mineral mapping studies such as those done at well known
localities like Cuprite, Nevada, this exercise tried to simulate a
operational situation often encountered in mineral exploration,
in which remote sensing is used as the first tool for defining
targets before the geologist sets foot on the ground. Therefore,
techniques that do not require a priori input of ground data
were favored and assessed in their ability to convert image data
to ground reflectance and for identifying surface materials.
3. STUDY AREA
The area selected for this study is the Bodie mining district and
part of the neighboring Paramount district located in Mono
County, California, USA (Figure 1). AVIRIS data for this area
were acquired in August 1992 by NASA's ER-2 aircraft. The
scene used in this study consists of 614 x 512 pixels (10.44 x
9.70 km) in 224 bands, at 16-bit radiometric resolution,
corresponding to approximately 141 MBytes of data. It covers
the Bodie district almost entirely and the eastern portion of the
Paramount district between Atastra and Rough creeks.
r 382 12’
119° 00’
Figure 1 - Location of the study area. The rectangle around Bodie marks the outline of the AVIRIS scene and the locations marked
as PA, SH and BB are refered in the text.
4. GEOLOGY AND MINERALIZATION OF THE
BODIE AND PARAMOUNT DISTRICTS
Bodie was an important gold-silver mining district in the
second half of the nineteenth century and a mercury mine was
exploited in the Paramount district. Tertiary (7.8 to 9.4 Ma)
intermediate to basic volcanic rocks (dacitic, andesitic and
rhyolitic lavas, plugs, tuffs and breccias) underlie both districts.
Hydrothermal alteration associated with precious metal
concentration at Bodie is probably the result of intense thermal
spring activity, some of which can still be found in this region
along fault zones (Silberman et al., 1995).
Bodie has mixed characteristics of a bonanza-type lode quartz
vein deposit and a large-scale stockwork system, with gold
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occurring in quartz veins and quartz-adularia-chalcedony
stockworks in the center of the district. Petrographic work by
Herrera et al. (1993) showed vertical and lateral zoning in the
alteration with silicification in the center surrounded by zones
of potassic, argillic and sericitic alteration and an outer zone of
propylitic alteration. Little information is available for the
Paramount district due to the lack of important mineralization,
but the district has recently been prospected for bulk tonnage
precious metal mineralization (Herrera et al., 1993). Geological
characteristics observed at Paramount are very similar to those
in Bodie and the origin of the alteration is believed to be similar
(Silberman et al., 1995).
5. DATA CALIBRATION TO SURFACE REFLECTANCE
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B7. Vienna 1996