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Use of Concentrated Solar Thermal Energy Systems to Enhance Sea Salt Production in Southern Spain
Robert Borja Flagg Díaz
The Pennsylvania State University
University Park, PA 16802 USA
Susan W. Stewart, Ph.D.
The Pennsylvania State University
University Park, PA 16802 USA
Jeffrey R.S. Brownson, Ph.D.
The Pennsylvania State University
University Park, PA 16802 USA
ABSTRACT
This study describes a simulation analysis to asses
increased productivity of salterns used for sea salt
production by implementing a solar parabolic trough
collector to accelerate the evaporation process. The
proposed system is designed for Southern Spain, to be
coupled with a heat exchanger submerged in the saltern’s
channel. A thermal-fluid analysis of the proposed system
was modeled using Engineering Equation Solver (EES) to
replicate the heat and mass transfer behavior of the system. Results provided through the simulation model show that
the added heat increases the pond solution layer
temperature, thereby increasing the evaporation rate and
the sea salt production rate.
1. INTRODUCTION
This work proposes implementing parabolic trough
collector technology to modernize the traditional salterns
of the Bay of Cádiz, in southern Spain. These salterns,
locally known as Las Salinas, are dedicated to producing salt mainly composed of NaCl. Unfortunately it is a dying
industry which cannot meet the competitive production
rates mandated by industrial and commercial competition.
The salinas, typically small-family businesses with limited
economic resources, have been conservative about
implementing technology. The traditional process currently
employed depends largely on daily temperature and the
prevailing winds to promote evaporation. This passive and
simple system has been used throughout the centuries,
dating back to the Phoenician time periods, with little
advances [1].
As a result, the production period is limited by the
meteorological conditions that promote an adequate
psychrometric balance, which only occur during the
summer months, typically between June and October. The
ideal meteorological conditions mainly consist of daily
high temperatures, partial pressure of water vapor in air,
and easterly winds. These eastern winds, known as el
viento del levante, refer to winds that originate in the
eastern Mediterranean (i.e. Syria, Lebanon, Israel,
Palestine, Jordan, and Iraq) and cross the Sahara Desert. As a result, these winds are composed of hot and dry air,
making them ideal to facilitate the evaporation process.
By employing parabolic trough collectors that heat a
working fluid which passes through a heat exchanger,
submerged in the Salinas channels, it is proposed that the
evaporative mass flux can be increased to promote the
production of sea salt. Additionally, it is proposed that the
production period of the Salinas can be expanded as the
added heat promotes evaporation during time periods
where simple solar radiation does not suffice.
This study therefore presents the results obtained from a
computer simulated model of the system. The simulation
incorporates models of parabolic trough collector
operations [2], a shell and tube heat exchanger model using
NTU method [3], and the modified Meyer evaporation flux
equation [4]. The computer model was programmed using
Engineering Equation Solver (EES), a software tool that
iteratively solves transcendental equations and has built-in
thermodynamic and transport property relations for many
different fluids [5].
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2. BACKGROUND
2.1 The Salinas
The salinas are composed of the estero (“water storage
pond”), three different channel types (the lucios, the retenidas, and the vueltas de Periquito), and finally the
tajos (“crystallization ponds”). An aerial view of a
traditional Salinas can be observed in Figure 1.
The salinas have a slight gradient that allows the water to
flow naturally thanks to gravitational pull. The channels
are created to typically be between 6 and 8 m wide and
between 0.5 and 2 m deep. These dimensions allow the
water to have a flow rate between 0.1 and 0.3 kg/s.
The evaporation, which averaged out throughout an entire
summer, is fairly constant compared to previous years. As
a result it is possible to characterize sections of these
channels with the concentration of the sea water.
Concentration indicators exist for a variety of reasons, be them biological occurrences or physical limitations of
precipitates. For example, different types of plankton can
be found at certain salinities [7]. Depending on the
presence of planktons, the channels walls can have a
certain colored tint. Likewise certain salts (other than
NaCl) precipitate at certain concentrations throughout the
salinas [8]. These precipitate also tint the salina’s walls.
2.2 Meteorological Conditions
According to Figure 2, the Köppen-Geiger Climate
Classification [9] categorizes southern Spain as having dry
and hot summers. Not surprisingly, the province of Cádiz,
including the Bay of Cádiz, suffers from moderate
temperature variations; between 16 C on average during
the winter months and 22 C on average throughout the
summer months [10].
