塔式太阳能电站聚光镜场的土地利用率研究

塔式太阳能热发电站的聚光镜场大多是由按一定规律排列的矩形定日镜组成,在相邻定日镜间无机械碰撞的情况下,聚光镜场的最大土地利用率仅为58%。文章提出了选用规则交错排列的聚光镜场布置方案,建立不同形状定日镜的土地利用模型,并计算出不同情况下的最大土地利用率。通过仿真得出,矩形定日镜和六边形定日镜在一定长宽比时可获得最大土地利用率,其中六边形定日镜的土地利用率最高,约为100%。     

An assessment on hydrogen production using central receiver solar systems

An assessment is presented on hydrogen production using a dedicated central receiver solar system concept coupled to two types of hydrogen producing processes, electrolysis and thermochemical. The study on solar electrolytic hydrogen was carried out using solar electricity and four different electrolytic technologies, namely industrial unipolar 1980 and 1983 technologies, industrial bipolar and solid polymer electrolyte technology. The thermochemical process was the sulphur/iodine cycle which is being developed by General Atomic Co. Systems which is capable of producing about 10⁶ GJ hydrogen per year were developed at the conceptual level and site specific computations were carried out. A general mathematical model was developed to predict the optical and thermal performance of the central receiver system coupled directly to the chemical plant. Cost models were developed for each sub-system based on the database published in the literature. Levelized and delevelized costs of solar hydrogen were then computed.     

Analysis and design of a field of heliostats for a solar power plant

For the design of the mirror field for the CNRS (Centre National de la Recherche Scientifique) project of a several MWe solar energy conversion power plant, an analysis of this concentration system is proposed. Using simulation programs, the problems of the choice of an optimal height of the tower and a convenient slope of the field are solved. By analysing the variation of the thermal power during five test days, it is shown that subject to certain assumptions the maximum output power is about 10 MWe.     

Low-profile heliostat design for solar central receiver systems

Heliostat designs intended to reduce costs and the effect of adverse wind loads on the devices were developed. Included was the low-profile heliostat consisting of a stiff frame with sectional focusing reflectors coupled together to turn as a unit. The entire frame is arranged to turn angularly about a center point. The ability of the heliostat to rotate about both the vertical and horizontal axes permits a central computer control system to continuously aim the sun's reflection onto a selected target. A schematic of the heliostat design is shown in Fig. 1. An engineering model of the basic device was built and is being tested. Control and mirror parameters, such as roughness and need for fine aiming, are being studied. The fabrication of these prototypes is in process. The model was also designed to test mirror focusing techniques, heliostat geometry, mechanical functioning, and tracking control. The model can be easily relocated to test mirror imaging on a tower from various directions. In addition to steering and aiming studies, the tests include the effects of temperature changes, wind gusting and weathering. The results of economic studies on this heliostat are also presented.     

Optimized working temperatures of a solar central receiver

Recent developments in solar tower technology, aimed at the achievement of high temperatures (above 1100 K) for the operation of advanced power conversion units (gas turbine and combined cycle), require careful analysis of their optimal operating parameters. This study presents a method of optimization for design parameters, such as the receiver working temperature and the heliostat field density. This method aims at maximizing the overall efficiency of the three major subsystems that constitute the entire plant, namely, the heliostat field and the tower, the receiver and its accompanying secondary optics, and the power block. The results of this optimization process are shown and analyzed. The principal result demonstrates that the operating temperature has an optimal value and its further increase can lower the overall efficiency of the system.     

Allowable flux density on a solar central receiver

The allowable flux density on a solar central receiver is a significant receiver parameter and is related to the receiver life span and economics. The allowable flux density has gradually increased as receiver technologies have developed and is related to various factors, such as the material characteristics, tube sizes, and internal tube flow conditions. A mathematical model was developed to calculate the allowable flux density for the Solar Two receiver which agrees well with published data. The model was then used to show that a higher allowable flux density can be obtained by increasing the allowable strain of the tube material and the fluid velocity and decreasing the tube thermal resistance, the convective thermal resistance, and the tube diameter and wall thickness. A sensitive analysis shows that the most important influence is the wall thickness, followed by the tube diameter and fluid velocity. Finally, a molten salt receiver gives a much higher allowable flux density than water/steam receivers and is even better than a supercritical steam receiver.     

