Distinguished New Zealand Geographer: Emeritus Professor John R. Flenley          下载免费PDF全文

Juliana Mansvelt  Michael Roche 《New Zealand geographer》2016,72(1):70-72

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Multicriteria analysis applied to landslide susceptibility mapping     

Juliana F. Lorentz  Maria Lucia Calijuri  Eduardo Gomes Marques  Alessandra Carreiro Baptista 《Natural Hazards》2016,81(1):41-54

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Sedimentary facies,fossil distribution and depositional setting of the late Ediacaran Tamengo Formation (Brazil)     

Kamilla Borges Amorim  Jhon Willy Lopes Afonso  Juliana de Moraes Leme  Cleber Quidute Clemente Diniz  Laura Carolina Montenegro Rivera  Juan Camilo Gómez-Gutiérrez  Paulo César Boggiani  Ricardo Ivan Ferreira Trindade 《Sedimentology》2020,67(7):3422-3450

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Derivation of Cloud Index from Geostationary Satellites and Application to the Production of Solar Irradiance and Daylight Illuminance Data     

P. Ineichen  R. Perez 《Theoretical and Applied Climatology》1999,64(1-2):119-130

Summary  We investigate in the present paper the relationship between satellite count, global irradiance and other solar and illumination resource components, bringing a particular attention to low solar elevation situations (below 20 °) which are very important in northern latitudes. Our investigation is based on data from two geostationary satellites, METEOSAT and GOES, backed by ground measurements in Switzerland and the northeastern USA. The study of different clear sky normalizations lead to the conclusion that a linear correlation between the global clearness index and the irradiance (like the heliosat method) would be inaccurate for low solar elevations, and therefore for high latitude regions. We developed a model that directly relates an elevation dependent clearness index to the could index. This methodology presents a definite advantage because it can be generalized to address the clearness index of other solar radiation components, besides global irradiance, such as direct irradiance, diffuse illuminance, etc. The correlations described in this paper were developed on the data from Geneva (in the frame of the EC program “Satellight”) and evaluated on two other independent data sets (Albany, USA and Lausanne, Switzerland). Their precisions, on a hourly basis, are respectively 30%, 40% and 60% for the global, diffuse and beam components) (90,55 and 95 W/m²). The use of independent data for thederivation and the validation of the models shows thatthose can be used in a wide range of locations, even if the applicability has to be assessed for very different climates. Received June 27, 1998 Revised February 26, 1999  相似文献   

When Fields Revert to Forest: Development and Spontaneous Reforestation in Post‐War Puerto Rico     

Thomas K. Rudel  Marla Perez‐Lugo  Heather Zichal 《The Professional geographer》2000,52(3):386-397

During the past 50 years forests have recolonized extensive areas of Puerto Rico. Between 1950 and 1990 forest cover increased from 9% to 37% of the island's land area. In proportional terms more land has reverted to forest in Puerto Rico than anywhere else on earth during the second half of the twentieth century. This paper explores the geography of this process by matching changes in land cover with the characteristics of the land and communities in Puerto Rico. The reversion of agricultural lands to forest occurred most frequently in humid, upland, coffee‐growing regions characterized by heavy out‐migration and populations of smallholders who earned some of their income from off‐farm sources. These findings suggest that changes in non‐farm labor markets, as well as changes in the political economy of agriculture, have important impacts on the prospects for converting agricultural lands into forests.  相似文献   

Sacred ground; the Maipés necropolis of north‐west Gran Canaria     

Valentin R. Troll  Alejandro Rodriguez‐Gonzalez  Frances M. Deegan  Francisco Jos Perez‐Torrado  Juan Carlos Carracedo  Konstantinos Thomaidis  Harri Geiger  Fiona C. Meade 《Geology Today》2019,35(2):55-62

