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	<title><![CDATA[Geosciences, Vol. 3, Pages 331-353: Geodynamic Reconstructions of the Australides—2:  Mesozoic–Cainozoic]]></title>
	<link>http://www.mdpi.com/2076-3263/3/2/331</link>
	<description>The present work, derived from a full global geodynamic reconstruction model over 600 Ma and based on a large database, focuses herein on the interaction between the Pacific, Australian and Antarctic plates since 200 Ma, and proposes integrated solutions for a coherent, physically consistent scenario. The evolution of the Australia–Antarctica–West Pacific plate system is dependent on the Gondwana fit chosen for the reconstruction. Our fit, as defined for the latest Triassic, implies an original scenario for the evolution of the region, in particular for the “early” opening history of the Tasman Sea. The interaction with the Pacific, moreover, is characterised by many magmatic arc migrations and ocean openings, which are stopped by arc–arc collision, arc–spreading axis collision, or arc–oceanic plateau collision, and subduction reversals. Mid-Pacific oceanic plateaus created in the model are much wider than they are on present-day maps, and although they were subducted to a large extent, they were able to stop subduction. We also suggest that adduction processes (i.e., re-emergence of subducted material) may have played an important role, in particular along the plate limit now represented by the Alpine Fault in New Zealand.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2013-06-04</prism:publicationDate>
	<prism:volume>3</prism:volume>
	<prism:number>2</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences3020331</prism:doi>
	<prism:startingPage>331</prism:startingPage>
		<prism:endingPage>353</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Geodynamic Reconstructions of the Australides—2:  Mesozoic–Cainozoic]]></dc:title>
    <dc:date>2013-06-04</dc:date>
	<dc:identifier>doi: 10.3390/geosciences3020331</dc:identifier>
    	<dc:creator>Christian Vérard</dc:creator>
		<dc:creator>Gérard Stampfli</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
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        <item rdf:about="http://www.mdpi.com/2076-3263/3/2/311">
	<title><![CDATA[Geosciences, Vol. 3, Pages 311-330: Geodynamic Reconstructions of the Australides—1: Palaeozoic]]></title>
	<link>http://www.mdpi.com/2076-3263/3/2/311</link>
	<description>A full global geodynamical reconstruction model has been developed at the University of Lausanne over the past 20 years, and is used herein to re-appraise the evolution of the Australides from 600 to 200 Ma. Geological information of geodynamical interest associated with constraints on tectonic plate driving forces allow us to propose a consistent scenario for the evolution of Australia–Antarctica–proto-Pacific system. According to our model, most geodynamic units (GDUs) of the Australides are exotic in origin, and many tectonic events of the Delamerian Cycle, Lachlan SuperCycle, and New England SuperCycle are regarded as occurring off-shore Gondwana.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2013-06-04</prism:publicationDate>
	<prism:volume>3</prism:volume>
	<prism:number>2</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences3020311</prism:doi>
	<prism:startingPage>311</prism:startingPage>
		<prism:endingPage>330</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Geodynamic Reconstructions of the Australides—1: Palaeozoic]]></dc:title>
    <dc:date>2013-06-04</dc:date>
	<dc:identifier>doi: 10.3390/geosciences3020311</dc:identifier>
    	<dc:creator>Christian Vérard</dc:creator>
		<dc:creator>Gérard Stampfli</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
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        <item rdf:about="http://www.mdpi.com/2076-3263/3/2/262">
	<title><![CDATA[Geosciences, Vol. 3, Pages 262-310: Mesozoic–Cenozoic Evolution of the Western Margin of South America: Case Study of the Peruvian Andes]]></title>
	<link>http://www.mdpi.com/2076-3263/3/2/262</link>
	<description>Based on the structural style and physiographic criteria, the Central Andes of Peru can be divided into segments running parallel to the Pacific coast. The westernmost segment, the Coastal Belt, consists of a Late Jurassic–Cretaceous volcanic arc sequence that was accreted to the South American craton in Cretaceous times. The Mesozoic strata of the adjacent Western Cordillera represent an ENE-vergent fold-and-thrust belt that formed in Eocene times. Tight upright folds developed above a shallow detachment horizon in the West, while more open folds formed above a deeper detachment horizon towards the East and in the neighboring Central Highlands. A completely different style with steeply dipping reverse faults and open folds affecting the Neoproterozoic crystalline basement is typical for the Eastern Cordillera. The Subandean Zone is characterized by mainly NE-vergent imbricate thrusting which occurred in Neogene times. A quantitative estimate of the shortening of the orogen obtained from balanced cross-sections indicates a total shortening of 120–150 km (24%–27%). This shortening was coevel with the Neogene westward drift of South America, occurred at rates between 3 and 4.7 mm/year and was responsible for the high elevation of the Peruvian Andes.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2013-06-04</prism:publicationDate>
	<prism:volume>3</prism:volume>
	<prism:number>2</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences3020262</prism:doi>
	<prism:startingPage>262</prism:startingPage>
		<prism:endingPage>310</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Mesozoic–Cenozoic Evolution of the Western Margin of South America: Case Study of the Peruvian Andes]]></dc:title>
    <dc:date>2013-06-04</dc:date>
	<dc:identifier>doi: 10.3390/geosciences3020262</dc:identifier>
    	<dc:creator>O. Pfiffner</dc:creator>
		<dc:creator>Laura Gonzalez</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
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        <item rdf:about="http://www.mdpi.com/2076-3263/3/2/240">
	<title><![CDATA[Geosciences, Vol. 3, Pages 240-261: Preservation and Recycling of Crust during Accretionary and Collisional Phases of Proterozoic Orogens: A Bumpy Road from Nuna to Rodinia]]></title>
	<link>http://www.mdpi.com/2076-3263/3/2/240</link>
	<description>Zircon age peaks at 2100–1650 and 1200–1000 Ma correlate with craton collisions in the growth of supercontinents Nuna and Rodinia, respectively, with a time interval between collisions mostly &amp;amp;lt;50 Myr (range 0–250 Myr). Collisional orogens are two types: those with subduction durations &amp;amp;lt;500 Myr and those ≥500 Myr. The latter group comprises orogens with long-lived accretionary stages between Nuna and Rodinia assemblies. Neither orogen age nor duration of either subduction or collision correlates with the volume of orogen preserved. Most rocks preserved date to the pre-collisional, subduction (ocean-basin closing) stage and not to the collisional stage. The most widely preserved tectonic setting in Proterozoic orogens is the continental arc (10%–90%, mean 60%), with oceanic tectonic settings (oceanic crust, arcs, islands and plateaus, serpentinites, pelagic sediments) comprising &amp;amp;lt;20% and mostly &amp;amp;lt;10%. Reworked components comprise 20%–80% (mean 32%) and microcratons comprise a minor but poorly known fraction. Nd and Hf isotopic data indicate that Proterozoic orogens contain from 10% to 60% of juvenile crust (mean 36%) and 40%–75% reworked crust (mean 64%). Neither the fraction nor the rate of preservation of juvenile crust is related to the collision age nor to the duration of subduction. Regardless of the duration of subduction, the amount of juvenile crust preserved reaches a maximum of about 60%, and 37% of the volume of juvenile continental crust preserved between 2000 and 1000 Ma was produced in the Great Proterozoic Accretionary Orogen (GPAO). Pronounced minima occur in frequency of zircon ages of rocks preserved in the GPAO; with minima at 1600–1500 Ma in Laurentia; 1700–1600 Ma in Amazonia; and 1750–1700 Ma in Baltica. If these minima are due to subduction erosion and delamination as in the Andes in the last 250 Myr; approximately one third of the volume of the Laurentian part of the GPAO could have been recycled into the mantle between 1500 and 1250 Ma. This may have enriched the mantle wedge in incompatible elements and water leading to the production of felsic magmas responsible for the widespread granite-rhyolite province of this age. A rapid decrease in global Nd and in detrital zircon Hf model ages between about 1600 and 1250 Ma could reflect an increase in recycling rate of juvenile crust into the mantle; possibly in response to partial fragmentation of Nuna.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2013-05-29</prism:publicationDate>
	<prism:volume>3</prism:volume>
	<prism:number>2</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences3020240</prism:doi>
	<prism:startingPage>240</prism:startingPage>
		<prism:endingPage>261</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Preservation and Recycling of Crust during Accretionary and Collisional Phases of Proterozoic Orogens: A Bumpy Road from Nuna to Rodinia]]></dc:title>
    <dc:date>2013-05-29</dc:date>
	<dc:identifier>doi: 10.3390/geosciences3020240</dc:identifier>
    	<dc:creator>Kent Condie</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/3/2/216">
