<?xml version="1.0" encoding="utf-8"?><rss version="2.0"><channel><title>SE - Latest Articles</title><link>http://www.solid-earth.net/</link><description>Solid Earth Latest Articles</description><language>en</language><item><title>Phanerozoic environments of black shale deposition and the Wilson Cycle</title><link>http://www.solid-earth.net/3/29/2012/</link><description>&lt;b&gt;Phanerozoic environments of black shale deposition and the Wilson Cycle&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 3, 29-42, 2012&lt;br /&gt;&lt;br /&gt;Author(s): J. Trabucho-Alexandre, W. W. Hay, and P. L. de Boer&lt;br /&gt;&lt;br /&gt;The spatial and temporal distribution of black shales is related to the
development of environments in which they accumulate and to a propitious
combination of environmental variables. In recent years, much has been done
to improve our understanding of the mechanisms behind the temporal
distribution of black shales in the Phanerozoic and of the environmental
variables that result in their deposition. However, the interpretation of
ancient black shale depositional environments is dominated by an
oversimplistic set of three depositional models that do not capture their
complexity and dynamics. These three models, the restricted circulation, the
(open) ocean oxygen minimum and the continental shelf models, are an
oversimplification of the variety of black shale depositional environments
that arise and coexist throughout the course of a basin's Wilson Cycle, i.e. the
dynamic sequence of events and stages that characterise the evolution of
an ocean basin, from the opening continental rift to the closing orogeny. We
examine the spatial distribution of black shales in the context of the
Wilson Cycle using examples from the Phanerozoic. It is shown that the
geographical distribution of environments of black shale deposition and the
position of black shales in the basin infill sequence strongly depend on
basin evolution, which controls the development of sedimentary environments
where black shales may be deposited. The nature of the black shales that are
deposited, i.e. lithology and type of organic matter, also depends on basin
evolution and palaeogeography. We propose that in studies of black shales
more attention should be given to the sedimentary processes that have led to
their formation and to the interpretation of their sedimentary environments.</description><pubDate>Thu, 02 Feb 2012 00:00:00 +0100</pubDate></item><item><title>Bio-chemostratigraphy of the Barremian-Aptian shallow-water carbonates of the southern Apennines (Italy): pinpointing the OAE1a in a Tethyan carbonate platform</title><link>http://www.solid-earth.net/3/1/2012/</link><description>&lt;b&gt;Bio-chemostratigraphy of the Barremian-Aptian shallow-water carbonates of the southern Apennines (Italy): pinpointing the OAE1a in a Tethyan carbonate platform&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 3, 1-28, 2012&lt;br /&gt;&lt;br /&gt;Author(s): M. Di Lucia, A. Trecalli, M. Mutti, and M. Parente&lt;br /&gt;&lt;br /&gt;Low biostratigraphic resolution and lack of chronostratigraphic calibration
hinder precise correlations between platform carbonates and coeval
deep-water successions. These are the main obstacle when studying the record
of Mesozoic oceanic anoxic events in carbonate platforms. In this paper
carbon and strontium isotope stratigraphy are used to produce the first
chronostratigraphic calibration of the Barremian-Aptian biostratigraphy of
the Apenninic carbonate platform of southern Italy. According to this
calibration, the segment of decreasing &amp;delta;&lt;sup&gt;13&lt;/sup&gt;C values, leading to
the negative peak that is generally taken as the onset of the Selli event,
starts a few metres above the last occurrence of &lt;i&gt;Palorbitolina lenticularis&lt;/i&gt; and &lt;i&gt;Voloshinoides murgensis&lt;/i&gt;. The following rise
of &amp;delta;&lt;sup&gt;13&lt;/sup&gt;C values, corresponding to the interval of enhanced
accumulation of organic matter in deep-water sections, ends just below the
first acme of &lt;i&gt;Salpingoporella dinarica&lt;/i&gt;, which roughly corresponds to the segment of peak &amp;delta;&lt;sup&gt;13&lt;/sup&gt;C values. The whole carbon isotope excursion associated with the
oceanic anoxic event 1a is bracketed in the Apenninic carbonate platform
between the last occurrence of &lt;i&gt;Voloshinoides murgensis&lt;/i&gt; and the &quot;Orbitolina level&quot;, characterized by
the association of &lt;i&gt;Mesorbitolina parva&lt;/i&gt; and &lt;i&gt;Mesorbitolina texana&lt;/i&gt;. Since these bioevents have been widely recognized
beyond the Apenninic platform, the calibration presented in this paper can
be used to pinpoint the interval corresponding to the Early Aptian oceanic
anoxic event in other carbonate platforms of central and southern Tethys.
This calibration will be particularly useful to interpret the record of the
Selli event in carbonate platform sections for which a reliable carbon
isotope stratigraphy is not available.</description><pubDate>Fri, 27 Jan 2012 00:00:00 +0100</pubDate></item><item><title>Influence of the Ringwoodite-Perovskite transition on mantle convection in spherical geometry as a function of Clapeyron slope and Rayleigh number</title><link>http://www.solid-earth.net/2/315/2011/</link><description>&lt;b&gt;Influence of the Ringwoodite-Perovskite transition on mantle convection in spherical geometry as a function of Clapeyron slope and Rayleigh number&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 315-326, 2011&lt;br /&gt;&lt;br /&gt;Author(s): M. Wolstencroft and J. H. Davies&lt;br /&gt;&lt;br /&gt;We investigate the influence on mantle convection of the negative Clapeyron slope ringwoodite to
perovskite and ferro-periclase mantle phase transition, which is correlated with the seismic discontinuity
at 660 km depth. In particular, we focus on understanding the influence of the magnitude of the Clapeyron slope
(as measured by the Phase Buoyancy parameter, &lt;i&gt;P&lt;/i&gt;) and the vigour of convection (as measured by the Rayleigh number, &lt;i&gt;Ra&lt;/i&gt;)
on mantle convection. We have undertaken  76 simulations of isoviscous mantle convection in spherical geometry, varying &lt;i&gt;Ra&lt;/i&gt; and &lt;i&gt;P&lt;/i&gt;.
