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Predicting Weather By The Moon - Xavier University Libraries

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Barometer<br />

Pascal also missed a previous opportunity by only<br />

two days. Had he gone up the mountain 4 days beforehand,<br />

when he had originally planned to, and taken note of the<br />

day and night differences in pressure at that height (which<br />

would have entailed staying up on the mountain); then compared<br />

them to those taken at sea-level over the same period<br />

he might have noted some pressure discrepancy<br />

changes over the course of a day that could be expressed<br />

as a function of height.<br />

<strong>The</strong> atmosphere can alter in height by several miles<br />

twice a day like the sea tide. Yet the barometer may not<br />

change, because it only measures, at sealevel, the weight<br />

of a column of air a square inch in ground area. <strong>The</strong> barometer<br />

does not and cannot measure the height of the atmosphere,<br />

only the weight. Such an experiment has yet to be<br />

done. I believe it has been.<br />

Harry Alcock, an umbrella maker from the Waikato,<br />

told me how he once fitted a filtered photographic exposure<br />

meter to a telescope aimed at the Sun. <strong>The</strong> filter was a<br />

lens from a discarded pair of sunglasses. <strong>The</strong> meter was<br />

graduated for a reading range of from 14.0 – 14.7. <strong>The</strong> telescope<br />

had an elevation angle calibration fitted, and readings<br />

were taken throughout the day so Sun angles could be<br />

catered for. Brightness values were recorded on every<br />

cloud-free day. Later, the experiment was repeated using a<br />

Cushing solar energy meter, yielding the same results. Why<br />

brightness? Because the less compacted the atmosphere,<br />

the duller will be the Sun, there being more interference to<br />

the passage of the Sun’s rays through the atmospheric layers.<br />

147

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