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AE 1350 Lecture #4

AE 1350 Lecture #4

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AE 1350 Lecture #4. PREVIOUSLY COVERED TOPICS. Preliminary Thoughts on Aerospace Design Specifications (“Specs”) and Standards System Integration Forces acting on an Aircraft The Nature of Aerodynamic Forces Lift and Drag Coefficients. TOPICS TO BE COVERED. - PowerPoint PPT Presentation

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Page 1: AE 1350 Lecture #4

AE 1350Lecture #4

Page 2: AE 1350 Lecture #4

PREVIOUSLY COVERED TOPICS

• Preliminary Thoughts on Aerospace Design

• Specifications (“Specs”) and Standards

• System Integration

• Forces acting on an Aircraft

• The Nature of Aerodynamic Forces

• Lift and Drag Coefficients

Page 3: AE 1350 Lecture #4

TOPICS TO BE COVERED• Why should we study properties of

atmosphere?

• Ideal Gas Law

• Variation of Temperature with Altitude

• Variation of Pressure with Altitude

• Variation of Density with Altitude

• Tables of Standard Atmosphere

Page 4: AE 1350 Lecture #4

Why should we study Atmospheric Properties

• Engineers design flight vehicles, turbine engines and rockets that will operate at various altitudes.

• They can not design these unless the atmospheric characteristics are not known.

• For example, from last lecture,

• We can not design a vehicle that will operate satisfactorily and generate the required lift coefficient CL until we know the density of the atmosphere, .

SV

LCL

2

21

Page 5: AE 1350 Lecture #4

What is a standard atmosphere?• Weather conditions vary around the globe, from

day to day.• Taking all these variations into design is

impractical.• A standard atmosphere is therefore defined, that

relates fight tests, wind tunnel tests and general airplane design to a common reference.

• This common reference is called a “standard” atmosphere.

Page 6: AE 1350 Lecture #4

International Standard Atmosphere

Standard Sea Level Conditions

Pressure 101325 Pa 2116.7 lbf/ft2

Density 1,225 Kg/m3 0.002378 slug/ft3

Temperature 15 oC or 288 K 59 oF or 518.4 oR

Page 7: AE 1350 Lecture #4

Ideal Gas Law orEquation of State

• Most gases satisfy the following relationship between density, temperature and pressure:

• p = RT– p = Pressure (in lb/ft2 or N/m2)– = “Rho” , density (in slugs/ft3 or kg/m3)– T = Temperature (in Degrees R or degrees K)– R = Gas Constant, varies from one gas to another.

– Equals 287.1 J/Kg/K or 1715.7 ft lbf/slug/oR for air

Page 8: AE 1350 Lecture #4

Speed of Sound• From thermodynamics, and compressible flow

theory you will study later in your career, sound travels at the following speed:

• • where,

– a = speed of Sound (m/s or ft/s) = Ratio of Specific Heats = 1.4

– R = Gas Constant– T = temperature (in degrees K or degrees R)

RTa

Page 9: AE 1350 Lecture #4

Temperature vs. Altitude

Temperature, degrees K

Altit

ude,

km

288.16 K

11km216.66K

25 km

47 km, T= 282.66 K

53 km

79 km165.66 K

90 km

TroposphereStratosphere

Page 10: AE 1350 Lecture #4

Pressure varies with Height

The bottom layers have to carry more weight than those at the top

Page 11: AE 1350 Lecture #4

Consider a Column of Air of Height dhIts area of cross section is A

Let dp be the change in pressure between top and the bottom

Pressure at the top = (p+dp)

Pressure at the bottom = p

dh

Page 12: AE 1350 Lecture #4

Forces acting on this Column of Air

Force = Pressure times Area = (p+dp)A

Force = p A

Weight of air= gA dh

dh

Page 13: AE 1350 Lecture #4

Force Balance

Force = (p+dp)A

Force = p A

gA dh

Downward directed force= Upward force(p+dp)A + g A dh = pA

Simplify:

dp = - g dh

Page 14: AE 1350 Lecture #4

Variation of p with T

dp = - g dh

Use Ideal Gas Law (also called Equation of State):

p = R T = p/(RT)

dp = - p / (RT) g dh

dp/p = - g/(RT) dh Equation 1

This equation holds both in regions where temperature varies,and in regions where temperature is constant.

Page 15: AE 1350 Lecture #4

Variation of p with T in Regionswhere T varies linearly with height

From the previous slide,

dp/p = - g/(RT) dh Equation 1

Because T is a discontinuous function of h (i.e. has breaks in its shape),we can not integrate the above equation for the entire atmosphere. We will have to do it one region at a time.

In the regions (troposphere, stratosphere), T varies with h linearly.

Let us assume T = T1 +a (h-h1)

The slope ‘a’ is called a Lapse Rate.

h

h=h1

T=T1

Page 16: AE 1350 Lecture #4

Variation of p with T when T varies linearly (Continued..)

From previous slide, T = T1 +a (h-h1)An infinitesimal change in Temperature dT = a dh

Use this in equation 1 : dp/p = - g/(RT) dh

We get: dp/p = -g/(aR)dT/T

Integrate. Use integral of dx/x = log x.

Log p = -(g/aR) log T + C Equation 2

where C is a constant of integration.

Somewhere on the region, let h = h1 , p=p1 and T = T1

Log p1 = -(g/aR) log T1 + C Equation 3

Page 17: AE 1350 Lecture #4

Variation of p with T when T varies linearly (Continued..)

Subtract equation (3) from Equation (2):

log p - log p1 = - g/(aR) [log T - log T1]

log (p/p1) = - g / (aR) log ( T/T1)

Use m log x = log (xm)

aR

g

T

T

p

p

11

loglog aR

g

T

T

p

p

11

Page 18: AE 1350 Lecture #4

Variation of with T when T varies linearly

From the previous slide, in regions where temperature varieslinearly, we get:

aR

g

T

T

p

p

11

Using p = RT and p1 = 1RT1, we can show that density varies as:

1

11

aR

g

T

T

Page 19: AE 1350 Lecture #4

Variation of p with altitude hin regions where T is constant

In some regions, for example between 11 km and 25 km, thetemperature of standard atmosphere is constant.

How can we find the variation of p with h in this region?

We start again with equation 1.

dp/p = - g/(RT) dh Equation 1

Integrate: log p = - g/(RT) h + C

Page 20: AE 1350 Lecture #4

Variation of p with altitude hin regions where T is constant (Continued..)

From the previous slide, in these regions p varies with h as:

log p = -g /(RT) h + C

At some height h1, we assume p is known and his given by p1.

Log p1 = - g/(RT) h1 + C

Subtract the above two relations from one another:

log (p/p1) = -g/(RT) (h-h1)

Or, 1

1

hhRT

g

ep

p

Page 21: AE 1350 Lecture #4

Concluding Remarks• Variation of temperature, density and pressure

with altitude can be computed for a standard atmosphere.

• These properties may be tabulated.

• Short programs called applets exist on the world wide web for computing atmospheric properties.

• Study worked out examples to be done in the class.