Question 8 of 8: Second-Order Dominant-Poles Models in s- and Frequency Domain
Nivaar worked solution (AI-drafted; not reviewed by a licensed engineer)
Notes on this paper
Paper format. National Exams, December 2019 —
16-Elec-A2, Systems & Control. Three hours, closed book
(approved Casio or Sharp calculator plus one double-sided handwritten 8.5×11″ formula
sheet). Eight questions of 20 marks each. Questions 1 and 2 are compulsory;
candidates then choose three of the remaining six, so five questions constitute a complete
paper (100 marks). A short table of Laplace transforms and a page of standard second-order
plots and formulae are supplied with the paper. Every one of the eight questions is
solved below, because the full set is the more useful study resource.
Reference texts.
Nise, Control Systems Engineering, 8th ed. — root locus (Ch. 8), frequency
response and Nyquist (Ch. 10), design via frequency response (Ch. 11), state space (Ch. 12).
Ogata, Modern Control Engineering, 5th ed. — Routh–Hurwitz (§5.6),
lead/lag design (Ch. 6), state-space controllability and observability (Ch. 9).
Dorf & Bishop, Modern Control Systems, 13th ed. — performance of
second-order systems (Ch. 5), stability (Ch. 6).
Franklin, Powell & Emami-Naeini, Feedback Control of Dynamic Systems, 8th ed.
— dominant-pole approximation and pole placement (Ch. 7).
Check: figure reads. Questions 2, 3, 5 and 8 depend on
plotted data. Every value quoted below was read from the printed figures. Chart reads carry a
tolerance of roughly the last quoted digit; where a graphical read drives a design, the exact
analytical value is given alongside it.
Question 8: Second-Order Dominant-Poles Models in s- and Frequency Domain (20 marks)
Given. $G_{cl}(s) = 60(s+50)/[(s+30)(s^2+4s+100)]$, together with two
plots. Read from Figure Q8.1: steady-state value 1.0, first peak 1.51 at $t_p = 0.32$ s. Read from
Figure Q8.2: low-frequency magnitude 1.0, resonant peak $M_r = 2.5$ at
$\omega_r \approx 9.6$ rad/s.
Find. A justification for the dominant-pair reduction and the analytic model
$G_{m1}$; the model $G_{m2}$ identified from the step plot; the model $G_{m3}$ identified from the
magnitude plot; and a comparison of the three.
Check: figure reads. The values above were read from the printed figures. Graphical reads carry roughly
$\pm 0.02$ on the peak amplitude and $\pm 0.02$ s on the peak time, which propagates to about
$\pm 2\%$ on $\zeta$ and $\omega_n$ — the level of agreement seen between the three models
below is therefore about as good as chart reading permits.
Approach. Factor the denominator to expose the pole pattern and test the
separation ratio, then read $\zeta$ and $\omega_n$ three independent ways — analytically from
the dominant pair, from overshoot and peak time on the step plot, and from resonant peak and
resonant frequency on the magnitude plot — normalising each model to the correct DC gain.
Factor and examine the poles (part 1). The quadratic factor gives
$$s = \frac{-4 \pm \sqrt{16-400}}{2} = -2 \pm j9.798$$
so the three closed-loop poles are $-30$ and $-2 \pm j9.798$, with a single finite zero at $-50$.
The real pole sits $30/2 = 15$ times further from the imaginary axis than the complex pair, and the
zero is further still. Since each mode decays as $e^{\sigma t}$, the mode at $-30$ dies out roughly
$e^{28t}$ times faster than the pair — it has effectively vanished within about 0.13 s, while
the oscillation persists for some 2 s. Both the far pole and the far zero therefore contribute
negligible residues, and a second-order dominant-poles model is appropriate. The
usual engineering threshold is a separation of at least five; here it is fifteen.