塔式太阳能热发电镜场中余弦效率仿真研究

参考eSolar塔式发电站中的矩形定日镜场,通过参数设计得到密集的轴对称交错排列布置方案;建立了余弦效率的数学模型,对一天中不同时刻的太阳入射角变化趋势进行了仿真,得出位于接收塔南北区域余弦效率状况;对矩形定日镜场的余弦效率分布做了进一步研究。仿真结果验证了太阳入射角的变化趋势,并得出塔的高度对余弦效率的影响。     

Receiver design considerations for solar central receiver hydrogen production

The status of the Solar Central Receiver or Power Tower developments is briefly reviewed. with particular consideration given to the application of this technology to thermochemical hydrogen production. Emphasis is on the general considerations in the receiver-chemical reactor interface. High solar flux densities of 1.5–3 MW M⁻² must be transformed to 50–100 kW M⁻² for catalytic decomposition of sulfuric acid such as in the General Atomic (GA) water-splitting reactions. The different methods considered to accomplish such reactions include cavities, external heat pipe receivers, a falling curtain of particles, and other direct absorption media coupled to chemical reactions.     

Site selection for hillside central receiver solar thermal plants

In this article, a new tool is introduced for the purpose of locating sites in hillside terrain for central receiver solar thermal plants. Provided elevation data at a sufficient resolution, the tool is capable of evaluating the efficiency of a heliostat field at any site location. The tool also locates suitable sites based on efficiency and average annual normal insolation. The field efficiency, or ratio of radiation incident to the receiver to direct normal solar radiation, is maximized as a result of factors including projection losses and interference between heliostats, known respectively as cosine efficiency, shading, and blocking. By iteratively defining the receiver location and evaluating the corresponding site efficiency by sampling elevation data points from within the defined heliostat field boundary, efficiency can be mapped as a function of the receiver location. The case studies presented illustrate the use of the tool for two field configurations, both with ground-level receivers and hillside heliostat layouts. While both configurations provide acceptable efficiencies, results from case studies show that optimal sites for ground-level receivers are ones in which the receiver is at a higher elevation than the heliostat field. This result is intuitive from the perspective of minimizing cosine losses but is nevertheless a novel configuration.     

Theoretical concentration of solar radiation by central receiver systems

Solar concentrations by central receiver systems have been calculated theoretically for various values of obliquity of the incident radiation, assuming that plane heliostat-mirrors, sufficiently small in dimension, cover a circular field without clearance. Through this calculation, the performance characteristics of this system such as the availability of the radiant energy incident on the heliostat-field, the distribution of interruption by an adjacent mirror, the optimum rim-angle for the mean area- and the mean volume-concentration and the attainable temperature were revealed. The study was extended towards the practical problem of decreasing the number of heliostats by increasing the dimensions of heliostat-mirrors, and the effect of increasing mirror-dimensions was argued for both plane and curved mirrors.     

Hydrogen as a vector for central receiver solar utilities

An assessment is presented to use hydrogen or hydrogen-rich fuels as a vector in the Central Receiver Solar Utility (CRSU) concept.

The CRSU is conceived to meet primarily the domestic energy requirements for space heating and hot water production of a community. It normally operates to provide low grade heat with sensible seasonal heat storage and district heating systems. However, there are institutional problems connected with using sensible heat storage and low grade energy distribution systems into dwellings.

