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Optimum design and performance of a solar dish microturbine using tailored component characteristics Giacomo Gavagnina, Sergio Rechb, David Sáncheza,∗, Andrea Lazzarettoc aUniversity of Seville, Camino de los descubrimientos s/n, 41092 Seville, Spain bInterdepartmental Center “Giorgio Levi Cases” for Energy Economics and Technology - University of Padova, via Marzolo 9, 35131 Padova, Italy cDepartment of Industrial Engineering - University of Padova, via Venezia 1, 35131,Padova, Italy Abstract The aim of the paper is to find the optimum design and performance of solar microturbines powered by parabolic dish collectors using an innovative methodology which integrates the design and off-design models of the total system. In contrast to the common practice of assigning an estimated efficiency to the engine turbomachinery (generalized performance maps), the procedure hereinafter produces the specific geometry and the characteristic maps of compressor and turbine, according to their inlet/outlet thermodynamic states and working cycle boundary conditions. With this global approach, a sensitivity analysis is performed to search for the pressure ratio that maximizes the solar-to-electric efficiency at design point for a constant air mass flow rate and turbine inlet temperature. Maximum values in the range 18.0% to 21.7% are obtained for a pressure ratio of 3.2 when the turbine inlet temperature changes between 800°C (base-case system) and 900°C. The methodology allows also to simulate the performance of the system when different design DNIs are considered with the aim to maximize the annual yield of the system. Simulations performed for Beijing, Seville and San Diego showed that quite different DNIs (610 to 815 W/m2) are to be chosen to get the maximum annual (average) efficiency: 11% to 16% for the base-case system and 14% to 19% for a more advanced design. ∗Corresponding author Email address: [email protected] (David Sánchez) Preprint submitted to Applied Energy September 11, 2018
Keywords: Microturbine, Solar dish, Volumetric cavity receiver, Design and off-design NOMENCLATURE αAbsorptivity ¯ηglobal Mean annual efficiency (global) ¯ Tair Average temperature of air in the cavity of the solar receiver ∆hsIsentropic enthalpy change δcl Clearance gap ˙ CHeat capacity ˙mMass flow rate ˙ Qint Receiver gross heat input ˙vVolumetric flow rate Emissivity ηEfficiency ΓFlux capture fraction γHeat capacity ratio νts,t Total-to-static velocity ratio ωAngular rotational speed φTotal radiant flux ψRim angle ρDensity σStefan-Boltzmann constant τTransmissivity εEffectiveness ςReflectivity ξInclination angle AAperture area amb Ambient bblade Blade height C∗Heat capacity ratio c0,is Spouting velocity dDiameter dsSpecific diameter DNI Direct Normal Irradiance DP Design Point EEnergy etot Total concentration error fpPressure loss factor fcapacity Capacity factor fdish Focal distance of dish fdumped Dumped energy factor GSpecific flow rate hEnthalpy HTArec Heat Transfer Area of recuperator 2
ISpecific irradiance kcv,ext External convective heat transfer coefficient of receiver window kcv,int Internal convective heat transfer coefficient of receiver window kdep Derating factor mGT micro Gas Turbine NRotational speed nsSpecific speed NTU Number of Transfer Units PPower pPressure Pmech Shaft power rcCompressor pressure ratio reTurbine pressure ratio rcv Receiver rec Recuperator rel Relative SR Simple recuperated TTemperature TwTemperature of glass window of solar receiver TIT Turbine Inlet Temperature TMY Typical Meteorolgical Year TOT Turbine Outlet Temperature ts Total-to-static tt Total-to-total UHeat transfer coefficient uBlade speed vcr Critical speed WSpecific power 1. Introduction Solar power is the most abundant and distributed primary energy source on Earth. In the last decades, academic and governmental organizations have attempted to develop power systems able to collect and convert this energy into electricity. Many of these efforts were aimed at demonstrating the technical and economic feasibility of systems that integrate solar energy collection and concentration devices with well established power generation systems. Among these conventional technologies, the focus has always been on the utilization of gas turbines for their small footprint and low capital cost [1–5]. One of the most recent attempts to develop small scale solar power generators based on micro gas turbine technology is the OMSoP project (Optimised Microturbine Solar Power Generator), funded by the European Commission within the 7th Framework Programme [6]. The OMSoP consortium has already published many works related to this type of systems 3