Write the analytic model $G_{m1}$. The dominant pair alone gives
$$\omega_n = |{-2+j9.798}| = \sqrt{4+96} = 10\ \text{rad/s}, \qquad
\zeta = \frac{2}{10} = 0.20$$
The model must reproduce the true DC gain, and
$G_{cl}(0) = (60)(50)/[(30)(100)] = 1$, so $K_{dc} = 1$ and
$$\boxed{\,G_{m1}(s) = \frac{100}{s^2+4s+100}\,}$$
Read the step plot (part 2). With a steady-state value of 1.0 and a first peak
of 1.51,
$$PO = \frac{1.51-1.0}{1.0}\times100 = 51\%
\;\Longrightarrow\;
\zeta = \frac{-\ln(0.51)}{\sqrt{\pi^2+\ln^2(0.51)}} = 0.2096$$
The peak time fixes the damped frequency, $t_p = \pi/\omega_d = 0.32$ s, so
$$\omega_d = \frac{\pi}{0.32} = 9.817\ \text{rad/s}, \qquad
\omega_n = \frac{\omega_d}{\sqrt{1-\zeta^2}} = 10.04\ \text{rad/s}$$
With $K_{dc} = 1$ read directly off the settled value,
$$\boxed{\,G_{m2}(s) = \frac{100.8}{s^2+4.208s+100.8}\,}$$
Read the magnitude plot (part 3). The resonant peak of a second-order system
relative to its DC gain is $M_r/K_{dc} = 1/(2\zeta\sqrt{1-\zeta^2})$. With $K_{dc} = 1$ and
$M_r = 2.5$, solving
$$2\zeta\sqrt{1-\zeta^2} = \frac{1}{2.5} = 0.4
\;\Longrightarrow\; \zeta = 0.2043$$
(the smaller of the two roots, the lightly damped one consistent with a tall peak). The resonant
frequency then gives $\omega_n$ through $\omega_r = \omega_n\sqrt{1-2\zeta^2}$:
$$\omega_n = \frac{9.6}{\sqrt{1-2(0.2043)^2}} = \frac{9.6}{0.9574} = 10.03\ \text{rad/s}$$
so
$$\boxed{\,G_{m3}(s) = \frac{100.6}{s^2+4.098s+100.6}\,}$$
Figure 8.1 — Step response of the full third-order Gcl(s) with the second-order model Gm1(s) overlaid. The two are almost indistinguishable, which is the dominant-pair reduction verified directly.
Figure 8.2 — Closed-loop magnitude response. The resonant peak of about 2.55 occurs near 9.6 rad/s, matching the reading taken from Figure Q8.2 of the paper.
Compare the three models (part 4). The agreement is close:
Model
Source
$\zeta$
$\omega_n$ (rad/s)
$K_{dc}$
$G_{m1}$
Analytic, from the pole pair
0.2000
10.00
1
$G_{m2}$
Step response, Fig. Q8.1
0.2096
10.04
1
$G_{m3}$
Magnitude plot, Fig. Q8.2
0.2043
10.03
1
All three natural frequencies agree to better than 0.5% and the damping ratios spread by under
5%, which is well inside chart-reading tolerance. The two graphical models both return a
slightly higher damping ratio than the analytic one, and that bias is real rather than
random: the neglected pole at $-30$ removes a little of the initial rise and the zero at $-50$
mildly reshapes the peak, so the measured overshoot and resonant peak are marginally smaller than a
pure second-order system with $\zeta = 0.20$ would produce, and inverting those relations returns a
slightly larger $\zeta$.
$G_{m1}$ is the most accurate. It is derived exactly from the known transfer
function, with no measurement uncertainty at all, and the two graphical models simply confirm it to
within reading error. $G_{m2}$ and $G_{m3}$ are nonetheless the more valuable techniques in
practice: they are the only ones available when the plant transfer function is unknown and all one
has is measured data. Of those two, the frequency-domain reading is usually the more reliable
because a resonant peak can be measured with a swept sine to high precision, whereas peak time on a
transient trace is difficult to pinpoint. The overlays above show both the full third-order
response and $G_{m1}$; the curves are almost indistinguishable, confirming the reduction.