Gran Canaria, like most of the Canary Islands, shows evidence for young basaltic volcanism in the form of cinder cones and valley‐hugging lava flows. These landforms were of no particular use to the aboriginal population, nor to the subsequent Spanish settlers, and young lava flows and lava fields are still referred to as ‘malpaís’ (badlands) in the Canary Islands. In north‐west Gran Canaria, one such lava flow fills the bottom of a steep‐sided valley, which reaches the sea at the present day village of Agaete. The lava flow erupted c. 3030 ± 90 yr bp and displays a total length of ～ 11 km. At its distal end, just outside Agaete, it hosts one of Europe’s largest and most important pre‐historic burial sites constructed of volcanic rock: the Maipés necropolis. Over 700 pre‐historic tombs (or tumuli) constructed from the aa‐type clinker materials have been identified on top of the valley‐filling lava flow. The up to soccer‐ball sized vesicular clinker fragments are sufficiently low in density to provide abundant, workable basalt blocks for the construction of the tumuli, allowing the pre‐hispanic aboriginal population to create a large and magnificent ‘sacred ground’ in an otherwise barren landscape.  相似文献   

A model for partitioning gases among brines and hydrocarbons in oil reservoirs: Examples from the IEA-GHG Weyburn CO₂ Monitoring and Storage Project, Saskatchewan, Canada     

Renee J. Perez  Maurice Shevalier  Ian Hutcheon  Bernhard Mayer 《Journal of Geochemical Exploration》2006,89(1-3):326

We derive a thermodynamic model useful for calculating the partitioning of gases in brine–oil closed systems. We assumed real binary mixtures of all components, and solved a set of equilibrium equations relating the solubility of gases in brines to the solubility of gases in petroleum liquids. We applied the model to understand the distribution of gases in the IEA-GHG Weyburn CO₂ Monitoring and Storage Project, in Saskatchewan, Canada, throughout the first and second year after commencement of CO₂ injection. Results indicate that a free-gas phase formed in the south-east of the field 363 days after injection, which increased in size and volume with time, but did not correlate with zones showing excess CO₂ production. We also observed overlaps between areas of ¹³C depleted HCO₃⁻ and areas with free-vapor phase. We conclude that gas injection leads to short-term CO₂ dissolution in liquids, followed by the creation of a CO₂-rich vapor phase.  相似文献   

Global environmental effects versus galaxy interactions     

J. Perez  P. Tissera  N. Padilla  M. S. Alonso  D. G. Lambas 《Monthly notices of the Royal Astronomical Society》2009,399(3):1157-1166

We explore properties of close galaxy pairs and merging systems selected from the Sloan Digital Sky Survey Data Release 4 in different environments with the aim to assess the relative importance of the role of interactions over global environmental processes. For this purpose, we perform a comparative study of galaxies with and without close companions as a function of local density and host halo mass, carefully removing sources of possible biases. We find that at low- and high-local-density environments, colours and concentration indices of close galaxy pairs are very similar to those of isolated galaxies. At intermediate densities, we detect significant differences, indicating that close pairs could have experienced a more rapid transition on to the red sequence than isolated galaxies. The presence of a correlation between concentration index and colours indicates that the physical mechanism responsible for the colour transformation also operates in the transformation of the luminous matter distribution. At fixed local densities, we find a dependence of the red galaxy fraction on dark matter halo mass for galaxies with or without a close companion. This suggests the action of host halo mass related effects. Regardless of dark matter halo mass, we show that the percentage of red galaxies in close pairs and in the control sample are comparable at low- and high-local-density environments. However, at intermediate local densities, the gap in the red fraction between close pairs and the control galaxies increases from ∼10 per cent in low-mass haloes up to ∼50 per cent in the most massive ones. Interestingly, we also detect that 50 per cent of merging systems populate the intermediate local environments, with a large fraction of them being extremely red and bulge dominated. Our findings suggest that in intermediate-density environments galaxies are efficiently pre-processed by close encounters and mergers before entering higher local density regions.  相似文献   

U–Pb dating of granites in the Neoproterozoic Sergipano Belt,NE-Brazil: Implications for the timing and duration of continental collision and extrusion tectonics in the Borborema Province     

Juliana Finoto Bueno  Elson Paiva Oliveira  Neal J. McNaughton  Jorge Henrique Laux 《Gondwana Research》2009,15(1):86-97

