Surface topography is of great importance in radar backscattering, but
the quantitative interpretation of data collected in the field is sti
ll a difficult problem. We present topographic profiles at 25-cm and 5
-cm horizontal resolution for three sites along a lava flow on Kilauea
Volcano, and use these data to illustrate techniques for surface roug
hness analysis. Height and slope distributions and the height autocorr
elation function are evaluated as a function of varying lowpass filter
wavelength for the 25-cm data. Rms slopes are found to increase rapid
ly with decreasing topographic scale and are typically much higher tha
n those found by modeling of Magellan altimeter data for Venus. A more
robust description of the surface roughness appears to be the ratio o
f rms height to surface height correlation length. For all three sites
this parameter falls within the range of values typically found from
model fits to Magellan altimeter waveforms. The 5-cm profile data are
used to estimate the effect of small-scale roughness on quasi-specular
scattering.