
2005
| Demaiffe,
D., Féménias, O., Berger, J. 2005. Variscan
Moho beneath the French Massif central: a xenolith
perspective from Puy Beaunit. Goldschmidt
Moscow, Idaho, USA. |
| 
|
Puy
Beaunit maar carries both mantle-derived and mafic-ultramafic
plutonic xenoliths [1] highlighting the complexity
of the shallow upper mantle and lower crust beneath
the French Massif Central.
The population of plutonic xenoliths commonly shows
asymmetric, mm to cm thick, layering. Layers are
pyroxenitic to gabbro-noritic, less commonly peridotitic
and anorthositic. They presumably derive from a
layered intrusion (Beaunit Layered Complex, BLC),
located at the crust–mantle boundary and emplaced
at 257±6 Ma (SIMS U-Pb zircon age, [2]).
BLC belongs to the large Permian within-plate mafic
(high-Mg) calc-alkaline magmatic event recognized
in W Europe and spatially controlled by post-Variscan
transcurrent basin tectonics in an intracontinental
setting [2]. Cumulate phases are ol, opx, cpx, gt
[3], am and pl. Rare intercumulus accessory phases
(phl, ilm, ap, ru, armacolite, srilankite and zircon)
are observed in the most differentiated layers [4].
The trace element contents of the cumulates are
similar to those of the Bushveld Lower Zone.
Mantle xenoliths range from fertile spinel lherzolites
to refractory dunites. Fertile peridotites have
registered a modal (amphibole-bearing) and cryptic
(LILE and Pb enrichment, negative Nb and Ta anomalies)
metasomatic event that took place before the Permian
melting episode. Depletion processes are related
to two melt extraction episodes. The first melting
and metasomatic event is attributed to a fluid/liquid
derived from a pre-Variscan subduction. It is sub-contemporaneous
with the texture acquisition and deformation of
the uppermost mantle (lithospheric delamination).
The second melting event produced high-Mg basalts
that gave rise to the BLC [5].
Sr and Nd isotopic data on the BLC (87Sr/86Sr257Ma:
0.7027 to 0.7062 and eNd257Ma: +6.2 to -6.4) and
on the mantle suite (87Sr/86Sr257Ma: 0.7033 to 0.7053
and eNd257Ma: +5.4 to -2.4) are largely overlapping,
confirming their genetic relationship. These values
plot outside the French Massif Central mantle array
and possibly record the pre-variscan subduction-related
mantle metasomatic enrichment.
References: [1] Féménias et al. 2001,
CRAS, 535-542. [2] Féménias et al.
2003, Chem Geol 199, 293-315. [3] Berger et al.
Eu J Min (submitted). [4] Féménias
et al. Lithos (accepted). [5] Féménias
et al. 2004, CMP 148, 13-28. |
| top... |
2004
| Féménias,
O., Nkono, C., Diot, H., Berza, T., Demaiffe, D. 2004.
Flowage differentiation in an andesitic dyke
of the Motru Dyke Swarm (Southern Carpathians, Romania):
Evidence from AMS, CSD and geochemical investigations.
RST, Strasbourg, France. |
|

|
From
a regional survey of a large Pan-African calc-alkaline
dyke swarm (of basaltic-andesitic-dacitic-rhyolitic
composition) of the Alpine Danubian window from
South Carpathians (Romania), two populations of
dykes have been described: thick (from 1 to 30 meters)
N-S trending dykes and thin (less than 1 m) E-W
dykes. These two populations crosscut the country
rocks without simple chronological relations between
them.
The thick dykes display asymmetrical fabrics that
involve a relatively long history of emplacement
and important distance of flow (Féménias
et al., JSG in press). The petrological implications
of such long time flowing are not well known. To
better understand these implications, two dykes
of different thickness (5.5m for TJ31 and 23m for
TJ34) have been studied with physical methods (crystal
size distribution –CSD- and anisotropy of magnetic
susceptibility -AMS) coupled to whole rock geochemistry
and mineral chemistry.
All the physical and chemical variations observed
along dyke’s width point to concordant results and
show that the variations of both the modal proportion
and size of the amphibole and biotite micro-phenocrysts
inside the dykes, deduced from the classical CSD
measurements, are the result of a mechanical segregation
of suspended crystals during magmatic transport.
