|
D.S.E. group of COMPANIES |
IN CENTRAL
SOLAR SYSTEM
Various single pass and
multipass central solar heating systems are studied
theoretically and examined from a system-life-cost aspect in order to arrive at
a configuration yielding the highest benefit/cost ratio.
Based on such modeling
and our extensive experience with various systems we submit that a Central
Solar Heating System based on a modified Slow Flow system 1 Phase Change
Material (P.C.M) in the storage circuit as designed and built by us meets these
desired criteria.
Accumulated experience
with dozen of systems based on our design and now operating over a prolonged
period support our design and energy storage concept; they have 2 the desired
high benefit/cost ratio.
1.
Introduction
Recent studies of
efficiency and cost effectiveness of thermosyphon
solar energy water heating systems [1-3] compared the performance of Multi-Pass
Systems (MPS) with that of Single Pass Systems (SPS) optional (and find them to
be of 3 equal efficiency). The MPS is based on the premise, which preswaited for a long time that “every possible energy gain
must be used”. In the MPS the water in the storage tank is caused to circulate
through the solar heat exchanger several times during one day so as to utilize
the solar energy to a maximum. This results in a system having relatively large
pumps and pipes, a small temperature raise per cycle, minor thermal
stratification in the water tanks and therefor small
water temperature differences within the tanks.
By control the SPS
or Slow Flow System. SFS is based on recirculation of the water through the
solar field approximately once per day, raising the water outlet temperature to
the desired usage temperature, in a single pass. The required storage tank
volume in SPS is such as to suffice for daily usage. The pumps and the pipes
used are smaller, slowing down the flow rate. Thermal stratification in the
water tanks
is significant and
the water outlet temperature is divide from the hottest water layer, nearest to
the top of the tank.
Tabor showed [1]
that under typical usage condition, and for climates as the type prevailing in
Israel, the SPS yields a thermal efficiency approximately equal to that of a
MPS, and that SPS has practical advantage that make it more cost effective. The
work of tabor [1] was confirmed by the publication of J.Gordon
and Y.Zarmi [2] who
extended the
validity of Tabor’s conclusions to various climatic conditions. The advantages
of the SPS using the slow flow principle as described by Tabor can found to
apply also to central solar system supplying a 4 of consumers as well as to
individual user systems.
In this paper we
shell discuss design improvements in Central Solar Systems (which become popular
in countries having many sunny days during the year) which offer short term and
long term ecological benefits and economical benefits as they reduce the 5 and
expenditures for required fossil fuels.
Central Solar
Systems include –3- major units,
namely; A backup heating
circuit,
A water storage circuit,
and A solar field circuit.
In the analysis, design and development of Central
Solar Heating Systems described below we first considered and compared various
features of the SPS and the MPS. In the solar heating system while we developed
a phase change material is include in the storage circuit of a modified SPS
while we have proven to be a cost effective system of high thermal efficiency.
Several dozen of such central systems were installed by the chromagen
Co’ in various locations and the accumulated experience validates the
advantages of our design. Local authorities and governments have been
subsidizing installation of Solar Heating System for
some time. We believe
that performance improvements based on advances in design and technology shell
help to substantially widen their usage in the near future.
2.
Modeling
and Design of Central Solar Water Heating System.
The function of a
Central Water Heating System is to supply hot water to a client (hotel,
apartment building, office building, etc) at a temperature and in quantities
required. The hot water must always be available. The basic structure of such a
system is shown schematically in fig 1.

Fig 1
Central Water
Heating System
For most practical
systems a hot water temperature in excess of 45 C deg is considered
satisfactory. We shell next consider the:
2.1
Flow
Rates and Attainable Efficiency in
SPS. (The Slow Flow System).
In Slow Flow
Systems one must control the water temperature so that it is at list at 45 C
deg at the entrance level to tank #1 of fig 1.
Thermal loss in
the solar heat exchanger and in the connecting pipes and the temperature
difference need in order to maintain heat transfer in the heat exchanger
regards a water temperature at the exit from the solar heat exchanger which is
5 C deg higher than the water storage temperature. A solar field water exit
temperature of 50 C deg is, therefore, typically used.
The water outlet
Tout from the solar field system is calculated on the basis of A.Whillier’s efficiency equation:
(1)
= FR (
- UL
T/It)
(2)
T/It
= [0.5 (Tin + Tout) –Ta]/It
And the heat balance
equation [ ]:
(3) Qout/Qin = m Cp (Tout-Tin)/It
(4) Tout ={1/ (2 m Cp+FR UL)}[Tin (2 m Cp-FR
UL)+2 Ta FR UL+2 It
FR
].
The outlet temperature
from the solar field (Tout) can be controlled by varying the flow rate (m).
To investigate the
various performance aspects resulting from use of the Slow Flow technique and
the performance of a SPS, let as examine the various parameters in “Whiller’s” efficiancy equation:
(5) FR = F’ F” F’ is the collector
efficiency factor.
(6) F’ = Co Ffe Ffe
is the fin efficiency factor.
Co is a coupling
parameter influenced by the thermal resistance between the pipe and the water
flowing in the pipe, and by the thermal resistance mainly due to the joint
between the pipe and the sunray collection surface fin.
In solar collectors
using high-quality joints (such as collectors in which the fin is
ultrasonically welded to the water conduits), the parameter Co depends mainly
on the thermal resistance between the water and the pipe. The fin efficiency Fef is given by [ ] as:
(7) Ffe = tanh (m
W/2)/(m W/2)
(8) m =
The flow factor F” is
given by [ ] as:
(9) F” = Ao [1-exp (-1/Ao)]
(10) Ao = m Cp/(Ac Ul F’)