Three domains of behaviour were found: layered convection for high &lt;i&gt;Ra&lt;/i&gt; and more negative &lt;i&gt;P&lt;/i&gt;, whole mantle convection for low &lt;i&gt;Ra&lt;/i&gt;
and less negative &lt;i&gt;P&lt;/i&gt;, and transitional behaviour in an intervening domain. The boundary between the layered and transitional domain
was fit by a curve &lt;i&gt;P = &amp;alpha; Ra&lt;sup&gt;&amp;beta;&lt;/sup&gt;&lt;/i&gt; where &lt;i&gt;α&lt;/i&gt; = −1.05, and &lt;i&gt;β&lt;/i&gt; = −0.1, and the fit for the boundary between the transitional
and whole mantle convection domain was &lt;i&gt;α&lt;/i&gt; = −4.8, and &lt;i&gt;β&lt;/i&gt; = −0.25. These two curves converge at &lt;i&gt;Ra&lt;/i&gt; ≈ 2.5 × 10&lt;sup&gt;4&lt;/sup&gt; (well below Earth mantle vigour) and &lt;i&gt;P&lt;/i&gt; &amp;approx; &amp;minus;0.38.
Extrapolating to high &lt;i&gt;Ra&lt;/i&gt;, which is likely earlier in Earth history, this work suggests a large transitional domain. It is therefore likely that convection in the
Archean would have been influenced by this phase change, with Earth being at least in the transitional domain, if not the layered domain.</description><pubDate>Mon, 19 Dec 2011 00:00:00 +0100</pubDate></item><item><title>Domains of Archean mantle lithosphere deciphered by seismic anisotropy &amp;ndash; inferences from the LAPNET array in northern Fennoscandia</title><link>http://www.solid-earth.net/2/303/2011/</link><description>&lt;b&gt;Domains of Archean mantle lithosphere deciphered by seismic anisotropy &amp;ndash; inferences from the LAPNET array in northern Fennoscandia&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 303-313, 2011&lt;br /&gt;&lt;br /&gt;Author(s): J. Plomerová, L. Vecsey, V. Babuška, and LAPNET Working Group&lt;br /&gt;&lt;br /&gt;An international LAPNET array (2007–2009, &lt;a href=&quot;http://www.oulu.fi/sgo-oty/lapnet&quot; target=&quot;_blank&quot;&gt;http://www.oulu.fi/sgo-oty/lapnet&lt;/a&gt;)
of the POLENET/LAPNET sub-project of the POLENET-IPY consortium, related to
seismic and geodetic studies in the Arctic regions, consisted of about 60
broadband seismic stations located on the territory of northern Finland and
adjacent parts of Sweden, Norway and Russia. We analyze relative P-wave
travel-time deviations evaluated for a subset of 90 teleseismic events
recorded by the LAPNET array and show examples of lateral variations of
shear-wave splitting to demonstrate variability of fabrics of the Archean
mantle lithosphere. The initial results clearly demonstrate the Archean
mantle lithosphere consists of domains with consistent fabrics reflecting
fossil anisotropic structures. 3-D self-consistent anisotropic models with
inclined symmetry axes accommodate two independent sets of body-wave
anisotropic observations. Individual domains are delimited by boundaries
(sutures), where the anisotropic parameters change. The results obtained
from the LAPNET array fill a gap in structural studies of the upper mantle
beneath northern Fennoscandia.</description><pubDate>Thu, 15 Dec 2011 00:00:00 +0100</pubDate></item><item><title>Erosion rates deduced from seasonal mass balance along the upper Urumqi River in Tianshan</title><link>http://www.solid-earth.net/2/283/2011/</link><description>&lt;b&gt;Erosion rates deduced from seasonal mass balance along the upper Urumqi River in Tianshan&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 283-301, 2011&lt;br /&gt;&lt;br /&gt;Author(s): Y. Liu, F. Métivier, J. Gaillardet, B. Ye, P. Meunier, C. Narteau, E. Lajeunesse, T. Han, and L. Malverti&lt;br /&gt;&lt;br /&gt;We report measurements performed during two complete flow seasons on the Urumqi
River, a proglacial mountain stream in the northeastern flank of the Tianshan, an
active mountain range in Central Asia. This survey of flow dynamics and sediment
transport (dissolved, suspended and bed loads), together with a 25-year record
of daily discharge, enables the assessment of secular denudation rates on this
high mountain catchment of Central Asia. Our results show that chemical
weathering accounts for more than one-third of the total denudation rate.
Sediment transported as bed load cannot be neglected in the balance, given that
sand and gravel transport accounts for one third of the solid load of the river.