[7–12]. Giovannelli [7, 8] presents a review of the current state of the art in the area of small-scale concentrated solar thermal power systems based on dish collectors. Lanchi et al. [9] present the experimental solar unit developed by ENEA (Italian National Agency for New Technologies, Energy and Suitable Economic Development) for the OMSoP project. Cerri et al. [10] propose the integration of solar dishes with advanced semi-closed cycles micro-turbines. Sanchez et al. [11] analyze the potential of selected markets for the worldwide commercial deployment of OMSoP systems. Gavagnin et al. evaluate the manufacturing, transportation and installation costs of the simple recuperated solar-only and hybrid systems in [12] and the economic and financial appraisal of the project for simple recuperated, intercooled and intercooled/reheated advanced layouts in [13]. Micro gas turbines (mGT) have power outputs in the range from a few kilowatts [14] to half a megawatt [15], even if this upper limit might change between 250 kW and 1 MW depending on the source. They typically include single stage radial turbomachinery with moderate pressure ratio (though higher pressure ratios are possible in larger engines in combination with axial flow machinery) and an internal heat recovery device (compact heat exchanger [14]) to enhance efficiency. These components are typically arranged in a single shaft configuration although multiple-shaft layouts have also been considered [16]. Solar micro turbines typically make use of parabolic dish collectors to collect and concentrate solar energy onto a receiver which in turn converts it into heat. The concentration ratio of these collectors is very high and enables the very high temperature that is needed to attain high efficiency [17]. With the aforecited OMSoP project, the Royal Institute of Technology in Stockholm (KTH) tested two different solar receiver prototypes: a cavity volumetric pressurized receiver with foam absorber [18, 19] and an impingement cavity receiver [20]. The integration of volumetric receivers in several applications such as solar systems for off-grid energy production [21] and polygeneration in rural areas [22], either in simple or combined cycle configuration [23], was studied by Aichmayer et al. whilst Wang et al. [24] investigated an integrated dish-mGT design using solar systems with impingement receivers. These activities add to the past work on these systems for space, military and civil power applications: Kesseli et al. calculated the performance of a micro turbine engine composed by stock turbocharger components in [25] while Dickey presented the experimental performance of a Capstone micro turbine integrated with a field of heliostats in [26]. More recently, LeRoux and Meyer 4
made use of a lumped-volume approach to simulate the performance of a small-scale dish-mTG system using data from standard off-the-shelf Garrett turbocharger technology and a model of open-cavity tubular receivers [27]. Semprini et al. also employed models of solar-only and hybrid mGT systems based on lumped volumes and turbomachinery performance maps taken from literature [28]. In contrast to these past works, which rely on generalized performance maps of turbomachinery or on existing compressors/turbines (engines derived from turbochargers), the current paper presents a two-step integrated procedure i) to design solar mGT systems by determining optimum turbomachinery geometries and performance maps, and ii) to simulate the off-design behavior in order to evaluate the highest annual production of electricity for a specific location. This integrated approach to the design and off-design analyses of solar mGTs allows for the generation of "ad hoc" designs for a specific location and for the calculation of more reliable performance values along a typical year of operation as compared to those calculated with the "traditional" approach. 2. Dish-mGT integrated solar systems Power generators based on integrated dish-mGT systems are mostly based on the simple recuperated Joule-Brayton cycle, Fig. 1, even if other configurations including intercooling and reheat have been proposed in the literature [10, 13, 29]. The parabolic dish is responsible for the heat supply and is a well established technology with many different designs having been tested in the past. Most of this experimental activity aimed at the integration in dish-Stirling systems [30–32] but there are also prototypes with micro turbines. A complete dish-mGT assembly based on an engine derived from a turbocharger was studied in the mid 1980s by NASA (National Aeronautics and Space Administration) in the Brayton Power System and Solar Advanced Gas Turbine Engine projects [33, 34]. Amsbeck et al. reported the testing of a solar-hybrid mGT at the Plataforma Solar de Almeria [35] and Dickey et al. published test results of an adapted Capstone mGT operated on solar energy at the Weizmann Institute [36]. Finally, Kesseli et al. reported tests carried out by Brayton Energy with a system including dish collectors, micro gas turbines and a compressed air storage system [37]. Most of these units make use of solar volumetric receivers because of the higher efficiency as compared 5