	<title><![CDATA[Geosciences, Vol. 3, Pages 216-239: The Role of Regional and Local Structure in a Late Ordovician (Edenian) Foreland Platform-to-Basin Succession Inboard of the Taconic Orogen, Central Canada]]></title>
	<link>http://www.mdpi.com/2076-3263/3/2/216</link>
	<description>The Upper Ordovician (Edenian) Lindsay Formation of the Ottawa Embayment represents the final stage of carbonate platform development in the Taconic foreland periphery inboard of the northern Appalachian orogen. The succession overlies a narrow (~60 km) axis of a Neoproterozoic Laurentian rift extending across the Grenville orogen. The Lindsay Formation consists of a lower heavily bioturbated skeletal limestone that represents a warm-water shoal facies following an underlying outer ramp stratigraphy, and an upper division of renewed deep-water deposition with organic-rich shale and fossiliferous lime mudstone. Pyritic deep-water black shale of the westerly advancing Taconic foreland basin disconformably overlies this platform succession. Stratigraphic correlation through the central embayment identifies likely synsedimentary faults and seaward-directed erosion bounding the Lindsay Formation in a region of older Ordovician faults and a change in the lithotectonic character of the crystalline basement. The Late Ordovician shallowing and localization of structural/erosional features are interpreted to record a structural hinge: a local accommodation to, first, foreland periphery uplift, then rapid subsidence related to westerly diachronous foreland subsidence through the platform interior. Spatial association of structures of differing ages suggests that reactivation of inherited weakened crust influenced Late Ordovician sedimentary patterns.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2013-05-21</prism:publicationDate>
	<prism:volume>3</prism:volume>
	<prism:number>2</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences3020216</prism:doi>
	<prism:startingPage>216</prism:startingPage>
		<prism:endingPage>239</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[The Role of Regional and Local Structure in a Late Ordovician (Edenian) Foreland Platform-to-Basin Succession Inboard of the Taconic Orogen, Central Canada]]></dc:title>
    <dc:date>2013-05-21</dc:date>
	<dc:identifier>doi: 10.3390/geosciences3020216</dc:identifier>
    	<dc:creator>Ruth Gbadeyan</dc:creator>
		<dc:creator>George Dix</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/3/2/176">
	<title><![CDATA[Geosciences, Vol. 3, Pages 176-215: Structural Evolution of the East Sierra Valley System  (Owens Valley and Vicinity), California: A Geologic and Geophysical Synthesis]]></title>
	<link>http://www.mdpi.com/2076-3263/3/2/176</link>
	<description>The tectonically active East Sierra Valley System (ESVS), which comprises the westernmost part of the Walker Lane-Eastern California Shear Zone, marks the boundary between the highly extended Basin and Range Province and the largely coherent Sierra Nevada-Great Valley microplate (SN-GVm), which is moving relatively NW. The recent history of the ESVS is characterized by oblique extension partitioned between NNW-striking normal and strike-slip faults oriented at an angle to the more northwesterly relative motion of the SN-GVm. Spatially variable extension and right-lateral shear have resulted in a longitudinally segmented valley system composed of diverse geomorphic and structural elements, including a discontinuous series of deep basins detected through analysis of isostatic gravity anomalies. Extension in the ESVS probably began in the middle Miocene in response to initial westward movement of the SN-GVm relative to the Colorado Plateau. At ca. 3–3.5 Ma, the SN-GVm became structurally separated from blocks directly to the east, resulting in significant basin-forming deformation in the ESVS. We propose a structural model that links high-angle normal faulting in the ESVS with coeval low-angle detachment faulting in adjacent areas to the east.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2013-04-22</prism:publicationDate>
	<prism:volume>3</prism:volume>
	<prism:number>2</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences3020176</prism:doi>
	<prism:startingPage>176</prism:startingPage>
		<prism:endingPage>215</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Structural Evolution of the East Sierra Valley System  (Owens Valley and Vicinity), California: A Geologic and Geophysical Synthesis]]></dc:title>
    <dc:date>2013-04-22</dc:date>
	<dc:identifier>doi: 10.3390/geosciences3020176</dc:identifier>
    	<dc:creator>Calvin Stevens</dc:creator>
		<dc:creator>Paul Stone</dc:creator>
		<dc:creator>Richard Blakely</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/3/2/159">
	<title><![CDATA[Geosciences, Vol. 3, Pages 159-175: Syracuse Limestone: From the Past a Prospect for  Contemporary Buildings]]></title>
	<link>http://www.mdpi.com/2076-3263/3/2/159</link>
	<description>The conservation of the historic stone heritage has great importance when this material characterizes the image of a city, as it happens in Syracuse (Sicily). Its historical buildings are afflicted by a heavy state of deterioration due to the particular microclimate, to pollution and to neglect endured over time. This article reports the investigations made on limestone samples from historic façades of the city and from the neighboring quarries still in operation, in order to understand the petrographic typology, the reaction to the degradation over time, the possible maintenance and recovery interventions, and the correct applications in buildings of new construction. For this aim, bulk and surface analysis have been made both on the quarry materials and on the corresponding aged materials. It is therefore possible to define the types of rock most suitable for the use in contemporary architecture guaranteeing criteria of perfect biocompatibility. In this way a natural material can be employed in traditional and innovative uses and ensure both the sustainability of the interventions and the continuity of a consolidated tradition.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2013-04-11</prism:publicationDate>
	<prism:volume>3</prism:volume>
	<prism:number>2</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences3020159</prism:doi>
	<prism:startingPage>159</prism:startingPage>
		<prism:endingPage>175</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Syracuse Limestone: From the Past a Prospect for  Contemporary Buildings]]></dc:title>
    <dc:date>2013-04-11</dc:date>
	<dc:identifier>doi: 10.3390/geosciences3020159</dc:identifier>
    	<dc:creator>Alessia Giuffrida</dc:creator>
		<dc:creator>Enrico Ciliberto</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/3/2/140">
	<title><![CDATA[Geosciences, Vol. 3, Pages 140-158: Spatial Evolution of the Chromium Contamination in Soils from the Assopos to Thiva  Basin and C. Evia (Greece) and Potential Source(s): Anthropogenic versus Natural Processes]]></title>
	<link>http://www.mdpi.com/2076-3263/3/2/140</link>
	<description>The investigation of the contamination in soil, plants and groundwater revealed a spatial evolution, with an increasing trend in the Cr, Fe, Ni, Mn and Co contents in soils from the Assopos to Thiva basin, followed by C. Evia and Ni-laterite deposits, suggesting that the latter and their parent ophiolites are a potential source for these metals. In contrast, the contamination in groundwater by Cr(VI), ranging from 2 to 360 μg/L Cr, and a varying degree of salinization is probably due to both human activities and natural processes. A diverse source for the contamination of soil and groundwater in the Assopos-Thiva basins is consistent with the increasing trend of the Mg/Si ratio and Cr(VI) concentration in water. The use of deep karst-type aquifer instead of the shallow-Neogene one may provide a solution to the crucial environmental problem. The selective extraction by EDTA and alkaline solution showed that Cr and Fe are less available than Mn. The Cr contents in plants range from &amp;amp;lt;1 to tens of mg/kg, due probably to the high resistance of chromite. However, the average Crtotal contents in plants/crops are higher than normal or sufficient values, whilst Crtotal accumulation [(% metals in plants × 100)/metal in soil] and Cr(VI) accumulation are relatively low. There is a very good positive correlation between accumulation factors for Cr and Fe (R2 = 0.92), suggesting a similarity concerning their uptake.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2013-04-09</prism:publicationDate>
	<prism:volume>3</prism:volume>
	<prism:number>2</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences3020140</prism:doi>
	<prism:startingPage>140</prism:startingPage>
		<prism:endingPage>158</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Spatial Evolution of the Chromium Contamination in Soils from the Assopos to Thiva  Basin and C. Evia (Greece) and Potential Source(s): Anthropogenic versus Natural Processes]]></dc:title>
    <dc:date>2013-04-09</dc:date>
	<dc:identifier>doi: 10.3390/geosciences3020140</dc:identifier>
    	<dc:creator>Maria Economou-Eliopoulos</dc:creator>
		<dc:creator>Ifigeneia Megremi</dc:creator>
		<dc:creator>Cathy Atsarou</dc:creator>
		<dc:creator>Christina Theodoratou</dc:creator>
		<dc:creator>Charalambos Vasilatos</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/3/1/114">
	<title><![CDATA[Geosciences, Vol. 3, Pages 114-139: Evolution of Endemic Species, Ecological Interactions and Geographical Changes in an Insular Environment: A Case Study of Quaternary Mammals of Sicily (Italy, EU)]]></title>
