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    Geochemical and environmental controls on the genesis of solubleeforescent salts in Coastal Mine Tailings Deposits: A discussion based onreactive transport modeling

    S.A. Bea a,, C. Ayora a, J. Carrera a, M.W. Saaltink b, B. Dold c

    a Institute of Environmental Assessment and Water Research (IDAEA), CSIC, c/Lluis Sol Sabars, s/n, 08028 Barcelona, Spainb Technical University of Catalonia (UPC) c/Jordi Girona 1-3, 08034, Barcelona, Spainc Institute of Applied Economic Geology University of Concepcin, Victor Lamas 1290, 4070386 Concepcin, Chile

    a r t i c l e i n f o a b s t r a c t

    Article history:

    Received 19 April 2009

    Received in revised form 30 November 2009

    Accepted 11 December 2009

    Available online 24 December 2009

    Water-soluble eforescent salts often form on tailings in hyperarid climates. Their high

    solubility together with the high risk of human exposure to heavy metalssuch as Cu, Ni,Zn, etc.,

    makes this occurrence a serious environmental problem.

    Understanding their formation (genesis) is therefore key to designing prevention and

    remediation strategies.

    A signicant amount of these eforescences has been described on the coastal area of Chaaral

    (Chile). There, highly soluble salts such as halite (NaCl) and eriochalcite (CuCl22H2O) form on

    4 km2 of marine shore tailings. Natural occurrence of eriochalcite is rare: its formation requires

    extreme environmental and geochemical conditions such as high evaporation rate and low

    relative air humidity, and continuous Cl and Cu supply from groundwater, etc. Its formation

    was examined by means of reactive transport modeling.A scenario is proposed involvingsea water andsubsequently a mixture of seawater/freshwater

    in the groundwater composition in the formation of these eforescences. The strong

    competition from other halides (i.e. halite and silvite (KCl)) for the Cl may inhibit the

    precipitation of eriochalcite. Therefore, the Cl/Na ratio trend N1 is a key parameter in its

    formation. Cation-exchange between Na+ and other major ions such as K+, Ca2+, Mg2+ and

    Cu2+ in the clay fraction of tailings is proposed to account for realistic Cl/Na ratios.

    With regard to preventing the formation of eriochalcite, a capillary barrier on the tailings

    surface is proposed as a suitable alternative. Its efciency as a barrier is also tested by means of

    reactive transport models.

    2009 Elsevier B.V. All rights reserved.

    Keywords:

    Reactive transport modeling

    NaClCuCl2system

    Pitzer

    Tailings

    MultiphaseowUnsaturated zone

    Water-soluble eforescences

    1. Introduction

    Water-soluble eforescent salts often form on tailings in

    arid climates. Their formation on the surface increases the

    risk of human exposure to heavy metals such as Cu, Ni, and Zn

    through wind transport. Signicant amounts of eforescence

    salts (mainly halite (NaCl), eriochalcite (CuCl22H2O) and

    gypsum (CaSO42H2O)) form on 4 km2 of a porphyry copper

    tailings deposit in the coastal area of Chaaral (Chile, Fig. 1A).In 1983, the Chaaral contamination case was classied by

    the United Nations Environmental Programme (UNEP) as one

    of the most serious cases of contamination in the Pacic area.

    Despite the fact that Cl and Cu are widespread elements in

    the Earth, eriochalcite (also termed antofagastite, eriocalcite or

    erythrocalcite) is a highly soluble salt, commonly obtained in a

    laboratory, but rarely occurring under natural conditions.In fact,

    eriochalcite has never before been reported as eforescence in

    tailings (Dold, 2006). Its natural occurrence is mainly asso-

    ciated with fumaroles of volcanoes, e.g. Mt. Vesuvius (Italy)

    or associated with copper mineralization, e.g. Mina Quetena,

    Journal of Contaminant Hydrology 111 (2010) 6582

    Corresponding author. University of British Columbia, 6339 Stores Road,

    Vancouver, Canada V6T 1Z4, BC. Tel.: +1 604 827 5607; fax: +1 604 822 9014.

    E-mail address:[email protected](S.A. Bea).

    0169-7722/$ see front matter 2009 Elsevier B.V. All rights reserved.doi:10.1016/j.jconhyd.2009.12.005

    Contents lists available at ScienceDirect

    Journal of Contaminant Hydrology

    j o u r n a l h o m e p a g e : w w w. e l s ev i e r. c o m / l o c a t e / j c o n h yd

    mailto:[email protected]://dx.doi.org/10.1016/j.jconhyd.2009.12.005http://www.sciencedirect.com/science/journal/01697722http://www.sciencedirect.com/science/journal/01697722http://dx.doi.org/10.1016/j.jconhyd.2009.12.005mailto:[email protected]
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    west of Calama, Chile. In the latter case, eriochalcite is

    accompanied by other copper halides such as blandylite

    (CuB2

    O4

    CuCl2

    4H2

    O) and atacamite (CuCl2

    3Cu(OH)2

    ) in a

    leached zone above massive iron suldes(Palache and

    Foshag, 1938). Previous works dealing with the environ-

    mental problem in Chaaral include those devoted to the

    impact on the local and regional marine fauna (Castilla,

    1983; Farina, 2001; Lee and Correa, 2005; Lee et al., 2001),

    and the study of mobilization of contaminant elements such

    as Cu, Zn and Ni, and oxyanions such as As and Mo (Dold,

    2006). Environmental and geochemical conditions are parti-

    cular for formation of the eriochalcite. A range of water

    activity between 0.61 and 0.68 was measured in a solution

    saturated in halite and eriochalcite (Filippov et al., 1986). As

    a consequence, their natural occurrence is restricted to

    extremely arid climates such as the Atacama region in Chile.Moreover, a continuous supply of Cl and Cu is necessary.

    Thus, this limits their formation, for instance, to coastal areas

    (Cl supply) and to cupric tailings (Cu supply). A priori, these

    particular environmental and geochemical conditions are

    important for the precipitation of eriochalcite. However, its

    rare natural occurrence suggests complex mechanisms in its

    formation.

    Reactive transport modeling in a vadose zone is relatively

    uncommon. This may be attributed to the lack of codes

    necessary to deal with multiphase ow associated with

    geochemical reactions, and also to the difculty encountered

    in obtaining reliable sets of eld or experimental data to

    compare with model results. Therefore, the majority of earlier

    works to develop reactive transport models for the vadose

    zone of mine tailings have assumed time-invariable boundary

    conditions and thermohydraulic properties and have ap-

    proached it as a single reactor (Bain et al., 2000; Gerke et al.,1998; Gerke et al., 2001; Mayer et al., 2002; Wunderly et al.,

    Fig. 1.(A) Location map of Chaaral's tailings. (B) A sketch of geochemical zones in Chaaral tailings. Three geochemical zones are observed: (1) an evaporation

    zone mainly formed by eforescences, (2) an oxidation zone characterized by secondary ferric mineralogy (i.e. goethite and K-jarosite), (3) a primary zone

    preserving the initial mineralogy of the tailings.

    66 S.A. Bea et al. / Journal of Contaminant Hydrology 111 (2010) 6582

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    1996). In those studies which have takenuctuating bound-

    ary conditions or thermohydraulic properties into account,

    a simplied reactive transport problem (usually with pyrite

    as the only mineral phase present in the system) has been

    considered (Lefebvre et al., 2001a; Lefebvre et al., 2001b; Xu

    et al., 2000). In some cases, the developed models have been

    used as a tool for predicting the long-termevolution of sulde

    wastes. The objective of this paper is to propose the probable

    mechanisms in the origin of eriochalcite, so as to design the

    best remediation measures. In nding the hypothesis that

    best explains the observed eforescences, we will shed light

    on the climatic and geochemical conditions that favor preci-

    pitation of eriochalcite. To accomplish this, different scenarios

    based on the predominance of a particular groundwater and

    solute source were simulated. The results of the calculations

    were compared with chemical analysis of interstitial water

    and sequential extractions of the solid phase from boreholes

    in Chaaral (Dold, 2006). The analysis of the multiphaseow,

    dissolution/precipitation of the eforescent crust, and sulde

    oxidation was carried out by means of reactive transport

    modeling. The atmospheric boundary conditions set in the

    model account for the hyperarid features of the climate.