An alternative to this would be to produce hydrogen and hydrogen-rich fuels by using an advanced conversion technology and eliminate low grade heat storage and distribution systems. Two developing technologies, namely high temperature electrolysis and thermochemical processes, are considered for production of the vector. Then, an assessment is carried out at the conceptual level for fully dedicated Central Receiver Solar Utility Plants which integrate a central receiver system, thermochemical plant or electrical power generating system and synthetic fuel production plant with necessary auxiliary sub-systems.

It is shown that for a 10% capital recovery factor, the cost of hydrogen at the plant will be about $18 per GJ using thermochemical processes and about $20 per GJ using high temperature electrolysis processes.

The solar-hydrogen can also be converted to a more easily stored fuel for domestic use such as methanol, ethanol, ammonia or fuel oil. In this case, there is a distinct possibility that by using waste heavy fuels, tar sands and biomass, the cost of synthetic fuel can be considerably reduced.     

反射塔底式太阳能集热装置及镜场分析

提出了塔式太阳能热发电站反射塔底式集热装置,并与传统的塔式太阳能集热装置进行了能量损失分析比较,对反射塔底式太阳能集热装置的镜场进行了建模分析。通过对反射塔底式集热装置模型及对定日镜场的分析,显示了定日镜对塔顶二次反射器面积效应的影响,推荐了定日镜的形状参数。     

An optimization tool to design the field of a solar power tower plant allowing heliostats of different sizes

The design of a solar power tower plant involves the optimization of the heliostat field layout. Fields are usually designed to have all heliostats of identical size. Although the use of a single heliostat size has been questioned in the literature, there are no tools to design fields with heliostats of several sizes at the same time. In this paper, the problem of optimizing the heliostat field layout of a system with heliostats of different sizes is addressed. We present an optimization tool to design solar plants allowing two heliostat sizes. The methodology is illustrated with a particular example considering different heliostat costs. Copyright © 2017 John Wiley & Sons, Ltd.     

Exergetic analysis and economic evaluation of central tower receiver solar thermal power plant

This article presents the analytical evaluation of a central tower receiver solar thermal power plant with air‐cooled volumetric receiver using exergy analysis. The energetic and exergetic losses as well as the efficiencies of a typical central tower receiver‐based solar thermal power plant have been carried out under the specific operating conditions. The enhancement in efficiency of the plant from the variation in power input to constant power input achieved by thermal storage backup condition has been determined. It is found that the year round average energetic efficiency can be increased from 24.15% to 25.08% and year round average exergetic efficiency can be increased, from 26.10% to 27.10% for the selected location Jodhpur. The unit cost of electric energy generation (kWh_e) is found to be INR 10.09 considering 30‐year lifespan of the solar plant along with a 10% interest rate. The present study provides a base for the development of future solar thermal power plants in India. Copyright © 2013 John Wiley & Sons, Ltd.     

Performance of optimized solar central receiver systems as a function of receiver thermal loss per unit area

Recent efforts in solar central receiver research have been directed toward high-temperature applications. Associated with high-termperature processes are greater receiver thermal losses due to thermal radiation and convection. This article examines the performance of central receiver systems having optimum heliostat fields and receiver aperture areas as a function of receiver thermal loss per unit area. The results address the problem of application optimization, where the receiver design, temperature and consequently thermal loss per unit area may vary. A reasonable range of values for the primary independent variable L (the average thermal loss per unit area of receiver aperture) and a reasonable set of design assumptions were first established. Heliostat field analysis and optimization required a detailed computational analysis. Results are discussed for tower focal heights of 150 and 180 m. Values of L ranging from 0.04 to 0.50 MW per square meter were considered, roughly corresponding to working fluid temperatures in the range of 650–1650°C. As L increases over this range, the receiver thermal efficiency and the receiver interception factor decrease. The optimal power level drops by almost half, and the cost per unit of energy produced increases by about 25% for the base case set of design assumptions. The resulting decrease in solar subsystem efficiency (relative to the defined annual input energy) from 0.57 to 0.35 is about 40% and is a significant effect. Unoptimized systems would experience an even greater degradation in cost-effectiveness.     