Figure 1: Single-shaft recuperative microturbine with integrated solar receiver: compressor (C), recuperator (R), solar receiver (S), turbine (T) and generator (G). to cavity receivers in either tubular or impingement configuration [38, 39]. The knowledge gained from these experimental activities is complemented by the thorough theoretical analysis exploring the advantages and disadvantages of using adapted turbochargers or small gas turbines designed from scratch [40–45]. In the recuperated Brayton-Joule cycle shown in Fig. 1, the available heat carried by the gases leaving the expander is used to preheat the air delivered by the compressor before this enters the combustor, with the aim to increase the thermal efficiency of the engine. This layout is best exploited when associated with low pressure ratios which enable the utilization of singlestage radial turbomachinery coupled to a solar receiver as a mere substitute for the combustor of a conventional mGT [16]. The flow diagram is as follows. Ambient air enters the compressor (C) where it is pressurized (1-2). This air stream then flows into the cold side of the counter-flow compact recuperator (R) where it is heated by the hot exhaust air flowing out from the turbine (2a-3a). Once preheated, the air enters the solar receiver (S) where it is heated up further by the solar energy collected by the parabolic dish and concentrated onto the focal point where the solar receiver is mounted. This component is a volumetric, pressurized receiver with a SiC foam absorber and a quartz glass window that lets solar energy in whilst reducing both pressure and convective heat losses. The concentrated solar beams entering the receiver heat the foam absorber which, in turn, raises the temperature 6
of air flowing through it (air acts as a coolant for the absorber). The air exiting the receiver flows into the turbine (T) where it is expanded (4-5) and then sent to the hot end of the recuperator where it is cooled down by the compressor delivery air before being released to the atmosphere (5a-6). When the available solar radiation exceeds a maximum value (upper threshold), a fraction of the total mass flow through the engine bypasses both sides of the recuperator, thus reducing the inlet temperature to the solar receiver (3) and avoiding overheating of the system. The electric generator (G) is mounted on the same shaft as the turbine and compressor, hence rotating at a very high, variable speed (in the range 100-150 krpm). This means that power electronics are required to ensure that voltage and frequency of the electric output are stable and in compliance with the requirements of the grid. Two technology levels of the mGT are considered here, corresponding to different values of turbine inlet temperature (TIT) and recuperator effectiveness (εrec,DP ): base-case (800°C-85%) and advanced system (900°C-90%). This choice is based on techno-economic considerations. Temperatures lower than 800°C would bring about a drastic efficiency drop whereas temperatures above 900°C would imply using more expensive ceramic materials in the turbine [16, 46]. Recuperator effectiveness lower than 85% would bring a too low internal heat recuperation whereas a value higher than 90% would imply a very heavy and expensive component [16, 47]. Figure 2 shows the thermodynamic cycles of both the base-case and advanced systems. The differences lay on the position of station 4 (TIT effect) and in the relative position of station 5 with respect to station 3 (effect of εrec,DP ). The main deign specifications of the system are summarized in Table 1, where the range of DNI (DNIDP ) and pressure ratio (rc,DP ) considered in the sensitivity analysis are also given. Main system specifications DNIDP 800 W/m2(sensitivity 400 W/m2-1000 W/m2) rc,DP 3 (sensitivity 2.5-4) ˙mair,DP 0.1 kg/s TITDP 800 °C(base) 900 °C(adv.)εrec,DP 85 %(base) 90 %(adv.) Tamb,DP 25 °C pamb,DP 101325 Pa fp,rec,c,DP 97.0 %fp,rec,h,DP 98.5 % fp,rcv,DP 96.0 %fp,in/out,DP 99.5 % ηmech,DP 99.0 %ηel,DP 90.0 % ∆Tturb,DP 5°C ns,t,DP 0.55 Table 1: Independent variable set (input parameters). 7
Figure 2: Temperature-entropy (left) and pressure-enthalpy (right) diagrams of the basecase and advanced systems. 3. Methodology The methodology used to find the optimum design and performance of the solar-mGT system is based on an integrated procedure which combines the design and off-design performances of the system. Both models are solved with a modular-sequential approach which relies on the conservation of mass, momentum and energy and on established correlations to characterize components performance and efficiency. The working fluid is air which is considered to be dry real gas with the thermodynamic properties provided by Coolprop®[48]. The complete model is implemented in Matlab®on the assumption that all processes take place in equilibrium [49]. The first stage of the design model consists in calculating the working cycle and the characteristics of the main system components. To this end, both one dimensional (1-D) and zero dimensional (0-D) approaches are used: radial turbomachinery (1-D), solar receiver (0-D), recuperator (0-D) and solar dish (0-D). The design space is limited by a sufficiently large range of pressure ratios (2.5-4, see Section 5.1) wherein potential designs are explored in order to attain the highest solar-to-electric efficiency at the design point. The basic geometry of the turbomachines, which includes the meridional flow path and blades, is then used to produce the corresponding performance maps that will later be used by the off-design model (see Fig. 4) to evaluate the behavior of the system when subjected to boundary conditions different from the design ones. This off-design model relies on a suitable control strategy which ensures the safe operation of the system within a certain range of 8
