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Swing equation
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A consists of a number of operating synchronously under all operating conditions. Under normal operating conditions, the relative position of the rotor axis and the resultant axis is fixed. The angle between the two is known as the power angle, torque angle, or rotor angle. During any disturbance, the rotor decelerates or accelerates with respect to the synchronously rotating air gap magnetomotive force, creating relative motion. The equation describing the relative motion is known as the swing equation, which is a non-linear second order differential equation that describes the swing of the rotor of synchronous machine. The power exchange between the mechanical rotor and the electrical grid due to the rotor swing (acceleration and deceleration) is called Inertial response.


Derivation
A synchronous generator is driven by a prime mover. The equation governing the rotor motion is given by: J\frac{d^2{\theta_\text{m}}}{dt^2} = T_a = T_\text{m} - T_\text{e}, where:

  • J is the total moment of inertia of the rotor mass in kg-m2
  • \theta_\text{m} is the angular position of the rotor with respect to a stationary axis in radians (rad)
  • t is time in seconds (s)
  • T_a is the net accelerating , in N-m
  • T_\text{m} is the mechanical torque supplied by the prime mover in N-m
  • T_\text{e} is the electrical torque output of the alternator in N-m

Neglecting losses, the difference between the mechanical and electrical torque gives the net accelerating torque T_a. In the steady state, the electrical torque is equal to the mechanical torque and hence the accelerating power is zero. During this period the rotor moves at synchronous speed \omega_s in rad/s. The electric torque T_\text{e} corresponds to the net air-gap power in the machine and thus accounts for the total output power of the generator plus |I|^2 R losses in the armature winding.

The angular position \theta is measured with a stationary reference frame. Representing it with respect to the synchronously rotating frame gives: \theta_\text{m} = \omega_\text{sm}t + \delta_\text{m}, where the mechanical power angle \delta_m is the angular position with respect to the synchronously rotating reference frame. The derivative of the above equation with respect to time is: \frac{d\theta_\text{m}}{dt} = \omega_\text{sm} + \frac{d\delta_\text{m}}{dt}. The above equations show that the rotor angular speed is equal to the synchronous speed only when d\delta_m /dt is equal to zero. Therefore, the term d\delta_m /dt represents the deviation of the rotor speed from synchronism in rad/s.

By taking the second order derivative of the above equation it becomes: \frac{d^2\theta_\text{m}}{dt^2} = \frac{d^2\delta_\text{m}}{dt^2}. Substituting the above equation in the equation of rotor motion gives: J\frac{d^2{\delta_\text{m}}}{dt^2} = T_a = T_\text{m} - T_\text{e}. Multiplying both sides by the angular velocity of the rotor, given by \omega_\text{m} = \frac}{dt}, results in J\omega_\text{m}\frac{d^2{\delta_\text{m}}}{dt^2} = P_a = P_\text{m} - P_\text{e}, where P_a, P_\text{m} and P_\text{e} respectively are the accelerating, mechanical and electrical (active) power in (W). Intuitivley, the equation can also be derived by taking the time derivative of the rotational energy.

The J \omega_{\text{m}} is the angular momentum of the rotor at synchronous speed \omega_{\text{sm}}. In machine data supplied for stability studies this coefficient is often denoted by M and called the of the machine. In practice, \omega_{\text{m}} does not differ significantly from synchronous speed when the machine is in steady state \omega_{\text{sm}}; allowing for another constant of inertia: H = \frac{\frac{1}{2}J\omega_\text{sm}^2}{S_{\text{rated}}}= \frac{\frac{1}{2}M \omega_\text{sm}}{S_{\text{rated}}}= \frac{\text{stored kinetic energy in mega joules at synchronous speed}}{\text{machine rating in MVA}}, where S_{\text{rated}} is the three phase rating of the machine in . Substituting in the above equation 2H\frac{S_{\text{rated}}}{\omega_\text{sm}^2}\omega_\text{m}\frac{d^2{\delta_\text{m}}}{dt^2} = P_\text{m} - P_\text{e} = P_a. Since P_\text{m}, P_\text{e} and P_a in the machine data are given in MW, dividing them by the generator MVA rating gives these quantities in per unit. Dividing the above equation on both sides by S_{\text{rated}} gives \frac{d^2{\delta}}{dt^2} = P_\text{m} - P_e = P_a per unit |cellpadding= 5 |border |border colour = #0073CF |bgcolor=#F9FFF7 with the electrical power angle and electrical angular velocity given by \delta = \frac{p}{2}\delta_m, \qquad \omega = \frac{p}{2}\omega_m, \qquad \omega_s = \frac{p}{2}\omega_{sm}, where p is the number of poles of the synchronous machine.

The above equation describes the behaviour of the rotor dynamics and hence is known as the swing equation. The angle \delta is that of the internal EMF (E) of the synchronous generator and dictates the amount of power that can be transferred. This angle is therefore called the power angle. Neglecting the machine's resistive losses, the corresponding power angle equation is: P_e = P_{max} \sin (\delta)=3\frac

{X}\sin (\delta), where X is the machine reactance and V the system (i.e. grid) voltage. The angle \delta is also referred to as the torque angle as the electrical torque T_e can be derived from this equation as T_e = \frac{P_e}{\omega_m}=3\frac
{\omega_m X}\sin (\delta). Hence, for synchronous machines the swing equation is a non-linear function of \delta and can be solved numerically using, e.g., the fourth-order Runge-Kutta algorithm. When \delta is small, the equation can be linearized as P_e \approx P_{max}\delta.


See also


Notes

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