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11.
José Angel Docobo Josep Maria Trigo-Rodríguez Jiri Borovicka Vakhtang S. Tamazian Vera Assis Fernandes Jordi Llorca 《Earth, Moon, and Planets》2008,102(1-4):537-542
A daylight bolide was observed over Galicia (NW Spain) and Minho (N. Portugal) on March 1, 2005 at 15 h10 min ± 3 min UTC.
We interviewed 23 eyewitnesses of the event in order to obtain the azimuth, altitude, and slope of the fireball’s trajectory.
Reports suggest an atmospheric ending height below 20 km, indicating that meteorite survival was likely. From the reconstructed
trajectory and the fireball’s duration, we obtained the approximate heliocentric orbits for the meteoroid. Assuming an entry
velocity higher than 20 km s−1 which is consistent with its estimated duration, the meteoroid originated in the asteroid belt. 相似文献
12.
Alan L. Mayo Jiri Bruthans David Tingey Jaroslav Kadlec Steve Nelson 《Quaternary Research》2009,72(2):275-283
Timpanogos Cave, located near the Wasatch fault, is about 357 m above the American Fork River. Fluvial cave sediments and an interbedded carbonate flowstone yield a paleomagnetic and U–Th depositional age of 350 to 780 ka. Fault vertical slip rates, inferred from calculated river downcutting rates, range between 1.02 and 0.46 mm yr− 1. These slip rates are in the range of the 0–12 Ma Wasatch Range exhumation rate ( 0.5–0.7 mm yr− 1), suggesting that the long-term vertical slip rate remained stable through mid-Pleistocene time. However, the late Pleistocene (0–250 ka) decelerated slip rate ( 0.2–0.3 mm yr− 1) and the accelerated Holocene slip rate ( 1.2 mm yr− 1) are consistent with episodic fault activity. Assuming that the late Pleistocene vertical slip rate represents an episodic slowing of fault movement and the long-term (0–12 Ma) average vertical slip rate, including the late Pleistocene and Holocene, should be 0.6 mm yr− 1, there is a net late Pleistocene vertical slip deficit of 50–75 m. The Holocene and late Pleistocene slip rates may be typical for episodes of accelerated and slowed fault movement, respectively. The calculated late Pleistocene slip deficit may mean that the current accelerated Wasatch fault slip rate will extend well into the future. 相似文献
13.
Two pedogenic models for paleoclimatic records of magnetic susceptibility from Chinese and Siberian loess 总被引：3，自引：0，他引：3
The magnetic susceptibility (MS) of Chinese loess showing a general proportional relationship to pedogenic grade has been widely recognized and used for reconstruction of paleoclimate by Quaternary scientists. The in-situ pedogenic enhancement of ferrimagnetic content is normally believed to be the main reason for the increase of susceptibility in soil units. However, this pattern of high magnetic susceptibility in palaeosols, and low values in loess, are not replicated in some loess deposits. Siberian loess deposits display a completely opposite susceptibility behavior: high values in loess and low values in palaeosols. This inverse relationship has been explained by the idea that magnetic susceptibility is reflecting the magnitude of an aeolian ferrimagnetic component of consistent mineralogy, the grain size of which is related to average wind velocity. Our magnetic study of Siberian samples in this paper suggests that there are notable differences in magnetic properties between Siberian loess and developed palaeosols, not only in magnetic grain-size and concentration but also in magnetic mineralogy. This evidence is difficult to explain fully through variation in wind strength alone, but implies that the low magnetic susceptibility values in the Siberian paleosol units are a reflection, at least in part, of the alteration of the ferrimagnetic content by post-depositional processes. The Loess Plateau is a very arid area where potential evaporation is always higher than precipitation; pedogenesis occurs under dry oxidising conditions. The Siberian Kurtak region is located on the edge of the tundra where it is always wet and saturation during interglacials will lead to a reducing pedogenic environment. Ferrimagnetic minerals under this condition will be destroyed, resulting in lower magnetic susceptibility. Therefore, great care should be taken when using susceptibility values for paleoclimatic reconstruction. 相似文献
14.
Modelling the effects of changes in rainfall event characteristics on TSS loads in urban runoff 
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下载免费PDF全文 The effect of changes in rainfall event characteristics on urban stormwater quality, which was described by total suspended solids (TSS), was studied by means of computer simulations conducted with the Storm Water Management Model for a climate change scenario for northern Sweden. The simulation results showed that TSS event loads depended mainly on rainfall depth and intensity, but not on antecedent conditions. Storms with low‐to‐intermediate depths and intensities showed the highest sensitivity to changes in rainfall input, both for percentage and absolute changes in TSS wash‐off loads, which was explained by the contribution of pervious areas and supply limitations. This has significant implications for stormwater management, because those relatively frequent events generally carry a high percentage of the annual pollutant load. Copyright © 2013 John Wiley & Sons, Ltd. 相似文献
15.
