21.03.2013 Views

Exploring the Unknown - NASA's History Office

Exploring the Unknown - NASA's History Office

Exploring the Unknown - NASA's History Office

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

ty will determine <strong>the</strong> departure from an adiabatic lapse rate, while <strong>the</strong> degree of cloudiness<br />

(moisture) will help an analyst to decide whe<strong>the</strong>r to use <strong>the</strong> moist or <strong>the</strong> dry adiabatic<br />

lapse rate as <strong>the</strong> limiting one.)<br />

Vertically developed cloud will also aid in determining <strong>the</strong> temperature gradient of<br />

<strong>the</strong> surrounding area. This is true because of <strong>the</strong> fact that <strong>the</strong> vertical shear, as indicated<br />

[18] by <strong>the</strong> slope of towering cumulus and cumulonimbus clouds, orients <strong>the</strong> direction of<br />

<strong>the</strong> higher and lower temperatures in <strong>the</strong> areas. This method is employed by taking <strong>the</strong><br />

direction of vertical shear as being from <strong>the</strong> low levels toward <strong>the</strong> high levels. If one <strong>the</strong>n<br />

faces in <strong>the</strong> direction of shear in <strong>the</strong> nor<strong>the</strong>rn hemisphere, <strong>the</strong> lower temperature will be<br />

on <strong>the</strong> observer’s left and <strong>the</strong> higher on <strong>the</strong> observer’s right (see Fig. 3).<br />

This relationship holds for <strong>the</strong> nor<strong>the</strong>rn hemisphere. In <strong>the</strong> sou<strong>the</strong>rn hemisphere <strong>the</strong><br />

directions of decreasing and increasing temperature in relations to vertical shear are<br />

reversed.<br />

Pressure<br />

Fig. 3—Vertical wind shear—temperature gradient relationship<br />

It is apparent that no quantitative values of pressure are forthcoming from this analysis.<br />

Fur<strong>the</strong>rmore, it is virtually impossible even to make a quantitative estimate o<strong>the</strong>r than<br />

to state whe<strong>the</strong>r <strong>the</strong> area is thought to be under <strong>the</strong> influence of a high- or a low-pressure<br />

system. Charts of average pressures for various times of <strong>the</strong> year in different areas of <strong>the</strong><br />

world are available. Using <strong>the</strong>se and <strong>the</strong> wea<strong>the</strong>r situation at <strong>the</strong> time, trends of pressure<br />

may be established. This information when applied in conjunction with known wea<strong>the</strong>r<br />

may be a very useful tool for forecasting purposes. Little work has been attempted on this<br />

subject in this pilot study, and <strong>the</strong> above should serve only as a possible starting point for<br />

any detailed research along <strong>the</strong>se lines.<br />

C. F. Brooks 15 points out some fur<strong>the</strong>r pressure information that may be obtained<br />

from clouds. He says, in effect, that, since in <strong>the</strong> presence of any constant vertical shear<br />

<strong>the</strong> cumulus clouds will tend to lean or slope (<strong>the</strong> amount of departure from <strong>the</strong> vertical<br />

being a resultant of <strong>the</strong> vertical velocity and <strong>the</strong> rate of change of wind velocity with<br />

height), any cloud that has a uniform rate of vertical growth and a 90˚ slope throughout<br />

is an indication of <strong>the</strong> “uniformity of wind velocity in all layers pierced.” This indicates a<br />

decrease of horizontal pressure gradient with height. (This can be shown very simply by<br />

an examination of <strong>the</strong> geostrophic wind equation<br />

V g = 1 ( p) 1,<br />

p ( n) λ<br />

where V g = <strong>the</strong> geostrophic wind velocity<br />

p = density o air<br />

p/ n = horizontal pressure gradient<br />

λ = Coriolis parameter.<br />

EXPLORING THE UNKNOWN 199<br />

[19] It can be seen that since λ, which depends on <strong>the</strong> sine of <strong>the</strong> latitude, will remain<br />

constant and p decreases with height, p/ n must also decrease for V g , to remain constant.)<br />

This decrease turns out to be very small when actual values are used. In <strong>the</strong> case of<br />

a uniformly growing cumulus that slopes in its lower layers and <strong>the</strong>n straightens or even<br />

15. C. F. Brooks, “Clouds in Aerology and Forecasting,” B. Amer. Meteorol. Soc., Vol. 22, November, 1941,<br />

pp. 335–345.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!