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James W. Gregory Introduction to Flight Testing
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p
SL
μ
dynamic viscosity
ν
kinematic viscosity
ρ
density
σ
density ratio,
ρ
/
ρ
SL
θ
temperature ratio,
T
/
T
SL
Subscripts
ref
reference conditions at the base of a given atmospheric layer
SL
sea level
trop
tropopause
1
beginning of an atmospheric layer
2
end of an atmospheric layer
Acronyms and Abbreviations
AGL
height above ground level
ICAO
International Civil Aviation Organization
MSL
height above mean sea level
NOAA
National Oceanic and Atmospheric Administration
References
Anderson, J.D. Jr. (2016). Introduction to Flight, 8e. New York: McGraw‐Hill.
Carmichael, R. (2018). Public domain aeronautical software for the aeronautical engineer. http://www.pdas.com/atmos.html (accessed 28 December 2020).
ICAO (1993). Manual of the ICAO Standard Atmosphere (Extended to 80 Kilometres (262 500 Feet)), 3e, ICAO Document 7488. Montréal, QC: International Civil Aviation Organization.
NOAA, NASA, and USAF (1976). U.S. Standard Atmosphere, 1976, NOAA‐S/T‐76‐1562, NASA‐TM‐X‐74335. Washington, DC: U.S. Government Printing Office. http://hdl.handle.net/2060/19770009539.
Sartorius, S. (2018). Standard Atmosphere Functions, v. 2.1.0.0. MathWorks File Exchange. https://www.mathworks.com/matlabcentral/fileexchange/28135-standard-atmosphere-functions.
Sutherland, W. (1893). LII. The viscosity of gases and molecular force. The London, Edinburgh, and Dublin Philosophical Magazine and Journal of Science, Series 5 36 (223): 507–531. https://doi.org/10.1080/14786449308620508.
3
Aircraft and Flight Test Instrumentation
This chapter fundamentally deals with how we will measure the various aircraft performance characteristics. We will cover common instruments used in the aircraft cockpit (both traditional and modern avionics systems), as well as instrumentation found in external data acquisition (DAQ) systems. This fundamental understanding is important for developing an appreciation of the capabilities and limitations of each instrument and sensor system. We will begin with a discussion of various sensors and instrumentation hardware used in flight testing (these instruments can be either the standard cockpit instrumentation or supplemental instrumentation dedicated for flight testing purposes).
A discussion of instrumentation and DAQ must begin by detailing what we wish to measure and how we will measure it. For aircraft flight testing, we essentially need to know the vehicle's state – we need to know the aircraft's position and orientation as a function of time. Practically speaking, this requires measurements of the vehicle's velocity, acceleration, orientation (pitch, roll, and yaw angle relative to a defined set of coordinate axes), altitude, and magnetic heading.
Aircraft instruments are generally calibrated to report quantities in the English unit system, sometimes using nonstandard units. Speed is most often reported in knots (nautical miles per hour), altitude is in feet, vertical speed is in feet per minute, distance is in nautical miles, angles are in degrees, and angular rates are in degrees per second. When analyzing flight test data from these measurements, it is critical to convert to standard consistent units before further analysis. All analysis must be done in a single, consistent unit system with standard units (e.g., English: ft/s, ft, deg, and deg/s, or SI: m/s, m, deg, and deg/s). After completion of the analysis, the results may be converted to any desired units for reporting. This section provides an orientation to the instruments installed in general aviation (GA) aircraft cockpits, including both classical “steam gauge” instruments and more modern glass panel instrument displays. We will first discuss the traditional instruments, followed by glass panel avionics systems.
3.1 Traditional Cockpit Instruments
In traditional flight testing methods at the university level, many of the desired parameters are hand‐recorded from cockpit indicators such as the airspeed indicator (ASI), attitude indicator, heading indicator, and altimeter, which are illustrated in Figures 3.1 and 3.2 for a traditional “steam gauge” cockpit. The traditional instruments are arranged in a “six pack” configuration (Figure 3.2): starting at the upper left and moving clockwise, the instruments are the ASI, attitude indicator, altimeter, vertical speed indicator (VSI), heading indicator (also known as the directional gyro), and turn/slip indicator (also known as the turn coordinator). We will group these instruments into two types. The first group, consisting of the attitude indicator, heading indicator, and the turn/slip indicator, is based on gyroscopes. The second group, consisting of the ASI, altimeter, and VSI, is based on physical measurements of pressure. We will discuss each group of instruments in more detail as follows. Interested readers can also consult various publications such as Chapter 7 of the Pilot's Handbook of Aeronautical Knowledge (2008), Chapter 5 of the Instrument Flying Handbook (2012), and the Advanced Avionics Handbook (2009) for more details.

