Detailed study of the reflected phases from the Moho, identified in th
e seismic reflection recordings of the 1986 Nevada PASSCAL lithospheri
c seismic experiment, place important constraints on the fine structur
e and geological nature of the Mohorovicic discontinuity. Two differen
t spectral ratio techniques are used to estimate the reflectivity of t
he Moho. We evaluate the ratio of the reflected PmP phase to the incid
ent source amplitude. We also calculated the spectral ratio of the PmP
phase with a reference reflection. Reflectivity estimates, calculated
using both spectral ratio techniques, are very consistent. High refle
ctivity within the range 0.28-0.39 was obtained. The analysis of the s
pectral characteristics suggests a layered structure for the Moho with
an average thickness between 85 and 250 m. These results require a la
yered Moho structure with high impedance contrasts. Amplitude modeling
using a reflectivity algorithm demonstrates that constructive interfe
rence from a 1.0-1.5-km-thick layered structure produces amplitudes an
d waveforms comparable to the data. To achieve such high reflectivitie
s, 20-25% of the Moho consists of layers with velocities below 6.5 km/
s. The remaining layers have velocities between 7.7 and 8.1 km/s. Geol
ogically, the low velocities are consistent with velocities characteri
stics of basaltic magmas (partial melts). The high velocities are char
acteristic of mantle material. The partial melts may represent an expr
ession of present-day underplating.