Solar Photovoltaic Integration in Monopolar DC Networks via the GNDO Algorithm
Abstract
:1. Introduction
1.1. General Context
1.2. Motivation
1.3. State-of-the-Art Review
1.4. Contribution and Scope
- i.
- The application of the GNDO approach to the problem regarding the optimal placement and sizing of PV sources in monopolar DC distribution networks by improving the existing literature results reported in [22] via the application of the discrete-continuous VSA.
- ii.
- The combination of the GNDO approach with the efficient successive approximation power flow method using a master–slave optimization strategy. The main advantage of this combination lies in its reduced processing times (less than 10 min) to solve the studied problem in the DC versions of the IEEE 33- and IEEE 69-bus grids, with excellent numerical results.
1.5. Document Structure
2. Mathematical Formulation
3. Solution Methodology
3.1. Generalized Normal Distribution Optimization Algorithm
- ✔
- An initial population is generated with a normal distribution throughout the solution space. This initial population evolves through the solution space to explore and exploit its promissory sub-regions. During the first stages of the optimization process, the variances regarding the positions of the solution individuals show minimal variations, and the location of the decision variables concerning the global optimal solution can be considered to be randomly distributed with a normal structure.
- ✔
- As the evolution process through the solution space advances, the main position and the standard deviation are continuously decreased. This is done in order to pass from the exploration phase to the exploration of the solution space, i.e., refining the solution around the best solution reached.
- ✔
- At the end of the optimization process, the variance of the positions between all the solution individuals and the distance between the mean position and the optimal solution reach minimum values.
3.1.1. Local Exploration
3.1.2. Global Exploration
3.2. Power Flow Solution
3.3. Summary of the Optimization Methodology
Algorithm 1: Application of the GNDO method to locate and size PV sources in monopolar DC networks. |
4. Test Feeder Characteristics and Problem Parametrization
4.1. First Test Feeder
4.2. Second Test Feeder
4.3. Parametrization of the Studied Problem
5. Computational Validation
5.1. Results for the First Test Feeder
- ✔
- The reduction concerning the benchmark case with the CBGA was about USD/year 981,318.19, which corresponds to . The reduction reached with the DCVSA was about USD/year 981,617.69, (), and the best solution for the benchmark case was reached with the proposed GNDO approach, with USD/year 981,671.42, i.e., a reduction of . These results show that all the optimizers yield an annual expected reduction of USD 981,300.00 per year of operation. Furthermore, comparing the best literature report (solution with the DCVSA in [22] with the proposed GNDO approach, an improvement of about USD/year 53.73 is achieved, which makes it the best result reported in the current literature for the 33-bus grid with a DC monopolar configuration.
- ✔
- The three algorithms detected that one of the best sites to locate a PV source is node 31, where injections of power higher than 1540 kW are listed. This location demonstrates that the 33-bus grid is one of the most sensitive nodes to install PV sources concerning the expected improvement of the objective function. In addition, the total PV capacity installed with the CBGA is kW, kW with the DCVSA, and kW with the proposed GNDO. These values show that, for the 33-bus grid, the proposed GNDO installed less power with better objective function values, which a better nodal selection can explain in comparison with the CBGA and the DCVSA.
5.2. Results for the Second Test Feeder
- ✔
- The proposed GNDO approach achieves the best reduction with respect to the benchmark case, with a value of USD/year 1,032,408.85, i.e., . The DCVSA reached an annual reduction of USD/year 1,031,881.8, corresponding to an improvement of , and the CBGA reduced the expected annual operating costs by about USD/year 1,031,821.52, i.e., with respect of the benchmark case.
- ✔
- The nodes to locate PV generators for the proposed GNDO and the CBGA are the same, i.e., nodes 19, 61, and 64. However, the sizes assigned to the PV sources in these nodes differ between them. This behavior is explained by using the Gaussian distribution functions and decreasing the radius in the GNDO approach, which allows shifting from exploring the solution space to exploiting it.