These variations cannot be linked to different pulses
of flow during ascent of the magma. Despite a pene-contemporaneous
regional tectonic, the flow-induced differentiation
in the large dyke, characterised by the concentration
of pre-existing crystals (Ti-rich pargasite-tschermakite,
clinopyroxene and plagioclase) in the core and the
concomitant extraction of differentiated liquid
near the walls, contributed to a slight chemical
differentiation. As a result, the core has an andesitic
basalt composition whereas the margins are andesitic.
The chilled margins appear as a slightly more evolved
liquid with a Newtonian behaviour when compared
to the average composition of the dyke. The localisation
of the liquid on both sides of the dyke has certainly
facilitated the ascent of the central part of the
dyke that behaved as a Binghamian mush.
|
| top... |
2003
| Féménias,
O., Diot, H., Berza, T., Gauffriau, A., Demaiffe,
D. 2003. Asymmetrical to symmetrical magnetic
fabric of dykes: Paleo-flow orientations and Paleo-stresses
recorded on feeder-bodies from the Motru Dyke Swarm
(Romania). EUG XII, Nice, France. |
| 
|
Puy
Beaunit maar carries both mantle-derived and mafic-ultramafic
plutonic xenoliths [1] highlighting the complexity
of the shallow upper mantle and lower crust beneath
the French Massif Central.
The population of plutonic xenoliths commonly shows
asymmetric, mm to cm thick, layering. Layers are
pyroxenitic to gabbro-noritic, less commonly peridotitic
and anorthositic. They presumably derive from a
layered intrusion (Beaunit Layered Complex, BLC),
located at the crust–mantle boundary and emplaced
at 257±6 Ma (SIMS U-Pb zircon age, [2]).
BLC belongs to the large Permian within-plate mafic
(high-Mg) calc-alkaline magmatic event recognized
in W Europe and spatially controlled by post-Variscan
transcurrent basin tectonics in an intracontinental
setting [2]. Cumulate phases are ol, opx, cpx, gt
[3], am and pl. Rare intercumulus accessory phases
(phl, ilm, ap, ru, armacolite, srilankite and zircon)
are observed in the most differentiated layers [4].
The trace element contents of the cumulates are
similar to those of the Bushveld Lower Zone.
Mantle xenoliths range from fertile spinel lherzolites
to refractory dunites. Fertile peridotites have
registered a modal (amphibole-bearing) and cryptic
(LILE and Pb enrichment, negative Nb and Ta anomalies)
metasomatic event that took place before the Permian
melting episode. Depletion processes are related
to two melt extraction episodes. The first melting
and metasomatic event is attributed to a fluid/liquid
derived from a pre-Variscan subduction. It is sub-contemporaneous
with the texture acquisition and deformation of
the uppermost mantle (lithospheric delamination).
The second melting event produced high-Mg basalts
that gave rise to the BLC [5].
Sr and Nd isotopic data on the BLC (87Sr/86Sr257Ma:
0.7027 to 0.7062 and eNd257Ma: +6.2 to -6.4) and
on the mantle suite (87Sr/86Sr257Ma: 0.7033 to 0.7053
and eNd257Ma: +5.4 to -2.4) are largely overlapping,
confirming their genetic relationship. These values
plot outside the French Massif Central mantle array
and possibly record the pre-variscan subduction-related
mantle metasomatic enrichment.
References: [1] Féménias et al. 2001,
CRAS, 535-542. [2] Féménias et al.
2003, Chem Geol 199, 293-315. [3] Berger et al.
Eu J Min (submitted). [4] Féménias
et al. Lithos (accepted). [5] Féménias
et al. 2004, CMP 148, 13-28.
|
| top... |
S. Brassinnes,
E. Balaganskaya and D. Demaiffe. 2003. MAGMA
GENESIS AND EVOLUTION IN THE
KOLA ALKALINE-CARBONATITE PROVINCE. A Pb-Sr-Nd ISOTOPE
STUDY. EUG XII, Nice, France. |
| 
|
The
Kola Peninsula (NW Russia) is well known for its
late Devonian (380-360Ma) ultramafic, alkaline and
carbonatitic magmatic province, that comprises more
than 20 intrusions including the two giant massifs
of agpaitic nepheline syenite of Khibina and Lovozero
and numerous smaller annular differentiated complexes
(i.e. : Kovdor, Vuorijarvi, ...). These massifs
intrude the Archean to Proterozoic crustal terranes.
