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Exploring the Unknown - NASA's History Office

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182<br />

OBSERVING THE EARTH FROM SPACE<br />

storms, size and intensity would vary geographically. A meteorologist given a clear picture<br />

of <strong>the</strong> cloud distribution, as here portrayed, could without difficulty sketch in a very useful<br />

wea<strong>the</strong>r chart showing location of <strong>the</strong> various stormy and fair wea<strong>the</strong>r areas; in fact, he<br />

would have a much better idea of <strong>the</strong> large-scale wea<strong>the</strong>r distribution than his Earthbound<br />

colleague, who is forced to rely on scattered observations taken at or near <strong>the</strong><br />

Earth’s surface.<br />

As for obtaining two or more “fixes” on storms within 12 hours, this would be possible<br />

as <strong>the</strong> vehicle makes successive passages toward <strong>the</strong> Poles—and <strong>the</strong> closer to <strong>the</strong> Pole<br />

<strong>the</strong> storm is located <strong>the</strong> more such fixes could be made. For example, <strong>the</strong> large fully developed<br />

storm depicted over Hudson Bay would be visible first on one leg of <strong>the</strong> path, again<br />

4 hours later on <strong>the</strong> next leg, and again 4 hours later on a third leg. This would, by reference<br />

to known surface features, enable tracking of <strong>the</strong> storm in <strong>the</strong> 12-hour interval. A<br />

word of caution is necessary since <strong>the</strong> clouds which on one hand make possible <strong>the</strong> visual<br />

identifications of <strong>the</strong> storm will hinder its location with respect to known surface features.<br />

Nor would trying to track <strong>the</strong> storm by observing <strong>the</strong> edge of its cloud shield<br />

necessarily give an accurate track, since <strong>the</strong> changing cloud pattern associated with such<br />

large, usually dissipating storms may give spurious motions, as <strong>the</strong>y form on one side and<br />

dissipate on <strong>the</strong> o<strong>the</strong>r. Thus, <strong>the</strong>re will not be too good an accuracy for tracking <strong>the</strong>se<br />

large storms, but this is not too important since <strong>the</strong>ir speed of motion is usually slow anyway.<br />

On <strong>the</strong> o<strong>the</strong>r hand, <strong>the</strong> incipient or developing storm, so important for future wea<strong>the</strong>r<br />

developments, is faster moving and has a less extensive cloud system associated with it<br />

so that more accurate fixes should be possible. The hurricane, with its cloud bands, similar<br />

to <strong>the</strong> arms of a spiral nebula, and its open “eye” at <strong>the</strong> centre, will be a much easier<br />

storm to detect and follow accurately. Cloud systems associated with cold fronts and squalllines<br />

will also lend <strong>the</strong>mselves to accurate tracking.<br />

As <strong>the</strong> days pass, however, and <strong>the</strong> Earth moves in its orbital motion about <strong>the</strong> Sun,<br />

<strong>the</strong> vehicle will cross each latitude about 4 minutes earlier than <strong>the</strong> preceding day. Thus,<br />

if motion northward is started at noon on March 21, this will change on June 21 to 6 a.m.<br />

moving north, and 6 p.m. moving south; in this case, <strong>the</strong> field of view in daylight will be<br />

mostly to <strong>the</strong> east (going north) and to <strong>the</strong> west (going south) and <strong>the</strong> efficiency of <strong>the</strong><br />

vehicle as a cloud patrol will have diminished considerably. On September 21 its efficiency<br />

will increase again as it moves south at noon and north at midnight. However, on<br />

December 21 its efficiency will drop again—and to its lowest point as far as <strong>the</strong> Nor<strong>the</strong>rn<br />

Hemisphere is concerned. It will move north at 6 p.m. and south at 6 a.m.—but because<br />

of <strong>the</strong> low solar declination at this time and consequent lack of daylight hours, its usefulness<br />

as a cloud and storm detector will be greatly impaired. This is a serious defect because<br />

<strong>the</strong> winter season is <strong>the</strong> busiest period for storms in <strong>the</strong> Nor<strong>the</strong>rn Hemisphere. This suggests<br />

as a better [276] solution that <strong>the</strong> preceding plan, <strong>the</strong> initial movement northward<br />

or southward at noon on December 21. This will <strong>the</strong>n give optimum conditions for winter<br />

wea<strong>the</strong>r patrol—excluding <strong>the</strong> Arctic and some distance south where little or no daylight<br />

will prevail.<br />

This visual cloud reconnaissance might be taken automatically by a television camera<br />

in an unmanned vehicle and relayed to Earth to various collection centres for study, analysis<br />

and exchange with o<strong>the</strong>r forecast offices to obtain a truly global wea<strong>the</strong>r picture. If <strong>the</strong><br />

vehicle could be properly manned and equipped, <strong>the</strong>n o<strong>the</strong>r valuable geophysical and<br />

solar data could be obtained as follows:—<br />

(a) Temperature of <strong>the</strong> Earth’s surface and a rough average temperature of <strong>the</strong> intervening<br />

atmosphere by observing <strong>the</strong> infrared spectrum.<br />

(b) Precipitation Areas (rain, snow, etc.) could be detected by radar as well as <strong>the</strong><br />

heights of <strong>the</strong>ir formation above <strong>the</strong> surface; also <strong>the</strong> height of <strong>the</strong> freezing level<br />

which shows as a bright band in <strong>the</strong> radar scope.

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