An analysis of the terminal concentrator concept for solar central receiver systems

One of the most interesting approaches to the large scale development of solar energy for electric power production is the Central Receiver System Concept. The Central Receiver System contains a large number of individually guided heliostats that reflect sunlight towards a central receiver high above the field of heliostats. The system resembles a giant Fresnel mirror and provides a substantial concentration of the solar beam. If high concentration is desired, a terminal concentrator may be included.The terminal concentrator is a device designed to increase the concentration of solar flux reflected from the collector field. Our study depends on two assumptions: (1) the beam width formula for the reflected beams and (2) the uniformly bright collector field which is a gross simplification allowing us to deal with the terminal concentrator. We obtained the necessary design relations, including a lower bound for the rim angle φ_m, the average fraction reflected $\text{?}\text{(φ}{}_{\mathrm{m}}\text{)}$, a radiative stagnation temperature for the aperature, and the concentration ratios. The temperature and concentration ratio curves determine the optimum rim angle φ_m for each of several designs. When designed to provide maximum concentration, the terminal concentrator becomes excessively large. Consequently, we consider a design which produces 90 per cent of the maximum concentration and reduces the size of the conical reflector by 5–6 times. The effectiveness of this compromise design permits us to conclude that a practical terminal concentrator of the conical variety can almost double the concentration without any appreciable loss of total power. There will be losses due to reflectivity but not due to beam spillage because of the reduced aperture. The terminal concentrator will be economically desirable for small central receiver systems if it is cheaper than the incremental cost of the heliostat field due to the additional focusing required to produce the same concentration.     

Photochemically assisted solar energy storage using eriochrome black-T in solar flat collector

The criteria for cis-trans photoisomerization of eriochrome black-T (EBT) in the flat-plate collector system, which consists of endoergic photochemical reaction, has been investigated. The efficiencies of this collector in both summer and winter have been compared with blank (distilled water only) and colored liquid (non-isomer-dye-absorbing in the same wavelength range). The photochemical storage efficiency was found to be higher in winter than in summer. The optimum efficiency for this photoisomerization-thermal reversion cycle was found by varying with the pumping rate of the liquid to match the value of rate constant of cis to trans reaction. The stability of (EBT) has been studied under different environmental conditions.     

Measurements of solar flux density distribution on a plane receiver due to a flat heliostat

An experimental facility is designed and manufactured to measure the solar flux density distribution on a central flat receiver due to a single flat heliostat. The tracking mechanism of the heliostat is controlled by two stepping motors, one for tilt angle control and the other for azimuth angle control. A x-y traversing mechanism is also designed and mounted on a vertical central receiver plane, where the solar flux density is to be measured. A miniature solar sensor is mounted on the platform of the traversing mechanism, where it is used to measure the solar flux density distribution on the receiver surface. The sensor is connected to a data acquisition card in a host computer. The two stepping motors of the heliostat tracking mechanism and the two stepping motors of the traversing mechanism are all connected to a controller card in the same host computer. A software “TOWER” is prepared to let the heliostat track the sun, move the platform of the traversing mechanism to the points of a preselected grid, and to measure the solar flux density distribution on the receiver plane. Measurements are carried out using rectangular flat mirrors of different dimensions at several distances from the central receiver. Two types of images were identified on the receiver plane—namely, apparent (or visible) and mirror-reflected radiation images. Comparison between measurements and a mathematical model validates the mathematical model.     

Detailed analysis of the solar power collected in a beam-down central receiver system

The design of a beam-down solar power plant represents a very complex problem, being its performance dependent on many interrelated parameters. A systematic analysis of these parameters is proposed in the present study. The effect of the hyperboloid eccentricity on both the sunshape and the size of the heliostats is analyzed. Optimal values of the characteristic parameters of the compound parabolic concentrator are also proposed and on the basis of these considerations, extensive calculations are presented to evaluate yearly solar power collection.