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Journal of Petrology Advance Access originally published online on December 10, 2004
Journal of Petrology 2005 46(2):339-354; doi:10.1093/petrology/egh078
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Journal of Petrology vol. 46 issue 2 © Oxford University Press 2004; all rights reserved

Experimental Petrology of the 1991–1995 Unzen Dacite, Japan. Part II: Cl/OH Partitioning between Hornblende and Melt and its Implications for the Origin of Oscillatory Zoning of Hornblende Phenocrysts

HIROAKI SATO1,*, FRANCOIS HOLTZ2, HARALD BEHRENS2, ROMAN BOTCHARNIKOV2 and SETSUYA NAKADA3

1 DEPARTMENT OF EARTH AND PLANETARY SCIENCES, FACULTY OF SCIENCE AND GRADUATE SCHOOL OF SCIENCE AND TECHNOLOGY, KOBE UNIVERSITY, KOBE, 657-8501 JAPAN
2 INSTITUTE FOR MINERALOGY, UNIVERSITY OF HANNOVER, WELFENGARTEN 1, D-30167, HANNOVER, GERMANY
3 EARTHQUAKE RESEARCH INSTITUTE, UNIVERSITY OF TOKYO, YAYOI 1-1-1, BUNKYO, TOKYO, 113-0032 JAPAN

RECEIVED NOVEMBER 10, 2002; ACCEPTED AUGUST 11, 2004


    ABSTRACT
 TOP
 ABSTRACT
 INTRODUCTION
 PETROGRAPHY AND PHASE CHEMISTRY...
 EXPERIMENTAL STUDY
 DISCUSSION
 REFERENCES
 
High-temperature–pressure experiments were carried out to determine the chlorine–hydroxyl exchange partition coefficient between hornblende and melt in the 1992 Unzen dacite. Cl in hornblende and melt was analyzed by electron microprobe, whereas OH in hornblende and melt was calculated assuming anion stoichiometry of hornblende and utilizing the dissociation reaction constant for H2O + O = 2(OH) in water-saturated melt, respectively. The partition coefficient strongly depends on the Mg/(Mg + Fe) ratio of hornblende, and is expressed as ln K1 = (Cl/OH)hb/(Cl/OH)melt = 2·37 – 4·6[Mg/(Mg + Fe)]hb at 2–3 kbar and 800–850°C. The twofold variation in Cl content in the oscillatory zoned cores of hornblende phenocrysts in the 1991–1995 dacite cannot be explained by the dependence of the Cl/OH partition coefficient on the Mg/(Mg + Fe)hb ratio, and requires c. 80% variation of the Cl/OH ratio of the coexisting melt. Available experimental data at 200 MPa on Cl/OH fractionation between fluid and melt suggest that c. 1·2–1·8 wt % degassing of water from the magma can explain the required 80% variation in the Cl/OH ratio of the melt. The negative correlation between Al content and Mg/(Mg + Fe) ratio in the oscillatory zoned cores of the hornblende phenocrysts is consistent with repeated influx and convective degassing of the fluid phase in the magma chamber.

KEY WORDS: chlorine; element partitioning; hornblende; oscillatory zoning; Unzen volcano


    INTRODUCTION
 TOP
 ABSTRACT
 INTRODUCTION
 PETROGRAPHY AND PHASE CHEMISTRY...
 EXPERIMENTAL STUDY
 DISCUSSION
 REFERENCES
 
