<?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>Candidates for multiple impact craters?: Popigai and Chicxulub as seen by the global high resolution gravitational field model EGM2008</title><link>http://www.solid-earth.net/1/71/2010/</link><description>&lt;b&gt;Candidates for multiple impact craters?: Popigai and Chicxulub as seen by the global high resolution gravitational field model EGM2008&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 1, 71-83, 2010&lt;br /&gt;&lt;br /&gt;Author(s): J. Klokočník, J. Kostelecký, I. Pešek, P. Novák, C. A. Wagner, and J. Sebera&lt;br /&gt;&lt;br /&gt;In 2008 the new Earth Gravitational Model (EGM2008) was released. It
contains a complete set of spherical harmonic coefficients of the Earth's
gravitational potential (Stokes parameters) to degree 2190 and order 2159
and selected orders to degree 2190, that can be used for evaluation of
various potential quantities with both the unprecedented accuracy and high
spatial resolution. Two such quantities, the gravity anomaly and
second-order radial derivative of the disturbing potential, were computed
over selected areas with known impact craters. The displays of these
derivatives for two such sites clearly show not only the strong
circular-like features known to be associated with them but also other
symmetrical structures which appear to make them multiple impact sites. At
Popigai, Siberia, the series of circular features fall in a line from the
&quot;primary crater&quot; in the southeast (SE) direction. At Chicxulub,
Yucatán, there appears to be one more crater close to the &quot;primary&quot; in
the northeast (NE) direction, as well as possibly others in the vicinity of
the main crater (SW). Gravity information alone is not, however, proof of
impact craters but it is useful in identifying &lt;i&gt;candidate sites&lt;/i&gt; for further study, for
examination by geologists and geophysicists. In the case of Chicxulub, a
very recent single seismic profile suggests that a more likely explanation
for the observed circular like gravity signal from EGM2008 NE of the
&quot;primary&quot; is a pre-impact basin.</description><pubDate>Wed, 21 Jul 2010 00:00:00 +0200</pubDate></item><item><title>Rheological control on the dynamics of explosive activity in the 2000 summit eruption of Mt. Etna</title><link>http://www.solid-earth.net/1/61/2010/</link><description>&lt;b&gt;Rheological control on the dynamics of explosive activity in the 2000 summit eruption of Mt. Etna&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 1, 61-69, 2010&lt;br /&gt;&lt;br /&gt;Author(s): D. Giordano, M. Polacci, P. Papale, and L. Caricchi&lt;br /&gt;&lt;br /&gt;In the period from January to June 2000 Mt. Etna exhibited an exceptional
explosive activity characterized by a succession of 64 Strombolian and
fire-fountaining episodes from the summit South-East Crater. Textural
analysis of the eruptive products reveals that the magma associated with the
Strombolian phases had a much larger crystal content (&amp;gt;55 vol%) with
respect to the magma discharged during the fire-fountain phases (~35
vol%). Rheological modelling shows that the crystal-rich magma falls in a
region beyond a critical crystal content where small addition of solid
particles causes an exponential increase of the effective magma viscosity.
When implemented into the modeling of steady magma ascent dynamics (as
assumed for the fire-fountain activity), a large crystal content as the one
found for products of Strombolian eruption phases results in a one order of
magnitude decrease of mass flow-rate, and in the onset of conditions where
small heterogeneities in the solid fraction carried by the magma translate
into highly unsteady eruption dynamics. We argue that crystallization on top
of the magmatic column during the intermediate phases when magma was not
discharged favoured conditions corresponding to Strombolian activity, with
fire-fountain activity resuming after removal of the highly crystalline top.
