experimental investigations on top loss coefficients
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Abstract—The flat plate collector is one of the most widely used
device for harnessing the solar energy. The measurement of the flat
plate collector performance is the collector efficiency. The collector
efficiency is the ratio of the useful energy gain to the incident solar
energy over a particular period of time. The useful energy gain in
turn depends on the energy loss from the top surface of the collector
both due to convective & radiative heat transfer processes. The losses
from the bottom and from the edges of the collector do exist but their contribution is not as significant as the losses from the top. Hence
investigations are carried out to study the losses by changing the
collector tilt to determine the top loss coefficient.
Keywords—Collector, Tilt angle, Losses, Top loss coefficient
I. I NTRODUCTION
HE technology of harnessing the solar energy has reached
to the state of commercialization on mass scale. The
greatest advantage of using solar energy is that it is an
inexhaustible and pollution free source of energy. The Lord
Sun gives approximately 1.8 x 1011 MW power, which is
many thousand times higher than the present consumption rateon earth. This makes it one of the most promising of the
unconventional sources of energy.
II. NOMENCLATURE
A p Area of absorber plate, m2
Qs Losses of heat from sides, W
Q b Losses of heat from bottom, W
Qt Losses of heat from top, W
Ein Energy input, W
β Collector tilt angle, degrees
N No. of covers
σ Stefan Boltzmann constant 5.67 x 10-8 W/m2K -4
∈ p Emissivity of plate
∈c Emissivity of cover
T b Temperature of bottom cover of collector, K
Tc1 Mean temperature of 1st cover, K
Tc2 Mean temperature of 2nd cover
Tc Thickness of cover, m
M. K. Bhatt is with the S. V. National Institute of Technology, Surat,
Gujarat State, India (Phone: 91-9898082293, Fax: 91-261-2227334, email:
S. N. Gaderia is with the S. V. National Institute of Technology, Surat,
Gujarat State, India (email: [email protected] )
S. A. Channiwala is with the S. V. National Institute of Technology, Surat,
Gujarat State, India (email: [email protected])
Ut Top heat loss co-efficient, W/m2K
UL Over all heat loss co-efficient of collector, W/m2K
Th Temperature of heater plate, K
T p Temperature of absorber plate, K
hw wind induced convective heat transfer co-efficient,
W/m2K
hC1-2 Convective heat transfer co-efficient between 1st and
2nd
cover, W/m2K
K c Thermal conductivity of cover, W/m2K
h p-c Convective heat transfer co-efficient between
absorber plate & cover, W/m2K
hc-a Convective heat transfer co-efficient between cover &
atmosphere, W/m2K
F p-c Radiation shape factor between plate & cover
∈g Emmisivity of glass cover
Qu Useful energy gain, W
S Flux absorbed by collector, W/m2
III. FLAT PLATE COLLECTOR
The flat plate collector shown in Fig. 1 is one of the most
widely used device for harnessing solar energy. In any solar collection device, the principle usually followed is to expose a
dark surface to solar radiation so that the radiation is
absorbed. A part of the absorbed radiation is then transferred
to a fluid like air or water. When no optical concentration is
done; the device in which the collection is achieved is called
the flat plate collector. The flat plate collector is the most
important type of solar collector because it is simple in design,
has no moving parts and requires little maintenance. It can be
used for a variety of applications in which temperature
ranging from 40 °C to 100 °C is required.
Fig. 1 Solar flat plate collector
IV. PERFORMANCE ANALYSIS OF FLAT PLATE COLLECTOR
An energy balance on the absorber plate yields the
Experimental Investigations on Top Loss Co-
efficients of Solar Flat Plate Collector atDifferent Tilt AngleM. K. Bhatt, S. N. Gaderia, and S. A. Channiwala
T
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following equation for steady state:
qu = A p S - q1 (1)
where, qu = useful heat gain, i.e., the rate of heat transfer to
the working fluid; S = incident solar flux absorbed in the
absorber plate; A p = area of the absorber plate and q1= rate of heat loss.