boundary conditions. 3.1. Design model The structure of the design model shown in the flowchart in Fig. 3 is common to the base-case and advanced systems (Section 2) and the input data to the model are listed in Table 1. Upon calculation of the working cycle with the input data in Table 1, the "Thermodynamic cycle 1" module calculates the inlet conditions (pressure and temperature) to each turbomachinery along with the corresponding turbine expansion ratio (re,DP =p4/p5) for a given pressure ratio of the compressor (rc,DP =p2/p1). Pressure losses across the solar receiver, recuperator and inlet/outlet ducts are taken into account by means of the pressure loss factors (fp=pout/pin) in Table 1. With this information, the turbomachinery 1-D design modules ("Turbine" and "Compressor") calculate the draft geometries of turbine and compressor, also providing their isentropic efficiencies and rotational speed. These data are then used to complete the simulation of the thermodynamic cycle by calculating the outlet states of each turbomachinery and the complete heat balance of the recuperator. With the thermodynamic cycle calculated fully, the recuperator is designed using the ε−NTU approach to calculate the Number of Transfer Units (NTU). This provides the total heat transfer area of the selected counter-flow configuration that yields the target effectiveness specified originally. The tools to design the solar subsystem include the parabolic dish and receiver modules. The aperture (dish) and window (receiver) area of these elements are optimized for the nominal conditions obtained in the design model of the mGT by minimizing of heat losses. Inputs to the parabolic dish model are the design DNI and the heat input to the receiver with which the receiver model calculates the air outlet temperature (TIT). Two iterative loops are finally used to optimize the aperture area of collector and receiver: 1. The inner loop searches for the optimum size of the receiver. This stems from a balance between heat input from the collector and heat losses to the environment. 2. The outer loop corrects the dish aperture area until the receiver outlet temperature is equal to the specified TIT at the rated conditions. A detailed description and the equations of the design models of the mGT components are given in Appendix A. 9
individual models of the constituents were previously validated against theoretical or experimental data and hence the model of the complete system is expected to provide trustful results. In particular: •The performance models of the compressor and turbine are well known and have been validated by Aungier against a large set of experimental data taken from real applications [52, 53]. Moreover, the specific models of the compressor developed for the solar application have been validated in a previous work for air and sCO2[54]. For the turbine, a specific validation against experimental data was done by NASA, as a function of the relative size of the clearance gap. The total-to-total and total-to-static efficiencies at the design point obtained experimentally [55], the results of the model and the corresponding errors are shown in Table 2. δcl,rel Ref [55] Model Error Total-to-total efficiency 0.25% 89.2% 90.2% 1.05% 3% 84.7% 86.0% 1.62% 7% 79.3% 82.3% 3.64% Total-to-static efficiency 0.25% 87.0% 84.1% 3.51% 3% 82.8% 80.5% 2.88% 7% 77.7% 77.0% 0.87% Table 2: Validation of turbomachinery design models. •The design and off-design models of the solar components (parabolic dish and volumetric receiver) have both been validated against data obtained at the test rig at the Royal Institute of Technology in Stockholm (KTH) [18, 19]. •The off-design model of the electric generator is derived from experimental data obtained by ENEA directly [8]. •The properties of dry air with real gas behavior are computed with Coolprop®whose accuracy is widely acknowledged within the industrial and scientific communities [48]. 5. Results This last Section presents three different sets of results: 16
