Message from 2014 Best Paper Award Winners     

Martí Lloret-Cabot  Gordon A. Fenton  Michael A. Hicks 《Georisk: Assessment and Management of Risk for Engineered Systems and Geohazards》2015,9(2)

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Morphostructure and evolution of the central and Eastern Bransfield Basins (NW Antarctic Peninsula)   总被引：2，自引：0，他引：2  

Eulàlia Gràcia  Miquel Canals  Marcel Lí Farràn  Maria José Prieto  Jordi Sorribas  Gebra Team 《Marine Geophysical Researches》1996,18(2-4):429-448

The Bransfield Basin is a narrow and elongated active rift basin located between the Antarctic Peninsula and the South Shetland Islands. The Bransfield Basin is composed of three small basins, and two of them, the Central and Eastern Bransfield Basins, were surveyed during a recent cruise (GEBRA 93). The full swath bathymetry coverage as well as the single-channel seismic reflection and magnetic profiles that have been acquired, help us to better understand the morphostructure and recent evolution of the Bransfield Basin. Six large volcanic edifices aligned with the basin axis stick out of the sedimented seafloor of the Central Bransfield Basin. In contrast, the Eastern Bransfield Basin is characterised by four deep troughs displaying a rhombic-shape, and small, scattered volcanic cones located in the southwestern half basin. Seamount volcanism plays an important role in the formation of new crust in the Bransfield Basin. The larger seamounts of the Central Bransfield Basin are located at the intersection of the two main orthogonal sets of faults (longitudinal ENE-WSW and transversal NNW-SSE). Morphological analysis of the seamounts indicates a multi-staged volcano-tectonic construction. The distribution and shape of these edifices suggests that both volcanism and extension are concentrated at the same preferential areas through time. This might be related to the fracturation style of the continental crust. The Central and Eastern Bransfield Basins are very different in morphostructure, volcanism, and sedimentary cover. The Central Bransfield Basin shows evidence of NW-SE extensional faulting and focused active MORB-volcanism interpreted as result of incipient seafloor spreading. The Eastern Bransfield Basin is still in a rifting stage, mainly dominated by a NW-SE extension and some left-lateral strike-slip component probably related to the South Scotia Ridge.J. Acosta, J. Baraza, P. Bart, A.M. Calafat, J.L. Casamor, M. De Batist, G. Ercilla, G. Francés, E. Ramos, J.L. Sanz, and A. Tassone.  相似文献   

Extreme precipitation and long-term precipitation changes in a Central European sedge-grass marsh in the context of flood occurrence     

Jiří Dušek  Šárka Hudecová  Stanislav Stellner 《水文科学杂志》2017,62(11):1796-1808

This study offers a detailed analysis of the extreme precipitation and long-term precipitation changes in a sedge-grass marsh in the “Wet Meadows” area in the Czech Republic (Central Europe) in the context of flood occurrence. Namely, trends in annual maxima of daily precipitation and trends in the occurrence and amount of rainfall are investigated. The analysis is based on daily measurements of precipitation from 1977 to 2015. We found out that extreme precipitation has become significantly more frequent in recent years, and there are also other significant changes in the rainfall distribution. Possible negative effects on the wetland can be linked to a change of carbon exchange between the ecosystem and the atmosphere and a change of biodiversity. Awareness of these changes is necessary for possible positive human intervention when a desirable wetland functioning is threatened.  相似文献   

Modeling biodiversity loss by global warming on Pantepui, northern South America: projected upward migration and potential habitat loss     

Sandra Nogué  Valentí Rull  Teresa Vegas-Vilarrúbia 《Climatic change》2009,94(1-2):77-85

This work aims to estimate the potential effects of the global warming projected for the twenty-first century on the biodiversity of a remote and pristine region of the Neotropics called Pantepui. Habitat loss and fragmentation by upward migration of bioclimatic conditions is analyzed using Species-Area Relationships (SAR) and Altitudinal Range Displacement (ARD) analysis. The ARD is a tool that uses the present-day lapse rate to estimate the upward migration of the species based on the global warming predicted by the IPCC. The results show that around 80% of the vascular flora, ca. 1,700 species of which up to 400 would be Pantepui endemics, are threatened of extinction. These estimates should be considered preliminary, but the danger is real. Therefore, suitable conservation or mitigation strategies are needed.  相似文献   

