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Learning goals

Reading

Classical swing model (teaching form)

A common classical-machine SMIB model (per-unit power, radian angles) is:

δ˙=ω−ω0,2Hω0ω˙=Pm−Pe(δ)−D (ω−ω0),\begin{aligned} \dot{\delta} &= \omega - \omega_0, \\ \frac{2H}{\omega_0}\dot{\omega} &= P_m - P_e(\delta) - D\,(\omega - \omega_0), \end{aligned}

with electrical power of the form Pe=EVXsin⁡δP_e = \frac{E V}{X}\sin\delta (details and bases documented in the lab notebook).

Teaching estimands in Lab 3: inertia HH and damping DD. Keep units and the per-unit base in the dataset manifest.

Event stages

StageNetwork / drivingTypical use
PrefaultIntact network, equilibriumInitial condition
Fault-onReduced PeP_e capability (e.g. bolted fault)Energy input / acceleration
PostfaultCleared topologyStability vs loss of synchronism

Critical clearing time (CCT) later asks: how long can fault-on last before postfault trajectories are unstable under a stated rule? See Stability and CCT.

Worked example

For fixed HH, plot qualitative δ(t)\delta(t) after a short fault vs a long fault. Which parameter mainly scales the “inertia” of the swing?

Lab

Further reading

Common misconceptions

References
  1. Kundur, P., & Malik, O. P. (2022). Power System Stability and Control (Second). McGraw-Hill Education. https://openlibrary.org/isbn/9781260473544
  2. Kundur, P., Paserba, J., Ajjarapu, V., Andersson, G., Bose, A., Canizares, C., Hatziargyriou, N., Hill, D. J., Stankovic, A., Taylor, C., Van Cutsem, T., & Vittal, V. (2004). Definition and Classification of Power System Stability IEEE/CIGRE Joint Task Force on Stability Terms and Definitions. IEEE Transactions on Power Systems, 19(3), 1387–1401. 10.1109/TPWRS.2004.825981