The Sergipano Belt is the outcome of collision between the Pernambuco–Alagoas Massif and the São Francisco Craton during Neoproterozoic assembly of West Gondwana. Field relationships and U–Pb geochronology of granites intruded in garnet micaschists of the Macururé Domain are used to constrain the main collisional event (D₂) in the belt. The granites are divided into two groups, the pre-collisional granites (pre- to early-D₂) and the syn-collisional granites (syn- to tardi-D₂), the latter were emplaced as sheets along the S₂ axial plane foliation or they were collected at the hinge zones of F₂ folds. A U–Pb SHRIMP zircon age of 628 ± 12 Ma was obtained for the pre-collisional Camará tonalite. Two U–Pb TIMS titanite ages were obtained for the syn-collisional granites, 584 ± 10 Ma for the Angico granite and 571 ± 9 Ma for the Pedra Furada granite, and these ages are close to the garnet-whole rock Sm–Nd isochron of 570 Ma found for the peak of metamorphism in the Sergipano Belt. The ages of the Camará tonalite (628 Ma) and the Pedra Furada granite (571 Ma) mark respectively the maximum age for beginning of the D₂ event and minimum age for the end in the Macururé Domain. Using these ages, the main Neoproterozoic D₂ collisional event has been in operation in the Sergipano Belt for at least 57 million years. Correlation with coeval granitoids farther north in the Borborema Province indicate that while in the Sergipano Belt the syn-D₂ granites (ca. 590–570 Ma) were emplaced under compression, in the Borborema Province they emplaced under extensional conditions related to regional strike-slip shear zones. These contrasting emplacement settings for contemporaneous Neoproterozoic granitoids are explained by a combination of continent–continent collision and extrusion tectonics.  相似文献   

Life inhabits rocks: clues to rock erosion from electron microscopy of pisolite at a UNESCO heritage site in Brazil     

Kazue Tazaki  Ryuji Asada  Zara Gerhardt Lindenmayer  Tatsuya Shirotori  Juliana Missiaggia Vargas  Carlos Henrique Nowatzki  Osmar Wöhl Coelho 《International Journal of Earth Sciences》2009,98(1):227-238

Rock erosion is attracting increasing attention from scientists worldwide. The area encompassing the Saint John Baptist Church, Saint John Village, XVII century ruins in Rio Grande do Sul at the UNESCO World Heritage Site is considered a Brazilian treasure. However, the risk of damage to this site from rock erosion has recently increased tremendously. Generally, the rocky construction such as fence, wall and tomb stone, seems strong but is actually extremely sensitive to erosion caused by lichens, fungi, molds and bacteria. Because of biological erosion and massive exposure, the fresh rock is dominated by clays and microorganisms. Water-adsorbing clays and microorganisms influence the mechanisms of the rock erosion. In this study, the formation of bio-clay-minerals in porous structure of pisolite was demonstrated using electron microscopy. Bacterial clay mineralization can deform the rock structure and even produce organic materials. Biological activity could easily corrode rocky constructions around the Saint John Baptist Church site. The rocks are pisolitic laterites possibly formed in Tertiary over the Kretaceous Parana flood Basalts. Samples inhabited by lichens and fungi were collected from a collapsed wall in the ancient church. The zonal reddish-brown pisolites are 4 mm in diameter in a matrix of clays associated with porous and empty spaces. Elemental distribution maps from X-ray fluorescence microscopy show iron-rich spherules of pisolite, whereas the matrix is composed of Al, Si, Mn, and Sr; thus producing goethite and kaolinite. Transmission electron microscopic observation showed that various types of bacteria inhabit the spherule and are associated with clay minerals and graphite. STEM elemental analysis confirmed the bio-clay-mineralization with Al, Si, S, and Fe, around bacterial cells. The results presented here will improve our understanding of nm-scale bio-mineralization and bio-erosion in lateritic rocks. Electronic supplementary material  The online version of this article (doi:) contains supplementary material, which is available to authorized users.  相似文献