1. The results obtained by running the design model for the base-case (TIT = 800°Cand εreg,DP = 0.85) and advanced (TIT = 900°Cand εreg,DP = 0.90) systems for a design DNI of 800 W/m2and an air flow rate of 0.1 kg/s (see Table 1). In this analysis, the sensitivity to the rated pressure ratio is also assessed. 2. The off-design performance maps and the results of the annual simulation of the two systems mentioned in the previous bullet point. 3. The results of a sensitivity analysis with respect to the design DNI for three different locations (Beijing, Seville and San Diego). 5.1. Results at the design point The following performance metrics are used to characterize the aforecited systems: •The global (solar-to-electric) efficiency (ηglobal) is defined as the ratio from net electric output (Pel) to total heat input to the system (DNI ·Adish), Eq. (1). It can be applied to either design or off-design conditions. •The specific output can be referred to the air mass flow rate ( ˆ Pel, Eq. (2)) or to the aperture area of the parabolic dish ( ˆ Psolar,DP , Eq. (3)). It can also be applied to either design or off-design conditions. •The efficiencies of the parabolic dish collector (ηdish,DP ), solar receiver (ηrcv,DP ) and mGT (ηmGT,DP ), defined by Eqs. (4-6). ηglobal =Pel DNI ·Adish (1) ˆ Pel =Pel ˙m1 (2) ˆ Psolar =Pel Adish (3) ηdish =˙ Qint,DP DNIDP ·Aa,dish (4) ηrcv,DP =˙ Qmgt,DP ˙ Qint,DP (5) 17
ηmGT,DP =Pel,DP ˙ Qmgt,DP (6) A complete sensitivity analysis of system and component performance against pressure ratio (rc,DP ) is shown in Fig. 9 for the base-case and advanced systems (green and blue lines respectively). Firstly, it is worth noting that both systems achieve maximum ηglobal for a pressure ratio of about 3.2, even if a higher pressure ratio would have been expected for the advanced case. This is mostly because of the higher recuperator effectiveness of the advanced case which promotes a lower pressure ratio to exploit the recuperative potential fully, Table 1. The efficiency of the parabolic dish is independent from rc,DP as shown in Section Appendix A.5, whereas the efficiency of the receiver increases slightly with pressure ratio because of the higher density of air. Shaft speed also increases because more compression work is needed whereas the aperture areas of dish and receiver increase with rc,DP due to the higher heat input that comes about because of the decreasing inlet temperature to the receiver (lower turbine exhaust temperature). In the light of the information in Fig. 9 and in order to maintain a feasible shaft speed of some 130 krpm, a lower pressure ratio equal to 3 is finally selected, even if the rated efficiency shown is slightly lower than the optimum value. Table 3 summarizes the dependent variables calculated in the design process. The base-case system produces more than 7 kWewith an aperture area of 50 m2while the advanced system generates almost 9 kWe(about 25% more) with a 3% larger aperture area only. This power gain is mainly due to the higher TIT and reg,DP which raise the mean temperature of heat addition to the working cycle, transformations 30 −40and 300 −400 in Fig. 2. 18
Figure 9: Global (solar-to-electric) efficiency vs. pressure ratio and specific power (above), turbomachinery total-to-total efficiencies vs. pressure ratio (center) and shaft speed and dish/receiver aperture areas vs. pressure ratio (below). Base-case and advanced systems shown in green and blue respectively. 19
Base-case system Pel,DP 7.19 kWeηs,t,DP 82.44 % Adish (ddish) 50.0 m2(8.0 m) ηs,c,DP 76.52 % Arcv (drcv) 167 cm2(14.6 cm) ηdish,DP 90.35 % HT Arec 5570 m2ηrec,DP 82.79 % NT Urec,DP 5.45 ηmGT,DP 24.03 % NDP 129690 rpm ηglobal,DP 17.97 % ˆ Psol,DP 0.144 kWe/m2ˆ Pel,DP 71.9 kWe/(kg·s) Advanced system Pel,DP 8.96 kWeηs,t,DP 81.64 % Adish (ddish) 51.5 m2(8.1 m) ηs,c,DP 76.97 % Arcv (drcv) 171 cm2(14.8 cm) ηdish,DP 90.34 % HT Arec 8757 m2ηrec,DP 82.04 % NT Urec,DP 8.58 ηmGT,DP 29.34 % NDP 132540 rpm ηglobal,DP 21.74 % ˆ Psol,DP 0.174 kWe/m2ˆ Pel,DP 89.6 kWe/(kg·s) Table 3: Main design specifications of the base-case and advanced systems for 800 W/m2 and the optimum rc,DP . 5.2. Results of the annual simulations The off-design model shown in Section 3.2 is used here to calculate the solar-mGT performance maps linking power output and efficiency to the DNI at given ambient temperatures. These maps are then utilized to evaluate the annual yield (production of energy) for given annual distributions of DNI and ambient temperature in a specified location. In order to analyze the results of the off-design model, the following three additional performance metrics are introduced: •The mean annual conversion efficiency (¯ηglobal, Eq. (7)) is the ratio from the net annual electricity (Eel,net) to the available solar energy input (Esol) over the year. It must be noted that the latter may differ from the solar energy actually harvested by the system (Qsol) due to periods when the system is not in operation because of the very high or very low DNI:DNI < DNIcut−in or DNI > DNIcut−off , Fig. 6. •The capacity factor of the system (fcapacity, Eq. (8)) is the ratio from the annual yield (Eel,net) to the electric energy that would be produced if the system worked at the nominal output (Pel,DP ) throughout the year (8760 hours). •The dumped solar energy factor fdumped, Eq. (9), is the ratio from the solar energy that is available but not harvested by the system (Esol − Qsol) to the available solar energy input (Esol). This metric is used to 20
