INTENSITIES AND POLARIZATION RATES OF WHISTLER-MODE VLF SIGNALS OBSERVED FROM A GROUND NETWORK NEAR L=4

VLF signals transmitted from Siple station in Antarctica that propagat ed through the ionosphere and magnetosphere to the northern hemisphere and triggered emissions generated by the Siple signals in the magneto sphere are radiated from wave exit areas on the ionospheric lower boun dary. The locations and extent of the wave exit areas are deduced from the wave intensity distributions measured on the ground. In this meth od we use measurements of wave magnetic intensity made simultaneously at six stations. The validity of this method is assessed by comparing the results with values simply estimated from a mathematical evaluatio n and with results of full wave calculations carried out by Nagano et al. (1986, 1987). We find close agreement among results obtained from the three methods and conclude that the wave intensity distribution an alysis is valid. The observed distribution of polarization rate also a grees well with the results of the full wave calculations carried out by Nagano et al. (1986, 1987) and with those obtained by the mathemati cal evaluation. As a result of analyzing a triggered emission in detai l, the extent of the wave exit area of the downgoing triggered emissio n is estimated to be 25-50 km or so at an altitude of 80 km. We believ e that this value relates to the horizontal extent of the duct through which the triggered emission propagated in the magnetosphere and iono sphere and that essentially only direct waves transmitted from the wav e source arrive within a range of 200 km from the wave intensity peak on the ground.