A plot of fin efficiency Fef on m W
is shown in Fig 3 with t as a parameter.
Fig 3
fin efficiency Fef .

A plot of the flow factor F” as number of collectors
is show in fig 4 (spec. flow value is parameter).
Fig 4
F” flow factor.
For climatic conditions
in the northern Mediterranean basin a chromagen
CR-120 collector typically provides solar field temperatures of 50 C Deg. As
the specific flow rates in the range of 8 l/m^2h to 20 l/m^2h. Under climatic
condition of central and northern
2.2
Heat
Transfer Efficiency As a Function of Water Flow Through the
Collectors.
The rate of heat
transfer from the collection surface to the flowing in the conduit was seem to
be determined by Fef and F”, were:
Fef – the fin efficiency (Fig 3) depends
on geometry and on k, the thermal conductivity of the collection surface
material.
F” – the flow factor (Fig 4) depends on the water conduit
flow rate. In order to operate in the slow flow regime and to obtain required
field outlet temperatures of 50 C deg. The specific flow rate common in MPS
should be typically reduced by a factor of 3 to 4. Such a reduction
significantly reduce the flow factor F” value and causes an appreciable
decrease in the efficiency of individual solar collectors.
The
achievement of high overall field efficiencies at low specific flow rates
requires maintenance of a high flow factor in every collector in the solar
field.
This can be attained by
a series connection of the collectors as shone in Fig 5.
Fig 5
Series
(Serpentine) connection of collectors

A parallel connection as shone in fig 6 is also
possible.
Fig 6
A parallel connection of collectors
For a parallel
connection as shone in Fig 6 the number of joint is greater, the piping is
longer, the hydraulic resistance is higher, and the heat losses from the
connecting pipes are greater.
2.1
Solar
Field Efficiency for a Series (Serpentine – Connected) Collector System.
Use of a serpentine connection solves the efficiency
problem due to slow flow, but leads to a decrease in efficiency, due to flow in
a direction opposite to the thermosyphon direction.
Efficiency of a solar collector, with reverse flow was
examined in an experiment performed in the solar laboratory of Lordan Ltd. In
The observed results can be expressed by the following
flow factor equation which contains a correction factor [ ].
( 11 ) Rff = Ao’[1-exp(-1/Ao’)]
( 12 ) Ao’
= m Cp /[Ac Ul (F’/F”’)]
Eq. (11) and (12):
Rff is the Reverse
flow factor.
F”’ is the Reverse
collector efficiency and the other symbols are as previously describe.
With serpentine
connected collectors flow in the thermosyphone
direction takes place in about half of the collectors; flow in the opposite
direction takes place in the remaining collectors.