In order to determine the flux, ‘S’ absorbed by the absorber
a term called the transmitivity absorptivity product (τα)
which is defined as the ratio of the flux absorbed in the
absorber plate to the flux incident on the cover system, is
evaluated and is given by ‘S’.
S= I b R b (τα) b + Id R d (τα)d+ (I b + Id) R r . (τα)d (2)
Where
τ = transmitivity of glass cover system.
α = absorptivity of absorber plate.
(τα) b = transmitivity absorptivity product for the beam
radiation falling on the collector.
(τα)d = transmitivity absorptivity product for the diffuse
radiation falling on the collector.
Now, rate of the heat loss is given by,
ql = Ul A p (T pm – Ta) (3)
Where,
Ul= overall loss coefficient
A p= area of absorber plate.
T pm= average temperature of the absorber plate, andTa= temperature of surrounding air.
The heat loss from the collector is the sum of the heat loss
from the top, the bottom and the sides.
Ql = qt + q b + qs (4)
Where,
Qt = Ut A p (T pm – Ta) (5)
Q b = U b A p (T pm – Ta) (6)
Qs = Us A p (T pm – Ta) (7)
Ul = Ut + U b + Us (8)
Here, Ut , U b and Us are the top, the bottom and the side
loss co-efficients respectively.
V. TOP LOSS COEFFICIENT
The top loss co-efficient Ut is evaluated by considering the
convection and the radiation loss from the absorber plate in
the upward direction. For the purpose of calculation, it is
assumed that
1) The transparent covers and the absorber plate constitute a
system of infinite parallel surface and flow of the heat isone dimensional and steady.
2) Temperature across the thickness of the cover is
negligible and that the interaction between the incoming
solar radiation absorbed by the covers and the outgoing
loss may be neglected
A schematic diagram of two-cover system is shown in theFig. 2.
Fig. 2 schematic diagram of two-cover system
In steady state the heat is transferred by convection and
radiation between the following:
1) The absorber plate and the first cover.
2) The first cover and the second cover and
3) The second cover and the surrounding must be equal.
( )( )
( )1
4 4
1
1 1/1/ 1/ 1
pm c
p p c pm c
p c
T T q A h T T
σ
−
−= − +
∈ + ∈ −
(9)
( )( )
( )2
4 4
1 2
1 21/ 1/ 1
c c
p c c c
p c
T T h T T
σ
−
−= − +
∈ + ∈ −(10)
( ) 4 4
2 2 2( )
w c a c skyh T T T T σ = − + ∈ −(11)
Eqs. 9 to 11 constitute a set of three nonlinear equations,
which can be solved iteratively by assuming Tc1 and Tc2 for
which qt/A p is same by all these equations.
There exists few correlations for calculating h p-c, hw, and Ut
which have been derived based on different experiments andtechniques which may not be representative of real life
collector.
The present work is an attempt to present the comparative
assessment of these correlations, based on systematic
experiments, on an experimental research collector which is a
representative of real life collector and to study the effect of
collector tilt angle on top losses and top loss co-efficient.
VI. EXPERIMENTAL SET-UP & METHODOLOGY
An experimental research collector as shown in Fig. 3 is the
representative of real life collector developed during the
course of this work. It essentially consists of a cover plate of 5
mm thick glass, powder coated black absorber of copper [∈ p
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= 0.9] having size as 1210 mm x 710 mm x 1 mm, two
reflective electric heaters of 0.5 kW capacity, kept below the
absorber to produce uniform heat flux, and wooden housing
filled with cerwool insulation (K=0.03 W/m-k) at the back
and glass wool (K = 0.04, W/m-k) at the sides.
Fig. 3 photograph of research collector
The experiments are conducted in a laboratory with black
curtains on the windows so as to avoid any infiltration of
external radiation. The electricity is supplied to the two
heaters by two variacs at a predecided controlled rates varying
from 200 to 700 W through double stabilized power sources
and the collector is allowed to reach to its steady state which
takes nearly 4 to 5 hours for each heat input. The steady state
temperature levels are measured by 48 calibrated chromel
alumel thermocouples of 26 gauge mounted on the bottom of
the glass cover, absorber plate, heater plate, bottom, sides,
edges and covers of housing. The wind is created by three
adjustable height pedestal fans whose input is also controlled
by variacs for creating different speeds. The wind velocity is
measured by vane type anemometer over six different points
on the collector, Fig. 3 gives the photographic view of
experimental set-up.