The numerical simulations also provide a consistent interpretation of the
association between fire-fountain activity and emergence of lava flows from
the crater flanks.</description><pubDate>Thu, 01 Jul 2010 00:00:00 +0200</pubDate></item><item><title>The stochastic quantization method and its application to the numerical simulation of volcanic conduit dynamics under random conditions</title><link>http://www.solid-earth.net/1/49/2010/</link><description>&lt;b&gt;The stochastic quantization method and its application to the numerical simulation of volcanic conduit dynamics under random conditions&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 1, 49-59, 2010&lt;br /&gt;&lt;br /&gt;Author(s): E. Peruzzo, M. Barsanti, F. Flandoli, and P. Papale&lt;br /&gt;&lt;br /&gt;Stochastic Quantization (SQ) is a method for the approximation of a
  continuous probability distribution with a discrete one. The
  proposal made in this paper is to apply this technique to reduce the
  number of numerical simulations for systems with uncertain inputs,
  when estimates of the output distribution are needed. This question
  is relevant in volcanology, where realistic simulations are very
  expensive and uncertainty is always present. We show the results of
  a benchmark test based on a one-dimensional steady model of magma
  flow in a volcanic conduit.</description><pubDate>Tue, 22 Jun 2010 00:00:00 +0200</pubDate></item><item><title>Particle size distributions by laser diffraction: sensitivity of granular matter strength to analytical operating procedures</title><link>http://www.solid-earth.net/1/25/2010/</link><description>&lt;b&gt;Particle size distributions by laser diffraction: sensitivity of granular matter strength to analytical operating procedures&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 1, 25-48, 2010&lt;br /&gt;&lt;br /&gt;Author(s): F. Storti and F. Balsamo&lt;br /&gt;&lt;br /&gt;We tested laser diffraction particle size analysis in poorly coherent
carbonate platform cataclastic breccias and unfaulted quartz-rich eolian
sands, representing low- and high-strength granular materials, respectively.
We used two different instruments with different sample dispersion and
pumping systems and several wet analytical procedures that included
different pump speeds, measurement precision tests with and without sample
ultrasonication, and different dispersant liquids. Results of our work
indicate that high strength material is not strongly affected by analytical
operating procedures, whereas low strength materials are very sensitive to
the pump speed, ultrasonication intensity, and measurement run time. To
reduce such a data variability, we propose a workflow of analytical tests
preliminary to the set up of the most appropriate SOP.</description><pubDate>Mon, 19 Apr 2010 00:00:00 +0200</pubDate></item><item><title>Earth's surface heat flux</title><link>http://www.solid-earth.net/1/5/2010/</link><description>&lt;b&gt;Earth's surface heat flux&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 1, 5-24, 2010&lt;br /&gt;&lt;br /&gt;Author(s): J. H. Davies and D. R. Davies&lt;br /&gt;&lt;br /&gt;We present a revised estimate of Earth's surface heat flux that is based
upon a heat flow data-set with 38 347 measurements, which is 55% more
than used in previous estimates. Our methodology, like others, accounts for
hydrothermal circulation in young oceanic crust by utilising a half-space
cooling approximation. For the rest of Earth's surface, we estimate the
average heat flow for different geologic domains as defined by global
digital geology maps; and then produce the global estimate by multiplying it
by the total global area of that geologic domain. The averaging is done on a
polygon set which results from an intersection of a 1 degree equal area grid
with the original geology polygons; this minimises the adverse influence of
clustering. These operations and estimates are derived accurately using
methodologies from Geographical Information Science. We consider the
virtually un-sampled Antarctica separately and also make a small correction
for hot-spots in young oceanic lithosphere. A range of analyses is
presented. These, combined with statistical estimates of the error, provide
a measure of robustness. Our final preferred estimate is 47&amp;plusmn;2 TW,
which is greater than previous estimates.</description><pubDate>Mon, 22 Feb 2010 00:00:00 +0100</pubDate></item><item><title>The Eons of Chaos and Hades</title><link>http://www.solid-earth.net/1/1/2010/</link><description>&lt;b&gt;The Eons of Chaos and Hades&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Solid Earth, 1, 1-3, 2010&lt;br /&gt;&lt;br /&gt;Author(s): C. Goldblatt, K. J. Zahnle, N. H. Sleep, and E. G. Nisbet&lt;br /&gt;&lt;br /&gt;We propose the &lt;i&gt;Chaotian Eon&lt;/i&gt; to demarcate geologic time from
the origin of the Solar System to the Moon-forming impact on Earth.
This separates the solar system wide processes of planet formation
from the subsequent divergent evolution of the inner planets. We
further propose the division of the Hadean Eon into eras and periods
and naming the proto-Earth &lt;i&gt;Tellus&lt;/i&gt;.</description><pubDate>Tue, 02 Feb 2010 00:00:00 +0100</pubDate></item></channel></rss>