Consider a model composed of Series collectors
connected in serpentine as shown
In Fig. 7
The overall efficiency
for such a model is given by:
(11)
FR
={
[1-(1-K)N]/(NK) (FR
)1
Where (FR
)1 and (FR UL)1 are
the values for the original test of the collector that was made according to
the standard.
(12) FR
UL={ [1-(1-K)N]/(NK) (FR UL)1
Were
(13)
K = (FR UL)1 /
(m N Cp)
And N is the number of collectors connected in serial.
The efficiency of a row of collectors (the efficiency of a
row is equals the efficiency of the solar field when the rows are thermally
balanced) is given by:
(14)
Field = FR
(
-UL
T/It)
Fig 8 represents the solar field efficiency (the
efficiency of a row of collectors as a function of specific flow rate and of
the number of the collectors connected in serpentine.
N = the number of collectors in a row.
2.2
Schemes
for Efficient Improvements in MPS.
A commonly used
collector connection for a MPS is shown in Fig 9.
*[[The efficiency of
the solar field using a connection as shone in Fig 9 is a parameter of the flow
rate through the collector, the heat loss and the reverse thermosyphon
flow in the connecting piping]].
The efficiency of the
solar field, improved if the outlet temperature from each row of collectors is
identical.
Riner, Croy and Felix Peuser [4] point out a significant improvement in the
hydraulic balance of the solar field and an increase in the solar efficiency if
one employs a serpentine connection, instead of the common type of connection
as shone in Fig 9.
The pressure drop along
a row of serpentine-connected collectors is high and permits good hydraulic-
balance even at low flow rats in systems employing small-bore piping and other
small bore accessories.
The use of flow rates
which are three to four times lower, by using of serpentine connection
significantly reduces the cost of pump, the cost of the electricity consumed in
operating it, and the piping as a result of reduction diameter.
3.
Flow
Rate Control Strategies and Efficiency Optimization in MPS and SPS.
The flow rate control strategy in MPS is such as to take
full advantage of every possible energy gain; use of a differential thermostat
enable implementation of this strategy.
The control strategy in SPS dictates activation of the
pump in the solar field circuit, when the water temperature at the outlet from
the solar field, is equal to, or above 50 C Deg and activation of the storage
pumps when the temperature at the input to the storage tank is above 45 C Deg.
A control system, which regulates the flow rate and
ensures that the outlet temperature is lower then a set control value is
suitable for implementation of this control strategy.
In MPS, the water is cased to circulate through the
storage system several times per day and the water temperature increases by a
few degrees for each cycle.
Rapid circulation of water in the system causes mixing in
the tanks and results in a small temperature difference between the various
storage tanks and between water layers with no stratification its need to wait
until water is heated to user temperature.
In a SPS the water flow rate is controlled by monitoring
the water temperature at the outlet from the solar field. The flow rate in the
solar field and in the storage circuit is controlled so as to keep A desired
temperature of the water leaving the solar heat exchanger and entering the
storage circuit.
This control strategy causes stratification of temperature
in the storage tank. Wuestling [7] presented
simulation study results indicating a energy utilization of 66% as a result of
slow flow and a highly stratified layer of a solar system operating in the sloe
flow regime in comparison to a multi pass system, where the solar energy
utilization reaches only 48% as a result of water mixing.
In order to reduce the operating time (and reduced
consumption) of the Backup Heating System (BHS) the BHS should be installed as
a water flow heater near the outlet of the storage circuit. Thus the heated
water enters the circulation circuit at a usable temperature and returns to the
storage circuit at a lower temperature. This results in a saving of energy
stemming from heat loss reduction due to lower water temperature of the storage
circuit and of the connecting piping.
Low storage temperatures also reduce build up of calcium
deposits in the system.
4.
Improved
Energy Storage System.
A major problem encountered in the design and installation
of a central solar system in existing buildings is a shortage of storage
capacity. Enlargement of storage capacity is costly, problematic, and often
difficult to carry out. Unique method for storing energy in central solar
system was developed.
Tank containing (phase change material) PCM within the
storage circuit.