Compositional zoning in phenocryst minerals in volcanic rocks may record various magmatic processes. Oscillatory zoning has been interpreted as a consequence of kinetically controlled oscillation in crystal growth (e.g. Haase et al., 1980Go), repeated replenishment of the magma chamber (e.g. Davidson & Tepley, 1997Go), intermittent turbulent mixing of the chamber by tidal oscillation (Anderson, 1984Go), and boundary layer convection and mixing (Nakada et al., 1994Go). Patchy zoning (sieve texture) is another story and may be formed by rapid cooling (Kawamoto, 1992Go), rapid decompression (Nelson & Montana, 1992Go), or dissolution of crystals at hyperliquidus conditions (Nakamura & Shimakita, 1998Go). Minor element behaviour often helps to resolve the processes of compositional variation in minerals (e.g. Blundy & Shimizu, 1991Go), although there are possible effects of diffusion in modifying trace element zoning in minerals, as recently demonstrated for Mg in plagioclase (Costa et al., 2003Go). During the course of petrographic examination of the 1991–1995 dacite of Unzen volcano, Japan, we observed oscillatory, patchy and reverse zoning in the hornblende phenocrysts in back-scattered electron images, which reflects the variation of Mg/(Mg + Fe) ratio in the hornblende. We further identified correlations among Cl, Al, Mg and Fe in the oscillatory zoned cores of the hornblende phenocrysts. The chlorine content of the oscillatory zoned cores of the hornblende phenocrysts in the Unzen dacite varies from 0·035 to 0·075 wt %.

Chlorine is strongly partitioned into any fluid phase separating from magmas (Shinohara, 1994Go), and, if the distribution coefficients between minerals and melt are known, can be utilized to reveal the degassing history of magmas through the analysis of chlorine zoning in Cl-bearing minerals. Icenhower & London (1997)Go experimentally determined the distribution coefficient of Cl and F between biotite and silicic melt at 800°C and 200 MPa, and showed their strong dependence on the Mg/(Mg + Fe) ratio of biotite. The strong effect of Mg/(Mg + Fe) ratio of biotite and hornblende on the distribution of Cl and F has been predicted from crystal-chemical considerations (Volfinger et al., 1985Go; Oberti et al., 1993Go); that is, the large anionic size of chlorine (181 pm; Shannon & Prewitt, 1969Go) is readily accommodated in the crystal lattice of Fe-rich biotite and amphibole.

In this study, we describe the compositional zoning of hornblende in the 1991–1995 Unzen dacite. Then, we present experimental results for partitioning of Cl–OH between hornblende and melt in dacitic systems. Based on the experimental results, we evaluate quantitatively the processes responsible for the Cl zoning observed in hornblende phenocrysts in the 1991–1995 Unzen dacite.


    PETROGRAPHY AND PHASE CHEMISTRY OF HORNBLENDE IN UNZEN DACITE
 TOP
 ABSTRACT
 INTRODUCTION
 PETROGRAPHY AND PHASE CHEMISTRY...
 EXPERIMENTAL STUDY
 DISCUSSION
 REFERENCES
 
Host rocks
The 1991–1995 eruption of Unzen volcano was mostly effusive with extrusion of viscous magmas accompanied by numerous collapse-type pyroclastic flows. Only two vulcanian explosions were recorded in the early stages of the activity (Nakada et al., 1999Go). Most of the samples are poorly vesiculated with porosity of 10–20 vol. %; however, bread-crust bombs and blocks from the vulcanian explosions of 8 and 11 June 1991 exhibit variable vesicularity, ranging from 0 to 70 vol. %. The eruption products are entirely dacitic in bulk-rock composition. SiO2 contents vary from 64·5 to 66 wt %, and total phenocryst contents vary from 20 to 30 vol. % (Nakada & Motomura, 1999Go). Phenocryst phases include plagioclase, hornblende, biotite, quartz, apatite, magnetite, ilmenite, and trace amounts of augite and orthopyroxene. Groundmass constituents are pargasite, plagioclase, magnetite, ilmenite, apatite, orthopyroxene, augite and glass. Later eruption products in 1994–1995 contained silica minerals in the groundmass. The glass content of the groundmass varies from 50 to 80 vol. %. Phenocryst minerals often show compositional zoning; that is, oscillatory, spike (isolated zone in otherwise uniform core) and patchy zoning in the core, dusty and reverse zoning at the rim of plagioclase and hornblende phenocrysts, and reverse zoning (increase in Ti toward the rim) in magnetite (Nakamura, 1995Go; Nakada & Motomura, 1999Go). The reverse zoning at the rims of the phenocrysts of plagioclase, hornblende, and magnetite has been interpreted as evidence of magma mixing, which took place just before the eruption (Nakamura, 1995Go; Nakada & Motomura, 1999Go; Venezky & Rutherford, 1999Go; Holtz et al., 2005Go).

