Question 1 of 7: Standard-atmosphere altitudes, Pitot-static reading and stagnation pressure
Nivaar worked solution (AI-drafted; not reviewed by a licensed engineer)
Notes on this paper
Paper format. National Examinations,
December 2013 — 07-Mec-B7 Aero and Space Flight. Three hours,
OPEN BOOK, any non-communicating calculator permitted. Seven
questions are printed and all carry equal value; the paper states that
any six constitute a complete examination and that only the first six
appearing in the answer book will be marked, so each question is worth 20 of
the 120 marks a candidate can attempt. The printed marking key splits every
question into its sub-parts, and those weights are reproduced in the headings
below. All seven questions are solved here, because this set is
a study resource rather than a timed sitting. The paper also instructs the
candidate to state any assumption made where a required quantity has been
omitted; that instruction is used explicitly in Questions 4 and 5, where the
thrust lapse with altitude and the ground-run averaging method are not given.
Reference texts. Solutions follow the conventions of the
texts recommended for this examination code:
J. D. Anderson Jr., Introduction to Flight, 9th ed. — the
standard atmosphere and the four altitudes (Ch. 3), incompressible
aerodynamics and the Pitot-static tube (§3.4, §4.11), airplane
performance (Ch. 6), atmospheric entry (§8.11). This is the primary
reference throughout.
J. D. Anderson Jr., Fundamentals of Aerodynamics, 6th ed. —
finite-wing theory and induced drag (Ch. 5), transonic flow and
drag divergence (Ch. 11).
B. N. Pamadi, Performance, Stability, Dynamics and Control of
Airplanes, 3rd ed. — take-off and landing field lengths (Ch. 2),
turning flight and the load factor (Ch. 2), static stability (Ch. 3).
W. F. Phillips, Mechanics of Flight, 2nd ed. — the parabolic
drag polar, minimum-drag and maximum-climb speeds (Ch. 3).
P. H. Oosthuizen & W. E. Carscallen, Introduction to Compressible
Fluid Flow, 2nd ed. — critical Mach number and compressibility
effects (Ch. 1, Ch. 8).
H. J. Allen & A. J. Eggers, A Study of the Motion and Aerodynamic
Heating of Ballistic Missiles Entering the Earth's Atmosphere at High
Supersonic Speeds, NACA Report 1381 (1958) — the closed-form
ballistic-entry solution used in Question 7.
SI units are used throughout, matching the paper. The International Standard
Atmosphere constants are taken as
$p_{0}=101.325\ \text{kPa}$, $T_{0}=288.15\ \text{K}$,
$\rho_{0}=1.225\ \text{kg}\,\text{m}^{-3}$, lapse rate
$L=0.0065\ \text{K}\,\text{m}^{-1}$ through the troposphere,
$R=287.05\ \text{J}\,\text{kg}^{-1}\,\text{K}^{-1}$ and
$g=9.80665\ \text{m}\,\text{s}^{-2}$ inside the atmosphere model. Aircraft
weights use the rounded $g=9.81\ \text{m}\,\text{s}^{-2}$ that Canadian
examination practice expects. All pressures are absolute.
Question 1: Standard-atmosphere altitudes, Pitot-static reading and stagnation pressure (20 marks — a 8, b 6, c 6)
Find. The pressure, temperature and density altitudes
corresponding to the measured cruise state, the ambient density that produces the
density altitude, the Pitot-minus-static pressure difference at the second
condition, and the maximum (stagnation) pressure on the blunt body at the third.
The four altitudes compared. Only the geometric height is a geometric fact; the other three are ISA look-ups — the height at which the standard atmosphere reproduces the measured temperature, pressure and density respectively.
Approach. Each of the three altitudes is the height at which
the standard atmosphere alone reproduces one measured property, so each is
found by writing the ISA relation for that property and inverting it for height;
parts (b) and (c) are then two applications of the same incompressible Bernoulli
statement, once to read dynamic pressure off a probe and once to add it to the
ambient static pressure at a stagnation point.
Part (a) — write the troposphere model and get the temperature
altitude directly. Below $11\ \text{km}$ the ISA temperature falls
linearly, $T=T_{0}-Lh$, so the height at which the standard atmosphere is as cold
as the measurement follows immediately:
$$\begin{aligned}
h_{T} &= \frac{T_{0}-T}{L} \\
&= \frac{288.15-233.15}{0.0065} \\
&= 8461.5\ \text{m}
\end{aligned}$$
The aeroplane is at $10{,}000\ \text{m}$ but the air around it is as warm as
standard air at only $8460\ \text{m}$: this day is warmer than standard aloft.
