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Advanced electrical engineering: 50 upper-level concepts

Upper-level electrical engineering: Laplace and Z transforms, Bode and Nyquist stability, DSP, transmission lines, Maxwell’s equations, power systems and noise.

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Laplace transform (unilateral)

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  1. 1
    Laplace transform (unilateral)
    F(s)=∫0−∞f(t) e−st dtF(s) = \displaystyle\int_{0^-}^{\infty} f(t)\,e^{-st}\,dt
    s=σ+jωs = \sigma + j\omega is the complex frequency. Differentiation becomes multiplication by ss: L{f′}=sF(s)−f(0−)\mathcal{L}\{f'\} = sF(s) - f(0^-).
  2. 2
    Final value theorem
    lim⁡t→∞f(t)=lim⁡s→0sF(s)\displaystyle\lim_{t \to \infty} f(t) = \lim_{s \to 0} sF(s)
    Valid only if every pole of sF(s)sF(s) lies in the open left half-plane, so that f(t)f(t) actually settles.
  3. 3
    Z-transform
    X(z)=∑n=−∞∞x[n] z−nX(z) = \displaystyle\sum_{n=-\infty}^{\infty} x[n]\,z^{-n}
    A delay of one sample multiplies the transform by z−1z^{-1}.
  4. 4
    Transfer function
    H(s)=Y(s)X(s)H(s) = \dfrac{Y(s)}{X(s)}, the ratio of the output and input transforms with all initial conditions zero
    It is also the Laplace transform of the impulse response.
  5. 5
    Poles and zeros of a transfer function
    Zeros are the roots of the numerator of H(s)H(s); poles are the roots of the denominator
    On a pole-zero plot, poles are drawn as crosses and zeros as circles.
  6. 6
    Stability condition for a continuous-time LTI system
    Every pole of the transfer function lies in the open left half of the s-plane
    A pole in the right half-plane makes the response grow without bound; simple poles on the imaginary axis give sustained oscillation.
  7. 7
    Stability condition for a discrete-time LTI system
    Every pole of H(z)H(z) lies strictly inside the unit circle, ∣z∣<1|z| < 1
    The mapping z=esTz = e^{sT} sends the left half of the s-plane inside the unit circle.
  8. 8
    Bode phase of a real left-half-plane pole
    It falls from 0∘0^\circ to −90∘-90^\circ, passing −45∘-45^\circ at the corner frequency
    Most of the change happens within a decade either side of the corner, from 0.1 ωc0.1\,\omega_c to 10 ωc10\,\omega_c.
  9. 9
    Right-half-plane zero on a Bode plot
    Its magnitude rises at 20 dB20\ \mathrm{dB} per decade like a normal zero, but its phase falls by 90∘90^\circ like a pole
    Systems with one are called non-minimum phase; the step response often starts in the wrong direction.
  10. 10
    Standard second-order transfer function
    H(s)=ωn2s2+2ζωns+ωn2H(s) = \dfrac{\omega_n^2}{s^2 + 2\zeta\omega_n s + \omega_n^2}
    ωn\omega_n is the natural frequency and ζ\zeta the damping ratio; 0<ζ<10 < \zeta < 1 is underdamped.
  11. 11
    Percent overshoot of an underdamped second-order step response
    %OS=100 e−ζπ/1−ζ2\%\mathrm{OS} = 100\,e^{-\zeta\pi/\sqrt{1 - \zeta^2}}
    It depends only on ζ\zeta: about 16% at ζ=0.5\zeta = 0.5 and 4.3% at ζ=0.707\zeta = 0.707.
  12. 12
    Routh–Hurwitz criterion
    The number of sign changes in the first column of the Routh array equals the number of roots in the right half-plane
    It tests the stability of a characteristic polynomial without solving for its roots.
  13. 13
    Nyquist stability criterion