Hornblende zoning
Hornblende phenocrysts range from 0·3 to 5 mm in length and 0·1 to 1 mm in width. They usually show idiomorphic crystal forms. In some cases, the hornblende phenocrysts are surrounded by a thin breakdown corona (width <20 µm in most cases) composed of plagioclase, pyroxenes, iron–titanium oxides, and glass. Hornblende phenocrysts contain inclusions of plagioclase, biotite, magnetite, ilmenite, pyrrhotite, apatite, zircon and glass. Compositional zoning of the hornblende phenocryst can be classified into oscillatory, spike or patchy zoning in the core, and reverse zoning at the rim. The boundary between the core and rim of the hornblende phenocrysts is generally sharp, but often showing irregular corroded features. The groundmass pargasite is 5–50 µm across and crystals are often skeletal and/or rounded (Sato et al., 1999Go).

Figure 1 shows back-scattered electron images of hornblende phenocrysts in the 1991–1995 Unzen dacite. In the images, bright zones represent iron-rich compositions, and dark zones correspond to magnesium-rich areas. Out of 50 images of hornblende phenocrysts, 20% have reversely zoned Mg-rich rims (Fig. 1c and d), and 80% are without rims (Fig. 1a and b). The thickness of the rim is 5–30 µm, averaging c. 10 µm. In these zoned outer rims (Fig. 1d), the zoning is of normal character. Oscillatory zoning in the core of hornblende phenocrysts varies from 5 to 100 µm in width, mostly between 20 and 50 µm. The zones usually show inner Fe-rich (FeO 14·0–14·5%; MgO 12·6–14·0%) and outer Mg-rich parts (FeO 13·0–14·0%; MgO 14·0–14·8%). These parts show gradation as illustrated in the back-scattered electron images. The Fe-rich part often truncates the Mg-rich part of the inner zone (Fig. 1a and b). These textures are similar to the oscillatory zoning of plagioclase phenocrysts in the 1991–1995 Unzen dacite. In plagioclase phenocrysts, each zone shows a gradual decrease of Ca/(Ca + Na) ratio toward the outer part, which is often truncated by a new zone with high Ca/(Ca + Na) ratio. The correspondence of An-rich zones in plagioclase and iron-rich zones in hornblende cannot be explained by simple magmatic differentiation processes but suggests some other process, such as magma replenishment, for the formation of oscillatory zoning of the phenocrysts; this will be discussed subsequently.



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Fig. 1. Back-scattered electron images of hornblende phenocrysts in the 1991–1995 Unzen dacite. Scale bars represent 100 µm. (a) Bright zones are rich in Fe, and overgrow corroded, Mg-rich, dark zones. Sample 95101703-hb-3. (b) Oscillatory zoning often showing gradual transition from bright to dark zone and abrupt overgrowth of bright Fe-rich zone. Arrow shows the position of line scan shown in Fig. 2a. Sample 91K524E-hb-5. (c) Dark pargasitic rim of 20 µm thickness on Fe-rich oscillatory zoned core of hornblende phenocryst. Arrow shows the position of line scan of Fig. 2b. Sample 91K524E-hb-3. (d) Fe-rich ‘spike’ zone in otherwise fairly uniform core. The dark outer rim is corroded and encloses the crystal core. Sample 95101703A-hb-9.