Invert the ISA pressure law for the pressure altitude.
Integrating the hydrostatic equation with the linear lapse rate gives the
pressure ratio as a power of the temperature ratio,
$$\begin{aligned}
\frac{p}{p_{0}} &= \left(1-\frac{Lh}{T_{0}}\right)^{g/(LR)}, \\
\frac{g}{LR} &= \frac{9.80665}{0.0065\times287.05}=5.2559
\end{aligned}$$
Solving that relation for the bracket and then for the height,
$$\begin{aligned}
\theta_{p}&=\left(\frac{24.5}{101.325}\right)^{1/5.2559}=(0.24180)^{0.19026}=0.76325\\
h_{p}&=\frac{T_{0}}{L}\,(1-\theta_{p})=\frac{288.15}{0.0065}\times0.23675=10{,}495\ \text{m}
\end{aligned}$$
so a pressure altimeter set to $1013.25\ \text{hPa}$ would indicate about
$10{,}495\ \text{m}$, roughly $500\ \text{m}$ above the true height.
Get the ambient density from the perfect-gas equation. The
question asks for the density built from the two measured values rather
than read from a table, which is what makes the density altitude a genuinely
independent third answer:
$$\begin{aligned}
\rho &= \frac{p}{RT} \\
&= \frac{24\,500}{287.05\times233.15} \\
&= 0.3661\ \text{kg}\,\text{m}^{-3}
\end{aligned}$$
Invert the ISA density law for the density altitude. Dividing
the pressure law by the temperature law lowers the exponent by one:
$$\frac{\rho}{\rho_{0}}=\left(1-\frac{Lh}{T_{0}}\right)^{g/(LR)-1}
=\left(1-\frac{Lh}{T_{0}}\right)^{4.2559}$$
With $\rho/\rho_{0}=0.3661/1.225=0.29883$ the bracket is
$\theta_{\rho}=(0.29883)^{1/4.2559}=0.75292$, and therefore
$$\boxed{\;h_{T}=8462\ \text{m},\quad h_{p}=10{,}495\ \text{m},\quad
\rho=0.366\ \text{kg}\,\text{m}^{-3},\quad h_{\rho}=10{,}953\ \text{m}\;}$$
The density altitude is the highest of the three, which is the physically
important statement: engine and wing behave as though the aeroplane were nearly a
kilometre higher than it is.
Part (b) — evaluate the standard density at 2500 m. The
question directs that ISA density be used, so the same power law is applied
forwards rather than inverted:
$$\begin{aligned}
\theta &= 1-\frac{0.0065\times2500}{288.15}=0.94361, \\
\rho_{2500} &= 1.225\times(0.94361)^{4.2559}=0.9569\ \text{kg}\,\text{m}^{-3}
\end{aligned}$$
Read the probe difference as dynamic pressure. For
incompressible flow the Pitot hole senses $p_{0}=p+\tfrac{1}{2}\rho V^{2}$ while
the static ports sense $p$, so the cell between them reads exactly the dynamic
pressure. With $V=240/3.6=66.667\ \text{m}\,\text{s}^{-1}$,
$$\boxed{\;p_{0}-p=\tfrac{1}{2}\rho V^{2}
=\tfrac{1}{2}\times0.9569\times(66.667)^{2}=2126\ \text{Pa}=2.13\ \text{kPa}\;}$$
The Mach number here is only about $0.20$, so the incompressible reading is
accurate to well under one per cent and no compressibility correction is needed.
The probe senses stagnation pressure at the nose hole and ambient static pressure at the flush side ports; the cell between them reads the dynamic pressure directly.
Part (c) — add the sea-level dynamic pressure to ambient.
The highest pressure anywhere on a body in a steady incompressible stream is the
stagnation pressure at the forward stagnation point, where the flow has been
brought to rest isentropically along the dividing streamline:
$$\boxed{\;p_{0}=p_{\infty}+\tfrac{1}{2}\rho_{0}V^{2}
=101\,325+\tfrac{1}{2}\times1.225\times70^{2}=101\,325+3001=104{,}326\ \text{Pa}\;}$$
that is $104.3\ \text{kPa}$, about three per cent above ambient. Nowhere on the
body can the pressure exceed this value, because any other point still carries
some kinetic energy.