Puerto Lápice eucrite fall: Strewn field,physical description,probable fireball trajectory,and orbit     

Josep M. TRIGO‐RODRÍGUEZ  Jiří BOROVIčKA  Jordi LLORCA  José M. MADIEDO  Jaime ZAMORANO  Jaime IZQUIERDO 《Meteoritics & planetary science》2009,44(2):175-186

Abstract— The fall of the Puerto Lápice eucrite occurred on May 10, 2007, at 17 h 57 m 30 ± 30 s UTC. Its daylight fireball was witnessed by hundreds of people from Spain, and produced a meteorite fall associated with a large strewn field of fragments. There were no direct pictures of the fireball, but several pictures of the fireball's train were taken from different locations in Spain. Additional theodolite calibrations of visual records were made in order to find the most probable fireball trajectory based on the available data. The shape of the meteorite strewn field was considered as well. Although the orbit of the Puerto Lápice meteoroid could not be computed due to the absence of velocity data, we assumed a likely range of geocentric velocities and computed a range of possible orbits. All solutions show that the body was in an Apollo‐type orbit, with low inclination and perihelion distance just below 1 astronomical unit (AU). This is the first case that an orbit can be discussed for an HED meteorite fall.  相似文献   

Imprint of the 11-year solar cycle in reanalyzed and radiosonde datasets: a spatial frequency analysis approach   总被引：1，自引：0，他引：1  

Petr Pi?oft  Eva Holtanová  Peter Huszár  Ji?í Mik?ovsky  Michal ?ák 《Climatic change》2012,110(1-2):85-99

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Geochemical characterization of moldavites from a new locality,the Cheb Basin,Czech Republic     

Zdeněk Řanda  Jiří Mizera  Jaroslav Frána  Jan KuČEra 《Meteoritics & planetary science》2008,43(3):461-477

Abstract— Twenty‐three moldavites from a new locality, the Cheb Basin in Western Bohemia, were analyzed by instrumental neutron activation analysis for 45 major and trace elements. Detailed comparison of the Cheb Basin moldavites with moldavites from other substrewn fields in both major and trace element composition shows that the Cheb Basin is a separate substrewn field. The geochemical data obtained are discussed with respect to the source materials and processes leading to formation of moldavites. The data show that three groups of Cheb Basin moldavites exist. Ten samples of group 1 are characterized by the lowest content of Al, Fe, Na, and other elements representing phyllosilicate minerals, and by high Ca + Mg contents related probably to carbonates. They resemble the “poisonous green” moldavites, a subgroup of the Southern Bohemian moldavites. Seven samples of group 2 and 6 samples of group 3 are similar to typical moldavites of the Southern Bohemian substrewn field. These two groups differ from each other mainly in Al contents; with higher contents of Al and the elements associated with phyllosilicate minerals (namely Ba and Sr), group 3 also resembles the Moravian moldavites. Significant positive correlations between K, Ca, Mg, and Mn found in group 2 of the Cheb Basin moldavites and the enrichment in these elements observed generally in all moldavites, as well as other facts, e.g., high K/Na and K/Rb ratios and the reduced conditions during formation of moldavites, have been attributed to possible contribution to the moldavite source materials of the ash produced by burning of vegetation and soil organic matter present at the pre‐impact area.  相似文献   

New Plateau de Bure observations of M 1–92; unveiling the core     

Javier Alcolea  Valentín Bujarrabal  Roberto Neri 《Astrophysics and Space Science》2008,313(1-3):235-239