 
Figure 2 shows examples of line analytical profiles across hornblende phenocrysts. In the line profiles, Mg is positively correlated with Si, and inversely correlated with Fe, Al, Na and Cl in the core of the phenocrysts (Fig. 2). This contrasts with the core–rim compositional change, where Mg is positively correlated with Al, Ti, Na and K, and negatively correlated with Si, Fe and Cl (left side of Fig. 2b). Major element correlations similar to those observed in the core of oscillatory zoned hornblende phenocrysts in the Unzen dacite have been previously described from hornblende phenocrysts in the Fish Canyon Tuff by Bachmann & Dungan (2002)Go.



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Fig. 2. Line profiles of hornblende phenocrysts in the 1991 Unzen dacite. Step interval of the analyses is 3·2 µm. Vertical scale is modified as shown on the right-hand side of each figure. In (a) the inverse correlation between Mg, Si and Al, Fe, Cl, Ti and Na in the core of the phenocryst should be noted. (b) The rim shows concomitantly high Al and Mg content, which is in contrast to the inverse correlation of Al and Mg in the core of the hornblende phenocryst. Position of the line scans is indicated in Fig. 1.

 
Table 1 shows representative analyses of hornblende phenocrysts in the 1991–1995 Unzen dacite. The analytical conditions for the electron microprobe analyses are described in the legend to Table 1. Figure 3 shows compositional variations of Al vs Mg/(Mg + Fe) ratio. Within the oscillatory zoned cores of the amphiboles, Al is negatively correlated with Mg/(Mg + Fe) ratio (open symbols in Fig. 3). The amphibole rims have higher Al contents and Mg/(Mg + Fe) ratios when compared with the cores (Fig. 2b). The groundmass amphibole is pargasite (after Leake et al., 1997Go) and has the same composition as the rims of the hornblende phenocrysts. Other oxides, such as Na, Ti and K, also show a positive correlation with Mg/(Mg + Fe) ratio for the core to rim relation, and a negative correlation with Mg/(Mg + Fe) ratio for the core oscillatory zoning. These observations suggest that different processes are required to explain the origin of the compositional variations (1) within the cores and (2) between cores and rims of amphiboles. Figures 4 and 5 illustrate the chlorine content of hornblende phenocrysts. Figure 4 shows a positive correlation between Al2O3 and Cl for the oscillatory zoned cores of the hornblende phenocrysts (varying from c. 0·035 to 0·075 wt % Cl), whereas the Cl content of the rims is markedly lower (0·01–0·02 wt % Cl). Figure 5 demonstrates a negative correlation between chlorine and Mg/(Mg + Fe) ratio for the cores and rims of hornblende but it can be observed that different compositional trends are observed for the cores and the rims. As noted previously, Cl is more readily accommodated by Fe-rich hornblende from a crystal-chemical viewpoint. However, we need a quantification of the compositional effects on the partition coefficient of Cl/OH between hornblende and melt to evaluate the origin of Cl zoning in hornblende phenocrysts.



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Fig. 3. Al2O3 wt % vs Mg/(Mg + Fe) of hornblende in the 1991–1995 Unzen dacite. Open symbols are analyses of hornblende cores. Filled symbols are analyses of hornblende rims (phenocrysts) and groundmass hornblende.

 


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Fig. 4. Cl wt % vs Al2O3 wt % in hornblende phenocrysts and groundmass hornblende in the 1991–1994 Unzen dacite.

 


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Fig. 5. Cl wt % vs Mg/(Mg + Fe) in hornblende phenocrysts and groundmass hornblende in the 1991–1995 Unzen dacite. Calculated compositional trends assuming constant Cl/OH ratios in the melt are shown as dashed curves (see text for details).