quantify the fraction of available solar energy that cannot be harvested because the system is already running at full or minimum capacity. ¯ηglobal =Eel,net Qsol (7) fcapacity =Eel,net Pel,DP ·8760 (8) fdumped = 1 − Esol −Qsol Esol (9) Figure 10 shows the performance maps obtained for the base-case (green) and advanced (blue) systems. The inability to absorb a very high radiation becomes evident in the upper charts and translates into a drastic drop in efficiency (bottom charts) due to a large fraction of the available solar energy that is dumped off by the system at high DNI. Annual simulations are performed for three selected locations -Beijing (China), Seville (Spain) and San Diego (USA)- for which hourly values of DNI and ambient temperature are obtained from the System Advisory Model software [56]. This information is shown in Fig. 11, whose left chart shows the number of Sun hours (horizontal axis), peak DNI (vertical axis) and annual solar energy available (area subtended by the curve). Similar information is shown for ambient temperature on the right hand side of Fig. 11. According to the results shown in Table 4, the highest yield is obtained in San Diego where the base-case system achieves 15.87% annual conversion efficiency and 24.77% capacity factor, with just 10.69% of the available solar energy being dumped off the system. Seville shows similar performance but, in contrast, the efficiency in Beijing is just 11.13% and the capacity factor is 10.51%, mainly due to the high amount of dumped solar energy (more than 37%). It must be noted that the high fdumped in this location is not due to frequent overflows of solar energy (DNI > DNIcut−off ) but to long periods of time with DNI lower than the cut-in value (DNI < DNIcut−in). Finally, when the advanced systems are considered, these yield similar performances in terms of dumped solar energy and capacity factors whereas the annual efficiency is around 2.7-3.5 percentage points higher in all locations. 21
Figure 10: Performance maps of the base-case (left) and advanced (right) systems: net power output vs. DN I (above) and global (solar-to-electric) efficiency vs. DN I (below) Figure 11: Duration curves of hourly DNI (left) and ambient temperature (right) of the three selected locations in a Typical Meteorological Year (provided by SAM [56]). 22
Base-case system Locations Beijing Seville San Diego DNIDP [W/m2] 800 800 800 Esol [kWh] 59494 88676 98304 Qsol [kWh] 37223 76273 87797 Eel,net [kWh] 6622 13384 15605 ¯ηglobal 11.13% 15.09% 15.87% fdumped 37.43% 13.99% 10.69% fcapacity 10.51% 21.24% 24.77% Advanced system Locations Beijing Seville San Diego DNIDP [W/m2] 800 800 800 Esol [kWh] 61257 91304 101217 Qsol [kWh] 39424 79669 91087 Eel,net [kWh] 8463 16938 19581 ¯ηglobal 13.82% 18.55% 19.35% fdumped 35.64% 12.74% 10.01% fcapacity 10.78% 21.58% 24.95% Table 4: Performance of the base-case and advanced systems designed for 800 W/m2in a Typical Meteorological Year (TMY). 5.3. Sensitivity analysis. Impact of design DNI Sections 5.1 and 5.2 have shown that largely different performances can be obtained when the same system is operated under dissimilar boundary conditions. For this reason, a sensitivity analysis is now performed in order to assess to what extent the location impacts the reference value of DNI that is convenient to consider in the design process; i.e., DNIDP that yields highest annual efficiency ¯ηglobal, Eq. (7). This metric depends on the hourly distribution of DNI and on the performance maps of the system. The sensitivity analysis is performed following the procedure shown in Fig. 12. Mass flow rate and turbine inlet temperature are set to their rated values (0.1 kg/s and 800/900 °C for the base-case/advanced systems respectively) and the value of DNI at the design point (external loop) is changed in the range of interest (400-1000 W/m2). This means that the micro turbine design remains unaltered with respect to the original design for DNIDP =800 W/m2whereas the solar subsystem (parabolic dish and volumetric receiver) is re-sized according to the new value of DNIDP . The calculations for each DNIDP are based on non-dimensional performance maps of the system, obtained from those shown in Section 3.2 for the reference case at 800 W/m2. These maps shown in Fig. 10 are then dimensionalized again by merely multiplying the horizontal scale by the corresponding value of DNIDP . Even if the procedure is not utterly accurate, 23
Figure 12: Procedure to search for the optimum DN IDP . the error incurred does not bring about significant deviations in terms of annual system performance inasmuch as the efficiency of the parabolic dish is rather independent from its size within reasonable limits (see Eqs. (A.15) to (A.16)), while the efficiency of the receiver is only slightly affected by DNI for given TIT and Tamb. For the sake of verification of this statement, the performance maps obtained with the non-dimensional approach and those built using the complete off-design procedure in Section 3.2 are shown in solid blue and dotted white lines in Fig. 13, confirming that there is very good agreement in all cases. The non-dimensional performance maps of the base-case and advanced systems are shown in Fig. 14 where the non-dimensional power output is plotted against relative DNI for various ambient temperatures. The resulting variations of ¯ηglobal,fcapacity and fdumped of the base case and advanced systems when these performance maps are used are illustrated in Fig. 15. The lower optimal DNIDP is found for Beijing (660 W/m2for the base-case system and 610 W/m2for the advanced system) whilst the highest DNIDP,opt corresponds to San Diego (815 W/m2for both systems), with Seville laying 24
