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The major difference lies in the active power responses.
The BESS power responses are shown in Fig. 16.
Performance evaluation proves that CSIST-50-01 has fast power responses.
Open image in new window Fig. 14 BESS active power responses for ξ* = 10% in Kundur system.
Open image in new window Fig. 16 Zoom-in plot of BESS active power responses when T es = 50 ms.
Finally, the peak power responses were also highly reliable, and exploration of the three baseline trials indicated a significant reliability coefficient (Cronbach's α = 0.99, p = 0.00).
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By employing grid connected power inverters, RECSs can provide much faster power response than SGs.
Open image in new window Fig. 19 Zoom-in plot of BESS-4 active power response.
The oscillation properties were discriminated according to the components of power response in [10].
Open image in new window Fig. 12 Comparison of BESS active power response considering T es.
However, the predicted power response during the excursion phase did not match correctly the experimental tendency.
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