 

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Table 1: Representative compositions of hornblende in the 1991–1995 dacite of Unzen volcano

 

    EXPERIMENTAL STUDY
 TOP
 ABSTRACT
 INTRODUCTION
 PETROGRAPHY AND PHASE CHEMISTRY...
 EXPERIMENTAL STUDY
 DISCUSSION
 REFERENCES
 
Experimental methods
Most of the high-pressure and -temperature partitioning experiments were carried out using externally heated pressure vessels at the University of Hannover. The experimental conditions were 200–300 MPa and 800–850°C. The oxygen fugacities of most of the charges were controlled at NNO (nickel–nickel oxide) buffer conditions by inserting Ni + NiO powder in a bomb consisting of a nickel alloy. The starting materials were glasses prepared by melting at c. 1600°C in air for 5 h of either the bulk dacite or groundmass separates of the 1992 lava from Unzen. At this temperature, the Fe3+/(total Fe) ratio is calculated to be 0·51–0·52 using the equation of Kilinc et al. (1983)Go, which may have minimal effect on the redox state of the charge during the experiments. Some of the runs were carried out with FeO-doped starting materials. The compositions of the starting materials are shown in Table 2. The glass powder was inserted in Au or AgPd capsules together with NaCl or HCl aqueous solution. The concentration of NaCl or HCl in aqueous solution ranges from 2·5 to 11·2, mostly 4 wt %, and the amount of NaCl and HCl aqueous solution added to the charge ranges from 3·6 to 10·5 wt % (Table 3). The pressure was maintained at the nominal value monitored by a transducer, calibrated against a Heise gauge, and its uncertainty was within 5 MPa. The temperature was regulated by an automatic controller and is accurate to within 10 degrees. Experimental run duration was mostly 7 or 8 days (Table 3). The samples were quenched by cooling the bomb in air with c. 500°C drop of temperature within a minute. The run products were checked for possible volatile leakage both by weighing the capsule and by ensuring the presence of a vapor phase through identifying the vapor leak during opening of the capsule after the run. The run products were mounted in epoxy resin and polished thin sections were prepared for optical and electron microprobe analyses.


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Table 2: Composition of starting materials for the element partition experiments

 

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Table 3: Run conditions and phase assemblages of the experimental charges

 
The run conditions are listed in Table 3. Temperatures of the runs were either 800 or 850°C, and pressures were 185, 200 or 300 MPa. Table 4 lists the compositions of hornblende and glass in the run products, together with the standard error of the analyses. Most of the glass analyses gave totals of 92–95 wt %, which is consistent with the totals of H2O-rich glass quenched from vapor-saturated conditions in the experimental runs. The SiO2 content of the glass is in the range 69–76 wt % (anhydrous basis), and is similar to the estimated composition of the low-temperature Unzen end-member magma (prior to mixing) from which the hornblende phenocryst crystallized (Holtz et al., 2005Go). Hornblende in the charge is, in a strict sense, classified mostly as edenite (after Leake et al., 1997Go); i.e. Mg/(Mg + Fe) ratio is 0·47–0·71, Na + K p.f.u. is 0·38–0·72, Si p.f.u. is 6·92–7·37, and Al p.f.u. is 1·43–2·43.


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Table 4: Phase compositions of the experimental run products