	<link>http://www.mdpi.com/2076-3263/3/1/114</link>
	<description>The Quaternary mammals of Sicily are well known, and five faunal complexes have been distinguished on the basis of bioevents (extinctions and new arrivals) and evolution of endemic species. It is clear that the composition of mammal faunas is strictly related to the dispersal ability of each species and to the paleogeography of the area. Until now, researches have chiefly attributed paleogeographical changes as controlling these dispersals: the sea strait between the island and the Italian peninsula has had different widths and depths over time, operating different kinds of filters on the spreading of terrestrial mammals. Moreover, Sicily and its nearby mainland underwent changes in paleogeography. Some incongruence in bioevents has been attributed to the filter operated by the marine strait, which could have acted in differential ways on large and small mammals. However, the roles of ecological interactions among vertebrate species and their control on bioevents have been greatly underestimated. In this critical review, changes in mammals’ associations are reconsidered not only in terms of biochronology and dispersal ability of taxa through the marine strait, evolution of endemic features, in addition to the paleogeography of the island, but also considering the ecological role of each species and the interactions among the species with each faunal complex.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2013-02-05</prism:publicationDate>
	<prism:volume>3</prism:volume>
	<prism:number>1</prism:number>
	<prism:section>Review</prism:section>
	<prism:doi>10.3390/geosciences3010114</prism:doi>
	<prism:startingPage>114</prism:startingPage>
		<prism:endingPage>139</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Evolution of Endemic Species, Ecological Interactions and Geographical Changes in an Insular Environment: A Case Study of Quaternary Mammals of Sicily (Italy, EU)]]></dc:title>
    <dc:date>2013-02-05</dc:date>
	<dc:identifier>doi: 10.3390/geosciences3010114</dc:identifier>
    	<dc:creator>Antonella Marra</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/3/1/102">
	<title><![CDATA[Geosciences, Vol. 3, Pages 102-113: Verde Macael: A Serpentinite Wrongly Referred to as a Marble]]></title>
	<link>http://www.mdpi.com/2076-3263/3/1/102</link>
	<description>Serpentinites are used in both exterior and interior locations, but not all serpentinites are equal: they vary in physical-mechanical behavior and are not all suitable for similar uses. The serpentinites most commonly used worldwide come from India, Pakistan or Egypt. Spain has traditionally quarried two ultramafic massifs, one in Galicia (Verde Pirineos) and one in Andalucía (Verde Macael). Some of these quarries were small family-run businesses. In both cases, these rocks are commercially available as “green marble.” These serpentinites commonly have a high degree of carbonation, but the process does not always take place with the same intensity. Carbonate can act as a cementing agent of the other phases, increasing the mechanical strength parameters. As a result, an improvement in the strength conditions is achieved, but a misinterpretation of the suitability of the rock may occur because a perception among users that “green marble” is similar to geologically defined marble. This may lead to inappropriate applications as an ornamental stone. At a time of economic crisis in Europe, the natural stone sector is encouraged to invest in research to identify the best quality products that can compete profitably with those currently being imported from other countries. This paper provides a comparison of properties of the Verde Macael serpentinite with a true marble in the hope of contributing to improving the natural stone industrial sector.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2013-02-05</prism:publicationDate>
	<prism:volume>3</prism:volume>
	<prism:number>1</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences3010102</prism:doi>
	<prism:startingPage>102</prism:startingPage>
		<prism:endingPage>113</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Verde Macael: A Serpentinite Wrongly Referred to as a Marble]]></dc:title>
    <dc:date>2013-02-05</dc:date>
	<dc:identifier>doi: 10.3390/geosciences3010102</dc:identifier>
    	<dc:creator>Rafael Navarro</dc:creator>
		<dc:creator>Dolores Pereira</dc:creator>
		<dc:creator>Ana Gimeno</dc:creator>
		<dc:creator>Santiago Barrio</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/3/1/63">
	<title><![CDATA[Geosciences, Vol. 3, Pages 63-101: Rocks, Clays, Water, and Salts: Highly Durable, Infinitely Rechargeable, Eminently Controllable Thermal Batteries  for Buildings]]></title>
	<link>http://www.mdpi.com/2076-3263/3/1/63</link>
	<description>Materials that store the energy of warm days, to return that heat during cool nights, have been fundamental to vernacular building since ancient times. Although building with thermally rechargeable materials became a niche pursuit with the advent of fossil fuel-based heating and cooling, energy and climate change concerns have sparked new enthusiasm for these substances of high heat capacity and moderate thermal conductivity: stone, adobe, rammed earth, brick, water, concrete, and more recently, phase-change materials. While broadly similar, these substances absorb and release heat in unique patterns characteristic of their mineralogies, densities, fluidities, emissivities, and latent heats of fusion. Current architectural practice, however, shows little awareness of these differences and the resulting potential to match materials to desired thermal performance. This investigation explores that potential, illustrating the correspondence between physical parameters and thermal storage-and-release patterns in direct-, indirect-, and isolated-gain passive solar configurations. Focusing on heating applications, results demonstrate the superiority of water walls for daytime warmth, the tunability of granite and concrete for evening warmth, and the exceptional ability of phase-change materials to sustain  near-constant heat delivery throughout the night.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2013-01-25</prism:publicationDate>
	<prism:volume>3</prism:volume>
	<prism:number>1</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences3010063</prism:doi>
	<prism:startingPage>63</prism:startingPage>
		<prism:endingPage>101</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Rocks, Clays, Water, and Salts: Highly Durable, Infinitely Rechargeable, Eminently Controllable Thermal Batteries  for Buildings]]></dc:title>
    <dc:date>2013-01-25</dc:date>
	<dc:identifier>doi: 10.3390/geosciences3010063</dc:identifier>
    	<dc:creator>Alexandra Rempel</dc:creator>
		<dc:creator>Alan Rempel</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/3/1/46">
	<title><![CDATA[Geosciences, Vol. 3, Pages 46-62: Engineering Geology Maps for Planning and Management of Natural Parks: “Las Batuecas-Sierra de Francia” and “Quilamas” (Central Spanish System, Salamanca, Spain)]]></title>
	<link>http://www.mdpi.com/2076-3263/3/1/46</link>
	<description>Presented herein is a cartographic procedure that is easy to utilise and at low-cost, which facilitates the first stages of planning and management of a naturally protected space and considers the geotechnical parameters that influence human activity. This procedure uses geographical information systems technology by combining the cartographies for the most influential parameters on the stability of the area (lithology, hydrogeology, geomorphology, slopes, lineament/fractures and seismicity) with geomechanical mapping generated from geotechnical parameters obtained through field and laboratory tests. This geotechnical mapping facilitates the division of a territory into zones according to each type of problem and generates a cartography for natural hazards. Using this information, it is possible to produce a cartography of constructive conditions or geotechnical hazards. This methodology has been validated by application to two natural protected spaces, “Las Batuecas-Sierra de Francia” and “Quilamas”. The validation confirmed that the cartography procedure described herein is a preventive, and not a structural measure. It is a tool that delimits areas with different constructive use recommendations and limitations, and therefore, is useful for natural space managers.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2013-01-18</prism:publicationDate>
	<prism:volume>3</prism:volume>
	<prism:number>1</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences3010046</prism:doi>
	<prism:startingPage>46</prism:startingPage>
		<prism:endingPage>62</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Engineering Geology Maps for Planning and Management of Natural Parks: “Las Batuecas-Sierra de Francia” and “Quilamas” (Central Spanish System, Salamanca, Spain)]]></dc:title>
    <dc:date>2013-01-18</dc:date>
	<dc:identifier>doi: 10.3390/geosciences3010046</dc:identifier>
    	<dc:creator>Antonio Martínez-Graña</dc:creator>
		<dc:creator>José Goy</dc:creator>
		<dc:creator>Caridad Zazo</dc:creator>
		<dc:creator>Mariano Yenes</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/3/1/30">
	<title><![CDATA[Geosciences, Vol. 3, Pages 30-45: Hydrophobization by Means of Nanotechnology on Greek Sandstones Used as Building Facades]]></title>
	<link>http://www.mdpi.com/2076-3263/3/1/30</link>