Overall, the mean denudation rates are low, averaging 46 t × km&lt;sup&gt;−2&lt;/sup&gt; × yr&lt;sup&gt;−1&lt;/sup&gt;(17–18 m Myr&lt;sup&gt;−1&lt;/sup&gt;).
We furthermore analyse the hydrologic record to show that the long-term sediment
budget is not dominated by extreme and rare events but by the total amount of
rainfall or annual runoff. The rates we obtain are in agreement with rates
obtained from the mass balance reconstruction of the Plio-Quaternary gravely
deposits of the foreland but signicantly lower than the rates recently obtained
from cosmogenic dating of the Kuitun River sands, west of the Urumqi River.
We show that the resolution of this
incompatibility may have an important consquence for our understanding of the
interplay between erosion and tectonics in the semi-humid ranges of Central
Asia.</description><pubDate>Tue, 13 Dec 2011 00:00:00 +0100</pubDate></item><item><title>Remobilization of silicic intrusion by mafic magmas during the 2010 Eyjafjallajökull eruption</title><link>http://www.solid-earth.net/2/271/2011/</link><description>&lt;b&gt;Remobilization of silicic intrusion by mafic magmas during the 2010 Eyjafjallajökull eruption&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 271-281, 2011&lt;br /&gt;&lt;br /&gt;Author(s): O. Sigmarsson, I. Vlastelic, R. Andreasen, I. Bindeman, J.-L. Devidal, S. Moune, J. K. Keiding, G. Larsen, A. Höskuldsson, and Th. Thordarson&lt;br /&gt;&lt;br /&gt;Injection of basaltic magmas into silicic crustal holding chambers and
subsequent magma mingling or mixing is a process that has been recognised
since the late seventies as resulting in explosive eruptions. Detailed
reconstruction and assessment of the mixing process caused by such intrusion
is now possible because of the exceptional time-sequence sample suite
available from the tephra fallout of the 2010 summit eruption at
Eyjafjallajökull volcano in South Iceland. Fallout from 14 to 19 April
contains three glass types of basaltic, intermediate, and silicic
compositions recording rapid magma mingling without homogenisation,
involving evolved FeTi-basalt and silicic melt with composition identical to
that produced by the 1821–1823 AD Eyjafjallajökull summit eruption. The
time-dependent change in the magma composition suggests a binary mixing
process with changing end-member compositions and proportions. Beginning of
May, a new injection of primitive basalt was recorded by deep seismicity,
appearance of Mg-rich olivine phenocrysts together with high sulphur dioxide
output and presence of sulphide crystals. Thus, the composition of the
basaltic injection became more magnesian and hotter with time provoking
changes in the silicic mixing end-member from pre-existing melt to the solid
carapace of the magma chamber. Finally, decreasing proportions of the mafic
end-member with time in the erupted mixed-magma demonstrate that injections
of Mg-rich basalt was the motor of the 2010 Eyjafjallajökull explosive
eruption, and that its decreasing inflow terminated the eruption.
Significant quantity of silicic magma is thus still present in the interior
of the volcano. Our results show that detailed sampling during the entire
eruption was essential for deciphering the complex magmatic processes at
play, i.e. the dynamics of the magma mingling and mixing. Finally, the rapid
compositional changes in the eruptive products suggest that magma mingling
occurs on a timescale of a few hours to days whereas the interval between the
first detected magma injection and eruption was several months.</description><pubDate>Fri, 02 Dec 2011 00:00:00 +0100</pubDate></item><item><title>Paleointensities on 8 ka obsidian from Mayor Island, New Zealand</title><link>http://www.solid-earth.net/2/259/2011/</link><description>&lt;b&gt;Paleointensities on 8 ka obsidian from Mayor Island, New Zealand&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 259-270, 2011&lt;br /&gt;&lt;br /&gt;Author(s): A. Ferk, R. Leonhardt, K.-U. Hess, and D. B. Dingwell&lt;br /&gt;&lt;br /&gt;The 8 ka BP (6050 BCE) pantelleritic obsidian flow on Mayor Island, Bay
of Plenty, New Zealand, has been investigated using 30 samples from two
sites. Due to a very high paramagnetic/ferromagnetic ratio, it was not
possible to determine the remanence carriers. This is despite the fact that
the samples were studied intensively at low, room, and high temperatures. We
infer that a stable remanence within the samples is carried by single- or
close to single-domain particles. Experiments to determine the anisotropy of
thermoremanence tensor and the dependency on cooling rate were hampered due
to alteration resulting from the repeated heating of the samples to
temperatures just below the glass transition. Nonetheless, a well-defined
mean paleointensity of 57.0 ± 1.0  μT, based on individual high