VII. EXPERIMENTAL DETERMINATION OF VARIOUS PARAMETERS
Once the steady state is achieved the top loss, the overallloss and the convective heat transfer coefficients are evaluated
from the energy balance equation as follows:
Qin = Qt + Q b + Qs + Qc + Qe + Qsl (12)
Qin is the total energy supplied to the heaters which is same
as the heat losses from collector under steady state. The
bottom losses, Q b, side losses, Qs, edge losses, Qe, corner
losses, Qc are calculated as per the method suggested by
Channiwala. Sealing losses are assumed as 1% and hence top
losses are calculated by subtracting all these losses from input
energy Qin. Once Qt is obtained U1, Ut, h p-c and hw may be
evaluated as follows:
4 4
4 4
( )
( )
( )
( ) ( )
( )
( ) ( )
int
t
t
p ct p c
t cw c a
QU
Ap Tp Ta
Q
U Ap Tp Ta
F Tp TcQh
Ap Tp Tc Ap Tp Tc
Q Tc Tah h
Ap Tc Ta Ap Tc Ta
σ
σ
−
−
−
=−
= −
−= −
− −
∈ −= = −
− −
VIII. INVESTIGATION STAGES
Effect of Plate Temperature:
In this stage, the effect of plate temperature on the wind loss and the top loss coefficient
of solar flat plate collector is investigated with different heat
inputs, keeping collector in horizontal position under zero
wind velocity. For each set of experiments the steady state
conditions were obtained and all the temperature and power
inputs were recorded, based on which h p-c, hw, Ut and U1 are
evaluated.
Effect of Collector Tilt Angle: In second stage the effect of
tilt angle (β) is studied keeping the collector at various angles
varying from 0° to 90°, with respect to horizontal under zero
wind velocity.
Effect of Wind Velocity: In this stage, the effect of wind
velocity at zero degree of yaw angle has been studied with
different wind velocities varying from 0 to 5 m/s. For this,
three pedestal fans were used to generate necessary wind.
Anemometer was used to measure wind velocity at six
different points and the average velocity was used in
calculation.
Effect of Wind Direction: In final stage of this project work,
the effect of yaw angle was studied. The readings were taken
at various yaw angles like 0°, 45°, and 90° with respect to the
principle axis of solar collector. Further, for each yaw angle
observations have been made at different wind velocitiesranging from 0 to 5 m/s.
IX. R ESULTS AND DISCUSSION
The salient features of the results obtained are discussed
below:
It is apparent from the graphs 1 to 3 that there is an increase in
top loss at different tilt angles, which supports the fact that at
higher absorber plate temperature levels both radiative &
convective losses will increase, resulting in increase in top
losses. Both Ut and Ul are found to be increasing due to
increased convective & radiative losses. The graphs 4 to 6
shows that there is an increase in % top loss as tilt angle
increases.
(13)
(14)
(15)
(16)
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Graph. 1
Graph. 2
Graph. 3
Graph. 4
Graph. 5
Graph. 6
X. CONCLUSION
The tilt angle has very marginal effect of wind induced
convective heat transfer at a given constant absorber plate
temperature. The top loss co-efficient correlations in general
over predict the value of Ut by 5-15%. Samdarshi and
Mullick, Agrawal and Larson correlation seems to correlate
present experimental work by 10%. For any collector, tilt
between zero to ninety the top loss coefficient may be
evaluated as,
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Utβ = Uth [1 – 0.0006β]
Where
Utβ = top loss coefficient at angle of β degree
Uth = top loss coefficient for horizontal collector
With the increase in absorber plate temperature,
simultaneously the value of Ut and Ul increases at different tilt
angle. Thus the value of Ut and Ul are found increasing due to
increased convective and radiative losses.
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