	<description>Modern sustainable architecture indicates the use of local natural stones for building. Greek sandstones from Epirus (Demati, Greece, EN 12440) used as building facades meet aesthetic and have high mechanical properties, but the inevitable interaction between stone materials and natural or anthropogenic weathering factors controls the type, and extent of stone damages. In the present paper, samples of sandstone were treated with a conventional hydrophobic product and four solutions of the same product, enriched with nanosilica of different concentrations. The properties of the treated samples, such as porosity and pore size distribution, microstructure, static contact angle of a water droplet, and durability to deterioration cycles (freeze-thaw) were recorded and conclusions were drawn. The research indicates the increased hydrophobic properties in nanosilica solutions but also the optimum content in nanoparticles that provides hydrophobicity without altering the properties of the stone.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2013-01-18</prism:publicationDate>
	<prism:volume>3</prism:volume>
	<prism:number>1</prism:number>
	<prism:section>Technical Note</prism:section>
	<prism:doi>10.3390/geosciences3010030</prism:doi>
	<prism:startingPage>30</prism:startingPage>
		<prism:endingPage>45</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Hydrophobization by Means of Nanotechnology on Greek Sandstones Used as Building Facades]]></dc:title>
    <dc:date>2013-01-18</dc:date>
	<dc:identifier>doi: 10.3390/geosciences3010030</dc:identifier>
    	<dc:creator>Maria Stefanidou</dc:creator>
		<dc:creator>Katia Matziaris</dc:creator>
		<dc:creator>Georgios Karagiannis</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/3/1/1">
	<title><![CDATA[Geosciences, Vol. 3, Pages 1-29: Nacre in Molluscs from the Ordovician of the Midwestern United States]]></title>
	<link>http://www.mdpi.com/2076-3263/3/1/1</link>
	<description>Nacre was previously thought to be primitive in the Mollusca, but no convincing Cambrian examples are known. This aragonitic microstructure with crystal tablets that grow within an organic framework is thought to be the strongest, most fracture-resistant type of shell microstructure. Fossils described herein from the Ordovician of Iowa, Indiana, and Ohio provide supporting evidence for the hypothesis that sometime between the middle Cambrian and late Ordovician, nacre originated in cephalopod, bivalve, and possibly gastropod lineages. The correlation of independent origins of fracture-resistant nacre with increasing shell-crushing abilities of predators during the Cambrian-Ordovician suggests an early pulse in the evolutionary arms race between predators and molluscan prey.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2013-01-08</prism:publicationDate>
	<prism:volume>3</prism:volume>
	<prism:number>1</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences3010001</prism:doi>
	<prism:startingPage>1</prism:startingPage>
		<prism:endingPage>29</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Nacre in Molluscs from the Ordovician of the Midwestern United States]]></dc:title>
    <dc:date>2013-01-08</dc:date>
	<dc:identifier>doi: 10.3390/geosciences3010001</dc:identifier>
    	<dc:creator>Michael Vendrasco</dc:creator>
		<dc:creator>Antonio Checa</dc:creator>
		<dc:creator>William Heimbrock</dc:creator>
		<dc:creator>Steven Baumann</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/4/298">
	<title><![CDATA[Geosciences, Vol. 2, Pages 298-307: Hellenic Natural Zeolite as a Replacement of Sand in Mortar: Mineralogy Monitoring and Evaluation of Its Influence on Mechanical Properties]]></title>
	<link>http://www.mdpi.com/2076-3263/2/4/298</link>
	<description>HEU-type zeolite-rich volcaniclastic tuff (Hellenic natural zeolite) is used as a raw material for the production of lighter mortars. The addition of natural zeolite in mortar mixtures of sand and Portland cement leads to a decrease of up to 18.35% unit weight. The increase of the natural zeolite proportions increases the porosity and water absorption of the mortar and, at the same time, decreases the uniaxial compressive strength. These variations in the mortar’s mechanical properties are due to the addition of natural zeolite, which causes incomplete hydration of C2S (2CaO.SiO2) and retardation of the mortar’s hardening.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-11-22</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>4</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences2040298</prism:doi>
	<prism:startingPage>298</prism:startingPage>
		<prism:endingPage>307</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Hellenic Natural Zeolite as a Replacement of Sand in Mortar: Mineralogy Monitoring and Evaluation of Its Influence on Mechanical Properties]]></dc:title>
    <dc:date>2012-11-22</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2040298</dc:identifier>
    	<dc:creator>Dimitrios Vogiatzis</dc:creator>
		<dc:creator>Nikolaos Kantiranis</dc:creator>
		<dc:creator>Anestis Filippidis</dc:creator>
		<dc:creator>Evaggelos Tzamos</dc:creator>
		<dc:creator>Costas Sikalidis</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/4/277">
	<title><![CDATA[Geosciences, Vol. 2, Pages 277-297: A Site-Specific Index Based on Weathering Forms Visible in Central Oxford, UK]]></title>
	<link>http://www.mdpi.com/2076-3263/2/4/277</link>
	<description>The authenticity of much of the stone-work along Queen’s Lane in central Oxford, UK presented an opportunity to produce a photographic survey from which a weathering index could be established. This represents a site-specific approach to devising a weathering form. Because it is photo-based, weathering forms are visible for comparison and classification purposes across disciplines. Limestone pertaining to building ashlar and plinths along this roadway, which mainly belong to Queen’s College, St Edmund Hall, New College, and Hertford College, was classified according to this newly introduced weathering index, the size-extent (S-E) index, through consideration of type, size, extent, impact, and trigger. This size- (range) and extent-based classification system enables for the assessment of weathering forms of various types, including soiling and decay features as well as those potentially expected in the presence of vegetation and animals. Weathering forms of a range of sizes were present, with a slightly greater abundance of small types (mm-cm in the micro- to mesoscale) and more discrete types with a low extent. For this location in central Oxford, chemical weathering was found to be the predominant type of soiling and decay.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-11-12</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>4</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences2040277</prism:doi>
	<prism:startingPage>277</prism:startingPage>
		<prism:endingPage>297</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[A Site-Specific Index Based on Weathering Forms Visible in Central Oxford, UK]]></dc:title>
    <dc:date>2012-11-12</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2040277</dc:identifier>
    	<dc:creator>Mary J. Thornbush</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/4/260">
	<title><![CDATA[Geosciences, Vol. 2, Pages 260-276: Examining Local Climate Variability in the Late Pennsylvanian Through Paleosols: An Example from the Lower Conemaugh Group of Southeastern Ohio, USA]]></title>
	<link>http://www.mdpi.com/2076-3263/2/4/260</link>
	<description>Three temporally close stratigraphic sections were excavated in Glenshaw Formation of Athens County, Ohio. The described units are Upper Pennsylvanian (Gzhelian, 305–302 Ma) and located in the distal portion of the Appalachian foreland basin. Mudstone units interpreted as paleosols were identified across all three sections. Detailed field and micromorphological studies lead to the recognition of two separate paleosols within the profile. The profile consists of a composite paleosol composed of two cumulative paleosols. The lower paleosol is interpreted as a calcic Vertisol which formed in a seasonally dry environment whereas the upper paleosol is interpreted as a gleyed Inceptisol which formed in a seasonally wet environment. The change in paleosol types is the result of increased precipitation which led to saturation of the soil and surface ponding. Pedogenic carbonate nodules are a common feature throughout the entire profile as are stress cutans. A coalesced carbonate horizon (Bk) was observed approximate 120 cm from the top of the profile in all three sections. This carbonate horizon formed in the Vertisol and later served as a barrier which limited the downward movement of surface water. This limited the gleization of the bottom portion of the overprinted Vertisol resulting in a diffuse boundary with the overlying Inceptisol and producing a composite paleosol.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-11-01</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>4</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences2040260</prism:doi>
	<prism:startingPage>260</prism:startingPage>
		<prism:endingPage>276</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Examining Local Climate Variability in the Late Pennsylvanian Through Paleosols: An Example from the Lower Conemaugh Group of Southeastern Ohio, USA]]></dc:title>
    <dc:date>2012-11-01</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2040260</dc:identifier>
