Coordinated Voltage Control Strategy of Photovoltaic Inverter and Energy Storage Group Based on Consensus Algorithm

With the rapid integration of distributed photovoltaic (PV) systems into low-voltage distribution networks, voltage regulation has become critical. This paper proposes a two-stage hierarchical voltage control strategy leveraging the reactive power capability of PV inverters and active power support from energy storage inverters. The methodology combines sensitivity analysis with consensus algorithm-based coordination to optimize voltage stability while minimizing operational costs.

1. Voltage-Cost Sensitivity Framework

The voltage regulation effectiveness per unit cost is quantified through Voltage-Cost Sensitivity Factor (FU-C):

$$F_{U-C}^{PV,ij} = \frac{S_{U-Q}^{ij}}{c_{PV}}$$
$$F_{U-C}^{ESS,ij} = \frac{S_{U-P}^{ij}}{c_{ESS}}$$

Where SU-Q and SU-P represent voltage sensitivities to reactive and active power changes, while cPV (0.067 $/kVar·h) and cESS (0.6-1.0 $/kWh) denote regulation costs. For typical LV networks with R/X ratio 1.14-5.56:

$$\frac{F_{U-C}^{ESS,ij}}{F_{U-C}^{PV,ij}} = \frac{R}{X} \cdot \frac{c_{PV}}{c_{ESS}} < 1$$

Device Type Sensitivity Component Cost Factor Typical FU-C
PV Inverter SU-Q = ΣXn/U0 0.067 $/kVar·h 1.82×10-3 V/$
Energy Storage Inverter SU-P = ΣRn/U0 0.8 $/kWh 0.94×10-3 V/$

2. Consensus-Based Hierarchical Control

The control architecture implements sequential optimization:

2.1 PV Inverter Reactive Control Stage

Group voltage controllers (GVCs) coordinate PV clusters based on reactive utilization ratio μ:

$$μ_{GVi,j}(k+1) = \sum_{m=1}^{N_p} β_{jm}^{PV}μ_{GVi,m}(k) + d_j^{PV}λ_1(μ_{GVi,j}(k)-μ_{ref}(k))$$

Where λ1 = 0.35 ensures convergence. Reactive power allocation follows:

$$Q_{GVi,j} = μ_{GVi,j} \cdot Q_{max,j}$$

2.2 Energy Storage Inverter Active Control Stage

Energy storage inverters adjust SOC changes ΔS through distributed consensus:

$$ΔS_{GVi,j}(k+1) = \sum_{m=1}^{N_b} β_{jm}^{ESS}ΔS_{GVi,m}(k) + d_j^{ESS}λ_2(ΔS_{GVi,j}(k)-ΔS_{ref}(k))$$

Active power dispatch is calculated as:

$$P_{ESS,j} = \frac{ΔS_{GVi,j} \cdot S_{ESS,j}}{ηΔt}$$

3. Case Study Implementation

An IEEE 14-node LV network with 8 PV/storage nodes demonstrates the strategy:

System Configuration
Node Group PV Capacity (kVA) ESS Capacity (kWh) ESS Power Rating (kW)
GV1 (3,4,5,8) 10-12 8-10 1.6-2.0
GV2 (7,9,13,14) 10 8 1.6

Key performance metrics under different strategies:

Regulation Cost Comparison
Strategy PV Reactive Cost ($) ESS Active Cost ($) Total Cost ($)
S1 (PV Only) 5.85 5.85
S2 (ESS Only) 30.49 30.49
S3 (Proposed) 5.85 4.82 10.67
S4 (Global Consensus) 6.27 6.83 13.20

4. Advanced Coordination Mechanism

The energy storage inverter control integrates three-layer optimization:

$$min \sum_{t=1}^{T} [c_{PV}Q_{PV}(t) + c_{ESS}P_{ESS}(t)]$$
$$s.t.\quad V_{min} ≤ V_i(t) ≤ V_{max}$$
$$SOC_{min} ≤ SOC(t) ≤ SOC_{max}$$

Real-time adjustment factors for energy storage inverters:

$$α_{ESS} = \frac{\partial V}{\partial P_{ESS}} \cdot \frac{1}{c_{ESS}}$$
$$β_{ESS} = \frac{\partial SOC}{\partial P_{ESS}} \cdot \frac{1}{Δt}$$

5. Conclusion

The proposed hierarchical control strategy demonstrates 35% cost reduction compared with pure energy storage inverter solutions and 19.55% improvement over global consensus approaches. By prioritizing PV reactive support and coordinating energy storage inverters through sensitivity-optimized grouping, the method effectively addresses voltage violations while extending equipment lifespan through balanced utilization.

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