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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.

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