Whole rock Pb isotope data are reported for the
first time on these intrusions. Representative samples
of the Kovdor massif (carbonatites, ultramafic cumulates,
ijolitesmelteigites) have been analysed. Two U-rich
pyrochlore-bearing carbonatites have extremely high
measured 206Pb/204Pb and 207Pb/204Pb ratios (94.1
to 253.6 and to 19.6 to 28.2 respectively). Together
with 5 other samples, these carbonatites plot along
a linear array in the 207Pb/204Pb-206Pb/204Pb diagram.
Interpreted as a secondary isochron, this array
gives an age indication of 392±15 Ma (MSWD
= 22), in agreement with the U-Pb baddeleyite age
of 380±4 Ma. Crustal contamination or source
heterogeneity are hardly detectable with such radiogenic
Pb composition. Some samples of other massifs of
the Kola region (Khibina, Lovozero, Sebljavr and
Ozernaya Varaka) have also been analysed, they plot
reasonably close to the Kovdor Pb-Pb isochron, confirming
that all the complexes of the province are grossly
contemporaneous. Although most rocks plot in the
depleted mantle quadrant of the Sr-Nd diagram, the
data show some dispersion. The Kovdor ultramafic
cumulates and carbonatites have overlapping compositions
("Nd(t): +0.5 to +6 ; (87Sr/86Sr)I : 0.7031
to 0.7039) while the ijolites-melteigites tend to
have lower "Nd(t) (+0.5 to -3.4) and higher
(87Sr/86Sr)I (0.7035 to 0.7047) values. This dispersion
can be explained either by heterogeneities of the
mantle (or mixing between different geochemical
reservoirs) or by open system behaviour during complex
emplacement history and hydrothermalism. Crustal
contamination is difficult to ascertain by Sr and
Nd isotopes because most rocks have higher Sr and
REE contents than crustal materials. By contrast,
Pb isotopes are more sensitive to crustal contamination.
The initial 207Pb/204Pb and 206Pb/204Pb ratios (recalculated
at 380Ma) define a short linear trend, that could
represent a mixing line between a HIMU (or FOZO)
type of reservoir (with µ > 10, 87Sr/86Sr
< 0.703 and "Nd > 5) and average lower
crustal material (µ < 10, 87Sr/86Sr >
0.7045 and "Nd < -4). These magmas have
possibly undergone crustal contamination during
their ascent through the thick (55km) cratonic crust
of Kola.
|
| top... |
| S. Brassinnes, E. Balaganskaya,
D. Demaiffe. 2003. Magmatic evolution of the
differentiated ultramafic-alkaline and carbonatite
intrusion of Vuorijarvi (Kola Region, Russia): a LA-ICP-MS
study of apatite. EUROCARB, Canary. |
|
The small, elliptical Vuorijarvi
massif (3.5 x 5.5 km) belongs to Kola Alkaline
and Carbonatitic Province. It is a complex multi-phased
intrusion classically interpreted as resulting
from successive magma pulses. The core of the
massif is mainly represented by ultramafic cumulates
while alkaline silicate rocks of the ijolite-melteigite
series are found at the periphery. Two carbonatitic
stocks with associated phoscorites occur at Vuorijarvi:
an early one in the eastern part of the massif
and a later thick stock (c.a. 800m) in the south-eastern
part. Apatite is a common liquidus phase in the
three kinds of rocks (ultramafic cumulates, ijolites-melteigites
and carbonatites/phoscorites). Apatites from representative
clinopyroxenite, ijolite and carbonatites have
been analysed by LA-ICP-MS. All apatites are rich
to extremely rich in REE (SREE: 730 to 13800 ppm),
with LREE enrichment: La/Yb ratio varies from
70 up to 467. Apatite REE composition does not
define a regular geochemical evolution trend with
emplacement sequence. The crystallisation/fractionation
of other REE-rich accessory phases (pyrochlore,
perovskite, …) has partly controlled the REE pattern
of the apatites. There is an increase in REE content
from the clinopyroxenites to the early carbonatites.