    2. Site description

    2.1. Ore geology

    The Chaaral deposits were otation tailings from the El

    SalvadorPotrerillos mining district (Fig. 1A). The Potrerillos

    porphyry copper deposit was exploited until 1959. Produc-

    tion in El Salvador started that year. Therefore, it can be

    assumed that the lower portion of the Chaaral tailings comes

    from Potrerillos and that they are overlain by tailings from

    El Salvador (Dold, 2006).

    The Potrerillos deposit (1.8106 t Cu) is located in the

    Atacama Desert, 120 km east of Chaaral. It is characterized

    by a granodiorite intrusion affected by three hypogene alter-

    ation and mineralization events and an important supergene

    alteration. The early potassic and propylitic alterations are

    responsible for the K-feldspar, biotite, chlorite, quartz, ankerite,

    and anhydrite content. Associated suldes are chalcopyrite,

    bornite, pyrite, molybdenite, minor enargite, sphalerite, and

    galena (Camus, 2003).

    The El Salvador deposit (5.7106 t Cu) is located about

    100 km east of Chaaral. Primary mineralization is char-

    acterized by granodiorite with quartz veins and a matrix of

    K-feldspar, hornblende, biotite, minor oxides, anhydrite and

    suldes (Gustafson and Hunt, 1975; Gustafson and Quiroga,

    1995).

    2.2. Mineralogy of tailings

    Tailings grain size varies between silty/clayey to sandy

    toward the sea. A sketch of geochemical zones in the Chaaral

    tailings is shown in Fig. 1B. The tailings surface presents

    abundant greenish-blue and white eforescent salts. XRD

    analysis revealed that these were mainly halite (NaCl) and

    eriochalcite (CuCl2 2H2O) (Dold, 2006).

    The unsaturated zone is characterized by oxidation. Its

    depth varies between 0.73 and 1.88 m, with pH ranging from2.5 to 4, underlain by a primary zone of neutral pH. The

    oxidation zone is characterized by secondary ferric min-

    eralogy with a typical yellowish-brown color (dominated by

    K-jarosite) with ochre to orange streaks dotted with goethite.

    Gypsum is also present. Clay mineralogy is made up of illite,

    kaolinite and a vermiculite-type mixed-layer, the latter re-

    sulting from biotite alteration (Dold, 2006; Dold and Fontbote,

    2001). Mineralogy from the primary zone consists of quartz,

    plagioclase, muscovite, biotite, kaolinite, magnetite and rutile.

    In addition, pyrite with minor chalcopyrite and chalcocite are

    also observed.

    Sequential extractions are widely used for exploration

    purposes and for the study of element speciation in tailings. A

    seven-step sequence was applied to samples collected at

    Chaaral (Dold, 2003). Sequential extractions for Cu, Na, Ca

    and Mg, in samples corresponding to the rst meter of

    borehole CH1 are shown inTable 1. They showed a high level

    of Cu enrichment in the water-soluble fraction in the

    evaporation zone at the top of the tailings. This is consistent

    with the abundance of eriochalcite described in the previous

    section. Thus, eriochalcite content was estimated to be

    around 30 mol m3. However, a large fraction of Cu was

    associated with clay minerals (probably adsorbed on illite or

    as an interlayer ion-exchange cation in the vermiculite-type

    mixed-layer), or adsorbed to the surface and/or co-precipi-

    tated with Fe(III)-oxides and hydroxides (see Cu(ex) and Cu

    (ox) inTable 1, respectively). It is important to note that only

    a very small amount of Cu remains in the sulde fraction,

    indicating that most of the original chalcopyrite and chalco-

    cite has oxidized and dissolved in the last thirty-two years

    (see Cu(sph) inTable 1).

    Na is also present in the water-soluble fraction (mainly as

    halite) at the top (around 700 mol m3, see Na(sol) in

    Table 1). However, a signicant portion of the Na is found in

    the residual phase (around 440 mol m3, see Na(r) in

    Table 1). The sequential extractions indicate a halite/

    eriochalcite ratio in eforescences of about 20.

    2.3. Hydrological setting

    The west coast of South America, from northern Peru to

    Central Chile, is extremely arid (Fuenzalida, 1950). Aridity

    results from a combination of subsidence generated by a

    permanent high-pressure area over the Pacic Ocean and the

    Table 1Sequential extractions in mol for Cu, Na, Ca and Mg, in samples

    corresponding to the rst meter of borehole CH1 (Dold, 2003). sol = soluble

    fraction (Step I), ex = exchangeable fraction (Step II), ox = Fe(III) oxides

    and hydroxides fraction (Steps III and IV), sg = organic matter and Cu-

    supergene fraction (Step V), sph = primary suldes fraction (Step VI), r =

    residual fraction (Step VII) and t = total. A halite/eriochalcite ratio to 20

    could be estimated according to Na(sol)/Cu(sol).

    Step Cu Na Ca Mg

    I (sol) 33.77 684 152.56 59.0

    II (ex) 10.18 16.39 20.48 6.45

    III and IV (ox) 9 20.57 7.85 33.16

    V (sg) 0.4 6.82 4.4 6.45

    VI (sph) 0.68 20.59 10.62 47.95

    VII (r) 1.01 442.15 63.9 120.73

    Total (t) 53.63 1190.6 259.8 273.64

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    atmospheric stability induced by the cold northward-owing

    Humboldt Current.

    The climate in the coastal area of the Atacama region is

    classied as arid with abundant clouds (Fuenzalida, 1950;

    Fuenzalida, 1965). On an annual average 28% of the days are

    cloudy, 60% are partially cloudy and only 12% display clear

    skies. A cloudy sky means less solar radiation on the tailings

    surface and reduced evaporation.

    Average precipitation of 30 mm per year was recorded for

    Chaaral (Larrain et al., 2002). Therefore, the hydrological

    system of coastal tailings deposits at Chaaral is mainly

    controlled by tides, an inow of brine originating from Salar

    de Pedernales, and leakage from freshwater supply which

    feeds the village of Chaaral (Dold, 2006; Wisskirchen et al.,

    2006). The temperature in this coastal area is characterized

    by low variation between summer and winter and between

    day and night. (Thompson et al., 2003) provided a temporal

    record of temperature and relative humidity in Pan de Azcar

    Park, located 20 km north of Chaaral. There, ve meteoro-

    logical stations were established at different elevations

    (between 210 m and 800 m) and distances from the Pacic

    Ocean. Temperature and relative humidity were measured

    between June, 1999 and October, 2000 in a station located

    close to the Pacic Ocean. The variation in temperatures for

    the entire period does not exceed 10 C (approximately 21 C

    and 13 C for summer and winter, respectively), and the

    Vapor Pressure Decit (VPD) was highest during the summer

    (at 0.8 to 1.0 kPa), though not particularly high for desert

    ecosystems. Peak temperatures are observed in the months of

    January and February. The predominantly WSW winds form

    sand dunes, up to 1.5 m high, which migrate over the tailings

    surface toward the village of Chaaral. The portion of the

    tailings surface not covered by dunes displays abrasion

    marks, concordant with the predominant wind direction.

    2.4. Hydrogeology

    The distribution of major ions (see Na, K, Ca, Mg, Cl and

    SO4 in Fig. 2A) suggests that three different groundwater

    types were mixed in these tailings deposits (Fig. 2B)

    (1) Brine ows through the deepest portion of tailings. It

    may have originated at Salar de Pedernales, 150 km

    east of Chaaral (Dold, 2006). Therefore, it ows below

    the surface along its riverbed in the El Salado valley

    and discharges into the ocean.