quality paleointensity determinations, was obtained. This field value
compares very well to a paleointensity of 58.1 ± 2.9 μT, which
Tanaka et al. (2009) obtained for 5500 BCE at a site 100 km distant. Agreement
with geomagnetic field models, however, is poor. Thus, gathering more
high-quality paleointensity data for the Pacific region and for the southern
hemisphere in general to better constrain global field models is very
important.</description><pubDate>Mon, 21 Nov 2011 00:00:00 +0100</pubDate></item><item><title>An open ocean record of the Toarcian oceanic anoxic event</title><link>http://www.solid-earth.net/2/245/2011/</link><description>&lt;b&gt;An open ocean record of the Toarcian oceanic anoxic event&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 245-257, 2011&lt;br /&gt;&lt;br /&gt;Author(s): D. R. Gröcke, R. S. Hori, J. Trabucho-Alexandre, D. B. Kemp, and L. Schwark&lt;br /&gt;&lt;br /&gt;Oceanic anoxic events were time intervals in the Mesozoic characterized by
widespread distribution of marine organic matter-rich sediments (black
shales) and significant perturbations in the global carbon cycle. These
perturbations are globally recorded in sediments as carbon isotope
excursions irrespective of lithology and depositional environment. During
the early Toarcian, black shales were deposited on the epi- and
pericontinental shelves of Pangaea, and these sedimentary rocks are
associated with a pronounced (ca. 7 &amp;permil;) negative (organic) carbon isotope
excursion (CIE) which is thought to be the result of a major perturbation in
the global carbon cycle. For this reason, the lower Toarcian is thought to
represent an oceanic anoxic event (the T-OAE). If the T-OAE was indeed a
global event, an isotopic expression of this event should be found beyond
the epi- and pericontinental Pangaean localities. To address this issue, the
carbon isotope composition of organic matter (&amp;delta;&lt;sup&gt;13&lt;/sup&gt;C&lt;sub&gt;org&lt;/sub&gt; of
lower Toarcian organic matter-rich cherts from Japan, deposited in the open
Panthalassa Ocean, was analysed. The results show the presence of a major
(&gt;6 &amp;permil;) negative excursion in &amp;delta;&lt;sup&gt;13&lt;/sup&gt;C&lt;sub&gt;org&lt;/sub&gt; that, based on
radiolarian biostratigraphy, is a correlative of the lower Toarcian negative
CIE known from Pangaean epi- and pericontinental strata. A smaller negative
excursion in &amp;delta;&lt;sup&gt;13&lt;/sup&gt;C&lt;sub&gt;org&lt;/sub&gt; (ca. 2 &amp;permil;) is recognized lower in the
studied succession. This excursion may, within the current
biostratigraphic resolution, represent the excursion recorded in European
epicontinental successions close to the Pliensbachian/Toarcian boundary.
These results from the open ocean realm suggest, in conjunction with other
previously published datasets, that these Early Jurassic carbon cycle
perturbations affected the active global reservoirs of the exchangeable
carbon cycle (deep marine, shallow marine, atmospheric).</description><pubDate>Fri, 11 Nov 2011 00:00:00 +0100</pubDate></item><item><title>Metamorphic history and geodynamic significance of the Early Cretaceous Sabzevar granulites (Sabzevar structural zone, NE Iran)</title><link>http://www.solid-earth.net/2/219/2011/</link><description>&lt;b&gt;Metamorphic history and geodynamic significance of the Early Cretaceous Sabzevar granulites (Sabzevar structural zone, NE Iran)&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 219-243, 2011&lt;br /&gt;&lt;br /&gt;Author(s): M. Nasrabady, F. Rossetti, T. Theye, and G. Vignaroli&lt;br /&gt;&lt;br /&gt;The Iranian ophiolites are part of the vast orogenic suture zones that mark
the Alpine-Himalayan convergence zone. Few petrological and geochronological
data are available from these ophiolitic domains, hampering a full
assessment of the timing and regimes of subduction zone metamorphism and
orogenic construction in the region. This paper describes texture,
geochemistry, and the pressure-temperature path of the Early Cretaceous mafic
granulites that occur within the Tertiary Sabzevar ophiolitic suture zone of
NE Iran. Whole rock geochemistry indicates that the Sabzevar granulites are
likely derived from a MORB-type precursor. They are thus considered as
remnants of a dismembered dynamo-thermal sole formed during subduction of a
back-arc basin (proto-Sabzevar Ocean) formed in the upper-plate of the
Neotethyan slab. The metamorphic history of the granulites suggests an
anticlockwise pressure-temperature loop compatible with burial in a hot
subduction zone, followed by cooling during exhumation. Transition from a
nascent to a mature stage of oceanic subduction is the geodynamic scenario
proposed to accomplish for the reconstructed thermobaric evolution.