Levante, the easterly or northeasterly winds, result from the
Azores anticyclone weather phenomena. When the
anticyclone extends northeastwardly over Spain and
southern France, it creates a low pressure area over the
western Mediterranean, causing the levante to blow [11].
Typically the levante is a dry wind. The dryness of this wind results from its proximity to Northern Africa. This
can be observed in the Köppen-Geiger Climate
Classification Map (Fig. 2). The map also depicts northern
Africa as a hot and arid desert climate, implying it having
dry air. Because of the Azores anticyclone, air from
northern Africa is suctioned by the pressure differential
previously mentioned, driving the levante over the salinas
of Cádiz and the rest of southern Spain.
2.3 Evaporation Process
According to the Oceanographic Sciences Institute of
Andalucía, the evaporation process at the salinas can be
divided into several stages [12]. Stage 1 begins with
pleamar (“high tide”) when the damn to the estero is
Caño Santi
Petri
Tajos 2
Tajos 1
Retenidas 2 Retenidas 1
Vueltas de
Periquito 1
Vueltas de
Periquito 2
Lúcios
Estero 1
Estero 2
Fig. 1: Property outline of salinas San Vicente. The different
sections depicted include: Estero, Lucios, Retenidas,
Vueltas de Periquito, & Tajos. (Adapted from [6])
1]
N
Fig. 2: Köppen-Geiger Climate Classification for
Mediterranean Ocean. Red depicts: hot, arid desert climate; Yellow depicts: Dry, hot summer climate. (Adapted from
[9])
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opened allowing seawater inflow from the estuary. The
water is trapped in the estero until Stage 2 when a
secondary damn is opened allowing the water to drain into
the lucios. The lucios act as a passage way for the water,
channeling it into the retenidas (“retained water”) where
the evaporation process begins having a significant role. The water is then passed to the vueltas de Periquito for
Stage 3, where salt water reaches concentrations slightly
below the crystallization limit. These 3 stages, last for
several days depending on the climatological patterns and
account for the majority of the evaporation process and
preparation of the highly concentrated sea water. Stage 4
finalizes the process when the highly concentrated sea
water is passed through to the tajos. Here the last bit of
evaporation occurs leading to salt crystallization. At this
point a thin layer of salt is created in the tajos. The full
process is then repeated until enough salt has accumulated
permitting the workers to collect the salt for crushing, processing, and distribution.
3. DATA AND METHODS
3.1 Data
For this analysis hourly data was used to model the system
behavior. Data sets used included meteorological data,
solar radiation data and oceanic data. The data obtained
came from measurement stations, modeled meteorological
conditions, and TMY data.
Figure 3 depicts satellite imagery provided by Google
Earth of the analyzed area and the location of the different
data sets.
The Spanish Port Authority, a department of the Ministry
of Public Works (“Ministerio de Fomento”) provided historical oceanographic and meteorological data from
three different stations. Two of the stations, “Boya Costera
de Cádiz (1320)” and “Boya de Golfo de Cádiz (2342)” are
buoys. The other station, “La Estación Meteorológica de la
Bahía de Cádiz (4340)” is land-based. The scale provided
in Figure 3 allows to approximate the distance from the
stations to the studied salinas.
Surface temperature data was compiled between Stations
2342 and 1320 because the measurement systems aboard
these buoys fail, presenting gaps in the data. Priority was
given to the data obtained from station 1320 due to its proximity to the salinas. Because of its proximity, it is
expected to adequately represent the water temperature of
the salinas, which oscillate between 23 and 26 C during the
summer. This was confirmed by comparing data obtained
in Yúfera’s “Estudio Preliminar del Zooplancton de las
Salinas de Cádiz” [7].
Concentration measurements were obtained from station
2342’s because it was the only equipped with salinity
measurement instrumentation.
Salinas San
Vicente
Fig. 3: Satellite imagery depicting the Bay of Cádiz. The tagged sites depict the location of the corresponding
meteorological stations and Salinas San Vicente (Adapted from [6]).
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Average wind velocity measurements were obtained from
station 4340. This station was selected to provide the wind
data because it is located on a land-based pier. This is
convenient because this site’s wind shear behavior
approximates the wind shear experienced by the salinas
due to surface roughness. The data provided by this station was in 10-minute intervals. As a result, the data was
averaged out throughout each hour to match the hourly
format.