    Z=N+PZ = N + P: closed-loop right-half-plane poles equal the clockwise encirclements of −1-1 by L(s)L(s) plus the open-loop right-half-plane poles
    Stability needs Z=0Z = 0, so the plot must encircle −1-1 counterclockwise once for each unstable open-loop pole.
  14. 14
    Gain margin
    How much the loop gain can rise before instability: GM=1∣L(jωpc)∣\mathrm{GM} = \dfrac{1}{|L(j\omega_{pc})|}, where the phase of LL is −180∘-180^\circ
    ωpc\omega_{pc} is the phase-crossover frequency. In decibels, GM=−20log⁡10∣L(jωpc)∣\mathrm{GM} = -20\log_{10}|L(j\omega_{pc})|.
  15. 15
    Phase margin
    PM=180∘+∠L(jωgc)\mathrm{PM} = 180^\circ + \angle L(j\omega_{gc}), where ∣L(jωgc)∣=1|L(j\omega_{gc})| = 1
    ωgc\omega_{gc} is the gain-crossover frequency. A common design target is 45∘45^\circ to 60∘60^\circ.
  16. 16
    Nyquist–Shannon sampling theorem
    A signal band-limited to BB hertz can be reconstructed exactly from samples taken at a rate fs>2Bf_s > 2B
    Half the sampling rate, fs/2f_s/2, is called the Nyquist frequency.
  17. 17
    Aliasing
    After sampling, frequencies above fs/2f_s/2 fold back and appear as lower frequencies
    An anti-aliasing low-pass filter before the sampler prevents it. A 7 kHz7\ \mathrm{kHz} tone sampled at 10 kHz10\ \mathrm{kHz} appears at 3 kHz3\ \mathrm{kHz}.
  18. 18
    FIR vs IIR filters
    FIR filters have no feedback, are always stable and can have exactly linear phase; IIR filters use feedback and need fewer coefficients for a sharp response, but can be unstable
    An FIR filter with symmetric coefficients has linear phase, so it delays all frequencies equally.
  19. 19
    Discrete Fourier transform (DFT)
    X[k]=∑n=0N−1x[n] e−j2πkn/NX[k] = \displaystyle\sum_{n=0}^{N-1} x[n]\,e^{-j2\pi kn/N}
  20. 20
    Cost of the FFT vs a direct DFT
    O(Nlog⁡N)O(N\log N) operations instead of O(N2)O(N^2)
    The common radix-2 Cooley–Tukey algorithm needs NN to be a power of 2.
  21. 21
    Frequency resolution of an N-point DFT
    Δf=fsN\Delta f = \dfrac{f_s}{N}
    Bin kk sits at kfs/Nk f_s/N. Zero-padding interpolates the spectrum but doesn’t add resolution.
  22. 22
    Characteristic impedance of a lossless transmission line
    Z0=L′C′Z_0 = \sqrt{\dfrac{L'}{C'}}
    L′L' and C′C' are the inductance and capacitance per unit length. Coaxial cables are usually 5050 or 75 Ω75\ \Omega.
  23. 23
    Reflection coefficient at a load
    Γ=ZL−Z0ZL+Z0\Gamma = \dfrac{Z_L - Z_0}{Z_L + Z_0}
    A matched load gives Γ=0\Gamma = 0, a short circuit −1-1 and an open circuit +1+1.
  24. 24
    Voltage standing wave ratio (VSWR)
    VSWR=1+∣Γ∣1−∣Γ∣\mathrm{VSWR} = \dfrac{1 + |\Gamma|}{1 - |\Gamma|}
    It runs from 1 for a perfect match to infinity for total reflection.
  25. 25
    Quarter-wave transformer
    A λ/4\lambda/4 line of impedance Z0=ZinZLZ_0 = \sqrt{Z_{\text{in}} Z_L} matches a real load ZLZ_L to ZinZ_{\text{in}}
    A quarter-wave line transforms any load to Zin=Z02/ZLZ_{\text{in}} = Z_0^2/Z_L.
  26. 26
    Smith chart
    A plot of the reflection coefficient in the complex plane, overlaid with circles of constant normalized resistance and arcs of constant normalized reactance
    Moving along a lossless line rotates the point around the centre; one full turn is half a wavelength.
  27. 27
    Gauss’s law in differential form
