1. Introduction
To expedite the development of a clean, low-carbon, safe, and efficient energy system, China has prioritized the construction of extensive new energy bases in deserts, the Gobi, and wastelands [
1]. Nonetheless, the variability of new energy output in these areas, particularly its seasonal characteristics, often exacerbates the peak load pressures on thermal power units and limits the full utilization of the transmission capacity within new energy corridors. The “14th Five-Year Plan” for a modern energy system emphasizes enhancing the construction of interprovincial and cross-regional power transmission channels, aiming for an average utilization exceeding 4500 h annually for these DC transmission channels. Employing power system timing operation simulations—a fundamental tool for both planning and operational processes [
2]—to model the scheduling at new energy bases in desert and Gobi regions is crucial. This approach not only helps determine the power supply operational plan but also facilitates a quantitative assessment of the average utilization hours of the DC transmission channels. Such assessments are essential for improving the efficiency of new energy transmission channels and enhancing the consumption capacity at these new energy bases.
Timing operation simulation predominantly focuses on power production involving new energy sources. Extensive research has been conducted on the scheduling and planning of large-scale, multi-energy, multi-timescale new energy power systems. Serving as a crucial technical approach for studying large-scale multi-energy systems, mid/long-term time-series operation simulations are required to account for factors such as multi-energy complementarity, diverse power characteristics of different energy sources, and the uncertainty of new energy outputs [
3,
4,
5,
6]. A multi-timescale time-sequence operation simulation model for large-scale new energy power systems was introduced in [
7]. This model differentiates between medium- and long-term operation simulations that address the seasonal variations in new energy output and short-term models that tackle the stochastic nature of these outputs, yielding comprehensive and accurate simulation results. Consequently, the simulation of new energy base time series operations in desert and Gobi areas should initially analyze the volatility and randomness of wind and photovoltaic power, in alignment with the specific characteristics of new energy outputs in these regions.
Numerous scholars have developed various index systems to quantify the fluctuation characteristics of wind power. These systems include metrics such as the wind power capacity factor, credible capacity factor, and peak and valley coefficients, which facilitate a detailed analysis of wind power fluctuation distribution across diverse spatial and temporal scales [
8,
9,
10]. An improved scene reduction method, which integrates enhanced K-means clustering with the simultaneous backward generation elimination algorithm, was introduced in [
11]. This method aims to represent complex scenarios with a minimal set of representative scenes effectively. Additionally, a renewable energy scene reduction technique that combines clustering and optimization algorithms was proposed in [
12] to efficiently achieve scene reduction. However, expressing the volatility of wind PV is more suitably conducted probabilistically, and K-means clustering faces challenges with determining the optimal number of clusters.
In the realm of DC outgoing operation models, a high-voltage DC liaison line operation model was introduced in [
13] to enhance the regulation of inter-regional wind power. Addressing the challenge of large-scale wind power aggregation within the sender power system, a two-stage optimal scheduling model was developed in [
14]. This model facilitates day-ahead optimal scheduling for the sender power system. To fully leverage the flexible regulation capacity of the UHV DC liaison line, a multitemporal coordinated optimization method that considers the joint outflow of wind, photovoltaic, and photothermal energies was devised in [
15], significantly improving the utilization of wind and solar resources. Additionally, a joint scheduling plan model integrating flexible direct, pumped storage, and thermal power was proposed in [
16], aimed at optimizing the joint scheduling strategy to maximize new energy consumption. Lastly, a time-series simulation calculation method, performing week-by-week calculations across a full year of 8760 h, was proposed in [
17] to achieve reasonable optimization of the medium- and long-term operation modes of the DC outgoing system. Furthermore, a multi-objective optimization methodology for enhancing the overall transmission capacity of AC-DC hybrid interfaces is put in [
18]. This proposed methodology is designed to reduce the initial investment costs associated with the energy delivery system while simultaneously promoting the utilization of renewable energy sources.
Notwithstanding the comprehensive nature of the aforementioned studies, none of them investigated the influence of the DC transmission mode on the operational modeling of HVDC liaison lines. In the context of China’s market-based power trading, a singular transmission trading mode no longer reflects the actual production scenarios accurately. Additionally, while these studies primarily focus on maximizing new energy consumption, they do not necessarily ensure the efficient operation of the DC transmission channel. For instance, the Qishao UHV system, during its initial year and ten months of operation, transmitted a total of 9 billion kWh to Hunan, which is substantially lower than its designed annual capacity of 40 billion kWh. Consequently, the actual utilization rate fell below the design value.
