IGCP Board; 10th session; Report of the ... - unesdoc - Unesco
IGCP Board; 10th session; Report of the ... - unesdoc - Unesco
IGCP Board; 10th session; Report of the ... - unesdoc - Unesco
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interpretation for mineral and energy exploration,<br />
plant siting, waste disposal and <strong>the</strong> development<br />
<strong>of</strong> models for regional and continental<br />
tectonics. New spaceborne methods and associated<br />
technologies are being developed to produce<br />
data from which geologic information about<br />
large areas can be derived much more rapidly<br />
than by conventional techniques". The authors<br />
provide a generally balanced overview <strong>of</strong> progress<br />
and yet stress <strong>the</strong> spectral mapping approach<br />
to defining mineralized ground that <strong>the</strong>y<br />
have developed. As principal investigators <strong>of</strong><br />
SMIRR, <strong>the</strong>y tested <strong>the</strong> Landsat-D Thematic<br />
Mapper (TM) and <strong>the</strong> Shuttle Multispectral Infrared<br />
Radiometer (SMIRR) first from aircraft<br />
altitudes over Nevada and Utah mineral-rich<br />
test sites.<br />
1. Space Shuttle Flight: Two geological experiments<br />
were included in <strong>the</strong> scientific payload<br />
<strong>of</strong> <strong>the</strong> second flight <strong>of</strong> <strong>the</strong> Space Shuttle on 12-<br />
14 November, 1981. The objectives <strong>of</strong> <strong>the</strong><br />
SMIRR experiment were: (1) Obtain 10-channel<br />
radiometric data from orbit from a significant<br />
sample <strong>of</strong> geologic units world-wide in <strong>the</strong> spectral<br />
region 0.6 to 2.5 um with emphasis on <strong>the</strong><br />
region beyond 1.0 um; (2) Determine <strong>the</strong> value<br />
<strong>of</strong> <strong>the</strong> spectral bands chosen in <strong>the</strong> separation <strong>of</strong><br />
lithologie units based on <strong>the</strong>ir reflectances;<br />
(3) Determine <strong>the</strong> correlation between <strong>the</strong> radiances<br />
measured from orbit and <strong>the</strong> reflectance<br />
data obtained by a portable field spectrometer<br />
system; (4) Assess <strong>the</strong> effect <strong>of</strong> variable atmospheric<br />
absorption on <strong>the</strong> radiance values, particularly<br />
in <strong>the</strong> 2.0 to 2.5 um region; (5) Determine<br />
<strong>the</strong> spectral bands to be used in future multispectral<br />
scanners designed specifically for geological<br />
mapping uses; and (6) Test <strong>the</strong> value <strong>of</strong><br />
Shuttle as a platform for low-cost measurements<br />
<strong>of</strong> parameters vital to <strong>the</strong> design <strong>of</strong> new instrumentation<br />
for future flights.<br />
Measurements were made with a single 20-cm<br />
telescope containing a linear array <strong>of</strong> ten detectors<br />
and associated filters aligned along <strong>the</strong> spacecraft<br />
ground track. Data were obtained in<br />
100 x 100 m segments in a continuous strip along<br />
<strong>the</strong> subspacecraft track. A 16-mm framing camera<br />
was used to identify <strong>the</strong> position <strong>of</strong> <strong>the</strong><br />
ground track. Alex Goetz, Jet Propulsion Laboratory,<br />
Pasadena, California, is <strong>the</strong> principal<br />
investigator on SMIRR, and Larry Rowan, US<br />
Geological Survey, Reston, Virginia, is <strong>the</strong> coinvestigator.<br />
The results <strong>of</strong> that mission are<br />
being evaluated. Data were ga<strong>the</strong>red mainly<br />
over desert regions <strong>of</strong> Mexico, Spain, Italy,<br />
Greece, Turkey, Morocco, Egypt, and Saudi<br />
Arabia. Data are to be distributed to scientists<br />
where cooperating investigations have been established<br />
through this Project. Unfortunately,<br />
wea<strong>the</strong>r masses over <strong>the</strong> United States and Australia<br />
limited operations in <strong>the</strong>se areas.<br />
The o<strong>the</strong>r experiment was <strong>the</strong> Shuttle Imaging<br />
Radar (SIR-A). The objective <strong>of</strong> <strong>the</strong> Shuttle<br />