    (2) A lens of freshwater overlies the brine. These fresh-

    waters may have originated from leaks in Chaaral's

    freshwater supply (Wisskirchen et al., 2006).

    (3) Sea water, less dense than the brine described above.

    In Chaaral, the ocean level varies approximately 1 mduring the tidal cycle.

    2.5. Aqueous chemistry

    Three piezometer nests (CH1, CH2 and CH3) were

    installed to a maximum depth of 9 m, along a prole in the

    southern part of the tailings deposits, directly in the west of

    Fig. 2.Aqueous chemistry distribution and hydrogeology. (A) Vertical proles of pH and major ions (K, Ca, Mg, Cl and SO 4) corresponding to borehole CH1 (its

    location is shown inFig. 1A). (B) Hydrogeology: three different water types are identied in the hydrogeologic system: (1) a brine in the deepest part of thetailings, (2) a lens of freshwater, and (3) sea water.

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    the Chaaral village (seeFig. 1A). The 20 pore-water samples

    were analyzed for major chemical components (Na, K, Mg, Ca,

    Cl, NO2, NO3, and SO4), and trace metals (Fe, Al, Cd, Cu, Mn,

    Zn, Pb, V, Cr, Co, Ni, As, Se, Sr, Mo, Ba, Ti, and U) by (Dold,

    2006).

    Vertical proles for pH and major chemical components

    corresponding to borehole CH1 are shown in Fig. 2A. Pore-

    water pH ranged between2.6 and 4 in the oxidation zone,and

    increased sharply to neutral values below the oxidation front.

    Furthermore, redox potential (Eh) reached 600 mV in the

    oxidation zone and dropped to 200 mV in the reducing

    environment of the saturated zone. Majorions such as Ca, Mg,

    Na, Cl and SO4increase their concentrations in the oxidation

    zone of these tailings, whereas K decreases its concentration

    in the same zone.

    3. Conceptual and numerical model

    A conceptual model for the thermohydraulic and geo-

    chemical processes involved in the formation of eriochalcite

    is shown inFig. 3.

    3.1. Thermohydraulic model

    Several atmospheric processes are considered in the

    model: rain, evaporation, radiation and heat exchange

    between tailings/atmosphere. Water ux (jw, k g r s1)

    through the tailings surface results from

    jw = P+ E+ jwg +jsr 1

    wherePis rainfall, Eevaporation,jgw

    ux of water vapor and

    jsr of the surface runoff. The evaporation rate in Eq. (1) is

    given by an aerodynamic diffusion relation according to

    E= fva;za;z0eae

    t 2

    wheree

    a

    and e

    t

    are vapor pressures in the atmosphere andpore tailings, respectively, fis a constant of proportionality,

    which takes into account the wind speed (va, m s1), the

    roughness length (z0, m), and the screen height at which

    va and ea were measured (za, m). Vapor pressure in the

    atmosphere (ea) is computed from its relative humidity

    (Hr) and temperature (Ta) through the psychometric law

    (Edlefson and Anderson, 1943). However, the vapor pres-

    sure in pore tailings (et) depends on its temperature (Tt),

    salinity (through water activity), and the capillary proper-

    ties of tailings.

    On the other hand, the energy ux (Je, J m2 s1) consists

    of sensible heat (Hs), latent heat (Hc) and radiation (Rn)

    uxes. As with evaporation, Hs is a function of air tempera-ture, wind speed and the specic heat of the gas. Hc is equal to

    the evaporation rate times the latent energy of vapor. Rn is

    calculated according to direct solar short-wave radiation,

    long-wave atmospheric radiation, the albedo of the tailings

    surface, etc. The calculation of the direct solar short-wave

    radiation takes into account seasonal variations, local latitude

    and the cloud index (this index represents completely clear to

    completely cloudy conditions). The daily variation inRnis not

    considered in the model for the purposes of simplicity.

    Fig. 3.Flux, transport, geochemical and energy balance conceptual model for Chaaral tailings.

    69S.A. Bea et al. / Journal of Contaminant Hydrology 111 (2010) 6582

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    The low relative humidity during the summer causes eva-

    poration, making water ow upwards. Solute concentrations

    in the upowing water are dramatically increased, with sat-

    uration resulting in some salts forming an eforescent crust.

    As evaporation progresses, pore-water content is reduced,

    preventing liquidux from rising to the surface. Therefore,the

    evaporation front is displaced slightly downwards, and efo-

    rescences continue to grow within the pore volume. This

    causes the tailings top to become increasingly cemented by

    salts. The associated reduction in permeability favors an in-

    crease in downward vapor diffusion. Vapor condenses at depth

    and concentrations decrease.

    The model is conceptualized as a 1D clayey tailings ac-

    cording to grain size described for borehole CH1 by (Dold,

    2006). Physical parameters and constitutive laws used in the

    simulations are shown in Table 2. The 1D column is open

    at the top and bottom. Atmospheric boundary conditions are

    applied at the top, whereas prescribed gas and liquid pres-

    sures (approximately 0.1 MPa) are applied at the bottom in

    order to simulate the groundwater level.

    As for the atmospheric parameters, maximum and minimum

    mean values for temperature (Ta) and relative humidity (Hr)

    are calculated over a period of thirty-two years (19752007)

    from data reported by (Thompson et al., 2003). The relative

    humidity varies between 0.63 and 0.74 and the temperature

    between 21 C and 13 C from summer to winter, respec-

    tively. Thus, sinusoidal functions between these values are

    simulated. On the other hand, the mean value for temper-

    ature (17 C) is set at the bottom of the model.

    As laid out above, the wind speed and a clear/cloudy sky

    affect the evaporation rate on the tailings surface. Thus, a

    constant wind speed of 4 m s1 and a partially cloudy sky are

    considered in the model.

    3.2. Geochemical model

    In parallel to the reduction of liquid saturation, oxygen

    (O2(g)) diffuses downwards, activating oxidation reactions.

    Oxidation of pyrite (FeS2) and chalcopyrite (CuFeS2) pro-

    duces sulfate, metals and acidity. The initial pathway consists

    of oxidation of the disulde to sulfate by O2(aq). The second

    pathway for sulde oxidation is by reaction with Fe(III). Both

    pathways are fast. They yield a low pH and Fe(II), which may

    become oxidized by O2(aq) to Fe(III). This oxidation is known to

    beveryslow atlow pH(Singer and Stumm, 1970) except in the

    presence of microorganisms, which can increase the rate of Fe

    (III) production by up to six orders of magnitude.

    The decrease in pH produced by pyrite and chalcopyrite

    oxidation increases the dissolution rate of accompanying

    silicates, which become the main source of alkalinity in these

    environments.

    The evolution of tailings impoundments is also controlled

    by the precipitation of secondary phases into the pores

    of waste materials and/or over their surface. Thus, the SO4,

    Fe(III) and K generated from dissolution are consumed

    by gypsum (CaSO42H2O), K-jarosite (KFe(SO4)2(OH)6) and

    goethite (FeO(OH)).

    Furthermore, cation-exchange could occur on the clay

    fraction of these tailings (e.g. on the vermiculite-type mixed-

    layer and illite). Major cations such as Ca2+, Mg2+, Cu2+, Na+

    and K+ could be exchanged onto the clay fraction, thus mod-

    ifying the major cation relationships.