 
Results
From the compositions of hornblende and glass (i.e. melt), we calculated the exchange partition coefficient of Cl and OH between hornblende and melt; i.e. K1 = (Cl/OH)hb/(Cl/OH)melt. We used the water solubility model of Zhang (1999)Go to calculate the total water content in the melt. We neglected the presence of Cl in the vapor phase in calculating the water content of the melts, because the NaCl or HCl content of the aqueous solution added to the charge was fairly low (mostly 4 wt %). In calculating the OH content of the melt, the equilibrium constant for the dissociation reaction of water [H2O + O = 2(OH)] in rhyolitic melts is adopted from Nowak & Behrens (2001)Go, expressed as Kwd = 27·9 exp(–4210/T), which was obtained by in situ high-temperature IR spectrometry. We supposed a stoichiometric concentration of anions in hornblende (two for O = 23) to calculate the amount of OH in hornblende, and anions other than chlorine were neglected. Fluorine was analyzed in some of the hornblende in the run products, but was found to be mostly in the range of 0–0·1 wt % with large relative errors, and may therefore be neglected in calculating the Cl/OH partition coefficient. The results of calculation of the partition coefficient are shown in Table 5. The partition coefficient K1 varies from 0·32 to 1·53, and shows a dependence on the Mg/(Mg + Fe) ratio of hornblende (Fig. 6). As noted previously, the partition coefficient may depend on the Mg/(Mg + Fe) ratio of hornblende based on crystal-chemical arguments (Oberti et al., 1993Go). The least-squares regression line for ln K1 as a function of Mg/(Mg + Fe)hb is: ln K1 = 2·37 – 4·6[Mg/(Mg + Fe)]hb (R = 0·82). Compared with OH, Cl preferentially enters into hornblende with more iron-rich compositions [Mg/(Mg + Fe) < 0·5]. Other compositional parameters such as Al(IV), or Mg/(Mg + Fe) x Al(IV) as suggested by Sato et al. (1997)Go, do not show good correlations with K1, and addition of these parameters to the regression does not improve the correlation coefficient. K1 does not depend on pressure. The temperature effect on ln K1 is negative, and the following regression is obtained: ln K1 = 8·62 – 3·46[Mg/(Mg + Fe)]hb – 0·0062T, where T is the absolute temperature (R = 0·80). Although the data points in Fig. 6 show some scatter, mainly because of analytical errors in determining the compositions of phases, and possibly because of the assumption of the stoichiometric anionic contents of hornblende, we conclude that the most important controlling factor on the partition coefficient K1 is the Mg/(Mg + Fe) ratio of hornblende.



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Fig. 6. Experimentally determined relationship between K = (Cl/OH)hb/(Cl/OH)melt and Mg/(Mg + Fe) in hornblende. The dashed line represents the regression line for all the data points with the equation K1 = 10·67 exp[–4·58(Mg/(Mg + Fe)hb] with R = 0·82.

 

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Table 5: Calculation of partition coefficient of (Cl/OH) between hornblende and melt

 

    DISCUSSION
 TOP
 ABSTRACT
 INTRODUCTION
 PETROGRAPHY AND PHASE CHEMISTRY...
 EXPERIMENTAL STUDY
 DISCUSSION
 REFERENCES
 
Interpretation of chlorine variation in hornblende phenocrysts
In this section, we apply the newly derived partition coefficient to interpret the variation of chlorine content in hornblende phenocrysts in the Unzen dacite. As noted previously, the Cl content of hornblende is negatively correlated with the Mg/(Mg + Fe) ratio for both the core and rim (and groundmass) compositions. Figure 5 shows two dashed lines, which illustrate the calculated Cl content vs Mg/(Mg + Fe) ratio of hornblende assuming a constant Cl/OH ratio in the melt. The compositions of the rims (pargasite) mostly fit the lower dashed line with a molar (Cl/OH)melt ratio of 0·0031, suggesting that these amphiboles crystallized from a melt with a nearly uniform molar Cl/OH ratio. On the other hand, the compositions of the phenocryst cores define a steeper slope than the calculated dashed line, which represents hornblende compositions in equilibrium with a melt of constant (Cl/OH)melt ratio of 0·0124. The variation of the partition coefficient K1 with the Mg/(Mg + Fe) ratio of the hornblende (Fig. 6) can account for c. 20% of the total variation in chlorine content of the cores of the hornblende phenocrysts; that is, c. 80% of the observed variations of chlorine content in the core of the hornblende phenocrysts should be ascribed to the variation of the Cl/OH ratio in the melt.

Cl/OH fractionation is probably caused by degassing of magmas and fluid input. We carried out incremental degassing calculations for melt compositions as illustrated in Fig. 7. The exchange partition coefficient of Cl/H2O between fluid and melt at 200 MPa ranges from two to five based on the data of Webster (1992)Go, and we adopted values of two and four for the degassing calculation. Figure 7 shows that about 70% of the variation in the Cl content of the hornblende requires 1·2–1·8 wt % degassing of H2O from the magma. Thus, it is likely that during the crystallization of the oscillatory zoned cores of the hornblende phenocrysts, repeated degassing and fluid recharge of the magma took place.