Intensive crystallisation of apatite and other
REE-rich phases deplete the residual melt in REE,
the late magnesiocarbonatite are indeed poor in
REE (SREE: 120 ppm) and devoid of apatite. REE
partition coefficients for apatite crystallising
in a carbonatite melt are poorly known. They have
been tentatively estimated for some African carbonatites
(Homa mountain, Kalkfeld, Ondurakorume, Otjisazu,
Okorusu and North Ruri) by comparing the trends
of the apatite and of the whole rocks (Bühn
et al, 2001). The partition coefficients increase
regularly from La to Yb. We use the same approach
in this study by combining whole rocks analyses
and LA-ICP-MS on apatites. The Vuorijarvi carbonatites
display consertal (intergrowth) and polygonal
textures. The carbonatites occur as cm to m thick
veins suggesting quick cooling of the melt. Calcite
crystals (1-2mm) are zoned (CaO: 54.5-56.3wt%;
MgO: 0.23-1.9 wt%; SrO: 1.06-0.14wt%) suggesting
rapid growth leading to closed-system behaviour.
As the zoning of calcite is easily erased at high
to medium T° (800-500°C; Cherniak, 1998),
the presence of zoned calcite at Vuorijarvi testifies
a rapid cooling. Moreover, deformation in calcite
involves mechanical twinning rather than pressure-dissolution,
so the deformation process has not homogeneised
the composition of the grains. We will consider
that the REE composition of the liquid in equilibrium
with the apatite can be approximated by subtracting
the apatite contribution to the whole rocks carbonatite
REE content. The apatite/carbonatite liquid partition
coefficients for the Vuorijarvi carbonatites are
given in Table 1, they range from 7.6 to 3.5 for
La, 8.4 to 4.9 for Eu and 5.2 to 1.0 for Yb. The
REE distribution coefficient patterns are convex-upwards
as the apatite/silicate liquid partition coefficients
(Watson and Green, 1981). The REE patterns obtained
for Vuorijarvi are completely different from those
by Bühn et al (2001). This discrepancy can
be explained either by variations of melt composition
or by the fractionation of a co-existing LREE
enriched phase (i.e. perovskite, pyrochlore).Yttrium
and holmium contents are high in apatite from
early silicate carbonatites (775 and 33 ppm respectively)
and lower in later carbonatites (72 and 2.8 ppm).
As Y and Ho have the same charge and nearly the
same ionic radius, they do not commonly fractionate.
Nevertheless, the calculated DY/DHo ratio (0.89
and 0.68) implies a slight fractionation. Whole
rocks analyses plot along a well-defined linear
array (R2=0.9884), corresponding to an Y/Ho ratio
of 27.5, close to the chondritic value (28.7).
Apatite crystallisation would result in an increase
of the Y/Ho ratio of the residual melt. The apatite
Y/Ho ratio decreases in the sequence clinopyroxenite
(27)-ijolite (22.5)-carbonatite (19). The nearly
constant Y/Ho ratio of whole rocks implies that
apatite alone does not control the Y/Ho fractionation.
Two other processes could be invoked: 1) the fractionation
of an Y-rich mineral (i.e. monazite) and/or 2)
the depletion of Y by exsolution of CO2/H2O fluids
(Bau, 1996; Bühn et al, 2001).The apatites
of the early clinopyroxenites display slight negative
Ce anomaly (Ce/Ce*: 0.7 to 1.0), this anomaly
decreases progressively during differentiation,
suggesting a decrease in oxygen fugacity. For
all the analysed apatites, the Ca (p.f.u) content
decreases while the La+Ce+Na (p.f.u) content increases,
this feature has already been interpreted in terms
of isomorphic substitution 2Ca2+ = REE3++Na+ (Brassinnes
et al, 2003), related to fractional crystallisation
of a single batch of melt from the ultramafic
cumulates to the carbonatites. This is confirmed
by the similar Sr and Nd isotopic compositions
(0.70303-0.70318; eNd380Ma: +3.5 to 6.1 of all
the Vuorijarvi rocks.
REFERENCES:
Brassinnes S.et al (2003) Period. di Mineral,
in press; Bau M. (1996) Contrib. Minera. Petrol
123, 323-333; Bühn B. et al (2001), Contrib.