    Evaporation trends for water samples collected in Chaaral

    are simulated using CHEPROO code (Bea et al., 2009). The ionic

    strength of water samples rangedfromaround 0.5to 15 M, thus

    requiring the Pitzer ion interaction approach (Bea et al., in

    press). The evaporation trend for a sample located in the oxi-

    dation zone, 0.3 m below the tailings surface(sample CH1-1),is

    shown inFig. 4A. Here, evaporation progress is dened as the

    ratio between the initial and the remaining mass of water

    after the evaporation step.Halite precipitates whenthe evap-

    oration progress is approximately equal to 6. This sample

    presents a Cl/Na ratio higher than 1. Therefore, precipitation

    causes Na concentrations to decrease and Cl to increase but

    with a lower slope (geochemical divide). Copper speciation

    changes during evaporation. Cu2+ is the predominant

    species at the onset of evaporation whereas CuCl+ is pre-

    dominant after halite precipitation (Fig. 4A1). Eriochalcite

    precipitates after evaporation progress equal to 150, when

    the ionic strength of the solution is 8 M and water activity

    0.7. At this point, the total Cu in solution decreases and Cl

    concentration continues to increase.

    The previous evaporation trend implies that the key

    parameter for eriochalcite to form is the Cl/Na ratio of the

    starting solution. For a Cl/Na ratio less than 1, Cl decreaseswhen halite precipitates but Na does not decrease, and the

    Table 2

    Parameters and the most important constitutive laws used in the simula-

    tions.Slis the pore saturation (m3 m3),Pl,Pgand e are the liquid, gas and

    vapor pressures, respectively (MPa), W is the molecular weight of water

    (kg wmol1),Ris the universal gasconstant, Tthe temperaturein Kelvin, aw is

    the water activity in the pore-water, and lis the liquid density (kg m3).

    Parameter or constitut ive law Tailings

    Porosity, 0.4

    Intrinsic permeability (m2) 1014

    Retention curve a S1 = 1 + PgPl

    P0

    1

    1n

    n

    P0(MPa) 0.002

    n 0.19

    Liquid relative permeability, krl = krlCSl

    1

    Constant,C 1

    Residual saturation,Srl 0.01

    Maximum saturation,Sls 0.99

    Thermal conductivity, = S1sat +

    1Slsat

    sat = 1sol

    liq

    dry = 1sol

    gas

    solb (W m1 K1) 2

    gas(W m1 K1) 0.026liq(W m

    1 K1) 0.6

    Solid density,sol(kg m3) 1700

    Solid specic heat (J kg1 K1) 789

    Saturated vapor pressure, es(MPa) eS = awAexp B

    T

    A(MPa) 136,075

    B(K) 5239.7

    Psychrometric law c e= esexp PlPg

    RT1W

    Evaporation by aerodynamic diffusion (E) E= k2 va

    lnzaz0

    h i2tvav Wind speed,va, (m s

    1) 4

    Stability factor, 1

    Screen height,za(m) 2

    Roughness length,z0(m) 0.01

    Karman's constant,k 0.4

    a Van Genuchten model (Van Genuchten, 1980).b

    Computed from mean values of mineral phases in tailings.c Edlefson and Anderson (1943).

    70 S.A. Bea et al. / Journal of Contaminant Hydrology 111 (2010) 6582

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    solution never reaches eriochalcite saturation. This is the case

    of the sample CH14, for instance (Fig. 4B, located 0.3 m

    below the water-table). The Cl/Na ratio of the pore-water

    samples from the three boreholes is plotted in Fig. 5. Besides

    sea water, only three samples display a Cl/Na ratio higher

    than 1. Two of them are located in the upper part of the

    oxidation zone, below the evaporation front. The third is

    located in the brine, in the deepest part of the tailings. The

    higher Cl/Na ratiocould be due to:(1) the exchange of Na+ by

    Ca2+, Mg2+, Cu2+ and K+ onto the clay fraction, (2) the

    inuence of the marine aerosol on the tailings surface, and

    (3) the precipitation of Na secondary phases (e.g. mirabilite,

    Na2SO410H2O). In this work, the above-mentioned process-

    es are evaluated in the proposed alternative scenarios.

    In this study, the numerical nite element model CODE-

    BRIGHT (Olivella et al., 1994) and the object-oriented module

    CHEPROO (Bea et al., 2009) are applied to simulateow and

    reactive transport through tailings. The rst solves the

    multiphase ow processes in the unsaturated zone while

    the second solves the geochemical processes. Both codes are

    coupled by direct substitution of the chemical equations into

    the transport equations (Saaltink et al., 1998).

    Fig. 4.Evaporation trends of samples CH1-1 (Cl/Na ratio higher than 1), and CH14 (Cl/Na ratio less than 1). (A1 and B1) Evolution of the concentration for Cl, Na

    andcupric species (i.e. Cu2+, CuCl+ and CuCl2). (A2and B2)Evolution of water activity andionic strength.(A3 andB3) Evolution of thesaturation indices forhalite

    (NaCl) and eriochalcite (CuCl22H2O). Evaporation is dened as the ratio between initial and the remaining mass of water after the evaporation step.

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    The domain for reactive transport modeling is 1 m of the

    unsaturated zone. The 1D nite element grid consists of 100

    vertical elements.

    Modeled aqueous species are Cu2+, CuCl+ and CuCl2(aq),

    Ca2+, Mg2+, MgOH+, Al3+, Na+, K+, Fe2+, Fe3+, SO42, HSO4

    ,

    Cl, SiO2(aq), H2O and OH. Virial coefcients for most of the

    ions are taken from (Harvie et al., 1984). Halite and

    eriochalcite solubility in the NaClCuCl2

    system were mea-

    sured by (Filippov et al., 1986). (Haung, 1989) modeled these

    experimental results and provided the best t for the constant

    equilibrium of the two minerals and Pitzer virial coefcients

    between dissolved ions. The same author included copper

    chloride complexes for a better t of experimental solubility.

    Modeled exchange complexes are CaX2, MgX2, CuX2, NaX and

    KX. Due to the absence of experimental exchange coefcients

    in Chaaral clays (mainly vermiculite and illite), we have

    tentatively used the selectivity coefcients given by (Appelo

    and Postma, 1993), and performed a sensitivity analysis of the

    inuence of these data on the nal results.

    The main reactions considered in the geochemical model

    are listed in Table 3. Homogeneous reactions are assumed to be

    in equilibrium except for Fe(II) oxidation, which is modeled

    using a modied kinetic expression provided by (Singer and

    Stumm, 1970). Once the oxidation rates of suldes have been

    dened in the model, the evolution of iron in the pore-water

    could only be made to t by calibrating simultaneously the

    scaling factor for rates of Fe(II)-oxidation and the precipitation

    of goethite and K-jarosite.A factorequal to 107 times the abiotic

    Fe(II)-oxidation rate is applied, which indicates that Fe(II)-

    oxidation in the pore-water is biocatalyzed.

    Fig. 5. Cl/Na ratio for water samples collected in boreholes CH1, CH2 and

    CH3. Besides sea water, only three samples display a Cl/Na ratio higher than

    1. Two of them are located in the upper part of the oxidation zone, below the

    evaporation front. The third is located in the brine, in the deepest part of the

    tailings.

    Table 3

    Reactions considered in the model. Equilibrium constants are taken of EQ3

    data base (Wolery and Daveler, 1992) at 25 C.