Figure 3.1 Overview of aircraft cockpit instrumentation for traditional “steam gauge” instruments.
Source: https://upload.wikimedia.org/wikipedia/commons/thumb/e/e7/Slingsby.t67c.panel.g-bocm.arp.jpg/1200px-Slingsby.t67c.panel.g-bocm.arp.jpg.

Figure 3.2 Detailed view of the six pack of key instruments in a traditional cockpit.
Source: Modified from photo by Mael Balland on Unsplash, https://unsplash.com/photos/V5hAryReZzo.
3.1.1 Gyroscopic‐Based Instruments
Before discussing the first group of instruments, it is helpful to briefly review the ideas behind gyroscopes. The operation of a gyroscope is based on the Newtonian principle of conservation of angular momentum. Due to conservation of angular momentum, the axis of rotation of a spinning object with a given angular momentum (L = Iω, where I is the moment of inertia and ω is the angular speed) will remain fixed unless acted upon by an external applied torque. (Think of how the axis of a child's spinning top remains upright as long as the top is spinning.) Over time, small external forces and moments that are present in any practical implementation of a physical gyro will lead to gyroscopic precession, which results in small changes in the axis of rotation that can grow over time.
The three gyroscopic instruments in a traditional six pack of instruments – the attitude indicator, heading indicator, and turn coordinator – all depend on gyroscopic principles. The rotational speed of the gyros in the attitude and heading indicators are traditionally powered by a vacuum system that flows air over a small turbine connected to the spinning disks in order to maintain rotation. The turn coordinator, on the other hand, is typically powered by the aircraft's electrical system. The attitude indicator provides an artificial horizon that provides an indication of the amount of bank and pitch that the aircraft has at a given moment. Essentially, the internal gyroscope (to which the artificial horizon is mounted) maintains its rigidity in space and the aircraft pitches and rolls about the internal gyro. Arcing along the top of the indicator, the first three white lines on either side of the centerline indicate increments of 10° bank angle (up to 30° bank). The next two lines on either side represent a 45° and 60° bank angles, respectively. The heading indicator is based on a geared gyro and simply indicates the magnetic heading of the aircraft (as long as the gyro has been set to match the magnetic compass). Both the attitude indicator and the heading indicator experience errors due to gyroscopic precession that must be occasionally corrected. For example, periodically in straight and level flight, the pilot may need to reset the heading indicator to match the indication on the magnetic compass. The turn coordinator, also based on a gyro, indicates the instantaneous rate of turn. The two white lines below the level lines each indicate a standard rate of turn of 3°/s to the right or left, which would require two minutes for the aircraft to complete a 360° turn.
3.1.2 Pressure‐Based Instruments
The second group of instruments is based on measurement of total pressure and static pressure on the aircraft. Total pressure is measured by a pitot probe, which is often mounted under the wing on GA aircraft (see Figure 3.3(a)). Static pressure is measured by flush‐mounted static pressure ports on the side of the aircraft fuselage (see Figure 3.3(b)). The pitot probe and static port are connected via tubing to the ASI, altimeter, and VSI mounted on the instrument panel (Figure 3.4).
Total pressure from the pitot tube and static pressure from the static port are fed into the ASI. The ASI is calibrated based on the assumption of standard sea‐level conditions with the isentropic Mach relation to convert a measured “impact pressure” (difference between total and static pressure) into indicated airspeed. For low‐speed, low‐altitude flight this is equivalent to converting a measured dynamic pressure to velocity by the Bernoulli equation. Further details on the functioning of the ASI are provided in Chapter 8 on calibration of the ASI.

Figure 3.3 Examples of the pitot tube (a) and static pressure port (b) on an aircraft.
The VSI, connected to the static pressure port, measures the time rate of change of pressure and converts this to a vertical speed. It is based on a mechanical comparison of the rate of change of static pressure with a known rate of change coming from a calibrated leak. Indications of vertical speed on the VSI tend to fluctuate so it is not as useful for measuring rate of climb or descent in a precise manner. Instead, for measurement of vertical speed in flight test, it is best to establish a steady rate and directly measure altitude from the altimeter and time with a stopwatch.
The altimeter (Figure 3.5) is based on a measurement of static pressure, which is converted into an indicated altitude. Altitude is displayed on the traditional altimeter by three hands, much like an analog clock displays time. The long, thin pointer with a triangle at the end indicates ten thousands of feet; the short, thick hand displays thousands of feet; and the medium length, slender hand displays hundreds of feet. So, the medium, slender hand makes a full revolution of the dial every 1000 ft; the short, thick pointer makes a complete revolution every 10,000 ft; and the long, slender pointer makes a full revolution every 100,000 ft. For example, the altimeter depicted in Figure 3.5 indicates an altitude of 10,180 ft.

Figure 3.4 Schematic of the pitot‐static system.
Source: Flight Instruments, Federal Aviation Administration.