    ∇⋅D=ρv\nabla \cdot \mathbf{D} = \rho_v
    The electric flux out of a region equals the free charge inside. In free space D=ε0E\mathbf{D} = \varepsilon_0\mathbf{E}.
  28. 28
    Gauss’s law for magnetism
    ∇⋅B=0\nabla \cdot \mathbf{B} = 0
    There are no magnetic monopoles, so magnetic field lines always close on themselves.
  29. 29
    Faraday’s law in differential form
    ∇×E=−∂B∂t\nabla \times \mathbf{E} = -\dfrac{\partial \mathbf{B}}{\partial t}
    A time-varying magnetic field produces a circulating electric field.
  30. 30
    Ampère–Maxwell law
    ∇×H=J+∂D∂t\nabla \times \mathbf{H} = \mathbf{J} + \dfrac{\partial \mathbf{D}}{\partial t}
    Maxwell’s displacement current term, ∂D/∂t\partial\mathbf{D}/\partial t, is what makes electromagnetic waves possible.
  31. 31
    Intrinsic impedance of free space
    η0=μ0ε0≈377 Ω\eta_0 = \sqrt{\dfrac{\mu_0}{\varepsilon_0}} \approx 377\ \Omega
    The ratio of the electric to the magnetic field strength in a plane wave travelling through a vacuum.
  32. 32
    Skin depth
    δ=2ωμσ=1πfμσ\delta = \sqrt{\dfrac{2}{\omega\mu\sigma}} = \dfrac{1}{\sqrt{\pi f \mu \sigma}}
    The depth at which current density falls to 1/e1/e of its surface value. In copper it is about 9 mm9\ \mathrm{mm} at 50 Hz50\ \mathrm{Hz} and 65 μm65\ \mathrm{\mu m} at 1 MHz1\ \mathrm{MHz}.
  33. 33
    Output voltage of an ideal buck converter
    Vout=D VinV_{\text{out}} = D\,V_{\text{in}}
    DD is the duty cycle, between 0 and 1, in continuous conduction mode.
  34. 34
    Output voltage of an ideal boost converter
    Vout=Vin1−DV_{\text{out}} = \dfrac{V_{\text{in}}}{1 - D}
    In continuous conduction mode; a duty cycle of 0.5 doubles the input voltage.
  35. 35
    Pulse-width modulation (PWM)
    Switching at a fixed frequency and varying the duty cycle D=ton/TD = t_{\text{on}}/T to control the average output
    Because the switch is either fully on or fully off, it dissipates little power.
  36. 36
    Inductor volt-second balance
    In periodic steady state, the average voltage across an inductor over one switching period is zero
    Applying it to the on and off intervals gives the conversion ratios of the buck and boost converters.
  37. 37
    Base impedance in a per-unit system
    Zbase=Vbase2SbaseZ_{\text{base}} = \dfrac{V_{\text{base}}^2}{S_{\text{base}}}
    In three-phase systems, use the line-to-line base voltage and the three-phase base power. Then Zpu=Z/ZbaseZ_{\text{pu}} = Z/Z_{\text{base}}.
  38. 38
    Converting a per-unit impedance to a new base
    Zpu,new=Zpu,old(Vbase,oldVbase,new)2Sbase,newSbase,oldZ_{\text{pu,new}} = Z_{\text{pu,old}} \left(\dfrac{V_{\text{base,old}}}{V_{\text{base,new}}}\right)^2 \dfrac{S_{\text{base,new}}}{S_{\text{base,old}}}
    Needed because nameplates give impedances on each machine’s own rating.
  39. 39
    Synchronous speed
    ns=120fpn_s = \dfrac{120 f}{p} revolutions per minute
    pp is the number of poles: a four-pole machine on 50 Hz50\ \mathrm{Hz} turns at 1500 rpm1500\ \mathrm{rpm}.
  40. 40
    Power–angle equation of a synchronous generator
    P=E VXssin⁡δP = \dfrac{E\,V}{X_s}\sin\delta
    Per phase, for a round-rotor machine with resistance neglected. EE is the internal EMF, XsX_s the synchronous reactance and δ\delta the power angle.
  41. 41
    Symmetrical components
