The very low frequency (VLF) NPM signal from Hawaii was recorded at tw
o closely spaced (similar to 50 km) receivers (located at Palmer and F
araday stations) on the Antarctic Peninsula. Measurements of character
istic amplitude and phase signatures of lightning-induced electron pre
cipitation (LEP) events were made on three different days in March 199
2. Both amplitude and, for the first time, phase measurements are quan
titatively interpreted using a three-dimensional model of VLF propagat
ion in the Earth-ionosphere waveguide in the presence of lower ionosph
eric disturbances. This is the first time such a study has been undert
aken with mirrored precipitation. Differences between the amplitude an
d phase changes at the two sites are accounted for by the location of
the LEP ionospheric disturbance transverse to the VLF signal propagati
on paths. The change in these differences is explained by the horizont
al movement of the disturbance region and, therefore, the causative wh
istler duct footprint across the transmitter-receiver paths. Trends in
the amplitude and phase changes on a timescale of order 1 hour are fo
und to be encompassed by the modeling of the passage of the day-night
terminator along the paths.