When framed with the regional scenario, results of this study point to
diachronous and independent tectonic evolutions of the different ophiolitic
domains of central Iran, for which a growing disparity in the timing of
metamorphic equilibration and of pressure-temperature paths can be expected
to emerge with further investigations.</description><pubDate>Fri, 11 Nov 2011 00:00:00 +0100</pubDate></item><item><title>New zircon data supporting models of short-lived igneous activity at 1.89 Ga in the western Skellefte District, central Fennoscandian Shield</title><link>http://www.solid-earth.net/2/205/2011/</link><description>&lt;b&gt;New zircon data supporting models of short-lived igneous activity at 1.89 Ga in the western Skellefte District, central Fennoscandian Shield&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 205-217, 2011&lt;br /&gt;&lt;br /&gt;Author(s): P. Skyttä, T. Hermansson, J. Andersson, M. Whitehouse, and P. Weihed&lt;br /&gt;&lt;br /&gt;New U-Th-Pb zircon data (SIMS) from three intrusive phases of the
Palaeoproterozoic Viterliden intrusion in the western Skellefte District,
central Fennoscandian Shield, dates igneous emplacement in a narrow time
interval at about 1.89 Ga. A locally occurring quartz-plagioclase
porphyritic tonalite, here dated at 1889 ± 3 Ma, is considered the youngest of the intrusive units, based on the new
age data and field evidence. This supports an existing interpretation of its fault-controlled emplacement
after intrusion of the dominating hornblende-tonalite units, in this study
dated at 1892 ± 3 Ma. The Viterliden magmatism was synchronous with the
oldest units of the Jörn type early-orogenic intrusions in the eastern
part of the district (1.89–1.88 Ga; cf. Gonzàles Roldán, 2010). A
U-Pb zircon age for a felsic metavolcanic rock from the hanging-wall to the
Kristineberg VMS deposit, immediately south of the Viterliden intrusion, is
constrained at 1883 ± 6 Ma in this study. It provides a minimum age for
the Kristineberg ore deposit and suggests contemporaneous igneous/volcanic
activity throughout the Skellefte District. Furthermore, it supports the
view that the Skellefte Group defines a laterally continuous belt throughout
this &quot;ore district&quot;. Tentative correlation of the 1889 ± 3 Ma
quartz-plagioclase porphyritic tonalite with the Kristineberg &quot;mine
porphyry&quot; suggests that these units are coeval at about 1.89 Ga. Based on
the new age determinations, the Viterliden intrusion may equally well have
intruded into or locally acted as a basement for the ore-hosting Skellefte
Group volcanic rocks.</description><pubDate>Wed, 26 Oct 2011 00:00:00 +0200</pubDate></item><item><title>The 11 May 2011 earthquake at Lorca (SE Spain) viewed in a structural-tectonic context</title><link>http://www.solid-earth.net/2/199/2011/</link><description>&lt;b&gt;The 11 May 2011 earthquake at Lorca (SE Spain) viewed in a structural-tectonic context&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 199-204, 2011&lt;br /&gt;&lt;br /&gt;Author(s): R. L. M. Vissers and B. M. L. Meijninger&lt;br /&gt;&lt;br /&gt;The Lorca earthquake of 11 May 2011 in the Betic Cordillera of SE Spain
occurred almost exactly on the Alhama de Murcia fault, a marked fault that
forms part of a NE-SW trending belt of faults and thrusts. The fault belt is
reminiscent of a strike-slip corridor, but recent structural studies have
provided clear evidence for reverse motions on these faults. Focal
mechanisms of the main earthquake, but also of a foreshock, are strikingly
consistent with structural observations on the Alhama de Murcia fault. This
strengthens the conclusion that, rather than a strike-slip fault, the fault
is at present a contractional fault with an oblique reverse sense of motion,
presumably in response to the NW-directed motion of Africa with respect to
Europe.</description><pubDate>Wed, 05 Oct 2011 00:00:00 +0200</pubDate></item><item><title>Positive geothermal anomalies in oceanic crust of Cretaceous age offshore Kamchatka</title><link>http://www.solid-earth.net/2/191/2011/</link><description>&lt;b&gt;Positive geothermal anomalies in oceanic crust of Cretaceous age offshore Kamchatka&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 191-198, 2011&lt;br /&gt;&lt;br /&gt;Author(s): G. Delisle&lt;br /&gt;&lt;br /&gt;Heat flow measurements were carried out in 2009 offshore Kamchatka during
the German-Russian joint-expedition KALMAR. An area with elevated heat flow
in oceanic crust of Cretaceous age – detected ~30 yr ago in the
course of several Russian heat flow surveys – was revisited. One previous
interpretation postulated anomalous lithospheric conditions or a connection
between a postulated mantle plume at great depth (&gt;200 km) as the source
for the observed high heat flow. However, the positive heat flow anomaly – as
our bathymetric data show – is closely associated with the fragmentation
of the western flank of the Meiji Seamount into a horst and graben
structure initiated during descent of the oceanic crust into the subduction
zone offshore Kamchatka. This paper offers an alternative interpretation,
which connects high heat flow primarily with natural convection of fluids in
the fragmented rock mass and, as a potential additional factor, high rates
of erosion, for which evidence is available from our collected bathymetric
image. Given high erosion rates, warm rock material at depth rises to nearer
the sea floor, where it cools and causes temporary elevated heat flow.</description><pubDate>Mon, 26 Sep 2011 00:00:00 +0200</pubDate></item><item><title>Dynamical geochemistry of the mantle</title><link>http://www.solid-earth.net/2/159/2011/</link><description>&lt;b&gt;Dynamical geochemistry of the mantle&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 159-189, 2011&lt;br /&gt;&lt;br /&gt;Author(s): G. F. Davies&lt;br /&gt;&lt;br /&gt;The reconciliation of mantle chemistry with the structure of the mantle
inferred from geophysics and dynamical modelling has been a long-standing
problem. This paper reviews three main aspects. First, extensions and
refinements of dynamical modelling and theory of mantle processing over the
past decade. Second, a recent reconsideration of the implications of mantle
heterogeneity for melting, melt migration, mantle differentiation and mantle
segregation. Third, a recent proposed shift in the primitive chemical
baseline of the mantle inferred from observations of non-chondritic
&lt;sup&gt;142&lt;/sup&gt;Nd in the Earth. It seems most issues can now be resolved, except
the level of heating required to maintain the mantle's thermal evolution.
&lt;br&gt;&lt;br&gt;
A reconciliation of refractory trace elements and their isotopes with the
dynamical mantle, proposed and given preliminary quantification by Hofmann,
White and Christensen, has been strengthened by work over the past decade.
