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Snow densities of the buried surface hoar and the layers
immediatelyabove and below show a trend similar to but
more pronounced than the time series from the previous
winter. Figure 6a shows that the densities of the surface
hoar and the snow above and below, within 2 cm, were
quite similar on 5 January. Again the adjacent snow lay-
ers densified at more rapid rates than the surface hoar.
Measurements of the surface-areato volume ratio provide
evidencethat grain growth accompaniedthe densification,
as shown in Figure 6b, while the buried surface hoar
showed little change.

GENERAL OBSERVATIONS AND DISCUSSION

Layers of buried surface hoar have microstructure that ex-
hibits extreme susceptibility to shear failure. The geom-
etry and spacing of the crystals as observed in the field
and on sections provide strong clues to the reasons. Sur-
face hoar crystals spread out as they grow upward (Lang
et al., 1985; Breyfogle, 1987), which can result in an um-
brella-like mechanism whennew snow falls. This depends
on weather eventssubsequentto hoar formation (Breyfogle,
1987). Both observations in the snow pit and on section
cuts showed large gaps between the surface hoar crystals
in this study. Figure 7a shows a classified section image
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Figure 4. Measured shear strength, rutschblock and grain sizes
plotted as time series with calculatedrutschblock score for surface
hoar layer buried 28 December 1995. Indicator shows time before
which avalanches were observed.
than 5.5 and none occurred when the calculated
rutschblock score was 5.5 or higher.
The heli-sking operation that surrounds the study site
reported natural and skier-triggered slab avalanches slid-
ing on the December 28th surface hoar on 7-10, 12 and 15
January, but none after 15 January 1996.
Initially we observed surface hoar crystals to 20 mm in
length. Although the following 11 weeks showed round-
ing and smoothing of the grains, 12 mm crystals were re-
ported on most test days including the final day. Analysis
of the digitized photographs supports these observations;
we measured little change in the average dimensions of
the surface hoar cr ystals. The photographs of the
disaggregated crystals do not show a decrease in crystal
size but rounding is apparent. The smallest reported crys-
tals, 2-6 mm, were reported on 6 February in the middle
of the observation period, which couq be due to spatial
variability. However, the subjective nature of collecting
and observingcrystals probably plays a role in thereported
variability.
Measurements of the layer thickness from the section
planes show the surface hoar settled by somewhat more
than 35% from 5 January to 18 January 1996, as shown in
Figure 5. After that the rate of compaction slowed sub-
stantially, as with the previous case. While the standard
deviation of the measurements remained low, again the
range of measurements overlapped for most of the test
period (Figure 5).
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Figure 6. Density(a) and surface-to-volume ratio (b) of layer of surface
hoar buried 28 December 1995 (V), and layers above (U) and below
(L). Measurements were made from section cuts.

as an example. The mechanical connectionacross the sur-
face hoar, from the layer above to the layer below, largely
relies on the bases of the surface hoar crystals.
Throughout the entire test period in both cases, the
averageslope-parallel cross section of ice grains (the mean
ice intercept) in the surface hoar layer was at least twice
that in the layers above and below. This means that the
individual crystals had higher strength than grains in ei-
ther the layer above or below. The number of ice connec-
tions between the buried surface hoar and snow above
and below was minimized at the base. Thus the number
of connections per unit area contributes to the very low
shear strength. Observations on section cuts show that this
variable does not change much over time, yet the shear
strength of the layer increases.
Mechanical tests and avalanchereleases show failures
at base of surface hoar layers in shovel, compression and
rutschblock tests, and in slab avalanches (Schweizer et
al., in preparation). Frequently surface hoar crystals grow
on a snow surface beneath which depth hoar or facet crys-
tals develop because the same meteorological conditions
can causeboth (e.g., Langet al., 1985). Figure 7aalso shows
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