Figure 13: Validation of the performance maps used in the search for the optimum DN IDP : maps calculated with the complete off-design procedure (white dots) and non-dimensional maps (blue line). Figure 14: Non-dimensional output of the base-case (top) and advanced (bottom) systems vs. relative DN I for different ambient temperatures. 25
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[70] M. Röger, C. Rickers, R. Uhlig, F. Neumann, C. Polenzky, Infraredreflective coating on fused silica for a solar high-temperature receiver, Journal of Solar Energy Engineering 131 (2) (2009) 021004. [71] J. R. Welty, C. E. Wicks, G. Rorrer, R. E. Wilson, Fundamentals of momentum, heat, and mass transfer, John Wiley & Sons, 2009. [72] W. B. Stine, R. W. Harrigan, Solar energy fundamentals and design, John Wiley and Sons, Inc., New York, NY, 1985. [73] W. B. Stine, M. Geyer, Power from the Sun, Power from the sun. net, 2001. [74] J. A. Harris, W. S. Duff, Focal plane flux distributions produced by solar concentrating reflectors, Solar Energy 27 (5) (1981) 403–411. [75] J. Noall, M. Forsha, Off-design turbomachinery performance mapping, Barber Nichols Inc., Internal Program Report. [76] A. J. Glassman, Turbine design and application. nasa sp-290, NASA Special Publication 290. Appendix A. Design models This Section presents the equations and solving procedures implemented in each design module of the flowchart in Fig. 3. Appendix A.1. Thermodynamic cycle The modules calculating the design thermodynamic cycle in Fig. 3 (“Thermodynamic cycle 1 and 2’’) are based on the application of mass and energy conservation and component efficiencies [57]. Thus, the outlet conditions from compressor and expander are calculated from the total-to-total pressure ratios and the isentropic efficiencies whilst the inlet and outlet states of the recuperator are computed from a fixed effectiveness and pressure loss factor (εreg,DP ,fp,cold,DP and fp,hot,DP in Table 1). With this information, the model calculates all the thermodynamic states in Fig. 1 along with the shaft output for a given mass flow rate at compressor inlet ( ˙m1=0.1 kg/s). The net electric output is then calculated by merely applying electric and mechanical efficiencies. 37
Appendix A.2. Turbomachinery The design modules of compressor and turbine provide the total-to-total isentropic efficiencies and the rotational speed of the sized stages [58], based on the one-dimensional approaches proposed by Aungier in [52] and [53]. In the main, this approach assumes constant flow field variables (velocity, temperature and pressure) at each cross-section of the flow passage (channel). These variables are obtained from steady-state mass, energy and momentum balance equations computed along the mean stream surface using empirical fluid dynamics and total pressure loss correlations. A boundary layer model is applied to take into account the total pressure loss due to skin friction between the fluid and passage walls, with the resulting variation of Reynolds number along the mean stream surface being used to evaluate the entropy rise and, in turn, the isentropic efficiency. The matching of compressor and turbine is initiated in the turbine assuming a reference specific speed ns,t=0.55 on the based on recommendations by Rodgers [59] and Aungier [53], Eq. (A.1). Based on this value, it is possible to calculate the rotational speed that yields highest turbine efficiency [60, 61]. This is then used along with the spouting velocity c0,is (velocity obtained in a total-to-static isentropic expansion) to calculate the tangential speed of the blade (utip,t) and the corresponding rotor diameter (dtip,t), Eq. (A.2) as described by Aungier [53]. ωDP =ns,t ∆h0.75 s,t √˙vout (A.1) νts,t =utip c0,is = 0.737 ·n0.2 s,t (A.2) The rotational speed of the compressor is the same as that of the expander and it can be used to calculate the specific speed (ns,c) and diameter (ds,c) of this machine, Eqs. (A.3,A.4). This information is obtained by interpolating the corresponding nsvs. dschart for maximum compressor efficiency (Cordier line, shown dashed red in Fig. A.1) in the range of application of radial turbomachinery: 50<ns,c<100 [62]. The specific diameter (ds,c) so obtained is used to calculate the tip diameter of the impeller (dtip,c). ns,c =ωDP √˙vin ∆h0.75 s,c (A.3) 38