    Reaction

    Homogeneous

    HSO4

    H+ + SO42

    MgOH+ + H+H2O+Mg2+

    OH+H+H2O

    Fe2 +0.25O2(aq)+H+Fe3+ +0.5H2O

    CuCl+Cu2+ + Cl a

    CuCl2(aq)Cu2+ +2Cl a

    Cation-exchange

    CuX2 +2Na+2NaX+Cu

    2+ b

    MgX2 +2Na+2NaX+Mg2+ b

    CaX2 +2Na+2NaX+Ca2+ b

    KX+Na+NaX+K+ b

    Dissolution/precipitation

    Pyrite+3.5 O2(aq)+H2O2 SO42 + Fe+2 +2H+

    Pyrite+14Fe3++ 8H2O2SO42 +15Fe+2 +16H+

    Chalcopyrite+4O2(aq)2 SO42+17Fe2+ +Cu2+16H+

    Chalcopyrite+16Fe 3+ + 8H2O2SO42+17Fe2+Cu2+ +16H+

    Albite+4.2H+2.95 SiO2(aq)+ 1.05 Al3+ +0.95Na+ +0.05Ca2+

    +2.1 H2O

    Anorthite+8H+2 Al3+ +2SIO2(aq)+Ca2+ + 4H2O

    EriochalciteCu2+ +2Cl+ 2H2O a

    HaliteNa+ + Cl a

    SylviteK+ +Cl

    Biotite+10H+3Al3+ +3SiO2(aq)Fe2+ + K+ +2Mg2+ +6H2OMuscovite+10H+3Al3+ +3SiO2(aq)+K

    + + 6H2O

    Geothite+3H+Fe3+ + 2H2O

    QuartzSiO2(aq)

    GypsumCa2+SO42+2H2O

    MirabiliteSO42+2Na+ +10H2O

    Kaolinite+6H+2Al3++2SiO2(aq)+5H2O

    Pickeringite2Al3+ + Mg2+ +4SO42+22H2O

    K-jarosite+6H+K+ +2 SO42+3 Fe3+ + 6H2O

    (K,Na)-jarosite+6H+0.5Na+ +0.5 K+ +2 SO42+3 Fe3++ 6H2O

    HexahydriteMg2+ +Fe2+ +SO 42+ 6H2O

    Halotrichite2Al3+ + Fe2+ +4SO42+22H2O

    Gas dissolution/exsolution

    O2(g)O2(aq)

    a

    Equilibrium constants taken fromHaung (1989).b Selectivity coefcients taken fromAppelo and Postma (1993).

    Table 4

    Summary of kinetic expressions used in the model.

    Reaction process Rate expression (mol m2 s1) Ref.

    Pyrite oxidation

    (oxygen path)

    R =108.19aH+0.11aO2(aq)

    0.5 (1) a

    Pyrite oxidation

    (Fe(III) path)

    R =106.7aFe3+0.93 aFe2+

    0.4 (1) a

    Chalcopyrite oxidation

    (oxygen path)

    R =1010.58aH+0.15 (1) b

    Chalcopyrite oxidation

    (Fe(III) path)

    R =106.75aFe3+0.43 (1) c

    Fe(II) oxidation R =103aO2(aq) (1) d

    Albite dissolution R =109.17aH+0.5 (1) e

    Anorthite dissolution R =109.17aH+0.5 (1) f

    Muscovite dissolution R =101223aH+0.38 (1) g

    Quartz dissolution R =1013.38 (1) h

    Kaolinite precipitation R =(1010.77aH+0.5 + 10166aH+

    0.3)(1) i

    Goethite precipitation R =10

    11(1) jK-jarosite precipitation R =104(1) j

    (K,Na)-jarosite

    precipitation

    R =104(1) j

    Biotite dissolution R =(108.5aH+0.57 + 1014.1aH+

    0.29)(1) k

    a Williamson and Rimstidt (1994).b Acero et al. (2007).c Rimstidt et al. (1994).d Modied after Singer and Stumm (1970), calibrated to reproduce

    observed iron evolution.e Chou and Wollast (1985).f Equal to albite.g Kalinowski and Schweda (1996).h Tester et al. (1994).i Nagy et al. (1991).j

    Calibrated to reproduce observed iron evolution.k Malmstrom and Banwart (1997).

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    Mineral dissolution reactions are modeled using kinetic laws.

    The kinetic rates presented inTable 4are based on the general

    expression presented byLasaga et al. (1994). Most secondary

    phasesareconsideredto precipitatein equilibrium.Theseinclude

    halite, eriochalcite, sylvite, gypsum, mirabilite, halotrichite,

    hexahydrite and pickeringite. K-jarosite, goethite and kaolinite

    are considered to precipitate kinetically (seeTable 4).

    Dissolved oxygen is modeled in equilibrium with the

    partial pressure of oxygen gas in pores (pO2 = 0.21 atm).

    A mixture of suldes (mainly pyrite and chalcopyrite) and

    aluminosilicates (mainly quartz, muscovite, biotite, and pla-

    gioclase) is considered as initial mineralogy. Their initial min-

    eral fractions are presented inTable 5. The volumetric fraction

    occupied by each mineral is calculated from its weight fraction

    by considering its density. Weight fractions are estimated from

    sequential extractions and mineralogical descriptions reported

    by (Dold, 2006). A total reactive surface corresponding to silty

    grain size tailings is considered (104 m2 m3). It is proportion-

    ally distributed in accordance with the volumetric fraction of

    each mineral phase. A vermiculite content of 3 wt.% is assumed

    in the model. Thus, the total exchange capacity considered in

    the calculations is computed from this clay content and the

    exchange capacity of Jeffersite vermiculite (Foscolos, 1968).

    The chemical composition of the initial and boundary

    solutions is shown inTable 6.

    3.3. Simulated scenarios

    Six scenarios (shown in Fig. 6) are simulated to account

    for the different genetic hypotheses about the formation of

    eforescences. The aim is to obtain a Cl/Na ratio higher than 1

    in the pore-water, while using the observed types of water.

    Sea water is imposed at the bottom in Scenarios I and II

    (SWCE and SW, with/without the cation-exchange, respec-

    tively), thus implying a sea water wedge reaching the inner

    portion of the tailings, which may well have been the case

    during early sedimentation. Mixtures (mixing proportion

    = 0.5) of sea water/freshwater and brine/freshwater are

    considered for Scenarios III and IV (SFWCE and BFWCE),

    respectively. Cation-exchange is also considered in both

    scenarios.

    There are situations in which the Cl/Na ratio is less than 1

    in the original groundwater composition and can be reversed

    through cation-exchange, or by adding marine aerosol. Both

    cases are tested in Scenarios V and VI (FWCE and FWMASL),

    respectively. With regard to the latter, a slow, constant ow

    of sea water (20 mm year1, its chemical composition is

    described in Table 6) is imposed at the upper 0.1 m of the

    model.

    4. Modeling results and discussion

    All simulations are run for thirty-two years, beginning

    after discharges from the El Salvador were stopped in 1975

    (period 19752007).

    Scenario I (SWCE) is chosen as the base case. Therefore,

    we thoroughly describe its features and results in the fol-

    lowing sections. Later, the remaining scenarios are analyzed

    and compared.

    Table 5

    Initial conditions. Summary of initial volumetric fraction and reactive surface

    used in the reactive transport model.

    Mineral phase vol.% Initial surface area (m2 m3)

    Pyrite 0.39 130

    Chalcopyrite 0.32 108

    Anorthite 18 5852

    Albite 6.8 2277

    Quartz 24 8231

    Goethite 0.18 61

    Muscovite 1.7 576

    Biotite 2.5 845

    Kaolinite 5.8 1920

    Gypsum 0 0

    Sylvite 0 0

    Halite 0 0

    Eriochalcite 0 0

    Mirabilite 0 0

    Pickeringite 0 0

    Hexahydrite 0 0

    (K,Na)-jarosite 0 0

    K-jarosite 0 0

    Halotrichite 0 0

    Total 60 20,000

    Table 6

    Chemical composition of initial, marine aerosol and boundary waters (mol kg w1).

    Initial solution Scenarios I, II and marine

    aerosol (sea water)

    Scenario III

    (0.5 sea-water+0.5 freshwater)

    Scenario IV

    (0.5 brine+0.5 freshwater)

    Scenarios V and VI

    (freshwater)

    pH 7.48 7.48 7.41 7.45 7.03

    Fe 6.35106 4.8106 6.8105 7.5104

    Cu 104 103 2.1105 8.0106 9.4106

    Zn 7.64108 104 9.0105 1.6106

    Ca 104 9.8103 1.06102 2.23102 1.1102

    Mg 107 5.2102 2.9101 8.7101 6.2103

    Na 107 5.0101 3.5101 1.4102 2101

    K 107 1.07102 7.21103 4.8106 3.7103

    Cl 5.75 101 5.75101 3.69101 8.7101 1.6101

    SO4 2.9102 2.9102 2.73102 2.27102 2.5102

    O2 2.5104

    Si

    Al

    Ionic strength 0.347 0.726 0.5 1.01 0.27

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    Fig. 6. Simulatedscenarios according to thecomposition ofthe water imposed at thebottom. Legend: S = seawater;F = freshwater; B = brine; W = water; MASL =

    marine aerosol; CE = cation-exchange.