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Fig. 7. Calculated variations of chlorine content of hornblende during degassing of magmas. K1 is determined from Fig. 6. K2 = (Cl/H2O)fluid/(Cl/H2O)melt is varied between two and four based on the data of Webster (1992)Go at 200 MPa. Incremental fractional vesiculation by 0·1 wt % of water was assumed.

 
Another possible cause of the change in (Cl/OH) melt ratio is the replenishment of the magma chamber by input of Cl-poor mafic magma and subsequent mixing of the magmas (Davidson & Tepley, 1997Go). This scenario, however, is not in agreement with the negative correlation between Al and Mg/(Mg + Fe) ratio observed in the oscillatory zoning of the hornblende phenocrysts. Replenishment of the magma chamber by mafic input will increase the Mg/(Mg + Fe) ratio and decrease the silica activity of the mixed magma, which may be reflected in concomitant increases of Mg/(Mg + Fe) ratio and Al content of hornblende such as observed in the reverse zoning of hornblende phenocrysts in Fig. 2b. Al in hornblende is affected by the composition of melt from which it crystallizes, and the following reaction indicates the increasing Al content of hornblende as a result of decrease of silica activity of the coexisting melt by magma replenishment: pargasite + 4SiO2 = hornblende + albite (e.g. Blundy & Holland, 1990Go). Decrease of silica activity shifts the reaction to the left-hand side of the equation, causing an increase in the Al content of the hornblende. Therefore, we should expect a positive correlation between Al and Mg/(Mg + Fe) ratio caused by replenishment of the magma chamber, which is opposite to the observed correlation in the oscillatory zoned cores of the hornblende phenocrysts. Therefore, the variation of Cl/OH as a result of magma replenishment is not a plausible mechanism for causing oscillatory zoning in the cores of the hornblende phenocrysts.

Convective degassing/fluid input in the chamber
Several arguments support the possibility of fluid input/degassing processes in the magma chamber to explain variations in the Cl content of hornblende. Generation of bubbles in a crystallizing mafic boundary layer in a stratified magma chamber has been proposed by Eichelberger (1980)Go as a mechanism for the formation of mafic inclusions. Simakin & Botcharnikov (2001)Go suggested that generation of bubbles in a stratified magma chamber may cause large-scale convective motion and mixing in the magma chamber, although Phillips & Woods (2002)Go argued that bubbles may separate and independently float up in the stratified chamber, and do not cause strong mixing in the magma chamber. Murphy et al. (2000)Go and Couch et al. (2001)Go suggested the input of fluid and vesiculated mafic inclusions into the upper layer of a stratified magma chamber at Soufrière Hills Volcano, Montserrat. These models assume the generation of fluid of magmatic origin by crystallization-induced volatile oversaturation in a deep high-temperature mafic magma within a stratified magma chamber (Fig. 8b).



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Fig. 8. Two possible models of fluid input–degassing explaining the chlorine zoning in the core of hornblende phenocrysts in the 1991–1995 Unzen dacite. (a) Chlorine is supplied from an uprising lower mafic magma chamber or heated surrounding saturated rocks into the upper phenocryst-rich magma chamber (Hattori, 1993Go), in which convective degassing takes place. The lower magma chamber may eventually connect to the upper magma chamber, which increases the uprise velocity (Takada, 1994Go) and initiates the eruption processes and mixing of magmas as recorded in the reverse zoning of the rims of hornblende phenocryst. (b) Crystallization-induced vapor saturation of the upper boundary of the lower mafic layer causes fluid and magma input into the overlying felsic layer of a stratified magma chamber as discussed by Eichelberger (1980)Go, Murphy et al. (2000)Go and Couch et al. (2001)Go.

