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Serpentine vegetation ofcuws within all of these zones. At the
lowest elevations, it differs from the surrounding vegetation by having
virtually no broadleaved evergreen tree species. The vegetation often consists
of a very open Jeffrey pine (Pinus jeffreyi) mixed grassland type often with
scattered manzanita (Arctostaphylos sp.). This contrasts with the much denser
surrounding vegetation which usually has an important broadleaf tree component.
At somewhat higher elevations (approximately 600m), other coniferous tree
species are present in the serpentine flora. The understory often has an open
cover of broadleaf tree species which are highly stunted. At this elevation,
non-serpentinized peridotite becomes an important associated ultramafic rock
type. This parent material can be vegetationally differentiated from the
serpentine vegetation by the much denser sclerophyll shrub and stunted broad-
leaf evergreen tree understory (Figure 1 illustrates this difference). At high-
er elevations (approximately 1,000m) the serpentine flora is distinct from the
surrounding flora by certain indicator species, many of which are stunted, and
a scattered shrub-grass understory. The broadleaf tree component, which is so
typical of the surrounding non-ultramafic rocks is virtually absent. Trees
which typically grow upon the higher elevation serpentine rocks include Port
Orford cedar (Chamaecyparis lawsoniana), Jeffrey pine, incense cedar, western
white pine (P. monticola), sugar pine (P. lambertiana), and Douglas fir.
Image Analysis
The primary imagery used in the analysis consisted of color and
color infrared aerial photography at scales varying between 1:15,840 and
1:130,000, and high altitude multispectral scanner imagery. The latter was
acquired by the NASA Ames Research Center over the study area on September 11,
1981. It was made with a modified Daedalus DEI-1260 scanner with ten operating
channels in the visible, near IR and thermal infrared (Table I). The imagery
was acquired at an altitude of 20,000m and , with a 1.25mrad IFOV, has a ground
resolution of approximately 25m X 25m.
The aerial photography was useful for separating the serpentine-
bearing rock types from the non-ultramafic rock types. A simulated false
color composite (FCC) made from the airborne scanner imagery was also useful
for separating those rock types. However, it required a ratio color composite
(made from ratioing the near IR to the red band, the red to a green band, and
the green to a blue band) and an enhanced 2.05 - 2.35 channel to separate
the serpentine from the non-serpentinized peridotite. A modified unsupervised
classification employing extensive ground data has been successful in a limited
area in separating those rock types. Attempts at using principal components
analysis techniques have so far not been successful for separating the
serpentine from the non-serpentinized peridotite. Further attempts will be made
with this technique.
JASPER RIDGE STUDY AREA
The Jasper Ridge Biological Preserve of Stanford University is
located 50km south of San Francisco and is situated on a low lying ridge on the
eastern flank of the Santa Cruz Mountains. It is bounded on the west by the
San Andreas Fault. Elevations within the study area range from 70m to 190m.
The study area receives most of its precipitation (approximately 70cm annually)
in the winter. Temperatures rarely reach freezing. Geologically, the ridge
consists of greenstone, chert, graywacke, and serpentine of the Jurassic-
Cretaceous Franciscan Formation and the Eocene Butano sandstone (Page and
Tabor, 1967).
The top of the ridge is a broad gently roll-ng plateau covered with
grassland. The surrounding north and east facing slopes are covered with