Figure A.1: Specific speed vs. specific diameter diagram of a compressor showing the Cordier line for radial stages in dashed red. Adapted from [62]. ds,c = 2.865 ·n−0.946 s,c =dtip ∆h0.25 s,c √˙vin (A.4) The sizing of the turbine is performed in the following order: rotor, nozzle, inlet volute and exhaust diffuser. For these elements, a draft geometry is produced from a set of default design specifications in combination with empirical correlations based on the reference specific speed, as suggested by Aungier [53]. These specifications include the spouting velocity of the stage, specific diameter of the rotor, inlet flow angle, number, chord and thickness of the blades and inlet-to-outlet radii ratio of the nozzle. The main design steps applied to these data are summarized below, as described in [53] where more details can be found: •The main geometrical parameters of the rotor are calculated from ns,t and dtip,t under the assumption that inlet velocity is radial (relative rotor inlet angle is 90°): –The meridional plane of the turbine is sized so as to minimize the variation of area between the inlet and outlet sections under the constant mass flow rate restriction, Fig. A.2. –The number, mean line geometry and thickness distribution of the blades is calculated with empirical correlations. –The feasibility of the resulting geometry is verified against the specific guidelines proposed by Aungier [53]. 39
•In order to size the nozzle, the minimum number of blades needed to yield radial relative flow at the inlet to the wheel and, at the same time, a blade loading lower than 1 is calculated. •An elliptical configuration is considered for the volute, where the variation of cross sectional area comes determined by mass conservation, a constant size parameter SP=1 and angular momentum conservation at nozzle inlet. SP =√˙vout ∆h0.25 s = 1 (A.5) •The design of the exhaust diffuser is obtained from empirical correlations on the assumptions that the ratio between outlet and inlet areas is equal to 1.5 and that the divergence angle is 11°. The aforedescribed procedure generates a draft geometry for the actual design point, yielding a certain mass flow rate and total-to-total expansion ratio. These values are then used to correct the design until the target values are attained. Once the final design is obtained, the corresponding performance map is produced by merely calculating the performance of the expander for different sets of boundary conditions, including the specific conditions for which sections of the machine get choked. The compressor design process does not start from a set of specifications but it is carried out directly by means of the empirical performance model proposed by Aungier [52]. In this, guessed values of the total-to-total isentropic efficiency and total pressure loss coefficient (from rotor inlet to volute outlet) are initially assumed and the geometry of each component of the compressor is evaluated as follows: •The impeller inlet section is sized in order to minimize the relative Mach number at the shroud, whilst the outlet diameter is influenced by the blade exit angle as a result of a trade-off between stage work and distortion, and slip factors for each dtip,c; this is shown in Eqs. (A.3,A.4) and in Fig. A.2. The number of blades results from the minimum value yielding a blade loading lower than 0.9. •The diffuser can be of the vaned or vaneless type. In the former case, the number of vanes, the area ratio and the divergence angle result from an optimization process to yield maximum efficiency with a total load lower than 0.3. 40
Figure A.2: Meridional flow passage of the compressor impeller (left) and turbine wheel (right) for the base-case (above) and advanced (below) systems. •The outlet radius of the volute is calculated iteratively by fixing a size parameter of 1.05. The radius distribution is then obtained from continuity by keeping the size parameter constant. To properly take into account the strong influence of the clearance gap between rotor and shroud (casing) [63, 64] the following definition is used: δcl =δcl,ref ·bblade bblade,ref 0.6 ,(A.6) where the reference blade height is bblade,ref = 5 mm and the reference gap δcl,ref is 0.4 mm and 0.3 mm for turbines and compressors, respectively. Finally, the effect of roughness is accounted for with a simple skin friction model based on boundary layer analysis in which a peak-to-valley roughness of 1 µm is assumed [65]. The performance maps of compressor and turbine for the base-case and advanced systems are shown in Fig. A.4. These maps show total-to-total isentropic enthalpy change and isentropic efficiency versus mass flow rate for shaft speeds ranging from 70% to 115% of the design point value. 41
Figure B.1: Electric efficiency of generator vs. shaft work and rotational speed (left) and maximum shaft power vs. rotational speed (right). Scales are non-dimensional. than upstream. The variations of the global heat transfer coefficient with the mass flow rate are evaluated using Eq. (B.7). U=UDP ·˙m ˙mDP 0.8 (B.7) The pressure losses of recuperator, solar receiver and inlet/outlet ducts are varied according to Eq. (B.8). ∆p= ∆pDP ·˙m ˙mDP 1.21 · ρDP ρ(B.8) 48