 
Another possible model was advocated by Hattori (1993)Go for the supply of sulfur in the silicic magma chamber at Pinatubo, in which uprising basic magma is saturated with a vapor phase, producing fluid pockets at the top of the mafic magma body. This fluid phase migrates along fractures towards the overlying silicic magma chamber as a result of buoyancy and the local stress field (Takada, 1994Go; Fig. 8a). Another possible source of the fluid is the heated meteoric water surrounding the lower magma chamber. The air-contaminated nature of the rare-gas isotopic composition of hornblende phenocrysts of the Unzen dacite (Hanyu & Kaneoka, 1997Go) supports a contribution of groundwater to the volatiles in the upper phenocryst-rich magma chamber. Input of fluid in this magma chamber results in the resorption of phenocrysts and a decrease in magma density triggers the convective uprise of magma in the chamber, which may vesiculate and degas at shallower depth. Degassing causes crystallization and an increase of magma density, and the degassed magma may descend in the chamber. Such fluid charge–convective degassing can occur repeatedly and oscillatory zoning of the phenocrysts may result. Equilibrium solubility of water in the dacitic melt at a depth of c. 11 km (c. 290 MPa) is c. 6·9 wt %, and at a depth of 8 km (210 MPa) is c. 5·8 wt %. These depths are indicated as pressure sources within the magma plumbing system beneath Unzen volcano by geodetic measurements (Ishihara, 1993Go; Nishi et al., 1999Go). Although we are not fully convinced of the existence of large-scale convective motion in the magma chamber, the model of Kazahaya et al. (1994)Go that explains degassing of large amounts of sulfur dioxide in many active volcanoes—that is, convective degassing through the conduit and magma chamber—reinforces the above model of convective degassing in deep magma chambers. Degassed dense magmas find their way down the conduit into the magma chamber accompanied by an upwelling of low-density volatile-rich magma, which may eventually vesiculate and degas in a shallower part of the conduit or chamber (Fig. 8b).

This study has demonstrated that large variations in chlorine content in the oscillatory zones of hornblende phenocrysts in the 1991–1995 Unzen dacite are probably caused by fluid input–output processes in the magma chamber, based on the experimental determination of Cl/OH exchange partitioning between hornblende and melt. Although plagioclase phenocrysts in the 1991–1995 dacite also show oscillatory, patchy, spike and reverse zoning, we have restricted the discussion to the origin of hornblende zoning, partly because there is rare-gas and Sr isotopic evidence for different sources for the hornblende and plagioclase phenocrysts in the Unzen dacite (Hanyu & Kaneoka, 1997Go; Chen et al., 1999Go). Another problem for interpreting the oscillatory zoning of plagioclase phenocrysts is the possible role of diffusion decoupling in the formation of trace element zoning in plagioclase as suggested by Costa et al. (2003)Go. We need further experimental studies and analyses to resolve these aspects of the origin of oscillatory zoning of phenocryst minerals in volcanic rocks.


    ACKNOWLEDGEMENTS
 
We appreciate discussions with Professor Wilhelm Johannes, Dr Youxue Zhang, Dr Atsushi Goto, Dr Susanne Ohlhorst and Dr Keiko Suzuki-Kamata. We also acknowledge technical assistance by Dr Jürgen Koepke, the late Dr Dieter Ziegenbein, Mr Otto Dietrich and other technical staff at the Institute for Mineralogy, University of Hannover. The paper benefited considerably from the critical reviews of Drs J. Barclay, M. Rutherford and Ian Smith, and from the final improvements of Dr J. Gamble. Financial support came from the Unzen Scientific Drilling Project, MECSST, Japan, the DFG projects Ho1337/7 and Ho1337/11, and JSPS project 14340162.


* Corresponding author. Telephone: 81-78-803-5732. Fax: 81-78-803-5757. E-mail: hsato{at}kobe-u.ac.jp


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