A schematic
diagram of a Central Solar Heating System employing PCMs
is shown in Fig 10
Fig 10
This technology and
method enable one to significantly increase the energy stored at small
additional cost without resorting to the construction of additional utility
rooms. Employment of this technology stabilizes the water temperature in the
storage circuit at 53-55 C Deg depending on the PCM used.
Use of PCM to increase
the Effective Storage Capacity
Conclusions
Central Solar Water
heating systems based on MPS and SPS were considered and SPS was examined in
great detail. In comparing the two system types one found that as far as: solar
field efficiency, storage circuit efficiency and cost of connecting pipes
accessories and pumps the SPS is the preferable system. As far as the cost of
the control system and the heat exchanger the MPS is at an advantage.
If an overall system
cost / profit value is taken as a yardstick for system efficiency the SPS
method is superior in pachculas if the PCM technology
is used in the storage circuit.
Conventional SPS were
originally developed for individual systems. Today about 50,000 individual
units are in use, most in
The SPS (or slow flow
systems) design and construction care subsequently extended to Central Systems.
Over 30 central systems were and operate
successfully in
Reference:
1)
H.Tabor., (1969)
A note on the Thermosyphon hot water heater.
Cooperation Mediterraneenne Pour L’Energie,
Bulletin No 17, pp. 33- 41.
2)
J.M.
Gordon and Y. Zarmi., (1981) Technical Note, Thermosyphon System: Single VS multi-pass.
Solar Energy Vol. 27 No
5, pp. 441-442.
3)
Y.F.
Wang, Z.L. Li and X.L. sun (1982).
A “ONCE-THROUGH” SOLAR
WATER HEATING SYSTEM.
Solar energy Vol. 29 No 6, pp. 541-547.
4)
Reiner Croy and Felix A. Peuser., (1994)
Experience With Solar Systems For Heating Swimming Pools In
Solar energy Vol. 53 No 1, pp. 47-52.
5)
A. Arbel and M. Sokolov., (1994)
Improving Load Matching Characteristics Of a Thermosyphonic
Solar System By Thermostatically Controlled Circulation.
Solar energy Vol. 52 No
4, pp. 347-358.
6)
1993
ISES Solar World Congress.
6.1 – Peter Fagerlund Carlsson., Heat Storage For Large Low Flow Solar Heating
Systems.
6.2 – M. Mack and C. Funfgeld., Low Flow
System Design Consideration.
6.3 – C. Funfgeld, M. Mack., Side By
Side Comparison Of a Low Flow and an
Advance Conventional
Solar Domestic Hot Water System.
6.4 – Karsen Duer
and Svend Svendsen.,
Conversion Of Indoor Measurements To Outdoor Long-term
Performances For Low Flow Solar Collectors.
6.5) – Simon Furbo., Optimum Design Of Small DHW Low Flow Solar Heating
Systems.
6.5)
John A.
Duffie., William A. Beckman., (1991) Solar
Engineering Thermal Processes. Jhon Wiley & Sons
Inc., Second Edition pp. 498.
DESIGN OF A SOLAR CENTRAL SYSTEM AT THE ROBINSON
LYTTOS HOTEL IN CRETA
Method, Design
Equipment and Cost.
The solar system will
be based on the “Slow Flow” Concept, which enables the operation at higher
efficiencies, compared to standard one. The solar system will be designed by
using different computer programs.
1.0 Design details
1.1 Program 1.
This program
performs solar calculation, which are based on average climatic data at a
specific location.
The program
analyses, the data builds a model that describes a characteristics day, using
this program for the calculation of a module day.
a. Number of collectors’ need?
·
Number
of collectors in a raw.
·
Pressure
drop on collector’s line.
b. Total volume of the storage tanks.
c. Power of the heat exchangers?
d. Pump flow rate and pressure drop?
1.2 Program 2.
Drawing software.
a. Solar field construction:
The collectors
will be drawn on the roof taking care on:
·
Obstacle.
·
Shadow
line.
·
Number
of collectors in a raw.
·
Cold
water line.
·
Hot
water line.
·
Sensor location
in the solar field.
·
A
characteristic collector line.
·
Expansion
tank (open/close).
b. Machine room construction:
The machine room will
be constructed, To enable the optimal operation with the Solar system. The new
design will include:
·
Number of storage tanks.
·
Total volume of storage tanks.
·
Configuration of the connecting pipes
between the storage tank, solar heat exchanger, backup system, backup heat
exchanger and mixing pump.
1.3 Program 3.
The hydraulic
software will be used for the calculation of the pipes diameters at the solar
field and in the machine room.
Attention will be
drawn to keep engineering standards: maximum allowed velocity, and further
engineering needs: like equal flow rate in any collector raw. The pump curves
will be included into the software and as a result the correct pump to suite
the flow and pressure which will be found.
1.4 Control and Monitoring System (C.M.S).
The Control System
operates the solar when energy is taken from, and operates the backup system when
needed.
The monitoring
system unit will collect and keep (in real time) the information when energy
produced by the solar system and or by the backup system.
The control will
be build as a module unit called “Brain”. The “Brain” will be constructed as a
box. The box assembly unit will include all the sub systems that need to
operate the solar system.
Sub systems:
·
Energy systems.
·
Pumping systems.
·
Control instruments.
·
Control systems.
·
Electrical systems.
The control module unit
will build to operate and check in
2.0
Cost
brake down.
2.3 Part list of the “Brain”:
We can’t give accurate
price, due to lack in information.

Remark: The “Brain”
will be mounted on a structure which will combine a compact unit .
Solar Field: diameter units
a. Copper pipes :
· main line: 2 ½” - 3”.
· Connecting pipes: 2 ½” -
¾”.
b. Ball valve: ¾”.
30
c. Automatic air valve: ¾” (120 C Deg). 60
d. Thermometer: ½” (120 C Deg). 7
e. Open expansion tank: SS-316 L, 100(l). 1
Storage system:
f.
Galvanized
pipe: 2 ½” - 3”.
g.
Ball
valve: 2 ½”
- 3”.
h.
Check
valve: 2 ½” - 3”.
i.
Fitting: 2 ½” - 3”.
j.
Storage
tank: 3,500
(l).
k.
Assembly
materials:
Communication cable:
l.
PT-100
cable (Between the solar field and machine room).
m.
Telephone
communication port.
n.
Internet connection.
Solar Field Drawings.






Solar System
layout.











Calculation &
Graphs.