Figure 3.5 Diagram of an aircraft altimeter. The reference pressure is set by the knob on the lower left side and indicated in the Kollsman window on the right side of the instrument.
Source: Bsayusd, A 3‐pointer pressure altimeter. Originally from en.wikipedia.
The calibration of the altimeter is based on the pressure lapse rate of the standard atmosphere (assuming standard temperature). As discussed in Chapter 2, the pressure lapse rate is extremely consistent, which enables the altimeter to provide a highly accurate measurement. However, the local barometric pressure can change significantly, which would have a first‐order impact on the indicated altitude provided by an altimeter. Thus, an altimeter must account for variations in local barometric pressure reading, which is done by setting a reference pressure. This reference pressure appears in a small window on the right side of the altimeter and is set by a knob on the lower left side of the instrument (see Figure 3.5). It is important to note that the reference pressure is not related in any way to the actual pressure at some arbitrary altitude. Instead, the reference pressure simply shifts the base of the calibration curve, providing an offset above or below standard sea level pressure in order to accommodate the actual local barometric pressure reading and providing a more accurate reading of altitude.
This type of altimeter – the so‐called sensitive altimeter – was first invented by Paul Kollsman, leading to the naming of the Kollsman window where the reference pressure is read on the altimeter (e.g., the reference pressure shown in Figure 3.5 is 29.92 inHg). The Kollsman setting essentially shifts the altimeter's calibration curve in order to account for local variations in sea level pressure, which is routinely encountered due to weather variations (e.g., low or high pressure regions moving through a geographical area). Since accurate measurement of altitude is critical in most flight testing work, we will devote some attention to the calibration and correct setting of the altimeter.
The most typical use of the altimeter under routine flight is to set the Kollsman reference pressure to the local barometric pressure, such that the indicated altitude is the aircraft's height above mean sea level (MSL). A pilot can easily obtain up‐to‐date readings of the local barometric pressure by listening to broadcasts from local weather stations (such as the Automated Weather Observing System, or AWOS, found at many airports). Alternatively, air traffic control (ATC) will often report the local barometric pressure setting, especially when aircraft are transitioning from one controller to another with responsibility for different geographical areas. Reporting of the local barometric pressure is an important function for ATC, since they aim to maintain consistent vertical separation between all aircraft. Thus, for a pilot to ensure an accurate reading of MSL altitude, the altimeter must be set to the correct local barometric pressure reading (viewed in the Kollsman window) by adjusting the Kollsman knob.
However, in flight testing, we often wish to know the pressure altitude, or the pressure at our flight altitude. This can be accomplished by setting the altimeter to a reference pressure of 29.92 inHg (1013 hPa) instead of the local barometric pressure reading. Under this situation, the altimeter will not provide an accurate indication of height above sea level; rather, it will indicate pressure altitude. A flight test engineer can readily take the measured pressure altitude and convert this to a value of the local freestream static pressure via the standard atmosphere, using the theory described in Chapter 2[3].
3.1.3 Outside Air Temperature
Knowledge of ambient (freestream) temperature of the flight environment is important for calculating the freestream density from the ideal gas law and for determination of true airspeed. The challenge of measuring outside air temperature (OAT) from a moving aircraft is related to the frame of reference of the air (the desired temperature) versus the aircraft reference frame (where temperature is measured). Since the air is moving relative to the aircraft, the temperature measured in the aircraft frame of reference will be higher. If a temperature probe completely stagnates the flow (i.e., with no loss of energy), the isentropic Mach relation,
(3.1)

may be used to find the freestream temperature (T∞) from measurements of the stagnation temperature (T0) and the freestream Mach number (M∞), where γ = 1.4 is the ratio of specific heats for air. However, most temperature probes do not fully recover the full stagnation temperature, so a recovery factor (k) must be introduced. Furthermore, there may be differences between the local Mach number (Mℓ) and the freestream Mach number, due to local acceleration or deceleration of the flow around the aircraft body. Thus, we can modify Eq. (3.1) to accommodate these two factors,
(3.2)

where Mℓ and k can be found by calibration (Gracey 1980).
3.1.4 Other Instrumentation
Other relevant instruments on a traditional cockpit panel include a clock (for timing various events), the engine tachometer (for measuring engine speed in RPM), manifold pressure for the engine air intake, fuel flow rate, and total fuel burned. In traditional flight testing at the university level, readings from the “steam gauge” instruments must be manually recorded via pen and paper. These manual data recording techniques can be effective, as long as the time scale of any transient characteristic of the flight maneuver is long relative to the speed at which data can be manually recorded. For example, the rate of climb in a sustained, steady climb can be easily recorded by hand with a stopwatch and the altimeter, while the level acceleration of an aircraft would be much more difficult to manually record since velocity is changing quickly over time.
3.2 Glass Cockpit Instruments
Glass panel avionics displays (Figures 3.6–3.8) are becoming increasingly common on small GA aircraft. Glass panels measure and display the same data as traditional instruments, but the organization and display of data is greatly improved for better scanning and interpretation by the pilot. The glass panel display is usually physically segmented into a primary flight display (PFD), where critical data such as airspeed, altitude, heading, and attitude are displayed (left screen in Figures 3.6 and 3.7), and a multifunction display (MFD) where secondary data such as engine performance, navigation, terrain, traffic, etc. are displayed (right screen in Figures 3.6 and 3.8). We will discuss the glass panel display of the same data streams that are found on a traditional six pack of instruments, followed by a few notes on recording data from glass panel avionics systems. The following discussion refers to Figures 3.7 and 3.8.

