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Frontiers in Energy

ISSN 2095-1701

ISSN 2095-1698(Online)

CN 11-6017/TK

邮发代号 80-972

2019 Impact Factor: 2.657

Frontiers in Energy  2021, Vol. 15 Issue (2): 513-528   https://doi.org/10.1007/s11708-019-0638-7
  本期目录
Thermal performance of a single-layer packed metal pebble-bed exposed to high energy fluxes
Shengchun ZHANG1, Zhifeng WANG1(), Hui BIAN2, Pingrui HUANG1
1. Key Laboratory of Solar Thermal Energy and Photovoltaic System, Chinese Academy of Sciences, Beijing 100190, China; Institute of Electrical Engineering, Chinese Academy of Sciences, Beijing 100190, China; University of Chinese Academy of Sciences, Beijing 100190, China; Beijing Engineering Research Center of Solar Thermal Power, Beijing 100190, China
2. Lanzhou University of Technology, Lanzhou 730050, China
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Abstract

It is difficult to accurately measure the temperature of the falling particle receiver since thermocouples may directly be exposed to the solar flux. This study analyzes the thermal performance of a packed bed receiver using large metal spheres to minimize the measurement error of particle temperature with the sphere temperature reaching more than 700°C in experiments in a solar furnace and a solar simulator. The numerical models of a single sphere and multiple spheres are verified by the experiments. The multiple spheres model includes calculations of the external incidence, view factors, and heat transfer. The effects of parameters on the temperature variations of the spheres, the transient thermal efficiency, and the temperature uniformity are investigated, such as the ambient temperature, particle thermal conductivity, energy flux, sphere diameter, and sphere emissivity. When the convection is not considered, the results show that the sphere emissivity has a significant influence on the transient thermal efficiency and that the temperature uniformity is strongly affected by the energy flux, sphere diameter, and sphere emissivity. As the emissivity increases from 0.5 to 0.9, the transient thermal efficiency and the average temperature variance increase from 53.5% to 75.7% and from 14.3% to 27.1% at 3.9 min, respectively. The average temperature variance decreases from 29.7% to 9.3% at 2.2 min with the sphere diameter increasing from 28.57 mm to 50 mm. As the dimensionless energy flux increases from 0.8 to 1.2, the average temperature variance increases from 13.4% to 26.6% at 3.4 min.

Key wordspacked bed    solar thermal power plants    high heat fluxes    radiative heat transfer
收稿日期: 2018-09-26      出版日期: 2021-06-18
Corresponding Author(s): Zhifeng WANG   
 引用本文:   
. [J]. Frontiers in Energy, 2021, 15(2): 513-528.
Shengchun ZHANG, Zhifeng WANG, Hui BIAN, Pingrui HUANG. Thermal performance of a single-layer packed metal pebble-bed exposed to high energy fluxes. Front. Energy, 2021, 15(2): 513-528.
 链接本文:  
https://academic.hep.com.cn/fie/CN/10.1007/s11708-019-0638-7
https://academic.hep.com.cn/fie/CN/Y2021/V15/I2/513
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Fig.10  
Equation name Equation Equation number
Energy equation in each sphere ρ s, ips, ic Ts,iτ= 1 r2r(λs,ir2Ts,i r )+1r2sin?2θ φ(λs,i Ts,i φ)+1r2sin?θ θ(λ s,isin?θTs,iθ) (11)
Initial condition T s,i|τ= 0= Ts0 (12)
Boundary condition λ s,iTs,i r |r=0=0 (13)
λ s,iTs,i r |r=R=qihs(Ts,i|r=RTa)+ EiA i (14)
Convective heat transfer coefficient h s=λfNuLL (15)
NuL=0.228 Re?L0.731? Pr?1/3 [29] (16)
Wall energy equation ρ w,icpw,i Tw,i τ= λw,i 2Tw,ix 2 (17)
Initial condition T s,i|τ= 0= Tw0 (18)
Boundary condition λw ,iTw,ix| x=0=qi hw(T w,i|x=0Ta)+EiAi (19)
λ w,iTw,i x |x=l=ha(TaT w,i|x= l) (20)
Convective heat transfer coefficient hw=0 (21)
Thermal radiation calculation A iqin,i= j= 1NAjFj, iqo,j (22)
qo,i=( 1εi)qin,i+εiσTi 4 (23)
qi= qin,i qo,i (24)
Tab.1  
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Fig.13  
Fig.14  
Fig.15  
Fig.16  
Fig.17  
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Fig.19  
Fig.20  
A Area/m2
Cp Specific heat/(J?(kg?K)–1)
D Variance
E Energy absorbed from the external irradiation/J
Eray Energy carried by each beam/J
F View factor
H Receiver height/m
HH Half of the difference between the center distance between two spheres and the sum of two spheroid radii/m
ict, NN Counter
l Wall thickness/m
m Mass/kg
n Total number of spheres in the receiver
N Number
Nu Nusselt number
O Center of the sphere
R Sphere radius/m or random number
Re Reynolds number
r Radial distance/m
r1 Contact radius between the spheres
rij Characteristic radius between particles
q Heat transfer between radiant surfaces
T Temperature/K
r Density/(kg?m–3)
q Polar angle/rad
j Azimuthal angle/rad
Pr Prandtl number
V Volume/m3
W Receiver width/m
x, y, z Coordinates
l Thermal conductivity/(W?(m?K) –1)
a Absorptivity
e Emissivity
h Thermal efficiency
t Time/min
s Stefan-Boltzmann constant/(W?(m–2?K–4))
L Bench height/m
i, j Indices
min Minimum
max Maximum
f Fluid
av Average
k Time step
w Wall
a Ambient
S Sphere
in Incidence
o Outgoing
t All radiant surfaces
gap Gap between the spheres
s0, w0 Initial
  
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