The apparent age of lead isotopes and the broad refractory-element
differences among and between ocean island basalts (OIBs) and mid-ocean
ridge basalts (MORBs) can now be quantitatively accounted for with some
assurance.

&lt;br&gt;&lt;br&gt;
The association of the least radiogenic helium with relatively depleted
sources and their location in the mantle have been enigmatic. The least
radiogenic helium samples have recently been recognised as matching the
proposed non-chondritic primitive mantle. It has also been proposed recently
that noble gases reside in a so-called hybrid pyroxenite assemblage that is
the result of melt from fusible pods reacting with surrounding refractory
peridotite and refreezing. Hybrid pyroxenite that is off-axis may not remelt
and erupt at MORs, so its volatile constituents would recirculate within the
mantle. Hybrid pyroxenite is likely to be denser than average mantle, and
thus some would tend to settle in the D&quot; zone at the base of the mantle,
along with some old subducted oceanic crust. Residence times in D&quot; are
longer, so the hybrid pyroxenite there would be less degassed. Plumes would
sample both the degassed, enriched old oceanic crust and the gassy, less
enriched hybrid pyroxenite and deliver them to OIBs. These findings can
account quantitatively for the main He, Ne and Ar isotopic observations.
&lt;br&gt;&lt;br&gt;
It has been commonly inferred that the MORB source is strongly depleted of
incompatible elements. However it has recently been argued that conventional
estimates of the MORB source composition fail to take full account of mantle
heterogeneity, and in particular focus on an ill-defined &quot;depleted&quot; mantle
component while neglecting less common enriched components. Previous
estimates have also been tied to the composition of peridotites, but these
probably do not reflect the full complement of incompatible elements in the
heterogeneous mantle. New estimates that account for enriched mantle
components suggest the MORB source complement of incompatibles could be as
much as 50–100 % larger than previous estimates.
&lt;br&gt;&lt;br&gt;
A major difficulty has been the inference that mass balances of incompatible
trace elements could only be satisfied if there is a deep enriched layer in
the mantle, but the Earth's topography precludes such a layer. The
difficulty might be resolved if either the Earth is depleted relative to
chondritic or the MORB source is less depleted than previous estimates.
Together these factors can certainly resolve the mass balance difficulties.</description><pubDate>Tue, 13 Sep 2011 00:00:00 +0200</pubDate></item><item><title>The role of karst in engineering and environmental geosciences</title><link>http://www.solid-earth.net/2/155/2011/</link><description>&lt;b&gt;The role of karst in engineering and environmental geosciences&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 155-158, 2011&lt;br /&gt;&lt;br /&gt;Author(s): H. C. Ho&lt;br /&gt;&lt;br /&gt;Karst is a unique landform developed by soluble rock. It usually relates to
the groundwater drainage system, and provides important water resources. Current
researches indicate that karst is closely related to the Earth system and
environmental protection, and it can also create potential natural hazards
such as sinkhole flooding and land subsidence in urban area. Its
relationship with hydrogeology has also been an important factor for
studying water pollution and nutrient cycles in engineering geosciences and
agricultural geology.</description><pubDate>Tue, 30 Aug 2011 00:00:00 +0200</pubDate></item><item><title>Optical method for measuring bed topography and flow depth in an experimental flume</title><link>http://www.solid-earth.net/2/143/2011/</link><description>&lt;b&gt;Optical method for measuring bed topography and flow depth in an experimental flume&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 143-154, 2011&lt;br /&gt;&lt;br /&gt;Author(s): A. Limare, M. Tal, M. D. Reitz, E. Lajeunesse, and F. Métivier&lt;br /&gt;&lt;br /&gt;We describe an optical method known as moiré for acquiring quasi-simultaneous
measurements of bed topography and flow depth in laboratory experiments. The moiré method
is based on projecting a fringe pattern (grating) on the bed and analyzing the deformation
of the pattern caused by the topography with respect to a reference plane. The height
of the object is encoded in the phase of the pattern and can be retrieved either through
Fourier transform or phase shifting algorithms. The methodology enables image-based
non-contact measurements over a continuous surface at very high spatial and temporal
resolutions. We use a commercial software package of a moiré method called Light3D to
map bed topography and flow depth in an experimental braided channel and demonstrate
how the method can be used to characterize a full range of statistics not previously possible.</description><pubDate>Thu, 28 Jul 2011 00:00:00 +0200</pubDate></item><item><title>First observational evidence for the CO&lt;sub&gt;2&lt;/sub&gt;-driven origin of Stromboli's major explosions</title><link>http://www.solid-earth.net/2/135/2011/</link><description>&lt;b&gt;First observational evidence for the CO&lt;sub&gt;2&lt;/sub&gt;-driven origin of Stromboli's major explosions&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 135-142, 2011&lt;br /&gt;&lt;br /&gt;Author(s): A. Aiuppa, M. Burton, P. Allard, T. Caltabiano, G. Giudice, S. Gurrieri, M. Liuzzo, and G. Salerno&lt;br /&gt;&lt;br /&gt;We report on the first
detection of CO&lt;sub&gt;2&lt;/sub&gt; flux precursors of the till now unforecastable
&quot;major&quot; explosions that intermittently occur at Stromboli volcano (Italy).
