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9.3 Drag 503<br />

The corresponding Reynolds number 1assuming v 1.57 <br />

10 4 ft 2 s2 is<br />

Re UD<br />

n<br />

91.2 ft s 10.125 ft2<br />

1.57 10 4 ft 2 s<br />

7.26 104<br />

For this value of Re we obtain from Fig. 9.21, C D 0.5. Thus,<br />

our assumed value of C D 0.5 was correct. The corresponding<br />

value of U is<br />

U 91.2 fts 62.2 mph (Ans)<br />

COMMENTS By repeating the calculations for various altitudes,<br />

z, above sea level (using the properties of the U.S. Standard<br />

Atmosphere given in Appendix C), the results shown in Fig.<br />

E9.11b are obtained. Because of the decrease in density with altitude,<br />

the hail falls even faster through the upper portions of the<br />

storm than when it hits the ground.<br />

Clearly, an airplane flying through such an updraft would feel<br />

its effects 1even if it were able to dodge the hail2. As seen from<br />

Eq. 2, the larger the hail, the stronger the necessary updraft.<br />

Hailstones greater than 6 in. in diameter have been reported. In reality,<br />

a hailstone is seldom spherical and often not smooth. However,<br />

the calculated updraft velocities are in agreement with measured<br />

values.<br />

U, mph<br />

140<br />

120<br />

100<br />

80<br />

60<br />

40<br />

20<br />

(0, 62.2 mph)<br />

0<br />

0 10,000 20,000 30,000 40,000<br />

z, ft<br />

F I G U R E E9.11b<br />

The drag coefficient<br />

is usually independent<br />

of Mach number<br />

for Mach<br />

numbers up to approximately<br />

0.5.<br />

Compressibility Effects. The above discussion is restricted to incompressible flows. If<br />

the velocity of the object is sufficiently large, compressibility effects become important and the<br />

drag coefficient becomes a function of the Mach number, Ma Uc, where c is the speed of sound<br />

in the <strong>fluid</strong>. The introduction of Mach number effects complicates matters because the drag<br />

coefficient for a given object is then a function of both Reynolds number and Mach number—<br />

C D f1Re, Ma2. The Mach number and Reynolds number effects are often closely connected because<br />

both are directly proportional to the upstream velocity. For example, both Re and Ma increase<br />

with increasing flight speed of an airplane. The changes in C D due to a change in U are due<br />

to changes in both Re and Ma.<br />

The precise dependence of the drag coefficient on Re and Ma is generally quite complex<br />

1Ref. 132. However, the following simplifications are often justified. For low Mach numbers, the<br />

drag coefficient is essentially independent of Ma as is indicated in Fig. 9.23. For this situation, if<br />

Ma 6 0.5 or so, compressibility effects are unimportant. On the other hand, for larger Mach number<br />

flows, the drag coefficient can be strongly dependent on Ma, with only secondary Reynolds<br />

number effects.<br />

For most objects, values of C D increase dramatically in the vicinity of Ma 1 1i.e., sonic<br />

flow2. This change in character, indicated by Fig. 9.24, is due to the existence of shock waves as<br />

3.0<br />

2.5<br />

U<br />

D<br />

2.0<br />

__________ <br />

U 2 bD<br />

1__<br />

2 ρ<br />

1.5<br />

C D =<br />

1.0<br />

0.5<br />

0<br />

0<br />

U<br />

b = length<br />

4D<br />

D<br />

0.5 1.0<br />

Ma<br />

F I G U R E 9.23<br />

Drag coefficient as a function<br />

of Mach number for<br />

two-dimensional objects in<br />

subsonic flow (Ref. 5).

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