    Any set of three unbalanced phasors can be written as the sum of balanced positive-sequence, negative-sequence and zero-sequence sets
    They use the operator a=1∠120∘a = 1\angle 120^\circ, and turn an unbalanced fault into three decoupled sequence networks.
  42. 42
    Fault current for a single line-to-ground fault
    If=3VfZ1+Z2+Z0+3ZfI_f = \dfrac{3V_f}{Z_1 + Z_2 + Z_0 + 3Z_f}
    Z1Z_1, Z2Z_2 and Z0Z_0 are the positive-, negative- and zero-sequence impedances at the fault, ZfZ_f the fault impedance and VfV_f the pre-fault voltage.
  43. 43
    Shannon–Hartley channel capacity
    C=Blog⁡2 ⁣(1+SN)C = B\log_2\!\left(1 + \dfrac{S}{N}\right) bits per second
    BB is the bandwidth in hertz and S/NS/N the signal-to-noise power ratio as a plain ratio, not in decibels.
  44. 44
    Amplitude-modulated (AM) signal
    s(t)=Ac [1+mcos⁡(ωmt)]cos⁡(ωct)s(t) = A_c\,[1 + m\cos(\omega_m t)]\cos(\omega_c t)
    mm is the modulation index, kept at or below 1 to avoid overmodulation. The bandwidth is twice the highest message frequency.
  45. 45
    Total power of an AM signal
    Pt=Pc(1+m22)P_t = P_c\left(1 + \dfrac{m^2}{2}\right)
    PcP_c is the carrier power. Even at m=1m = 1, only a third of the power is in the sidebands that carry the message.
  46. 46
    Carson’s rule for FM bandwidth
    B≈2(Δf+fm)B \approx 2(\Delta f + f_m)
    Δf\Delta f is the peak frequency deviation and fmf_m the highest modulating frequency; their ratio β=Δf/fm\beta = \Delta f/f_m is the modulation index.
  47. 47
    Thermal (Johnson–Nyquist) noise voltage
    vn,rms=4kTRBv_{n,\text{rms}} = \sqrt{4kTRB}
    kk is Boltzmann’s constant, TT the temperature in kelvin and BB the bandwidth. A 1 kΩ1\ \mathrm{k\Omega} resistor at room temperature gives about 4 nV/Hz4\ \mathrm{nV/\sqrt{Hz}}.
  48. 48
    Thermal noise floor at room temperature
    About −174 dBm/Hz-174\ \mathrm{dBm/Hz}
    The available noise power is kTBkTB: at 290 K290\ \mathrm{K} that is 4×10−21 W4 \times 10^{-21}\ \mathrm{W} per hertz of bandwidth.
  49. 49
    Noise figure
    NF=10log⁡10SNRinSNRout\mathrm{NF} = 10\log_{10}\dfrac{\mathrm{SNR}_{\text{in}}}{\mathrm{SNR}_{\text{out}}}, in decibels
    How much a stage degrades the signal-to-noise ratio, defined with the source at 290 K290\ \mathrm{K}. The linear ratio is the noise factor FF.
  50. 50
    Friis formula for cascaded noise factor
    F=F1+F2−1G1+F3−1G1G2+⋯F = F_1 + \dfrac{F_2 - 1}{G_1} + \dfrac{F_3 - 1}{G_1 G_2} + \cdots
    FiF_i and GiG_i are each stage’s noise factor and gain as linear ratios. The first stage dominates, which is why receivers start with a low-noise amplifier.

Frequently asked questions

Who is this deck for?

Third- and fourth-year students, graduate students, and working engineers reviewing for professional exams or interviews. It assumes the material in the basics and intermediate decks.

Which sign conventions do the cards use?

Common engineering ones: j for the imaginary unit, the unilateral Laplace transform from 0−, and the Nyquist criterion as Z = N + P with clockwise encirclements. Textbooks vary, so check yours before an exam.

Why do power engineers use per-unit values?

Expressing quantities as fractions of chosen base values removes the turns ratios of ideal transformers from the analysis, keeps numbers close to 1 and makes errors easy to spot.

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