Mineral. Petrol. 141, 572-592; Cherniak D.J. (1998),
Earth Planet. Sci. Lett. 160, 273-287; McDonough,
W.F. and Sun, S.-s. (1995), Chemical Geology 120,
223-253; Watson E.B. and Green T.H. (1981), Earth
Planet. Sci. Lett. 56, 405-421.
top...
|
| S. Brassinnes, O. Féménias,
N. Coussaert, V. Nivin, D. Demaiffe 2003. Two
stages of nepheline crystallisation in the layered
part of the Lovozero agpaitic syenite complex (Kola
Peninsula, Russia): Implications for the layering
and cooling processes. EUROCARB, Canary. |
| |
The Lovozero alkaline massif (Gerasimovsky
et al, 1966; Kogarko et al, 1995) is composed
of three major petrographic units; the main central
unit (80% of the volume) is a differentiated layered
complex that consists of numerous (29) rhythms
composed of several layers: the ideal sequence
is urtite-juvite-foyaite-lujavrite. A detailed
textural, mineralogical and geochemical study
of the complete rhythm II-7 allows to better constrain
the mode of emplacement and the differentiation
process.
Two distinct types of nepheline have been recognised:
1) inclusion-free euhedral nepheline occurs mainly
in urtites and as a minor phase in foyaites and
2) anhedral to subhedral nepheline containing
numerous inclusions of aegirine and arfvedsonite
occurs in all rock types. The inclusion-free nephelines
display rather homogeneous compositions (Ne56-68Ks14-19Q15-25),
characterised by high SiO2 (44 to 47.5 %) and
Fe2O3 (1.5 to >2 %) contents in comparison
with natural nephelines. The nepheline inclusions
in aegirine and alkali feldspar are comparable
to the inclusion-free nephelines. The inclusion-rich
nephelines also show quite homogeneous composition
(Ne69-79Ks20-25Q0-11) but are clearly distinct
from the inclusion-free nephelines; they are more
potassic and less enriched in SiO2 (<43.5 %)
and Fe2O3 (< 0.55%). The excess of Si over
that required by stoichiometry can be used as
a temperature indicator. The inclusion-free nephelines
crystallise at significantly higher temperatures
(800-1100°C) than the inclusion-rich nephelines
(<700°C). The high T° of crystallisation
(already noted by Kogarko et Romanchev, 1977)
of the inclusion-free nepheline is probably higher
than expected for slowly cooled plutons and is
attributed to the rapid cooling in a subvolcanic
environment (Woolley and Platt, 1986).
The morphological and textural characteristics
of each mineral phase in the urtite-lujavrite
rocks sequence can be discussed in terms of order
of crystallisation and cumulate (solid) and intercumulate
(liquid) origin. Alkali feldspar laths are ubiquitous
in the sequence; they are dominantly euhedral
but have been variously affected by a deformation
that occurred contemporaneously with the layering
development. Alkali feldspar can be considered,
without ambiguity, as a cumulate phase. Inclusion-free
high T° nepheline is also a cumulate phase
whereas subhedral to anhedral inclusion-rich low
T° nepheline is of intercumulate origin. In
the rhythm II-7, high T° nepheline is rare,
less than 10% of the total nepheline modal proportion;
the small (0.2-0.4mm) crystals with cubic-like
morphology suggest that nepheline results from
the destabilisation of a high T° polymorphic
phase (carnegieite?). The inclusion-rich nepheline
is common in all the rocks of the rhythm II-7;
it represents the main mineral phase of the basal
urtite layer of the rhythm. Aegirine-augite constitutes
the core of the large poikilitic augite crystals
that contain aegirine inclusions, it growths after
alkali feldspar and inclusion-free nepheline but
before inclusion-rich nepheline. It is tentatively
interpreted as a cumulate phase, characterised
by a high nucleation rate (numerous crystals have
been observed) but a low growth rate. Aegirine
and arfvedsonite crystallise lately around the
aegirine-augite cores or as large interstitial
or poikilitic grains.
Inside the rhythm II-7, strong variations of the
cumulate-liquid (L) proportions and of the nature
of the liquid have been observed. The liquid proportion,
estimated by the proportion of intercumulate phases,
decreases dramatically from the basal urtite (L
~ 90%) to the uppermost lujavrite (L ~ 10%). In
the urtite, the cumulate phases are represented
by rare feldspar laths and inclusion-free nepheline;
in lujavrite, euhedral feldspar laths are abundant.