    Fig. 7.Scenario I (SWCE): Vertical distribution of (A) temperature (C), (B) salinity, (C) water activity, and (D) pore saturation, at the last winter/summer.

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    4.1. Thermohydraulic evolution in Scenario I (SWCE)

    Spatial distribution of temperature, salinity, water activity

    and pore saturation are shown inFig. 7. The time evolution of

    temperature, evaporation rate and energy balance are plotted

    inFig. 8.

    As expected, these parameters uctuate seasonally. The

    tailings surface temperature declines in the winter as solar

    radiation and air temperature do the same (Figs. 7A and 8).

    This temperature: (1) is always higher than the atmosphere

    temperature, and (2) increases during the summer (approx-

    imately 3 C) and over time (Fig. 8A). Both observations are

    explained by the energy balance at the upper boundary

    (Fig. 8B). Net radiation is at its maximum and most of the

    inowing radiation is used in evaporating water. However,

    the mean evaporation rate decreases over time as a

    consequence of the increase in salinity of the pore-water.

    Thus, the latent heat ux (invested in evaporation) declines

    over years. To maintain the heat balance, the sensible heat has

    to be increased (Fig. 8B), which requires increasing the

    surface/air temperature differential (Fig. 8A). The evapora-

    tion is produced during the summer, but in the winter thereis

    slight condensation (Fig. 8B).

    During the summer as a consequence of the high level of

    evaporation (Fig. 7B), salinity increases in the uppermost

    portion of tailings. However, during the winter, salinity

    decreases slightly or undergoes a slight increase at the top

    of tailings.

    An opposite evolution is predicted for water activity

    (Fig. 7C). It decreases in the uppermost portion of tailings due

    to an increase in salinity during the summer. However, it

    increases at the top of tailings during the winter. It decreases

    slightly between 0.1 m and 0.5 m below the surface during

    the same season.

    The water saturation prole (Fig. 7D) shows that the

    water saturation reached a steady-state prole. The satura-

    tion declined from the initial saturated state to about Sl =0.68

    at the top andSl =0.99 at the base.

    4.2. Evolution of pore-water chemistry in Scenario I (SWCE)

    Vertical proles for Cl, K, Ca, SO4, Cu, Na and pH in the last

    winter/summer are shown in Fig. 9A to G. In general,

    concentrations of ions increase in the oxidation zone,especially at the top. As expected, seasonal uctuations are

    predicted for them. Concentrations of solutes decrease during

    Fig. 8. Scenario I (SWCE): (A)the time evolutionof temperature in theatmosphere andtailings. (B)The time evolutionof evaporation rate andenergy uxesin thetailings.

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    Fig. 9.Scenario I (SWCE): Vertical proles of the main species at the last winter/summer. (A) Cl, (B) K, vertical distribution corresponding to Scenario II (SW) isalso shown, (C) Ca, vertical distribution corresponding to Scenario II (SW) is also shown, (D) pH, (E) SO 4, (F) Cu, and (G) Na.

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    the winter in the upper part, but increase slightly below the

    evaporation front (between 0.1 m and 0.5 m, e.g. see Cl in

    Fig. 9A). Similar behavior is also predicted for Na, K, Cu, Ca,Mg, Al, Zn, Fe(total) and SiO2(aq). However, SO4 shows

    different behavior. It decreases its concentration in the upper

    part of the model during the summer (seeFig. 9E).

    pH is found to decrease in tailings as a consequence ofsulde oxidation (Fig. 9D). It increases sharply to neutral

    Fig. 10.Temporal evolution of eforescences obtained from probable scenarios: (A) Scenario I (SWCE), (B) Scenario III (SFWCE), and (C) Scenario IV (BFWCE).

    Vertical distribution of mineral volumetric contents in the last summer: (D) Pyrite and chalcopyrite, (E) geothite and K-jarosite, and (F) gyspum and kaolinite.

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    values below the oxidation front (located 0.8 m below the

    surface). pH increases slightly in the upper part of the model

    during the winter, and the oxidation front rises 0.1 m in the

    same season. The concentration of K decreases within the

    oxidation zone due to precipitation of K-jarosite and its

    exchange onto the clay fraction (Fig. 9B). Ca concentration

    increases mainly due to the exchange with Na and limited

    plagioclase dissolution (Fig. 9C).

    In general, concentration and pH proles are consistent

    with eld observations. The total concentration of Cu

    predicted after thirty two years is one order of magnitude

    higher than eld observations (Fig. 9F). Other processes (not

    considered in this model) could probably explain Cu

    depletion in the pore-water. For instance, the adsorption of

    Cu onto secondary Fe-oxides/hydroxides (i.e. onto goethite

    and K-jarosite, see Cu(ox) inTable 1). Although the trend ts

    the experimental one, the predicted concentrations of Cl are

    clearly higher than measured. A possible explanation for the

    calculated high Cu and Cl concentrations could also be an

    insufciently accurate solubility value for eriochalcite in such

    complex solutions.

    4.3. Precipitation of secondary phases and suldes oxidation in

    Scenario I (SWCE)

    Eforescences precipitate in the upper part of the model

    (Fig. 10A). However, seasonal variation in them is predicted.

    This process of formation starts in the summer and partial

    dissolution (total in the case of eriochalcite) is produced

    during the winter. The total dissolution of eriochalcite was

    veried in Chaaral tailings during the winter of 2008.

    Eriochalcite was only identied in eforescence samples

    collected during the summer.

    Halite increased over time, whereas eriochalcite almost

    reached a constant value (between 15 and 25 mol m3).

    Thus, the halite/eriochalcite ratio observed during the

    summer increased over time from 10 to 70 after thirty-two

    years.

    Goethite and K-jarosite form at the expense of Fe(II)

    oxidation (Fig. 10E). Their precipitated amount is consistent

    with that observed in Chaaral (0.07 wt.% K equivalent for K-

    jarosite). In agreement with the eld observations, gypsum

    (CaSO42H2O) and kaolinite (Al2Si2O5(OH)4) form through-

    out the oxidation zone (Fig. 10F). Kaolinite forms as a product

    of the dissolution of aluminosilicates (i.e. muscovite, biotite,

    and plasgioclase) in an acidic environment. Gypsum is mainly

    predicted in the upper part of the model, and its amount

    (150 mol m3) is consistent with Ca measured in the soluble

    fraction of soil samples (see Ca(sol) inTable 1).

    Pyrite and chalcopyrite oxidation is predicted in the

    model. However, a proportion of chalcopyrite remained

    after thirty-two years (Fig. 10E) despite the fact that it was

    practically exhausted in the analysis of the tailings (see Cu

    (sph) inTable 1). Due to the uncertainty in its initial value, it

    is probable that chalcopyrite was overestimated in the initial

    condition (1.2 pyrite and 0.8 chalcopyrite equivalent). Based

    on sequential extractions and assuming that suldes were

    preserved by the oxidation processes below the water-table, a

    lower initial proportion of pyrite and chalcopyrite equivalent

    could be considered (0.65 pyrite and 0.15 chalcopyrite). Chal-copyrite is exhausted in a simulation taking the latter wt.%

    as initial conditions after thirty-two years. After thirty-two

    years, all silicate proles remain essentially unchanged from

    their initial proles. However, the sum of all mineral volume

    changes induces a net mineral volume gain, which results in a

    maximum porosity decrease of about 0.3% mainly in the upper

    part with virtually no change in other parts (not represented).

