Elsevier

Energy

Volume 77, 1 December 2014, Pages 771-782
Energy

A numerical study of parabolic trough receiver with nonuniform heat flux and helical screw-tape inserts

https://doi.org/10.1016/j.energy.2014.09.049Get rights and content

Highlights

  • Incidence angle was analyzed to accurately simulate the heat flux distribution.

  • Transversal angle (β) obviously affects the Tmax and ΔT on absorber tube.

  • Helical screw-tape inserts within a receiver greatly decreases Qloss, Tmax and ΔT.

Abstract

Effect of solar incidence angle was analyzed in order to accurately simulate the heat flux distribution around the absorber tube outer surface. Helical screw-tape inserts was proposed to homogenize the absorber tube temperature distribution and improve the thermal efficiency. Three dimensional periodical models of flow and heat transfer were established and solved with the heat flux of different transversal angle (β). The results show that β affects the flux distribution more greatly than longitudinal angle (φ). Transversal angle (β) of 11.567 mrad increases the relative change of heat loss (Qloss) as inlet temperature rises, and also increases the maximum temperature on absorber tube (Tmax) and the maximum circumferential temperature difference (ΔT). But its effect reduces as Reynolds number rises. Within the range of studied Re, the helical screw-tape inserts of given geometrical parameters greatly reduce the Qloss, Tmax and ΔT, which indicates that helical screw-tape inserts is a feasible way to enhance the heat transfer inside the receiver.

Introduction

PTC (Parabolic trough collector) can be used on a large scale in solar thermal power generation [1], [2], as well as in refrigeration [3] and seawater desalination [4]. In the PTC, solar radiation is reflected and concentrated on a linear receiver in focal line. HTF (Heat transfer fluid) flowing through the receiver absorbs the heat for further power generation or other industrial heating. The thermal performance of PTC and receiver has been widely researched by many scholars [5], [6], [7], [8], [9], [10]. Most of the studies that probe into the theoretical calculations neglect the incidence angle of solar rays. Actually, the incidence angle determines the heat flux distribution on the absorber tube outer surface. Fig. 1 shows that the incidence angle (θ) can be decomposed into two components on two orthogonal planes: longitudinal angle (φ) and orientation angle error or transversal angle (β). In a collector with ideal concentration, solar incidence that lies in the longitudinal plane causes a circumferentially-nonuniform heat flux on the absorber tube. The nonuniform heat flux is normally treated as an important boundary condition of heat transfer in the receiver [11], [12]. More accurate calculated results were obtained when the nonuniform heat flux rather than a uniform heat flux was taken into account [13], [14]. The nonuniform heat flux also causes thermal stress in the absorber tube, leading to breaking risks of bellows [15], [16] and limiting the achievable temperature of selective film that is coated on the tube external surface [17]. Wind or inherent error of control scheme [18] may cause an overall deflection of collector and consequently leaves the receiver into a defocus status where the heat flux is more nonuniform. EuroTrough consortium estimates that tracking error using today's shadow-band technology is about 2 mrad and that wind-induced tracking error is about 4 mrad given a 5 m/s average wind [19]. So both the temperature distribution and thermal performance of a receiver with unsatisfactory tracking may be worse than with ideal concentration, especially for a PTC with long-term operations. However, the influence of incidence that deviates from the longitudinal plane on heat transfer has not been reported.

Improvement of thermal performance and homogenization of temperature distribution on the absorber tube outer surface can be achieved simultaneously by heat transfer enhancement inside the tube. Many enhancement forms [20], [21], [22], [23], [24], [25] have been put forward in the receivers, most of which are non-inserts and commonly used in heat exchangers. Service experiences of those non-inserts shows various drawbacks: impurities, great pressure loss and inconvenience for manufacture. For existing receivers, heat transfer enhancement via suitable inserts is favorable. Twisted tape is the most common inserts that enhances the heat transfer, and its performance in a receiver has been recently investigated [26]. Helical screw-tape is an improvement of the twisted tape and can be easily manufactured by coiling up annealed copper on a mandrel with a helical groove [27]. Comparing with twisted tape, helical screw-tape makes only part of in-tube fluid flow spirally by using less metal, and consequently avoids overmuch pressure loss [28]. More importantly, the screw-tape provides excellent performance at low Reynolds number (Re) and prevents the deposition of scaling [27].

In this paper, the performance and temperature around the absorber tube outer surface were simulated and analyzed by considering various conditions including solar incidence angle and helical screw-tape inserts. First, the heat flux around the absorber tube was obtained applying MCRT (Monte Carlo ray tracing) method and was simplified. Then, the heat flux of different transversal angle (β) was used as heat input to periodical three-dimensional models. Flow and heat transfer in the receiver with/without inserts were simulated. Collector and receiver from CAMDA New Energy Equipment Co., Ltd were used (see Table 1 for parameters) in the models. Flow rates in the simulations were about 1 order below the regimes experienced in some practical applications, because the real flow rate in the CAMDA solar field that is small and lacks sufficient solar irradiance must be reduced to get high outlet temperature. Preliminary studies of the incidence angle and the inserts may provide a reference for receiver performance and for design of working conditions in solar field.

Section snippets

Program and validation of Monte Carlo ray tracing

MCRT (Monte Carlo ray tracing) method which assumes solar rays as independent photons is applied to simulate the heat flux distribution with different incidence angle [29]. A program for LHF (local heat flux) around the tube was written and implemented in MATLAB (see Fig. 2), where a dimensionless LCR (local concentration ratio) and direct normal insolation (Ib) in the plane perpendicular to incidence were used to express LHF [30]: LCR = LHF/Ib. Each photon in the program represented a constant

Description of heat transfer and flow in receiver

Fig. 6 shows the cross section of a receiver with SAT-PTR (smooth absorber tube) and corresponding thermal network. The heat transfer in radial direction is complicated [36].The selective coating deposited on the absorber tube outer surface absorbs the concentrated solar radiation and converts it into heat. Some heat on the tube outer surface is conducted to the tube inner surface and then taken away by HTF through convection. Other heat is transferred to the glass envelope through radiation.

Results and discussion

The maximum temperature on absorber tube outer surface (Tmax) and the difference between the maximum and the minimum (ΔT = Tmax − Tmin), are important factors for receiver's technical feasibility such as stability of absorbing coating and strength of glass and steel tubes. Therefore, the primary points of interest in the calculated results are the influences of various factors such as working conditions, screw-tape inserts, and different flux distribution by different β on heat loss (Qloss), T

Conclusions and outlook

MCRT method was employed to simulate the heat flux distribution. Effect of solar incidence angle on heat flux distribution was analyzed. The heat loss (Qloss) of a receiver, the maximum temperature (Tmax) on absorber tube outer surface and the maximum circumferential temperature difference (ΔT) are investigated. Various working conditions, including inlet temperature, mass flow rate, irradiation level, helical screw-tape inserts and different flux distribution by different β, are considered as

Acknowledgments

This work is financially supported by the International Science & Technology Cooperation Program of China (No.2012DFG61930) and by a grant from the National High Technology Research and Development Program of China (No.2012AA050601).

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