Atmospheric pressure data was provided by the
Meteorological State Agency (“Agencia Estatal de
Meteorología”). The data was also measured from Station
4340. The data provided by this station was presented as a
daily average; as a result the data was distributed over the
24 hours to match the hourly format provided for the other
meteorological conditions.
The Council of Innovation, Sciences and Businesses
(“Consejería de Innovación, Ciencia y Empresa”) of the
Energy Agency of Andalucía (“Agencia Andaluza de la
Energía”) provided TMY data for direct normal solar
radiation. This data corresponds to the area surrounding the
Doña Blanca Castle Station, located at El Puerto de Santa
María. Doña Blanca Castle is approximately 16.8 km from
the studied salinas.
Ambient temperature was provided averaged over 4 hour
intervals by the Weather Research and Forecasting (WRF) model with 9-km resolution. Measured historical data
could not be used because the measurement
instrumentation equipped on the stations failed during the
time period studied for this location. Because the WRF 9-
km model only provides 4-hour intervals, the ambient
temperature was distributed over four hours to match the
hourly format provided for the other meteorological
conditions. There is approximately 10.4 km from the
detailed spot to the studied salinas.
Dew point measurements were obtained from the Global
Summary of the Day provided by the National Oceanic and Atmospheric Administration (NOAA) National Climate
Data Center (NCDC) Geographic Information System
(GIS) Map Services system. The data presented was
measured by the Weather-Bureau-Army-Navy (WBAN)
system for location identifier 13025. This identifier
corresponds to Naval Station Rota, Spain. The data
provided by this station was presented as a daily average;
as a result the data was distributed over 24 hours to match
the hourly data provided for the other variables. Dew point
was used with ambient temperature to calculate relative
humidity. Relative humidity was used with atmospheric pressure and ambient temperature to calculate partial
pressure of water vapor.
Because much of this data set had data holes, only a small
period of time had complete data. The obtained data,
therefore, only allowed analyzing the meteorological
conditions between July 21st, 2004 and September 30,
2004.
3.2 Method
3.2.1 Proposed System
The proposed system is depicted in Figure 4.
Parabolic trough collectors will be installed along the
jetties that shape the channels. These PTC’s should be installed to minimize obstruction from the wind. They will
act as the heat source that feeds the heat exchanger fluid to
the heat exchanger. The proposed heat exchanger will be
comprised of a collection of pipes that facilitate heat
transfer from the working fluid to the salt water. These
pipes would be slightly submerged under the surface of the
water since the temperature of pond solution layer dictates
the evaporation rate of water as presented by Manganaro &
Schwartz [4].
Parabolic Trough Collectors
According to Kalogirou, parabolic trough collectors are a
type of concentrated, sun-tracking collector that can
achieve high temperatures with high efficiency. They are
light structures that provide temperatures in the hundreds
of degrees Celsius at low costs [2]. The collectors are made
up of metal sheets that are bent into a parabolic shape as to
reflect solar radiation to a black metal tube placed along
the focal line [2]. This structure concentrates the solar
radiation from the Sun, heating up the working fluid
running through the black tube.
A horizontal north-south facing collector can collect
slightly more solar radiation than an east-west oriented
collector and also, the north-south collector collects more
Fig. 4: Artistic rendition provided by the author to facilitate
understanding of the proposed system.
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solar energy in the summer months than in the winter [2].
This is critical for the presented project.
A glass cover can be placed around the black tube with a
vacuum seal to reduce convective heat loss, therefore
reducing the overall heat loss coefficient [2]. One disadvantage from this is that the glass provides
transmittance losses [2].
The heat transfer behavior of the parabolic trough collector
was based off of equations obtained from Kalogirou,
S.A.’s Thermal Analysis of Parabolic Trough Collectors
[2].
Equation 1 [2], which describes the useful heat gain, Qu, by
the working fluid,
[ ( )] (1)
In this equation, FR is the collector heat removal factor, Aa,
is aperture area, S is the absorbed solar radiation per unit
area, Ar is the receiver area, UL is the collector overall heat
loss coefficient, Ti is the initial temperature, and Ta is the
ambient temperature.