Figure 3.6 Overview of aircraft cockpit instrumentation for a glass panel avionics display in a Cirrus SR20.

Figure 3.7 Detailed view of the primary flight display (PFD) on a Cirrus SR20, with key indications identified.
Measurements such as airspeed and altitude continue to be made in the same manner, where total pressure and static pressure are used to calculate the indicated airspeed. Since the calibration of airspeed is known, and real‐time measurements of pressure and OAT are available, the flight computer can calculate the true airspeed in real time. Since global positioning system (GPS) data are also available for measuring ground speed, the flight computer can also calculate the winds aloft, which represent the difference between true airspeed and ground speed. (See Chapter 8 for detailed definitions of these speeds, and details on how they are computed.) Indicated airspeed is prominently displayed on the left side of the glass panel on a linear, sliding scale along with a digital readout in the center of the scale. Altitude is also displayed on a linear sliding scale, but on the right side of the screen. The Kollsman setting (reference pressure) is displayed immediately beneath the altitude scale. On the right side of the altitude ticker is a display of the rate of climb in numerical and graphical form.
The attitude indicator is displayed in much the same way as it is on a traditional attitude indicator; one critical difference is that the artificial horizon completely spans the width of the display for better situational awareness for the pilot. The heading indicator is in the bottom center of the PFD, with heading information displayed in much the same way as on the analog instrument. Both the attitude indicator and the heading indicator are based on microelectromechanical systems (MEMS)‐based gyroscopes, magnetometers, and accelerometers. The details of these sensor schemes will be discussed in the following subsections. OAT is typically displayed on the lower left side of the PFD. Engine parameters such as engine speed, percent power, manifold pressure, fuel flow rate, fuel burned, exhaust gas temperature, oil pressure, oil temperature, etc. are displayed on the MFD (see Figure 3.8).

Figure 3.8 Detailed view of the multifunction display (MFD) on a Cirrus SR20, with key engine parameters identified.
The airspeed and altitude tickers, along with the heading indicator, have accompanying magenta trend bars (on the inside edge of each ticker or along the circumference of the heading indicator) that indicate the projected value that will be true 6 seconds in the future, based on current rates of change. Rate of turn can be inferred from the length of the magenta bar on the heading indicator (e.g., a standard rate turn would have a magenta bar extending 18° from the center).
Data from glass cockpit displays may also be recorded manually (pen and paper), or in some cases, limited data streams are available in digital form from the avionics suite itself. For example, the Avidyne FlightMax Entegra avionics suite records aircraft data including latitude, longitude, pressure altitude, density altitude, exhaust gas temperatures and cylinder head temperatures for all cylinders, oil temperature, oil pressure, engine RPM, OAT, and manifold pressure. While this data stream is predominantly focused on engine parameters (for engine health monitoring), it can be a useful supplement to other data streams used in flight testing. The avionics suite records the data at a rate of one sample per 6 seconds (0.167 Hz) and stores it in internal data storage. The data can be retrieved after the flight via the USB port on the front of the avionics panel.
The fundamental principles for the sensors at the heart of an aircraft's glass panel avionics are the same as those underlying traditional cockpit instruments. Glass cockpit sensors are based on gyroscopic principles and measurement of physical quantities such as pressure and temperature, but there are critical differences. Sensors such as magnetometers, accelerometers, and rate gyroscopes are grouped together into an inertial measurement unit (IMU), known as the attitude and heading reference system (AHRS), that fuses the sensor data streams to provide real‐time computations of an aircraft's heading and orientation in space. A second major subsystem is the air data computer (ADC), which computes aircraft speed, altitude, and rate of change of altitude based on measurements of total pressure, static pressure, and OAT. The third major subsystem used in glass panel avionics is the navigation instruments. In modern avionics, this primarily relies upon a global navigation satellite system (GNSS) receiver (i.e., a GPS receiver) but also includes radio receivers for radio‐based navigation aids. A significant advantage of glass panel avionics is that derived quantities such as winds aloft, density altitude, true airspeed, etc. can be determined real time in flight via the onboard computer at the heart of the avionics system.