    	<dc:creator>Nicole Dzenowski</dc:creator>
		<dc:creator>Daniel Hembree</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/4/235">
	<title><![CDATA[Geosciences, Vol. 2, Pages 235-259: Oxygen-Dependent Morphogenesis of Modern Clumped Photosynthetic Mats and Implications for the Archean Stromatolite Record]]></title>
	<link>http://www.mdpi.com/2076-3263/2/4/235</link>
	<description>Some modern filamentous oxygenic photosynthetic bacteria (cyanobacteria) form macroscopic tufts, laminated cones and ridges that are very similar to some Archean and Proterozoic stromatolites. However, it remains unclear whether microbes that constructed Archean clumps, tufts, cones and ridges also produced oxygen. Here, we address this question by examining the physiology of cyanobacterial clumps, aggregates ~0.5 mm in diameter that initiate the growth of modern mm- and cm-scale cones. Clumps contain more particulate organic carbon in the form of denser, bowed and bent cyanobacterial filaments, abandoned sheaths and non-cyanobacterial cells relative to the surrounding areas. Increasing concentrations of oxygen in the solution enhance the bending of filaments and the persistence of clumps by reducing the lateral migration of filaments away from clumps. Clumped mats in oxic media also release less glycolate, a soluble photorespiration product, and retain a larger pool of carbon in the mat. Clumping thus benefits filamentous mat builders whose incorporation of inorganic carbon is sensitive to oxygen. The morphogenetic sequence of mm-scale clumps, reticulate ridges and conical stromatolites from the 2.7 Ga Tumbiana Formation likely records similar O2-dependent behaviors, preserving currently the oldest morphological signature of oxygenated environments on Early Earth.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-10-11</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>4</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences2040235</prism:doi>
	<prism:startingPage>235</prism:startingPage>
		<prism:endingPage>259</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Oxygen-Dependent Morphogenesis of Modern Clumped Photosynthetic Mats and Implications for the Archean Stromatolite Record]]></dc:title>
    <dc:date>2012-10-11</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2040235</dc:identifier>
    	<dc:creator>Min Sub Sim</dc:creator>
		<dc:creator>Biqing Liang</dc:creator>
		<dc:creator>Alexander P. Petroff</dc:creator>
		<dc:creator>Alexander Evans</dc:creator>
		<dc:creator>Vanja Klepac-Ceraj</dc:creator>
		<dc:creator>David T. Flannery</dc:creator>
		<dc:creator>Malcolm R. Walter</dc:creator>
		<dc:creator>Tanja Bosak</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/4/221">
	<title><![CDATA[Geosciences, Vol. 2, Pages 221-234: Ocean Acidification and the End-Permian Mass Extinction: To What Extent does Evidence Support Hypothesis?]]></title>
	<link>http://www.mdpi.com/2076-3263/2/4/221</link>
	<description>Ocean acidification in modern oceans is linked to rapid increase in atmospheric CO2, raising concern about marine diversity, food security and ecosystem services. Proxy evidence for acidification during past crises may help predict future change, but three issues limit confidence of comparisons between modern and ancient ocean acidification, illustrated from the end-Permian extinction, 252 million years ago: (1) problems with evidence for ocean acidification preserved in sedimentary rocks, where proposed marine dissolution surfaces may be subaerial. Sedimentary evidence that the extinction was partly due to ocean acidification is therefore inconclusive; (2) Fossils of marine animals potentially affected by ocean acidification are imperfect records of past conditions; selective extinction of hypercalcifying organisms is uncertain evidence for acidification; (3) The current high rates of acidification may not reflect past rates, which cannot be measured directly, and whose temporal resolution decreases in older rocks. Thus large increases in CO2 in the past may have occurred over a long enough time to have allowed assimilation into the oceans, and acidification may not have stressed ocean biota to the present extent. Although we acknowledge the very likely occurrence of past ocean acidification, obtaining support presents a continuing challenge for the Earth science community.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-09-28</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>4</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences2040221</prism:doi>
	<prism:startingPage>221</prism:startingPage>
		<prism:endingPage>234</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Ocean Acidification and the End-Permian Mass Extinction: To What Extent does Evidence Support Hypothesis?]]></dc:title>
    <dc:date>2012-09-28</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2040221</dc:identifier>
    	<dc:creator>Stephen Kershaw</dc:creator>
		<dc:creator>Sylvie Crasquin</dc:creator>
		<dc:creator>Yue Li</dc:creator>
		<dc:creator>Pierre-Yves Collin</dc:creator>
		<dc:creator>Marie-Béatrice Forel</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/4/203">
	<title><![CDATA[Geosciences, Vol. 2, Pages 203-220: Remote Sensing and Geographic Information Systems (GIS) Contribution to the Inventory of Infrastructure Susceptible to Earthquake and Flooding Hazards in North-Eastern Greece]]></title>
	<link>http://www.mdpi.com/2076-3263/2/4/203</link>
	<description>For civil protection reasons there is a strong need to improve the inventory of areas that are more vulnerable to earthquake ground motions or to earthquake-related secondary effects, such as landslides, liquefaction or soil amplifications. The use of remote sensing and Geographic Information Systems (GIS) methods along with the related geo-databases can assist local and national authorities to be better prepared and organized. Remote sensing and GIS techniques are investigated in north-eastern Greece in order to contribute to the systematic, standardized inventory of those areas that are more susceptible to earthquake ground motions, to earthquake-related secondary effects and to tsunami-waves. Knowing areas with aggregated occurrence of causal (“negative”) factors influencing earthquake shock and, thus, the damage intensity, this knowledge can be integrated into disaster preparedness and mitigation measurements. The evaluation of satellite imageries, digital topographic data and open source geodata contributes to the acquisition of the specific tectonic, geologic and geomorphologic settings influencing local site conditions in an area and, thus, estimate possible damage to be suffered.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-09-27</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>4</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences2040203</prism:doi>
	<prism:startingPage>203</prism:startingPage>
		<prism:endingPage>220</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Remote Sensing and Geographic Information Systems (GIS) Contribution to the Inventory of Infrastructure Susceptible to Earthquake and Flooding Hazards in North-Eastern Greece]]></dc:title>
    <dc:date>2012-09-27</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2040203</dc:identifier>
    	<dc:creator>Barbara Theilen-Willige</dc:creator>
		<dc:creator>Paraskevas Savvaidis</dc:creator>
		<dc:creator>Ilias N. Tziavos</dc:creator>
		<dc:creator>Ioanna Papadopoulou</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/4/178">
	<title><![CDATA[Geosciences, Vol. 2, Pages 178-202: Recognizing Vertical and Lateral Variability in Terrestrial Landscapes: A Case Study from the Paleosols of the Late Pennsylvanian Casselman Formation (Conemaugh Group) Southeast Ohio, USA]]></title>
	<link>http://www.mdpi.com/2076-3263/2/4/178</link>
	<description>The Upper Pennsylvanian Casselman Formation of southeastern Ohio contains four distinct paleosol types that formed in alluvial systems within the distal Appalachian foreland basin. The properties of these paleosols as well as their small-scale lateral and vertical variations were studied to interpret the paleoenvironmental and paleoecological conditions within the alluvial settings in which they formed. The ichnofossils and pedogenic features preserved within the paleosols of the Casselman Formation record the local climactic, hydrologic, biotic, and topographic changes that occurred in the region during the Late Pennsylvanian. The four paleosols types of the Casselman Formation are interpreted as Alfisols (Type A, Type D), Vertisols (Type B), and Inceptisols (Type D). The four paleosol types indicate different degrees of changes in local moisture regimes including water table fluctuations due to seasonal precipitation and flooding events. The assemblages of ichnofossils within the paleosol types were produced by both soil arthropods and a diverse array of plants that formed part of the different soil ecosystems present within the alluvial environment. Although regional-scale studies are important for understanding the Late Pennsylvanian world, small-scale studies are also necessary to fully understand the local pedogenic, paleoenvironmental, and paleoecologic consequences of global scale changes in paleoclimate and paleogeography.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-09-26</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>4</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences2040178</prism:doi>
	<prism:startingPage>178</prism:startingPage>