Equation 2 describes the outlet temperature [2], To, after
the fluid has absorbed all the useful heat gain:
(2)
Ti is the inlet temperature, Qu is the useful heat gain from
Equation 1, is the mass flow rate, and Cp is the heat
capacity.
Heat Exchangers
A shell and tube heat exchanger was used to approximate
the heat transfer behavior from the working fluid to the sea
water in the salinas’ channel. Figure 5 depicts what a heat
exchanger of this type looks like. This approximation was
used since the sea water flows through a confined space
over tubes that transport the working fluid.
For the analysis of this heat exchanger the effective Number of Transfer Units (NTU) method was used, rather
than the log-mean temperature difference method. This is
because the NTU method is better at predicting the outlet
temperatures of the hot and cold fluid streams in a
specified heat exchanger [3].
This model can be used because heat exchangers usually
operate for long periods of time with no change in the
operating conditions [3]. For such steady-flow conditions
to be achieved it is important that the mass flow rate of
both fluids and their temperatures remain constant.
The specific heat of a fluid will change with temperature
but over a specified temperature range it can be treated as a
constant at some average value with little loss in accuracy.
Also, the heat exchanger is assumed to be perfectly
insulated, so that there is no heat loss to the surrounding
medium, and any heat transfer occurs only between the two
fluids [3].
Some of these approximations are not true in the proposed
system as the inlet temperature of water can change due to
the atmospheric conditions and because the proposed heat exchanger is not completely enclosed. But due to the
complexity of the proposed system, the approximation of
the heat exchanger will suffice for this study.
Equations 3 and 4 are relevant in modeling this system’s
behavior as they provide the outlet temperature for both the
sea water and the working fluid, respectively [3].
(3)
(4)
Tc,out is the outlet temperature of the seawater, Tc,in is the
inlet temperature of the sea water, Q is the actual rate of
heat transfer between fluids (same for both fluids), Cc is
the heat capacity rate of the working fluid, Th,out is the
outlet temperature of the working fluid, Th,in is the inlet
temperature of the working fluid, and Ch is the heat
capacity rate of the seawater.
It is also important to note that the NTU method does not
consider material properties. This is significant as in reality
the material used would be limited to those that are
corrosion resistant due to the corrosive behavior of
seawater. In such a case, it is proposed for future studies
Fig. 5: 1-shell-pass and n-tube-passes Heat Exchanger.
(Adapted from [3])
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consider analyzing stainless steel 316. This metal is highly
corrosion resistant and used in many maritime applications.
Also, it is important to address the working fluid used to
transfer heat from the parabolic trough collectors to the
salinas. It is proposed that water be the fluid of choice as it would not cause any internal corrosion of the system.
Likewise, in the case of system failure and leakage, water
would not contaminate the salinas. This is an important
consideration because the salinas must meet certain criteria
and regulations imposed on the food processing industry.
Evaporation Flux
This study uses the evaporation flux equation proposed by
Manganaro and Schwartz’s [4]. In brief, this section will
summarize the theory presented in this source.
Figure 6 presents a control volume for a solar salt pond
and also depicts the material and energy flows used to
model the evaporation process.
From this model and using a modified version of the
Meyer equation, Manganaro and Schwartz were able to
devise the Evaporation Flux equation (Equation 5), re, which governs a solar evaporative process for a pond in
terms of lb/hr-ft2.
( )( ) (5)
The fundamental variables driving the evaporation flux
equation include: the velocity of the wind, V3, measured in
mph; the partial pressure of water vapor in air, p3,
measured in mmHg; the geometric constant, C, which
usually is 0.5 for shallow pans or 0.36 for ponds or lakes; and the calculated vapor pressure of the water over the
pond solution, p1, provided in mmHg. Equation 6 describes
how all these variables come together,
( ) (6)
As shown, the vapor pressure of the water over the pond
solution depends on: the salt concentration in solution
bulk, c1, measured in terms of weight-fraction, and the
vapor pressure of pure water, pw0, measured in mmHg. The
vapor pressure of pure water may be calculated given the
temperature of pond solution layer, T1, measured in oC. The vapor pressure of pure water can be calculated with
Equation 7.