- ✔
- The improvement obtained with the GNDO with respect to the CBGA was USD 587.33 per year of operation, whereas, for the DCVSA, this improvement was about USD/year . These results demonstrate that the proposed master–slave optimizer is the best current solution reported for the 69-bus DC network with a monopolar configuration, i.e., the GNDO represents the reference point for future research in this area.
6. Conclusions and Future Work
Author Contributions
Funding
Institutional Review Board Statement
Informed Consent Statement
Data Availability Statement
Acknowledgments
Conflicts of Interest
References
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Node i | Node j | () | (kW) | Node i | Node j | () | (kW) |
---|---|---|---|---|---|---|---|
1 | 2 | 0.0922 | 100 | 17 | 18 | 0.7320 | 90 |
2 | 3 | 0.4930 | 90 | 2 | 19 | 0.1640 | 90 |
3 | 4 | 0.3660 | 120 | 19 | 20 | 1.5042 | 90 |
4 | 5 | 0.3811 | 60 | 20 | 21 | 0.4095 | 90 |
5 | 6 | 0.8190 | 60 | 21 | 22 | 0.7089 | 90 |
6 | 7 | 0.1872 | 200 | 3 | 23 | 0.4512 | 90 |
7 | 8 | 1.7114 | 200 | 23 | 24 | 0.8980 | 420 |
8 | 9 | 1.0300 | 60 | 24 | 25 | 0.8960 | 420 |
9 | 10 | 1.0400 | 60 | 6 | 26 | 0.2030 | 60 |
10 | 11 | 0.1966 | 45 | 26 | 27 | 0.2842 | 60 |
11 | 12 | 0.3744 | 60 | 27 | 28 | 1.0590 | 60 |
12 | 13 | 1.4680 | 60 | 28 | 29 | 0.8042 | 120 |
13 | 14 | 0.5416 | 120 | 29 | 30 | 0.5075 | 200 |
14 | 15 | 0.5910 | 60 | 30 | 31 | 0.9744 | 150 |
15 | 16 | 0.7463 | 60 | 31 | 32 | 0.3105 | 210 |
16 | 17 | 1.2860 | 60 | 32 | 33 | 0.3410 | 60 |
Node i | Node j | () | (kW) | Node i | Node j | () | (kW) |
---|---|---|---|---|---|---|---|
1 | 2 | 0.0005 | 0 | 3 | 36 | 0.0044 | 26 |
2 | 3 | 0.0005 | 0 | 36 | 37 | 0.0640 | 26 |
3 | 4 | 0.0015 | 0 | 37 | 38 | 0.1053 | 0 |
4 | 5 | 0.0251 | 0 | 38 | 39 | 0.0304 | 24 |
5 | 6 | 0.3660 | 2.6 | 39 | 40 | 0.0018 | 24 |
6 | 7 | 0.3810 | 40.4 | 40 | 41 | 0.7283 | 1.2 |
7 | 8 | 0.0922 | 75 | 41 | 42 | 0.3100 | 0 |
8 | 9 | 0.0493 | 30 | 42 | 43 | 0.0410 | 6 |
9 | 10 | 0.8190 | 28 | 43 | 44 | 0.0092 | 0 |
10 | 11 | 0.1872 | 145 | 44 | 45 | 0.1089 | 39.22 |
11 | 12 | 0.7114 | 145 | 45 | 46 | 0.0009 | 39.22 |
12 | 13 | 1.0300 | 8 | 4 | 47 | 0.0034 | 0 |
13 | 14 | 1.0440 | 8 | 47 | 48 | 0.0851 | 79 |
14 | 15 | 1.0580 | 0 | 48 | 49 | 0.2898 | 384.7 |
15 | 16 | 0.1966 | 45.5 | 49 | 50 | 0.0822 | 384.7 |
16 | 17 | 0.3744 | 60 | 8 | 51 | 0.0928 | 40.5 |