    4.4. Analysis of scenarios

    The precipitation of halite is predicted in all scenarios in

    the upper part of the model. However, precipitation of

    eriochalcite is only reached in scenarios I (SWCE), III (SFWCE)

    and IV (BFWCE) (Fig. 11). The time evolution of halite and

    eriochalcite for these scenarios is displayed in Fig. 10A to C.

    Notice that cation-exchange is considered in all three scenarios.

    In Scenario II (SW), precipitation of eriochalcite is in-

    hibited in several ways. First, the saturation rate of eriochal-

    cite is reduced as a consequence of Cl consumed by halite

    precipitation (i.e. geochemical divide, Fig. 4B2). Second,

    water activity decreased quickly in the upper part of the

    model due to high concentrations of other major ions such asMg and K, further preventing the saturation of eriochalcite. As

    shown in the previous section, the evaporation rate decreases

    for low values of water activity. Due to the high concentra-

    tions of K and Mg, the precipitation of other KMg salts such

    as silvite (KCl) and hexahydrite (MgFe(SO4)26H2O) is

    predicted.

    No secondary KMg minerals precipitated in scenarios

    with cation-exchange. In these cases, as a result of the ex-

    change between Mg2+ and K+ by Ca2+, hexahydrite and

    silvite did not reach saturation.

    Other eforescences are associated with halite in the

    scenario affected by marine aerosol (Scenario VI (FWMASL),

    mirabilite and silvite). None of these associated efores-cences have been found in Chaaral.

    Eriochalcite is also inhibited in Scenario V (FWCE) because

    its Cl/Na ratio continuously decreases in the pore-water. This

    is enhanced by the Cl/Na ratio of its boundary water (b1) and

    cation-exchange processes.

    After thirty-two years, scenarios III (SFWCE) and IV

    (BFWCE) predicted larger amounts of halite (Fig. 10B and C,

    approximately 1400 and 2200 mol m3, respectively). How-

    ever, a similar precipitated amount is predicted for eriochalcite

    Fig. 11. Evolution of the saturation index of eriochalcite (CuCl22H2O) as a

    function of water activity from different scenarios. Eriochalcite precipitationis only reached in Scenarios I (SWCE), III (SFWCE) and IV (BFWCE).

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    in all thesescenarios (between20 and 25 mol m3). Therefore,

    in both scenarios III and IV, the halite/eriochalcite ratio is much

    larger than observed.

    The time evolution of evaporation/condensation rates

    obtained from different scenarios are shown inFig. 12. All of

    them present a similar trend (i.e. the evaporation is produced

    during the summer, while there is slight condensation in the

    winter). However, some differences are predicted in Scenar-

    ios I (SWCE) and II (SW) in spite of the fact that sea water is

    imposed in both scenarios. The evaporation rate trend is

    mainly controlled by the water activity and eforescence

    evolution at the evaporation front. As seen above, different

    eforescences are predicted for both scenarios (i.e. halite

    eriochalcite and halitesilvitehexahydrite in Scenarios I

    (SWCE) and II (SW), respectively). The evolution of these

    eforescences is different and consequently, so is the evolu-

    tion of evaporation rates.

    The scenario affected by marine aerosol (Scenario VI,

    FWMASL) predicts a higher evaporation rate. The dissolution/

    precipitation of eforescences (i.e. halitesilvitemirabilite)

    controls the evolution of evaporation rates.

    4.5. Sensitivity analysis in Scenario I (SWCE)

    In order to gain further insight into the hydrogeochemical

    behavior of the Chaaral tailings, and to address parameter

    uncertainty, several additional simulation scenarios are run

    using Scenario I (SWCE) as the base case. Therefore, the

    following parameters are tested: (1) the grain size of tailings,

    (2) the radiation on the tailings surface, (3) the wt.% to the

    clay fraction, (4) the order of selectivity (i.e. through

    selectivity coefcients) for cation-exchange, and (5) the

    inuence of the tidal cycle.

    The results are compared with data on: (1) ef

    orescenceratios (i.e. halite and eriochalcite), (2) the pore-water

    chemistry, (3) the precipitated amount of secondary phases

    described in Chaaral (i.e. gypsum, K-jarosite, goethite,

    kaolinite), (4) the formation of eforescences not previously

    described in Chaaral (e.g. silvite, hexahydrite, mirabilite),

    and (5) the dissolution of suldes (i.e. pyrite and chalcopy-

    rite), and aluminosilicates (i.e. biotite and muscovite).

    With regard to sensitivity to grain size (i.e. varying the

    retention curve), sandy tailings are modeled. As set out above,

    sandy tailings are characteristic toward the sea. The base case

    is repeated here using the same geometry and mineralogy,

    but with a modied water retention curve for tailings

    (P0 =0.002 (MPa) and =0.6 for Van Genuchten parameters

    inTable 2). The modication had the effect of reducing the

    water retention capacity of tailings. As a consequence of

    evaporation, the liquid saturation decreases signicantly in

    the upper part, and the evaporation front is located

    approximately ve centimeters below the surface. As a

    consequence of this, the evaporation rate also decreases

    during the summer. Major ions such as Mg, Na and K are

    strongly exchanged onto the clay fraction and their concen-

    trations decrease in the pore-water. Cl concentration

    increases signicantly at the top, so eriochalcite saturation

    is immediately achieved. An amount similar to the base case

    is predicted for this eforescence. However, halite saturation

    occurs one year later as a consequence of the retardation in

    the Na front from groundwater. The halite/eriochalcite ratio

    reaches 1 during summers, a much lower ratio than observed.

    Only a minor amount of other secondary phases is predicted

    (i.e. gypsum, goethite, K-jarosite) due to the lower availabil-

    ity of K and SO4 from the groundwater. A clear sky means

    greater solar radiation on the tailings surface and increased

    evaporation. It affects mainly the amount of halite and

    eriochalcite (the precipitate almost doubled) but not their

    relative proportion (halite/eriochalcite). It also increases,

    however, the K concentration in the pore-water to much

    higher values than observed. Due to the higher evaporation

    rate in relation to the precipitation rate of K-jarosite, the K

    concentration increases in the pore-water.

    Low and high clay contents are evaluated (0.3 wt.% and

    30 wt.%, respectively). Each one is implemented in the model

    using the CEC (Cation-Exchange Capacity) parameter. A

    similar geochemical evolution is obtained for low CEC as in

    Scenario II (SW) (scenario without cation-exchange). How-

    ever, approximately 100 mol m3 of eriochalcite is predicted

    for high CEC. In this case, Na+ is strongly exchanged onto the

    clay fraction, increasing the Cl/Na ratio in the pore-water.

    Thus, saturation of halite is reached two years later. The

    precipitated halite/eriochalcite ratio is approximately 1,

    which is much lower than observed.

    Each type of clay has its own order of cation-exchange

    preference (i.e. order of selectivity). The order of selectivity

    used in the base case was typical for illite (K+NCa2+N(Cu2+,

    Mg2+)NNa+). However, a different order of selectivity was

    suggested by other clays (Foscolos, 1968). This varies

    according to selectivity coefcients. Sensitivity analysis was

    carried out on the NaCu selectivity coefcient in order to

    obtain two orders of selectivity: 1) Cu2+NK+NCa2+NMg2+N

    Na+ (high afnity for Cu2+), and 2) K+NCa2+NMg2+NNa+N

    Cu2+ (low afnity for Cu2+). The concentrations of Na+ and

    Cu2+ were modied in the initial solution in order to obtain

    the same exchanged equivalent fractions (i.e. for NaX and

    CuX2) as the base case simulation. When Cu2+ is strongly

    exchanged onto the clay its availability in solution is depleted,

    and a maximum of 15 mol m3 of eriochalcite is predicted to

    form. When the afnity of Cu2+ in the exchange complex is

    low the opposite behavior is obtained, and precipitation of

    32 mol m3 of eriochalcite is predicted. Therefore, although

    there are differences, the resulting halite/eriochalcite ratiosvary within the same order of magnitude with the selectivityFig. 12.The time evolution of evaporation rates on the tailings surface fromdifferent scenarios (period 19761980).