An automated survey of the crater plume emissions in the period 2006–2010, during which 12 such explosions happened,
demonstrated that these events are systematically preceded by a brief phase
of increasing CO&lt;sub&gt;2&lt;/sub&gt;/SO&lt;sub&gt;2&lt;/sub&gt; weight ratio (up to &gt;40) and CO&lt;sub&gt;2&lt;/sub&gt; flux
(&gt;1300 t d&lt;sup&gt;−1&lt;/sup&gt;) with respect to the time-averaged values of 3.7 and
~500 t d&lt;sup&gt;−1&lt;/sup&gt; typical for standard Stromboli's activity. These signals are best
explained by the accumulation of CO&lt;sub&gt;2&lt;/sub&gt;-rich gas at a discontinuity of the
plumbing system (decreasing CO&lt;sub&gt;2&lt;/sub&gt; emission at the surface), followed by
increasing gas leakage prior to the explosion. Our observations thus supports
the recent model of Allard (2010) for a CO&lt;sub&gt;2&lt;/sub&gt;-rich gas trigger of
recurrent major explosions at Stromboli, and demonstrates the possibility to
forecast these events in advance from geochemical precursors. These
observations and conclusions have clear implications for monitoring
strategies at other open-vent basaltic volcanoes worldwide.</description><pubDate>Tue, 19 Jul 2011 00:00:00 +0200</pubDate></item><item><title>Geophysical characterisation of two segments of the Møre-Trøndelag Fault Complex, Mid Norway</title><link>http://www.solid-earth.net/2/125/2011/</link><description>&lt;b&gt;Geophysical characterisation of two segments of the Møre-Trøndelag Fault Complex, Mid Norway&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 125-134, 2011&lt;br /&gt;&lt;br /&gt;Author(s): A. Nasuti, C. Pascal, J. Ebbing, and J. F. Tønnesen&lt;br /&gt;&lt;br /&gt;The Møre-Trøndelag Fault Complex (MTFC) has controlled the tectonic
evolution of Mid Norway and its shelf for the past 400 Myr through repeated
reactivations during Palaeozoic, Mesozoic and perhaps Cenozoic times, the
very last phase of reactivation involving normal to oblique-slip faulting.
Despite its pronounced signature in the landscape, its deep structure has
largely remained unresolved until now. We focused on two specific segments
of the MTFC (i.e. the Tjellefonna and Bæverdalen faults) and acquired
multiple geophysical datasets (i.e. gravity, magnetic, resistivity and
shallow refraction profiles).
&lt;br&gt;&lt;br&gt;
A 100–200 m-wide zone of gouge and/or brecciated bedrock steeply dipping to
the south is interpreted as being the Tjellefonna fault sensu stricto. The fault appears
to be flanked by two additional but minor damage zones. A secondary normal
fault also steeply dipping to the south but involving indurated breccias was
detected ~1 km farther north. The Bæverdalen fault, ~12 km
farther north, is interpreted as a ~700 m-wide and highly deformed
zone involving fault gouge, breccias and lenses of intact bedrock. As such,
it is probably the most important fault segment in the studied area and
accommodated most of the strain during presumably Late Jurassic normal
faulting. Our geophysical data are indicative of a Bæverdalen fault
dipping steeply towards the south, in agreement with the average orientation
of the local tectonic grain. Our findings suggest that the influence of
Mesozoic normal faulting along the MTFC on landscape development is more
complex than previously thought.</description><pubDate>Mon, 11 Jul 2011 00:00:00 +0200</pubDate></item><item><title>Re-evaluation of the Mentelle Basin, a polyphase rifted margin basin, offshore southwest Australia: new insights from integrated regional seismic datasets</title><link>http://www.solid-earth.net/2/107/2011/</link><description>&lt;b&gt;Re-evaluation of the Mentelle Basin, a polyphase rifted margin basin, offshore southwest Australia: new insights from integrated regional seismic datasets&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 107-123, 2011&lt;br /&gt;&lt;br /&gt;Author(s): D. Maloney, C. Sargent, N. G. Direen, R. W. Hobbs, and D. R. Gröcke&lt;br /&gt;&lt;br /&gt;Vintage 2-D (two-dimensional) seismic reflection surveys from the sparsely
explored Mentelle Basin (western Australian margin) have been reprocessed
and integrated with a recent high-quality 2-D seismic survey and
stratigraphic borehole data. Interpretation of these data sets allows the
internal geometry of the Mentelle Basin fill and depositional history to be
reanalysed and new insights into its formation revealed. Basin stratigraphy
can be subdivided into several seismically defined megasequences separated
by major unconformities related to both breakup between India-Madagascar and
Australia-Antarctica in the Valanginian-Late Hauterivian and
tectonically-driven switches in deposition through the Albian.
&lt;br&gt;&lt;br&gt;
Resting on the Valanginian-Late Hauterivian breakup unconformity are several
kilometre-scale mounded structures that formed during Late Jurassic to Early
Cretaceous extension. These have previously been interpreted as volcanic
edifices although direct evidence of volcanic feeder systems is lacking. An
alternative interpretation is that these features may be carbonate
build-ups. The latter interpretation carries significant climatic
ramifications since carbonate build-ups would have formed at high
palaeolatitude, ~60° S.
&lt;br&gt;&lt;br&gt;
Soon after breakup, initial subsidence resulted in a shallow marine
environment and deposition of Barremian-Aptian silty-sandy mudstones. As
subsidence continued, thick successions of Albian ferruginous black clays
were deposited. Internally, seismic megasequences composed of successions of
black clays show previously unresolved unconformities, onlapping and
downlapping packages, which reflect a complex depositional, rifting and
subsidence history at odds with their previous interpretation as open marine
sediments.
