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Exploring the Unknown - NASA's History Office

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188<br />

OBSERVING THE EARTH FROM SPACE<br />

Table 1*<br />

RESOLUTION OF CLOUDS BY SUNLIGHT<br />

(Image orthicon f/10 camera operated at 20:1; + signal-to-noise ratio<br />

at rates of 40, 10, and 4 exposure frames/sec; and a satellite height of 350 mi)<br />

Minimum Resolvable Surface Dimension<br />

Contrast Aperture 40 Frames/Sec 10 Frames/Sec 4 Frames/Sec<br />

(%) (in.) (ft) (ft) (ft)<br />

100 0.5 200± 100± 64±<br />

1.0 100± 50± 32±<br />

2.0 50± 25± 16±<br />

5.0 20± 10± 6±<br />

25 0.5 800 400± 250±<br />

1.0 400 200± 125±<br />

2.0 200 100± 64±<br />

5.0 80 40± 25±<br />

10 0.5 2,000 1,000 640<br />

1.0 1,000 500 320<br />

2.0 500 250 160<br />

5.0 200 100 64<br />

2.5 0.5 8,000 4,000 2,500<br />

1.0 4,000 2,000 1,250<br />

2.0 2,000 1,000 640<br />

5.0 800 400 250<br />

1 0.5 20,000 10,000 6,400<br />

1.0 10,000 5,000 3,200<br />

2.0 5,000 2,500 1,000<br />

5.0 2,000 1,000 640<br />

* The material contained in this table was prepared by Dr. R. S. Wehner and is included<br />

in RAND Report R-217 (see footnote 1 . . .).<br />

+ It should be noted that this table (and also Tables 2 and 3) is unrealistic in that <strong>the</strong><br />

20:1 signal-to-noise ratio is applicable only to 25 per cent contrast. For 10 per cent<br />

contrast, a signal-to-noise ratio of 50:1 is required. This would mean a required transmitter<br />

power increase by a factor of 2.5 (assuming a 2-in. aperture 1000 TV lines, and<br />

a frame frequency of 10 sec). This is still not prohibitive but does become so with a<br />

substantial increase in ei<strong>the</strong>r <strong>the</strong> number of TV lines or <strong>the</strong> frame frequency.<br />

± Values of computed resolution smaller than realizable with present commercial image<br />

orthicons.

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