Addressing the challenges outlined previously, this study introduces a simulation model for the time-sequence operation of new energy bases in desert and Gobi areas, with a focus on DC utilization hours. Given the volatility of wind power output in these regions, the number of Gaussian functions in the Gaussian Mixture Model (GMM) is determined by analyzing wind power and photovoltaic output data using “Gaussian Kernel Density Estimation (GKDE) + GMM”. Concurrently, a flexible DC transmission model that incorporates DC transmission modes is developed. This model primarily employs mid/long-term DC transmission modes, with spot DC transmission serving as a supplementary mechanism for the consumption of wind power and photovoltaic energy. In solving the time-series operation model, the dung beetle optimization algorithm with non-dominated sorting is utilized to reduce variable counts and decrease the computational times required by commercial solvers. Ultimately, a simulation model for the time-sequence operation of the desert and Gobi area New Energy Base is proposed, taking into account DC utilization hours, environmental factors, economic considerations, and operational flexibility. The model’s efficacy is demonstrated using a case study from the New Energy Base in Gansu Province, Northwest China. Results indicate that the model facilitates efficient utilization of the DC transmission channel and high levels of new energy consumption while accounting for economic, flexibility, and environmental factors.
This paper is organized as follows.
Section 2 analyzes the fluctuation characteristics of wind power and photovoltaic in desert, Gobi, and desert beach areas;
Section 3 constructs an operation model for new energy bases in desert, Gobi, and desert beach areas;
Section 4 describes the objective function and solution process of the operation simulation model for new energy bases in desert, Gobi, and desert beach areas; and in
Section 5, the simulation results of the basic scenarios as well as the time-sequence operation simulation with the addition of pumped storage are given, respectively, and the results are analyzed. The simulation results are analyzed. Finally,
Section 6 is the conclusion.
2. Analysis of the Volatility of Wind Power Output in the Gobi and Desert Area
The large volatility of wind power output in the desert and Gobi area is the main factor affecting DC transmission. At present, the k-means method is mostly adopted to analyze the clustering of wind power, but it is only able to strictly divide the data and cannot reflect the probability characteristics of the volatility. GMM could be an excellent solution to the above problems. Firstly, the Gaussian mixture model could fit all shapes theoretically. In addition, the clustering results of GMM are expressed through the form of probability, which does not force the data points to be divided into a certain class, and it is possible to better reflect the volatility and stochasticity of the scenic outflow of the desert and Gobi area. Therefore, it utilizes GKDE estimation in this paper for the initial processing of the scenery data. The kernel density estimation is the ability to analyze the extent to which the current dataset conforms to the Gaussian function, thus determining the number of Gaussian functions for the GMM.
The standard deviation is commonly employed to measure the fluctuation of new energy output, and to determine the fluctuation of two adjacent moments, the mean value in the standard deviation is replaced with the value of the scenery output at the previous moment. The formula is as follows Equation (
1):
where:
is the time scale of the calculation, a total of 168 h for one week,
and
denote the wind power or PV output data under the moments of
t and
, respectively.
In addition to the fluctuation timeshare as another indicator to describe the volatility of wind and light output, when the change in output from the previous moment to the next moment exceeds
, it is regarded as output fluctuation. The formula is as follows Equation (
2):
where:
is the time of the week when the wind or PV output fluctuates.
Calculate the level of fluctuation and the percentage of time of fluctuation for each week in the three desert regions of Tengger, Badanjilin and Kumutag. These data are analyzed with Gaussian kernel density estimation and the results are obtained as shown in
Figure 1 and
Figure 2.
According to the kernel density estimation results in the figures, the T-value of wind power and the S, T-value of PV output are bimodal in the volatility indicators of wind power and PV, indicating that they conform to two Gaussian distributions. The S-value of wind power output is single-peaked, indicating compliance with one Gaussian distribution. Therefore, the number of Gaussian functions of the Gaussian mixture model for wind power and PV is determined to be 2.
The results of the GMM analysis are shown in
Table 1. Based on the parameters in
Table 1 it is sufficient to calculate the probability that the fluctuating data of the wind and light outputs for each week belong to each Gaussian function, which is calculated by the following (
3) and (
4):
where:
and
denote the probability of wind power and PV output fluctuation characteristics belonging to Gaussian function
i, respectively.
and
denote the mixing coefficients of wind power and PV Gaussian function
i,
and
denote the center coordinates and covariance of wind power Gaussian function
i,
and
denote the center coordinates and covariance of PV Gaussian function
i,
S and
T denote the weekly fluctuation index of wind power,
and
denote the probability value of wind power and PV fluctuation index belonging to the probability value of the two-dimensional Gaussian function.
The probability calculation of the wind power
volatility data of the example scenario is shown in
Figure 3, where
and
denote the wind power Gaussian function 1 and the wind power Gaussian function 2, respectively, and
and
denote the PV Gaussian function 1 and the PV Gaussian function 2, respectively. As shown in
Figure 3, the lighter the color denotes the higher the probability of being affiliated with the current Gaussian function, and the darker the color denotes the lower the probability of being affiliated with the current Gaussian function. In this paper, the wind PV output is reconstructed based on the calculated probability values.