Step 1: The steady-state error (\( e_{ss} \)) for a given system is determined using the Final Value Theorem: \[ e_{ss} = \lim_{s \to 0} s E(s) \]
Step 2: For a Type 2 system, the open-loop transfer function contains two poles at the origin, meaning it has two integrators.
Step 3: The steady-state error for different inputs is determined using error constants:
- Position error constant \( K_p \) (for step input)
- Velocity error constant \( K_v \) (for ramp input)
- Acceleration error constant \( K_a \) (for parabolic input)
Step 4: For a unit acceleration input (\( R(s) = \frac{1}{s^3} \)), the steady-state error is given by: \[ e_{ss} = \frac{1}{K_a} \] where \( K_a \) is the acceleration error constant.
Step 5: Since a Type 2 system has two integrators, it can track acceleration inputs with finite error, given by \( \frac{1}{K_a} \).
Match the following: For 8086 microprocessor