter echo. The selected portion of the echo brightened the spot of a cathode ray tube, which was then photographed on a continuously