		<prism:endingPage>202</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Recognizing Vertical and Lateral Variability in Terrestrial Landscapes: A Case Study from the Paleosols of the Late Pennsylvanian Casselman Formation (Conemaugh Group) Southeast Ohio, USA]]></dc:title>
    <dc:date>2012-09-26</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2040178</dc:identifier>
    	<dc:creator>Angeline Catena</dc:creator>
		<dc:creator>Daniel Hembree</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/3/157">
	<title><![CDATA[Geosciences, Vol. 2, Pages 157-177: Homology and Potential Cellular and Molecular Mechanisms for the Development of Unique Feather Morphologies in Early Birds]]></title>
	<link>http://www.mdpi.com/2076-3263/2/3/157</link>
	<description>At least two lineages of Mesozoic birds are known to have possessed a distinct feather morphotype for which there is no neornithine (modern) equivalent. The early stepwise evolution of apparently modern feathers occurred within Maniraptora, basal to the avian transition, with asymmetrical pennaceous feathers suited for flight present in the most basal recognized avian, Archaeopteryx lithographica. The number of extinct primitive feather morphotypes recognized among non-avian dinosaurs continues to increase with new discoveries; some of these resemble feathers present in basal birds. As a result, feathers between phylogenetically widely separated taxa have been described as homologous. Here we examine the extinct feather morphotypes recognized within Aves and compare these structures with those found in non-avian dinosaurs. We conclude that the “rachis dominated” tail feathers of Confuciusornis sanctus and some enantiornithines are not equivalent to the “proximally ribbon-like” pennaceous feathers of the juvenile oviraptorosaur Similicaudipteryx yixianensis. Close morphological analysis of these unusual rectrices in basal birds supports the interpretation that they are modified pennaceous feathers. Because this feather morphotype is not seen in living birds, we build on current understanding of modern feather molecular morphogenesis to suggest a hypothetical molecular developmental model for the formation of the rachis dominated feathers of extinct basal birds.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-09-14</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>3</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences2030157</prism:doi>
	<prism:startingPage>157</prism:startingPage>
		<prism:endingPage>177</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Homology and Potential Cellular and Molecular Mechanisms for the Development of Unique Feather Morphologies in Early Birds]]></dc:title>
    <dc:date>2012-09-14</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2030157</dc:identifier>
    	<dc:creator>Jingmai K. O’Connor</dc:creator>
		<dc:creator>Luis M. Chiappe</dc:creator>
		<dc:creator>Cheng-ming Chuong</dc:creator>
		<dc:creator>David J. Bottjer</dc:creator>
		<dc:creator>Hailu You</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/3/147">
	<title><![CDATA[Geosciences, Vol. 2, Pages 147-156: Bythocythere solisdeus n. sp. and Cytheropteron eleonorae n. sp. (Crustacea, Ostracoda) from the Early Pleistocene Bathyal Sediments of Cape Milazzo (NE, Sicily)]]></title>
	<link>http://www.mdpi.com/2076-3263/2/3/147</link>
	<description>Two new fossil species of Ostracoda belonging to the genus Bythocythere Sars, 1866, Bythocythere solisdeus n. sp. and to the genus Cytheropteron Sars, 1866, Cytheropteron eleonorae n. sp. are described. The specimens come from the upper silty sand layers of the Globorotalia truncatulinoides excelsa Zone (“Sicilian” stage), cropping out in “Cala S. Antonino” along the western side of the Cape Milazzo Peninsula (NE Sicily). Both species belong to a typical Bathyal ostracod association characterized by very low temperatures.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-07-09</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>3</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences2030147</prism:doi>
	<prism:startingPage>147</prism:startingPage>
		<prism:endingPage>156</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Bythocythere solisdeus n. sp. and Cytheropteron eleonorae n. sp. (Crustacea, Ostracoda) from the Early Pleistocene Bathyal Sediments of Cape Milazzo (NE, Sicily)]]></dc:title>
    <dc:date>2012-07-09</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2030147</dc:identifier>
    	<dc:creator>Francesco Sciuto</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/2/130">
	<title><![CDATA[Geosciences, Vol. 2, Pages 130-146: Evolving Phytoplankton Stoichiometry Fueled Diversification of the Marine Biosphere]]></title>
	<link>http://www.mdpi.com/2076-3263/2/2/130</link>
	<description>The availability of nutrients and the quantity and quality of food at the base of food webs have largely been ignored in discussions of the Phanerozoic record of biodiversity. We examine the role of nutrient availability and phytoplankton stoichiometry (the relative proportions of inorganic nutrients to carbon) in the diversification of the marine biosphere. Nutrient availability and phytoplankton stoichiometry played a critical role in the initial diversification of the marine biosphere during the Neoproterozoic. Initial biosphere expansion during this time resulted in the massive sequestration of nutrients into biomass which, along with the geologically slow input of nutrients from land, set the stage for severe nutrient limitation and relatively constant marine biodiversity during the rest of the Paleozoic. Given the slow nutrient inputs from land and low recycling rates, the growth of early-to-middle Paleozoic metazoans remained limited by their having to expend energy to first “burn off” (respire) excess carbon in food before the associated nutrients could be utilized for growth and reproduction; the relative equilibrium in marine biodiversity during the Paleozoic therefore appears to be real. Limited nutrient availability and the consequent nutrient imbalance may have delayed the appearance of more advanced carnivores until the Permo-Carboniferous, when widespread orogeny, falling sea level, the spread of forests, greater weathering rates, enhanced ocean circulation, oxygenation, and upwelling all combined to increase nutrient availability. During the Meso-Cenozoic, rising oxygen levels, the continued nutrient input from land, and, especially, increasing rates of bioturbation, enhanced nutrient availability, increasing the nutrient content of phytoplankton that fueled the diversification of the Modern Fauna.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-05-31</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>2</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences2020130</prism:doi>
	<prism:startingPage>130</prism:startingPage>
		<prism:endingPage>146</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Evolving Phytoplankton Stoichiometry Fueled Diversification of the Marine Biosphere]]></dc:title>
    <dc:date>2012-05-31</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2020130</dc:identifier>
    	<dc:creator>Ronald Martin</dc:creator>
		<dc:creator>Antonietta Quigg</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/2/109">
	<title><![CDATA[Geosciences, Vol. 2, Pages 109-129: Squalicorax Chips a Tooth: A Consequence of Feeding-Related Behavior from the Lowermost Navesink Formation (Late Cretaceous: Campanian-Maastrichtian) of Monmouth County, New Jersey, USA]]></title>
	<link>http://www.mdpi.com/2076-3263/2/2/109</link>
	<description>Chipped and broken functional teeth are common in modern sharks with serrated tooth shape. Tooth damage consists of splintering, cracking, and flaking near the cusp apex where the enameloid is broken and exposes the osteodentine and orthodentine. Such damage is generally viewed as the result of forces applied during feeding as the cusp apex impacts the skeletal anatomy of prey. Damage seen in serrated functional teeth from sharks Squalicorax kaupi [1] and Squalicorax pristodontus [1] from the late Cretaceous lowermost Navesink Formation of New Jersey resembles that occurring in modern sharks and suggests similar feeding behavior. Tumbling experiments using serrated modern and fossil functional shark teeth, including those of Squalicorax, show that teeth are polished, not cracked or broken, by post-mortem abrasion in lowermost Navesink sediment. This provides further evidence that chipped and broken Squalicorax teeth are feeding-related and not taphonomic in origin. Evolution of rapid tooth replacement in large sharks such as Squalicorax ensured maximum functionality after feeding-related tooth damage occurred. Serrated teeth and rapid tooth replacement in the large sharks of the Mesozoic and Cenozoic afforded them competitive advantages that helped them to achieve their place as apex predators in today’s ocean.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-05-30</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>2</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences2020109</prism:doi>
	<prism:startingPage>109</prism:startingPage>
		<prism:endingPage>129</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Squalicorax Chips a Tooth: A Consequence of Feeding-Related Behavior from the Lowermost Navesink Formation (Late Cretaceous: Campanian-Maastrichtian) of Monmouth County, New Jersey, USA]]></dc:title>
    <dc:date>2012-05-30</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2020109</dc:identifier>
    	<dc:creator>Martin A. Becker</dc:creator>