Imaging Radar-A experiment was to evaluate <strong>the</strong><br />
potential <strong>of</strong> spaceborne imaging radars in geolo<br />
42<br />
gic mapping and to determine <strong>the</strong> advantages <strong>of</strong><br />
using radar imagery in conjunction with Landsat<br />
imagery for Earth resources observation.<br />
The SIR-A is a syn<strong>the</strong>tic aperture imaging radar<br />
which uses <strong>the</strong> coherent echo from <strong>the</strong> surface to<br />
generate a high-resolution image. It uses its<br />
own energy to illuminate <strong>the</strong> surface, and generates<br />
an image from <strong>the</strong> backscatter echoes. It<br />
provides an all-wea<strong>the</strong>r capability because <strong>the</strong><br />
relatively long waves (microwave) are not effectively<br />
reflected or scattered by cloud water droplets.<br />
The SIR-A sensor operates at L-band frequencies<br />
<strong>of</strong> 23. 5-cm wavelength. The incidence angle<br />
at <strong>the</strong> surface is 50° at <strong>the</strong> centre <strong>of</strong> swath and differs<br />
by± 3° at <strong>the</strong> edges. The sensor is designed to<br />
be sensitive to surface backscatter cross-sections<br />
between -8 dB and -28 dB. The SIR-A data were<br />
recorded optically on board <strong>the</strong> Shuttle and all but<br />
6 feet <strong>of</strong> its film was used during <strong>the</strong> mission.<br />
After <strong>the</strong> shuttle landing, <strong>the</strong> signal film was retrieved,<br />
developed, and processed. Then it was<br />
converted to an image using an optical correlator.<br />
Charles Elachi, Jet Propulsion Laboratory, Pasadena,<br />
California, is <strong>the</strong> SIR-A principal investigator.<br />
Data were collected at numerous sites<br />
located between 39° N latitude and 38° S latitude<br />
in both experiments.<br />
2. Preliminary Metallogenic Map <strong>of</strong> North America<br />
and Landsat Mosaic: Under <strong>the</strong> chairmanship<br />
<strong>of</strong> P.W. Guild (1981a, b, c) a team <strong>of</strong> six<br />
geologists representing Canada, Greenland, Mexico,<br />
and Central America published <strong>the</strong> first<br />
"Preliminary Metallogenic Map <strong>of</strong> North America"<br />
at a scale <strong>of</strong> 1: 5, 000, 000. It is accompanied by<br />
a complex explanation which categorise 4, 215 ore<br />
deposits by commodities according to size, geologic<br />
environment, age, and minéralogie nature.<br />
Two USGS Circulars (858-A and -B) provide (A)<br />
numerical listing <strong>of</strong> deposits and (B) an alphabetical<br />
listing <strong>of</strong> deposits. This remarkable map<br />
was reproduced on an equal area - bipolar oblique<br />
conic conformai projection by electronic colour<br />
scanning <strong>of</strong> a hand-coloured original map. It will<br />
serve as an excellent basis for formulating new<br />
mineral exploration strategies and, we believe,<br />
will be enhanced fur<strong>the</strong>r when a new, ail-digitally<br />
processed Landsat Image Mosaic and Lineament<br />
Map <strong>of</strong> <strong>the</strong> North American Plate are completed.<br />
Present plans, however, call for <strong>the</strong> mosaic to<br />
be cast on a Transverse Mercator projection.<br />
3. Geobotanical Anomalies related to Porphyry<br />
Copper Mineralization: Birnie and Francica<br />
(1981) described <strong>the</strong> results <strong>of</strong> using an airborne<br />
multichannel spectrometer with a range from<br />
450-1000 m m over <strong>the</strong> known Mesatchee Creek<br />
porphyry copper prospect in central Washington.<br />
The entire area is covered with Douglas Fir and<br />
lesser amounts <strong>of</strong> western larch. Spectra from<br />
within <strong>the</strong> pyrite halo were anomalously high at<br />
565 nm and anomalously low at 465 nm. Individual<br />
spectra with a 565 nm/465 nm reflected radiance<br />
ratio value greater than 1.7 fall dominant -<br />
ly within <strong>the</strong> pyrite halo. The zone <strong>of</strong> mineralization<br />
was defined clearly by <strong>the</strong> cluster <strong>of</strong> anomalous<br />
spectra.