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    coefcients for Cu2+. In all cases, exchanged copper decreases

    with ionic strength, primarily attributed to formation of metal

    chlorides (mainly CuCl+, CuCl2(aq)), as was veried exper-

    imentally with vermiculite (El-Bayaa et al., 2009).

    Regarding sensitivity to the tidal cycle, a tidal oscillation of

    0.5 m is imposed at the lower boundary. In this case, a higher

    hydrodynamic dispersion is induced by tides and saturation

    of halite and eriochalcite is reached much later than for the

    base case. However, once saturation is reached, the tidal cycle

    did not signicantly affect the evolution and mineral propor-

    tion of the eforescences in the upper part of the system.

    4.6. Remediation alternative

    In general, remediation strategies on tailings are con-

    cerned with the capacity of the systems to minimize water

    and oxygen percolation towards the bulk of tailings. How-

    ever, our remediationstrategy focuses mainly on reducing the

    evaporation rate on the tailings surface and then preventing

    eforescence precipitation. Therefore, a capillary barrier is

    proposed as a suitable alternative (Melchior et al., 1993). This

    would consist of two layers overlying tailings (seeFig. 13A):

    (1) a coarse sand layer (i.e. drainage layer), and (2) a geo-

    membrane. The latter has two main purposes: (a) to isolate

    the capillary barrier from the acid mine drainage system, and

    (b) to prevent oxygen percolation toward the tailings. The

    former could reduce the evaporation rate as a consequence of

    its low water content and thermal conductivity. On the other

    hand, this cover design might provide an additional organic

    soil layer for the development of vegetation (in the present

    conditions, vegetation does not grow on tailings due to the

    acidic conditions).

    The proposed cover design is evaluated through reactive

    transport modeling. Thus, the base case mesh was extended

    in order to simulate 0.15 m drainage layer and a thick geo-

    membrane. Their main physical parameters were (see Table 2

    for reference): intrinsic permeabilities, 1014 and 1020 (m2),

    respectively; retention curve parameter P0, 0.002 and 0.0001

    (MPa), respectively; retention curve parameter n, 0.6 and

    0.19 (), respectively; and thermal conductivity sol, 0.16

    (W m1 K1) for both layers.

    Regarding the results, evaporation is dramatically re-

    duced thus preventing eforescence formation (see the tem-

    poral evolution of the saturation index for eforescences in

    Fig. 13B).

    5. Concluding remarks

    Although eforescence formation on tailings is common in

    hyperarid climates, natural occurrence of eriochalcite is rare.

    According to the modeling exercise described above, this is

    due to the fact that several environmental and geochemical

    constraints are required for its precipitation. A high level of

    evaporation and low relative humidity (Hr) have to be

    reached. These parameters control water activity evolution

    in the pore-water chemistry. Therefore, eforescences form

    mainly during the summer when the relative air humidity is

    low and solar radiation is high, whereas their dissolution is

    produced during the winter when relative humidity increases

    and light condensation is produced on the tailings surface.

    The modeled result was veried during a visit to Chaaral

    tailings during the winter of 2008. Eriochalcite could only be

    collected as eforescence during summer.

    With regard to geochemical conditions, the Cl/Na ratio is a

    key parameter in the formation of eriochalcite. The strong

    competition of other cations for Cl may form halite and

    sylvite, and inhibit the precipitation of eriochalcite. Precipi-

    tation of halite creates a geochemical divide, allowing either

    Cl orNa+ concentrations to increase, depending on whether

    the Cl or Na+ concentration is higher in the pore-water.

    Fig. 13. Remediation alternative: capillary barrier on tailings. (A) Cover design (Melchior et al., 1993). (B) Temporal evolution of the saturation index foreforescences on the tailings surface considering and not considering the capillary barrier.

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    Eriochalcite forms only in those samples with a Cl/Na ratio

    higher than 1. Three mechanisms are proposed to obtain a

    higher Cl/Na ratio: (1) the exchange of Na+ by Ca2+, Mg2+,

    Cu2+ and K+ onto a vermiculite-type mixed-layer, (2) the

    inuence of the marine aerosol on the tailings surface, and

    (3) the precipitation of secondary Na phases. According to the

    mineralogy and solute concentration proles of the different

    modeling scenarios, cation-exchange is the most likely mech-

    anism to obtain a higher Cl/Na ratio in the Chaaral tailings.

    In fact, it is also supported by analytical evidence: (1) a sig-

    nicant fraction of Cu, Na, and Ca were exchanged at least in

    the oxidation zone of these tailings (e.g. see Cu(ex), Na(ex)

    and Ca(ex) inTable 1). In the case of Cu, it may be released

    from this vermiculite-type mixed-layer mineral from samples

    in the low pH oxidation zone (Dold, 2003), (2) water samples

    collected in the oxidation zone (below the evaporation front,

    corresponding to boreholes CH1, CH2 and CH3) present a

    Cl/Na ratioN1.In thiscase, noNamineral phases precipitate in

    this zone, and only cation-exchange processes could explain

    these ion ratios. With regard to the probable scenario for the

    formation of these eforescences, a scenario with two stages is

    proposed: a rst stage involving sea water (Scenario I (SWCE),

    or a mixture of sea water/freshwater (Scenario III (SFWCE)) in

    the groundwater composition, and a second stage with the

    intrusion of freshwater. The rst stage is based on the amount

    of eriochalcite formed, whereas the freshwater intrusion is

    required to explain the observed halite/eriochalcite ratio and

    the vertical concentration distribution in therst 0.5 m above

    the water-table.

    Sensitivity analysis of different physical and geochemical

    parameters is evaluated in the model. The result is particu-

    larly sensitive to the clay content, because Na exchanged and,

    then the Cl/Na ratio increases with the clay content. As a

    result of this, a higher amount of eriochalcite is predicted and

    a halite/eriochalcite ratio lower than observed. The model is

    less sensitive to the cation-exchange selectivity coefcients.

    Thus, although higher afnity for Cu2+ in the exchange

    complex decreases the amount of eriochalcite formed, the

    variations in the halite/eriochalcite ratio are kept close to the

    base case value.

    Moreover, the model is also sensitive to grain size. Thus, for

    more sandy tailings, theliquid content in the uppermost part of

    the model is markedly reduced. Then, eriochalcite precipitates

    immediately and a lower evaporation rate is predicted.

    Therefore, less capillary transport and precipitation of second-

    ary mineral phases (i.e. gypsum, goethite and K-jarosite) are

    predicted in the oxidation zone. However, for consistence

    between grain size and clay content, the latter should be

    reduced, and eriochalcite formation decreases accordingly.

    On the other hand, the model is not particularly sensitive to

    the tidal cycle. In this case, major hydrodynamic dispersion in

    the oxidation zone is predicted but it did not signicantly affect

    the evolution of eforescences in the upper part of the model.

    With regard to preventing the formation of eriochalcite, a

    capillary barrier on the tailings surface is proposed as a suitable

    alternative (previous excavation of precipitated efores-

    cences). Its efciency as a barrier is also tested through reactive

    transport (approximately 0.15 m in thickness was considered

    in the simulation). Precipitation of eriochalcite is inhibited

    because evaporation rate on the tailings surface is dramaticallyreduced.

    Acknowledgments

    This work was partially funded by a point action CSIC/

    CONYCIT (20082009), the project CTM2007-66724-C02/

    TECNO of the Spanish Government, and Swiss National Science

    Foundation projects No. 200020-117792/1 and 200021-

    105507/1. Thanks are also to anonymous reviewer for the

    valuable comments and suggestions that have signicantly

    improved thenal version of the paper.

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