		<dc:creator>John A. Chamberlain</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/2/90">
	<title><![CDATA[Geosciences, Vol. 2, Pages 90-108: The Location and Styles of Ice-Free “Oases” during Neoproterozoic Glaciations with Evolutionary Implications]]></title>
	<link>http://www.mdpi.com/2076-3263/2/2/90</link>
	<description>Evidence based on molecular clocks, together with molecular evidence/biomarkers and putative body fossils, points to major evolutionary events prior to and during the intense Cryogenian and Ediacaran glaciations. The glaciations themselves were of global extent. Sedimentological evidence, including hummocky cross-stratification (representing ice-free seas affected by intra-glacial storms), dropstone textures, microbial mat-bearing ironstones, ladderback ripples, and wave ripples, militates against a “hard” Snowball Earth event. Each piece of sedimentological evidence potentially allows insight into the shape and location, with respect to the shoreline, of ice-free areas (“oases”) that may be viewed as potential refugia. The location of such oases must be seen in the context of global paleogeography, and it is emphasized that continental reconstructions at 600 Ma (about 35 millions years after the “Marinoan” ice age) are non-unique solutions. Specifically, whether continents such as greater India, Australia/East Antarctica, Kalahari, South and North China, and Siberia, were welded to a southern supercontinent or not, has implications for island speciation, faunal exchange, and the development of endemism.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-05-29</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>2</prism:number>
	<prism:section>Review</prism:section>
	<prism:doi>10.3390/geosciences2020090</prism:doi>
	<prism:startingPage>90</prism:startingPage>
		<prism:endingPage>108</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[The Location and Styles of Ice-Free “Oases” during Neoproterozoic Glaciations with Evolutionary Implications]]></dc:title>
    <dc:date>2012-05-29</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2020090</dc:identifier>
    	<dc:creator>Daniel Paul Le Heron</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/2/64">
	<title><![CDATA[Geosciences, Vol. 2, Pages 64-89: Early Silurian (Aeronian) East Point Coral Patch Reefs of Anticosti Island, Eastern Canada: First Reef Recovery from the Ordovician/Silurian Mass Extinction in Eastern Laurentia]]></title>
	<link>http://www.mdpi.com/2076-3263/2/2/64</link>
	<description>An extensive late Aeronian patch reef swarm outcrops for 60–70 km on Anticosti Island, eastern Canada, located in the inner to mid-shelf area of a prominent tropical carbonate platform of southeastern Laurentia, at 20°–25° S paleolatitude of the southern typhoon belt. This complex, described here for the first time, includes more than 100 patch reefs, up to 60–80 m in diameter and 10 m high. Reefs are exposed three-dimensionally on present-day tidal flats, as well as inland along roads and rivers. Down the gentle 1°–2° paleoslope, the reefs grade into coral-sponge biostromes, and westerly they grade into inter-reef or deeper ‘crinoidal meadow’ facies. The reef builders were dominantly tabulate and rugose corals, with lesser stromatoporoids. Other components include crinoids, brachiopods, green algae (especially paleoporellids), and encrusting cyanobacteria: reefs display some of the earliest known symbiotic intergrowths of corals and stromatoporoids. Reefs were variably built on a base of crinoidal grainstones, meadows of baffling tabulate corals, brachiopod shells, or chlorophytes. These reefs mark an early phase of reef recovery after a prominent reef gap of 5–6 million years following the Ordovician/Silurian mass extinction events. The reefs feature a maximal diversity of calcifying cyanobacteria, corals and stromatoporoids, but low diversity of brachiopods, nautiloids and crinoids. Following the North American Stratigraphic Code, we define herein the Menier Formation, encompassing the lower two members of the existing Jupiter Formation.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-05-24</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>2</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences2020064</prism:doi>
	<prism:startingPage>64</prism:startingPage>
		<prism:endingPage>89</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Early Silurian (Aeronian) East Point Coral Patch Reefs of Anticosti Island, Eastern Canada: First Reef Recovery from the Ordovician/Silurian Mass Extinction in Eastern Laurentia]]></dc:title>
    <dc:date>2012-05-24</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2020064</dc:identifier>
    	<dc:creator>Paul Copper</dc:creator>
		<dc:creator>Jisuo Jin</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/2/42">
	<title><![CDATA[Geosciences, Vol. 2, Pages 42-63: Distribution and Diversity of Carboniferous and Permian Colonial Rugose Coral Faunas in Western North America: Clues for Placement of Allochthonous Terranes]]></title>
	<link>http://www.mdpi.com/2076-3263/2/2/42</link>
	<description>Colonial rugose corals are common in western cratonal North America and in some of the allochthonous terranes, now amalgamated against its western margin. Throughout the Late Paleozoic, the coral faunas in these two different settings were significantly different. Comparisons of these faunas suggest that during the Mississippian the Alexander terrane probably was southwest of Arctic Alaska and the Stikine terrane probably lay west of the southern part of the North American craton. The Cache Creek terrane lay far out in the Paleopacific Ocean. The Pennsylvanian faunas suggest that the Quesnellia and Eastern Klamath terranes were situated southwest of Arctic Alaska and the Alexander terrane was somewhat farther southwest and farther from cratonal North America. The Stikine terrane continued to be positioned west of the southern part of the North American craton. During the Early Permian, terranes with a cratonal faunal aspect may have lain 2000–3000 km west of cratonal North America and latitudinally generally southwest of their present positions. In the Middle Permian these terranes were carried southward relative to the North American craton. Simultaneously the Tethyan Realm expanded eastward.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-05-10</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>2</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences2020042</prism:doi>
	<prism:startingPage>42</prism:startingPage>
		<prism:endingPage>63</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Distribution and Diversity of Carboniferous and Permian Colonial Rugose Coral Faunas in Western North America: Clues for Placement of Allochthonous Terranes]]></dc:title>
    <dc:date>2012-05-10</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2020042</dc:identifier>
    	<dc:creator>Calvin H. Stevens</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/2/25">
	<title><![CDATA[Geosciences, Vol. 2, Pages 25-41: Cenozoic Mammals and Climate Change: The Contrast between Coarse-Scale versus High-Resolution Studies Explained by Species Sorting]]></title>
	<link>http://www.mdpi.com/2076-3263/2/2/25</link>
	<description>Many paleontologists have noticed the broadly similar patterns between the changes in Cenozoic mammalian diversity and taxonomic dominance and climate changes. Yet detailed studies of fossil population samples with fine-scale temporal resolution during episodes of climate change like the Eocene-Oligocene transition in the White River Group, and the late Pleistocene at Rancho La Brea tar pits, demonstrates that most fossil mammal species are static and show no significant microevolutionary response to major climate changes. This mismatch between patterns seems best explained by species sorting. As the punctuated equilibrium model demonstrated, over long time spans most fossil species are stable and do not respond to climate change. Instead, change occurs at the next hierarchical level, with species sorting adding and subtracting to the total diversity pattern revealed by coarse-scale taxon counting, apparently responding to longer-term changes in climate as revealed by proxies like the oxygen isotope record.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-04-13</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>2</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences2020025</prism:doi>
	<prism:startingPage>25</prism:startingPage>
		<prism:endingPage>41</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Cenozoic Mammals and Climate Change: The Contrast between Coarse-Scale versus High-Resolution Studies Explained by Species Sorting]]></dc:title>
    <dc:date>2012-04-13</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2020025</dc:identifier>
    	<dc:creator>Donald Prothero</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/2/11">
	<title><![CDATA[Geosciences, Vol. 2, Pages 11-24: Cretaceous Ichthyosaurs: Dwindling Diversity, or the Empire Strikes Back?]]></title>
	<link>http://www.mdpi.com/2076-3263/2/2/11</link>