[
( )
) (7)
4. RESULTS & DISCUSSION
The system analyzed comprised of a 20 m parabolic trough
collector with a 3.5 m wide aperture that had a reflectance
coefficient of 0.86. The reflected radiation’s focal point
focuses on a receiver surrounded by a glass cover, forming
a vacuum between the receiver and the cover. The glass
cover has a diameter of 0.09 m and emissivity of 0.87. The
receiver, modeled as stainless steel with blackened nickel
surface treatment, has a thermal conductivity of 15 W/m-
K, and an outer diameter of 0.05 m with a wall thickness of 0.0005 m. The receiver absorptivity is 0.97, the
transmissivity is 0.80, and the emissivity is 0.92. The heat
transfer coefficient inside the receiver is assumed to be 330
W/m2-K.
Water was used as the working fluid passing through the
parabolic trough collector and the heat exchanger because
it is non-toxic in the case a spill is to occur. Specific heat
of water was modeled to have 4250 J/kg-K and a mass
flow rate of 0.32 kg/s.
The heat exchanger was modeled as having 1-shell and 80-
tube passes, each tube having a length of 5 m. It was
estimated that the overall heat transfer coefficient was 310
W/m2-K.
The cold fluid entering the heat exchanger was the sea
water at 20 C. Seawater at this temperature correlates to a
specific heat of 3,940 J/kg-K.
For the evaporation rate, the constant C is usually 0.5 for
shallow pans or puddles and about 0.36 for a pond or lake.
For the salinas, C was estimated to be 0.36 [4].
Inputting the data above with the previously described
meteorological data into the EES model produced the plot
depicted in Figure 7 which depicts the evaporation rate of
the salt water in the Salinas. The blue line depicts the
evaporation rate resulting from the enhanced PTC and heat
exchanger system. The red line depicts the evaporation rate
resulting from traditional methods.
Fig. 6: Solar salt and pond model. (Adapted from [4])
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The peaks depicted in the graph correspond to the day time
hours, while the lower values correspond to night hours.
These peaks occur because evaporation increases during
the day time when the wind and solar radiation combine to
promote this effect. At night, with 0 W/m2direct normal
solar radiation, the parabolic trough collectors do produce the heat needed to accelerate the evaporation process.
As it can be observed from Figure 7, the evaporation rate
of the sea water is drastically increased with the enhanced
system compared to the evaporation rate through the
natural process. It is estimated that the enhanced system
evaporates water six to ten times faster than the natural
process.
5. CONCLUSION
According to the EES model, the implementation of the
parabolic trough collectors and heat exchangers to the
traditional salters could drastically increase the sea salt
production efficiency of the salinas. Therefore, by
increasing the production rates, it is possible that the
salinas can regain competitive market position.
It is recommended that further investigation to this topic
include payback analysis. Such analysis is required to
examine if investing in parabolic trough collectors and heat
exchangers to increase the evaporation rate of water is
feasible.
At the same time, it is important to note that this model is
based on theoretical calculations and estimated values,
therefore limitations to its accuracy exist. As a result,
experimental research is necessary in order to obtain
realistic measurements of the system. This will allow
updating the computational model to depict more
accurately the evaporation of the salinas.
Experimental research should address heat exchanger
options, as the shell and tube heat exchanger is not the
most adequate model. Also, it is advised to study the
behavior of the working fluid as phase changes can potentially effect the heat transfer dynamics. The data
obtained from this research would allow to furthering the
accuracy of this assessment.
0
5
10
15
20
25
30
35
40
4850 5050 5250 5450 5650 5850 6050 6250 6450
Evap
ora
tio
n F
lux,
kg/
m^2
-hr
Hourly Date in Year, hr
Salinas Evaporation Rates Enhanced
Natural
Sept 30, 2004
July 21, 2004
Fig. 7: Results graphing the evaporation rates of the enhanced model versus the natural system.
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6. REFERENCES
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teau, L. (2003) Las salinas de la bahia de Cadiz
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http://dialnet.unirioja.es/servlet/fichero_articulo?codig
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(2) Kalogirou, S. A. (2009). Solar Energy Engineering:
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(3) Cengel, Y. A. (2003). Heat Transfer: A Practical
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EES).
(6) Map of the Bay of Cádiz, Cádiz, Spain. Google Earth.
(36.446N, 6.164E)
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http://www.youtube.com/watch?v=4vFdnNk1jg0&feat
ure=player_embedded
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