M 1–92 is a very well studied bipolar pPN that can be considered an archetype of this type of sources; it shows a clear axial symmetry, along with the kinematics characteristic of this class of envelopes around post-AGB stars. We performed sub-arcsecond resolution observations of the J=2–1 rotational line of ¹³CO in M 1–92 with the new extended configurations of the IRAM Plateau de Bure interferometer, for studying the morphology and velocity field of the molecular gas better in the nebula, particularly in its central parts. We found that the equatorial structure dividing the two lobes is a thin flat disk, which expands radially with a velocity proportional to the distance to the central stellar system. The kinetic age of this equatorial flow is very similar to that measured in the two lobes, suggesting that the whole structure was formed as a result of a single event some 1200 yr ago, after which the nebula reached an expansion velocity field with axial symmetry. The small widths and velocity dispersion in the gas forming the lobe walls confirm that the acceleration responsible for the nebular shape could not last more than 100–120 yr. In view of the similarity to η Car, we speculate on the possibility that the whole nebula was formed as a result of a magneto-rotational explosion in a common-envelope system. The study of the possible importance of this mechanism in the context of global PNe and pPNe reshaping should be one on the fields in which future ALMA observations will make a crucial contribution. Based on observations carried out with the IRAM Plateau de Bure Interferometer. IRAM is supported by INSU/CNRS (France), MPG (Germany) and IGN (Spain).  相似文献   

On the formation of TeV radiation in LS 5039     

D. Khangulyan  F. Aharonian  V. Bosch-Ramon 《Monthly notices of the Royal Astronomical Society》2008,383(2):467-478

The recent detections of TeV gamma-rays from compact binary systems show that relativistic outflows (jets or winds) are sites of effective acceleration of particles up to multi-TeV energies. In this paper, we discuss the conditions of acceleration and radiation of ultrarelativistic electrons in LS 5039, the gamma-ray emitting binary system for which the highest quality TeV data are available. Assuming that the gamma-ray emitter is a jet-like structure, we performed detailed numerical calculations of the energy spectrum and light curves accounting for the acceleration efficiency, the location of the accelerator, the speed of the emitting flow, the inclination angle of the system, as well as specific features related to anisotropic inverse Compton (IC) scattering and pair production. We conclude that the accelerator should not be deep inside the binary system unless we assume a very efficient acceleration rate. We show that within the IC scenario both the gamma-ray spectrum and flux are strongly orbital phase dependent. Formally, our model can reproduce, for specific sets of parameter values, the energy spectrum of gamma-rays reported by HESS for wide orbital phase intervals. However, the physical properties of the source can be constrained only by observations capable of providing detailed energy spectra for narrow orbital phase intervals (Δφ≪ 0.1).  相似文献   

Effect of water excess on soil carbon dioxide,seepage water chemistry,and calcite speleothem growth: An experimental and modelling approach     

Marek Lang  Jiří Faimon 《水文研究》2020,34(22):4334-4349

The effect of the water excess in soil on soil gaseous carbon dioxide concentrations (c_CO2) was studied based on field experiments. The gradual water addition of 15 and 30 L m⁻² to leptosols and anthrosols, simulating 15 and 30 mm precipitation, respectively, caused the overall c_CO2 increase of 1.53 × 10⁻¹ mol m⁻³ (increase by 60%) and 1.61 × 10⁻¹ mol m⁻³ (increase by 112%) in the soil airs. The effect of the c_CO2 increment on seepage water, cave dripwater chemistry, and calcite speleothem overgrowths was deduced from geochemical modelling. It showed that the c_CO2 increments may lead to the increments in total dissolved carbon, aqueous calcium, and dissolved solids of 1.10 × 10⁻³ mol L⁻¹ (increase by 35%), 4.45 × 10⁻⁴ mol L⁻¹ (increase by 30%), and 1.55 × 10⁻³ mol L⁻¹ (increase by 34%), respectively. After the total degassing of CO₂ in the cave, the increment in the saturation index of dripwater, SI, could reach up to ΔSI = 0.31, which means an increase by hundreds of percent. The water excess of 5 L m⁻² following a dry period would cause the increment in saturation index ΔSI = 0.17. The modelling further showed that the c_CO2 increase associated with the 30 L m⁻² water excess could induce the calcite overgrowth up to 1 μm thick per 1 m² surface area. The effect of water excess with additional water supplies gradually weakens, probably due to reduced CO₂ diffusivity and soil microorganism activity. It can be assumed that the most contrasting peaks in dripwater chemistry are associated with the individual precipitation events after short dry periods. The increased supersaturation of dripwater is expected to lead to faster growth of speleothem and changes in calcite textures.  相似文献