The intercumulate assemblage of the urtite is
represented by the inclusion-rich nepheline and
rare aegirine and arfvedsonite, whereas in the
lujavrite, the proportion of the latter increases
and are roughly equal to the inclusion-rich nepheline.
The modal proportion of alkali feldspar and their
size increase from the bottom to the top in the
urtite-juvite-foyaite-lujavrite sequence of rhythm
II-7. Structural features suggest that each rhythm
was formed by in situ differentiation of a sill-like
sheet of liquid. The layering could result from
a sill-in-sill mode of emplacement rather than
from magma chamber processes.
REFERENCES:
Gerasimovsky V. et al (1966) Geochemistry of the
Lovozero alkaline massif, Nauka (Moscow), 365pp;
Kogarko L. and Romanchev B. (1977) Geokh., 2,
199-216; Kogarko L. et al (1995) Alkaline rocks
and carbonatites of the world. Pt2. Former USSR,
Chapman et Hall, 225pp; Woolley A.R. and Platt
R.G. (1986), Mineral. Mag. 50, 597-610.
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|
2002
| Féménias,
O., Demaiffe, D., Diot, H., Berza, T., Tatu, M., Liégeois,
J.P., Duchesne, J.C. 2002. Petrological data
from the Late Pan-African high-K calc-alkaline Motru
dyke swarm (Romania): evidence for the evolution in
a deep magma chamber from sub-surface observations.
Colloque en l’honneur de J.-C. Duchesne.
Modelling of Magma Chambers and Implications for the
Evolution of the Continental Crust, Liège.
Belgique. |
|
|
The
Pan-African basement of the Danubian window (S.
Carpathians, Romania) is crosscut by several major
dyke swarms. Among these, the subvolcanic Motru
swarm intruded between the Late Cambrian (it crosscuts
the Tismana pluton dated at 560 Ma) and the Silurian
(stratigraphic relation). This swarm represents
a large magmatic episode strongly controlled in
a geotectonic environment by a late- to post-Pan-African
transcurrent tectonics. The swarm consists of 1
to 3 m thick dykes composed of high-K calc-alkaline
volcanic to subvolvanic rocks defining a complete
differentiated series from andesitic basalt to rhyolite
(50–72 wt% SiO2).The most common rocks are aphyric
to microgranular porphyritic andesite, with euhedral
brown tschermakitic amphibole and/or plagioclase
phenocrysts and porphyritic dacite with euhedral
green magnesiohornblende and/or corroded quartz
phenocrysts. Plagioclase is often deeply retrogressed
to secondary phases and appears as ghost crystals.
The groundmass is composed of quartz, plagioclase,
ferro-magnesian phases (amphiboles and rarely pyroxenes),
Ti-magnetite and devitrified glass. Many dykes contain
complexly zoned brown amphibole or plagioclase phenocrysts.
Back scattered electron images and detailed microprobe
investigations on selected amphibole and plagioclase
phenocrysts allow to reconstruct the several stages
of complex growth and resorbtion history. P-T conditions
during this history are recorded by the amphibole
chemistry. P estimate is based on the Al-content
empirical barometer (Schmidt, 1992) and T estimates
are deduced from Ti-content (Otten, 1984). In all
rock types, amphibole phenocrysts were equilibrated
at about the same pressure, 6±1 kbar, but
their temperature of crystallisation range from
900-1000°C for the andesitic basalts to 600-700°C
for dacites. In rhyolites, magnesiohornblende phenocrysts
present a continuous range of P-T conditions from
700°C/6 kbar to 600°C/1 kbar. These data
suggest that a calc-alkaline magma was ponding in
a chamber at mid-crustal level (6 kbar, Conrad discontinuity?)
and started crystallising. Episodically, dykes were
emplaced at higher crustal levels (subvolcanic environment)
carrying pre-emplacement phenocrysts of amphibole
and plagioclase. At the scale of the Danubian window
(90 x 30 km) the regional variations in composition
of the dykes suggest that several small chambers
evolved independently. Preliminary isotopic compositions
(87Sr/86Sr550: 0.7062 – 0.7065 and eNd550: -3 to
-4) suggest a juvenile (= probably mantle-derived)
magma contaminated by an old crustal component during
the ponding and the beginning of crystallisation
at mid-crustal level. Our data demonstrate that
deep magma chamber processes can be tackled from
sub-surface magmatic activity.
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2001
2000
|