	<description>Recent descriptions of new taxa and recognition of survivorship of Jurassic genera across the Jurassic–Cretaceous boundary bring the total number of Cretaceous ichthyosaur genera to eight. Taxa currently known from the Cretaceous include Ophthalmosaurus, Caypullisaurus, Aegirosaurus, Platypterygius, Maiaspondylus, Athabascasaurus, Sveltonectes, and Acamptonectes. This review summarizes the occurrence of all Cretaceous genera. A discussion of morphological diversity demonstrates the different, though overlapping, ecological niches occupied by the different taxa, while the comparison of phylogenetic hypotheses shows the problems inherent in understanding the evolutionary relationships between Cretaceous genera. The Late Jurassic radiation indicated in the competing phylogenetic hypotheses may correlate with the opening of the Atlantic Ocean or additional dispersal routes established by the breakup of Gondwana. Inclusion of the stratigraphically oldest Platypterygius species may aid in resolving these evolutionary relationships.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-04-12</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>2</prism:number>
	<prism:section>Review</prism:section>
	<prism:doi>10.3390/geosciences2020011</prism:doi>
	<prism:startingPage>11</prism:startingPage>
		<prism:endingPage>24</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Cretaceous Ichthyosaurs: Dwindling Diversity, or the Empire Strikes Back?]]></dc:title>
    <dc:date>2012-04-12</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2020011</dc:identifier>
    	<dc:creator>Maria Zammit</dc:creator>
	
	<cc:license rdf:resource="http://creativecommons.org/licenses/by/3.0/" />
</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/2/1/1">
	<title><![CDATA[Geosciences, Vol. 2, Pages 1-10: The Extinction of the Conulariids]]></title>
	<link>http://www.mdpi.com/2076-3263/2/1/1</link>
	<description>Conulariids are unusual extinct metazoans most often considered to be a group of scyphozoan cnidarians or close relatives. Generally, the temporal range of conulariid fossils is perceived to be late Precambrian or Cambrian to Triassic, though a supposed Cretaceous conulariid from Peru was published 46 years ago. A re-evaluation of this fossil indicates it is not a conulariid, but instead a pinnacean bivalve (Pinna sp.), confirming that the geologically youngest conulariids are of Late Triassic age. However, a review of the Triassic conulariid fossil record indicates it is very sparse, with only eight published records. It does not provide a reliable basis for analyzing the structure of conulariid extinction. Nevertheless, conulariid extinction still appears to have taken place very close to the end of the Triassic. The cause of conulariid extinction may have been the onset of the Mesozoic marine revolution, in which durivorous predators developed new mechanisms for preying on the epifaunal benthos, including the conulariids.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2012-03-22</prism:publicationDate>
	<prism:volume>2</prism:volume>
	<prism:number>1</prism:number>
	<prism:section>Communication</prism:section>
	<prism:doi>10.3390/geosciences2010001</prism:doi>
	<prism:startingPage>1</prism:startingPage>
		<prism:endingPage>10</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[The Extinction of the Conulariids]]></dc:title>
    <dc:date>2012-03-22</dc:date>
	<dc:identifier>doi: 10.3390/geosciences2010001</dc:identifier>
    	<dc:creator>Spencer G. Lucas</dc:creator>
	
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        <item rdf:about="http://www.mdpi.com/2076-3263/1/1/26">
	<title><![CDATA[Geosciences, Vol. 1, Pages 26-43: Geoscience of the Built Environment: Pollutants and Materials Surfaces]]></title>
	<link>http://www.mdpi.com/2076-3263/1/1/26</link>
	<description>An overview of issues with environmental relevance that arise from the interaction between pollutants and surfaces of the built environment is presented in this paper. Two broad perspectives are considered: decay of materials and recording of pollution characteristics. In relation to the former, we consider the possible implications on human activities restrictions, materials and morphological options, consumption of resources and release of pollutants resulting from the alteration of materials, conservation and restoration procedures. In terms of pollution recording, the interest of the stony materials as passive monitors of pollution, the question of heterogeneous conditions on buildings and the interest of qualitative and quantitative studies are highlighted. The importance of longitudinal studies on new and cleaned surfaces is considered, both for the understanding of materials decay and for the assessment of pollution conditions. The use of tracers to record the characteristics of pollution sources, interaction with materials and pathways of pollutants is also discussed. Finally, some recommendations are presented, based on the issues discussed on this paper that might be relevant for environmental management programs, including environmental education.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2011-12-20</prism:publicationDate>
	<prism:volume>1</prism:volume>
	<prism:number>1</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences1010026</prism:doi>
	<prism:startingPage>26</prism:startingPage>
		<prism:endingPage>43</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Geoscience of the Built Environment: Pollutants and Materials Surfaces]]></dc:title>
    <dc:date>2011-12-20</dc:date>
	<dc:identifier>doi: 10.3390/geosciences1010026</dc:identifier>
    	<dc:creator>Carlos Alves</dc:creator>
		<dc:creator>Jorge Sanjurjo-Sánchez</dc:creator>
	
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        <item rdf:about="http://www.mdpi.com/2076-3263/1/1/3">
	<title><![CDATA[Geosciences, Vol. 1, Pages 3-25: The Central Italy Electromagnetic Network and the 2009 L&#039;Aquila Earthquake: Observed Electric Activity]]></title>
	<link>http://www.mdpi.com/2076-3263/1/1/3</link>
	<description>A network of low frequency electromagnetic detectors has been operating in Central Italy for more than three years, consisting of identical instruments that continuously record the electrical components of the electromagnetic field, ranging from a few Hz to tens of kHz. These signals are analyzed in real time and their power spectrum contents and time/frequency data are available online. To date, specific interest has been devoted to searching for any possible electromagnetic features which correlate with seismic activity in the same region. In this study, spectral analysis has evidenced very distinct power spectrum signatures that increased in intensity when strong seismic activity occurred near the stations of the 2009 L&#039;Aquila earthquake. These signatures have revealed horizontally oriented electric fields, between 20 Hz to 400 Hz, lasting from several minutes to up to two hours. Their power intensities have been found to be about 1 μV/m. Moreover, a large number of man-made signals and meteorologic electric perturbations were recorded. Anthropogenic signatures have come from power line disturbances at 50 Hz and higher harmonics up to several kHz, while radio transmissions have influenced the higher kHz spectrum. Reception from low frequency transmitters is also provided in relation to seismic activity. Meteorologic signatures cover the lower frequency band through phenomena such as spherics, Schumann resonances and rain electrical perturbations. All of these phenomena are useful teaching tools for introducing students to this invisible electromagnetic world.</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2011-12-08</prism:publicationDate>
	<prism:volume>1</prism:volume>
	<prism:number>1</prism:number>
	<prism:section>Article</prism:section>
	<prism:doi>10.3390/geosciences1010003</prism:doi>
	<prism:startingPage>3</prism:startingPage>
		<prism:endingPage>25</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[The Central Italy Electromagnetic Network and the 2009 L&#039;Aquila Earthquake: Observed Electric Activity]]></dc:title>
    <dc:date>2011-12-08</dc:date>
	<dc:identifier>doi: 10.3390/geosciences1010003</dc:identifier>
    	<dc:creator>Cristiano Fidani</dc:creator>
	
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</item>
        <item rdf:about="http://www.mdpi.com/2076-3263/1/1/1">
	<title><![CDATA[Geosciences, Vol. 1, Pages 1-2: Geosciences: An Open Access Journal on Earth and Planetary Sciences and Their Interdisciplinary Approaches]]></title>
	<link>http://www.mdpi.com/2076-3263/1/1/1</link>
	<description>On behalf of the Editorial Board and the editorial management staff of MDPI, it is my great pleasure to introduce this new journal Geosciences. Geosciences is an international, peer-reviewed open access journal, which publishes original papers, rapid communications, technical notes and review articles, and discussions about all interdisciplinary aspects of the earth and planetary sciences. Geosciences may also include papers presented at scientific conferences (proceedings) or articles on a well defined topic assembled by individual editors or organizations/institutions (special publications).</description>

	<prism:publicationName>Geosciences</prism:publicationName>
	<prism:publicationDate>2011-05-25</prism:publicationDate>
	<prism:volume>1</prism:volume>
	<prism:number>1</prism:number>
	<prism:section>Editorial</prism:section>
	<prism:doi>10.3390/geosciences1010001</prism:doi>
	<prism:startingPage>1</prism:startingPage>
		<prism:endingPage>2</prism:endingPage>
		<prism:issn>2076-3263</prism:issn>
	
	<dc:title><![CDATA[Geosciences: An Open Access Journal on Earth and Planetary Sciences and Their Interdisciplinary Approaches]]></dc:title>
    <dc:date>2011-05-25</dc:date>
	<dc:identifier>doi: 10.3390/geosciences1010001</dc:identifier>
    	<dc:creator>Jesus Martinez-Frias</dc:creator>
	
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