&lt;br&gt;&lt;br&gt;
Southwestwards migration of the Kerguelen hotspot led to thermal contraction
and subsidence to the present day water depth (~3000 m). This was
accompanied by Turonian-Santonian deposition of massive chalk beds, which
are unconformably overlain by pelagic Palaeocene-Holocene sediments. This
substantial unconformity is related to the diachronous breakup and onset of
slow spreading between Australia and Antarctica, which may have led to the
reactivation and inversion of basement faults and was followed by rapid
seafloor spreading from the Middle Eocene to the present.</description><pubDate>Thu, 07 Jul 2011 00:00:00 +0200</pubDate></item><item><title>Exploring the potentials and limitations of the time-reversal imaging of finite seismic sources</title><link>http://www.solid-earth.net/2/95/2011/</link><description>&lt;b&gt;Exploring the potentials and limitations of the time-reversal imaging of finite seismic sources&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 95-105, 2011&lt;br /&gt;&lt;br /&gt;Author(s): S. Kremers, A. Fichtner, G. B. Brietzke, H. Igel, C. Larmat, L. Huang, and M. Käser&lt;br /&gt;&lt;br /&gt;The characterisation of seismic sources with time-reversed wave
fields is developing into a standard technique that has already been
successful in numerous applications.
While the time-reversal
imaging of effective point sources is now well-understood, little
work has been done to extend this technique to the study of finite
rupture processes. This is despite the pronounced non-uniqueness in
classic finite source inversions.
&lt;br&gt;&lt;br&gt;
The need to better constrain the details of finite rupture
processes motivates the series of synthetic and real-data time
reversal experiments described in this paper. We address questions
concerning the quality of focussing in the source area, the
localisation of the fault plane, the estimation of the slip
distribution and the source complexity up to which time-reversal
imaging can be applied successfully. The frequency band for the synthetic
experiments is chosen such that it is comparable to the band usually employed for
finite source inversion.
&lt;br&gt;&lt;br&gt;
Contrary to our expectations, we find that time-reversal
imaging is useful only for effective point sources, where it yields
good estimates of both the source location and the origin time. In
the case of finite sources, however, the time-reversed field does
not provide meaningful characterisations of the fault location and
the rupture process. This result cannot be improved sufficiently
with the help of different imaging fields, realistic modifications
of the receiver geometry or weights applied to the time-reversed
sources.
&lt;br&gt;&lt;br&gt;
The reasons for this failure are manifold. They include the choice of the frequency band,
the incomplete recording of wave field information at the surface,
the excitation of large-amplitude surface waves that deteriorate the
depth resolution, the absence of a sink that should absorb energy
radiated during the later stages of the rupture process, the
invisibility of small slip and the neglect of prior information
concerning the fault geometry and the inherent smoothness of seismologically inferred Earth models that prevents
the beneficial occurrence of strong multiple-scattering.
&lt;br&gt;&lt;br&gt;
The condensed conclusion of our study is that the
limitations of time-reversal imaging – at least in the frequency band
considered here – start where the seismic source stops being effectively
point-localised.</description><pubDate>Tue, 21 Jun 2011 00:00:00 +0200</pubDate></item><item><title>Native American lithic procurement along the international border in  the boot heel region of southwestern New Mexico</title><link>http://www.solid-earth.net/2/75/2011/</link><description>&lt;b&gt;Native American lithic procurement along the international border in  the boot heel region of southwestern New Mexico&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 2, 75-93, 2011&lt;br /&gt;&lt;br /&gt;Author(s): K. E. Zeigler, P. Hogan, C. Hughes, and A. Kurota&lt;br /&gt;&lt;br /&gt;Multidisciplinary field projects can be very useful to a more fundamental understanding
of the world around us, though these projects are not as common as they should be.
In particular, the combination of archeology and geology combines our understanding of
human behavior and human use of the landscape with an intimate knowledge of geologic
processes and the materials available for human use in order to gain a broader understanding
of human-Earth interaction. Here we present data from a cross-disciplinary project that uses
a common dataset, archeological artifacts, to explore the anthropological and geologic
implications of useage patterns. Archeological excavations and surveys conducted by the Office
of Contract Archeology in 2007 along the route of the proposed international border fence reveal
patterns of use of geologic materials by Archaic, Formative and Protohistoric Native Americans
in the Boot Heel of southwestern New Mexico. Thousands of artifacts were recorded in multiple
sites from Guadalupe Pass in the southern Peloncillo Mountains to the Carrizalillo Hills west
of Columbus. We identified the lithologies of artifacts, ranging from projectile points to
groundstones, and then constructed material movement maps based on either known procurement
sites (&quot;quarries&quot;) or outcrops identified as the closest source to a given site for each
lithology. Not unexpectedly, the majority of the rock types utilized by native peoples
are local siliceous volcanic materials. However, several artifacts constructed from obsidian
were transported into the region from northern Mexico and eastern Arizona, indicating
long-distance travel and/or trade routes. We also examine useage pattern difference between
Archaic, Formative and Protohistoric sites. Additionally, a dramatic change in distribution
of sources for geologic materials occurs between one pre-Spanish site and one post-Spanish
site that are adjacent to one another.</description><pubDate>Tue, 14 Jun 2011 00:00:00 +0200</pubDate></item></channel></rss>