17 | 18 | 0.0047 | 60 | 51 | 52 | 0.3319 | 3.6 |
18 | 19 | 0.3276 | 0 | 9 | 53 | 0.1740 | 4.35 |
19 | 20 | 0.2106 | 1 | 53 | 54 | 0.2030 | 26.4 |
20 | 21 | 0.3416 | 114 | 54 | 55 | 0.2842 | 24 |
21 | 22 | 0.0140 | 5 | 55 | 56 | 0.2813 | 0 |
22 | 23 | 0.1591 | 0 | 56 | 57 | 1.5900 | 0 |
23 | 24 | 0.3460 | 28 | 57 | 58 | 0.7837 | 0 |
24 | 25 | 0.7488 | 0 | 58 | 59 | 0.3042 | 100 |
25 | 26 | 0.3089 | 14 | 59 | 60 | 0.3861 | 0 |
26 | 27 | 0.1732 | 14 | 60 | 61 | 0.5075 | 1244 |
3 | 28 | 0.0044 | 26 | 61 | 62 | 0.0974 | 32 |
28 | 29 | 0.0640 | 26 | 62 | 63 | 0.1450 | 0 |
29 | 30 | 0.3978 | 0 | 63 | 64 | 0.7105 | 227 |
30 | 31 | 0.0702 | 0 | 64 | 65 | 1.0410 | 59 |
31 | 32 | 0.3510 | 0 | 11 | 66 | 0.2012 | 18 |
32 | 33 | 0.8390 | 14 | 66 | 67 | 0.0047 | 18 |
33 | 34 | 1.7080 | 19.5 | 12 | 68 | 0.7394 | 28 |
34 | 35 | 1.4740 | 6 | 68 | 69 | 0.0047 | 28 |
Parameter | Value | Unit | Parameter | Value | Unit |
---|---|---|---|---|---|
0.1390 | US$/kWh | T | 365 | days | |
10 | % | 2 | % | ||
y | 20 | years | 1 | h | |
1036.49 | US$/kWp | 0.0019 | US$/kWh | ||
2400 | kW | 0 | kW | ||
3 | – | ±10 | % | ||
US$/V | US$/V | ||||
US$/W | US$/A |
Method | Site (Node)/Size (kW) | (US$/Year) |
---|---|---|
Bench. case | – | 3,644,043.01 |
CBGA | 2,662,724.82 | |
DCVSA | 2,662,425.32 | |
GNDO | 2,662,371.59 |
Method | Site (Node)/Size (kW) | (US$/Year) |
---|---|---|
Bench. case | – | 3,817,420.38 |
CBGA | 2,785,598.86 | |
DCVSA | 2,785,538.58 | |
GNDO | 2,785,011.53 |
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Montoya, O.D.; Gil-González, W.; Grisales-Noreña, L.F. Solar Photovoltaic Integration in Monopolar DC Networks via the GNDO Algorithm. Algorithms 2022, 15, 277. https://doi.org/10.3390/a15080277
Montoya OD, Gil-González W, Grisales-Noreña LF. Solar Photovoltaic Integration in Monopolar DC Networks via the GNDO Algorithm. Algorithms. 2022; 15(8):277. https://doi.org/10.3390/a15080277
Chicago/Turabian StyleMontoya, Oscar Danilo, Walter Gil-González, and Luis Fernando Grisales-Noreña. 2022. "Solar Photovoltaic Integration in Monopolar DC Networks via the GNDO Algorithm" Algorithms 15, no. 8: 277. https://doi.org/10.3390/a15080277
APA StyleMontoya, O. D., Gil-González, W., & Grisales-Noreña, L. F. (2022). Solar Photovoltaic Integration in Monopolar DC Networks via the GNDO Algorithm. Algorithms, 15(8), 277. https://doi.org/10.3390/a15080277