Markus Fuchs Sebastian Kreutzer Denis‐Didier Rousseau Pierre Antoine Christine Hatté France Lagroix Olivier Moine Caroline Gauthier Jiri Svoboda Lenka Lisá 《Boreas: An International Journal of Quaternary Research》2013,42(3):664-677
The Dolní Věstonice loess section in the Czech Republic is well known for its high‐resolution loess–palaeosol sequence of the last interglacial–glacial climatic cycle (Upper Pleistocene). The loess section is situated in a climatic transition zone between oceanic and continental climates and is therefore of great value in reconstructing past regional climate conditions and their interaction with climate systems, in particular that of the North Atlantic. Based on a combination of optically stimulated luminescence (OSL) ages, stratigraphic field observations and magnetic susceptibility measurements, a chrono‐climatic interpretation of the Dolní Věstonice loess section is presented. To establish a reliable Upper Pleistocene chronology, a quartz OSL approach was applied for equivalent dose (De) determination. Monomineralic quartz extracts of three distinct grain sizes, fine (4–11 μm), middle (38–63 μm) and coarse (90–200 μm), were used and compared. Within error limits, the calculated OSL ages are the same for the different grain sizes, and the OSL ages are in stratigraphic order. The established OSL chronology is in agreement with a Weichselian litho‐ and pedostratigraphy. The Dolní Věstonice loess section is characterized by four pedosedimentary subsequences. At the base of the profile, subsequence I is characterized by a distinct Early Glacial soil complex, OSL‐dated to c. 110 to 70 ka, representing one of the most complete records of environmental change in the European loess belt. Subsequence II is allocated to the Lower Pleniglacial and is characterized by laminated sandy loess. Middle Pleniglacial subsequence III is represented by a brown soil complex, and is followed by the uppermost subsequence IV, characterized by a thick body of laminated sandy loess, indicating strong wind activity and a high sedimentation rate of more than ～1 mm a?1 during the Upper Pleniglacial. According to the OSL chronology, as well as to the sedimentological and palaeopedological investigations, it is likely that the sequence at Dolní Věstonice has recorded most of the climatic events expressed in the NGRIP δ18O reference record between 110 and 70 ka. 相似文献
16.
Vladimir Greif Martin Brcek Jan Vlcko Zuzana Varilova Jiri Zvelebil 《Landslides》2017,14(4):1441-1455
The paper discusses the results of research devoted to the preservation of a natural heritage site carried out at Pravcicka Brana Rock Arch, the largest natural sandstone bridge in Europe, located in the Bohemian Switzerland National Park, Czech Republic. One of the objectives of the study was to explore natural diurnal and annual temperature oscillations at the shallowest part of the rock mass and to acquire an insight into the heat balance both at the surface and within the rock mass. In 2009, four thermocouples were embedded at two positions (eastern and western sides) in a longitudinal direction sequence: rock surface and three different depths 0.10, 0.40, and 0.90 m. Calculation of heat flux inside the rock mass was treated with Fourier’s series which analyzes periodic temperature variation into a set of harmonics of the dominant diurnal or annual waves. Based on the results of Fourier’s analysis, fundamental thermophysical parameters were determined. These were used as the input data to establish a numerical model of temperature distribution in the near surface depth and thermomechanical (kinematic) behavior of the rock arch. Apart from in situ temperature monitoring data, the displacement time series data for the period 1993–2012 recorded by portable crack gauges in 1-month intervals were available. Finally, the rate of displacements in the model simulations was analyzed and compared with those recorded by on site displacement monitoring. Model simulations detected the existence of thermally driven deformation comprising both quasi-cyclic (reversible) movements and irreversible (plastic) deformations which in fact affirm the idea that temperature oscillations are the most contributing factor to the total displacement rate observed at the Pravcicka Brana Rock Arch. Based on the results of model simulation, the authors address the key issue whether the actual deformation mechanism and dynamics will have any influence on the stability of the Pravcicka Brana Rock Arch. 相似文献
17.
The Orlica-Snieznik and Jeseník Mountains correspond to three main domes from west to east: the Snieznik, Keprnfk and Desna domes. They are composed of a basement of autochthonous gneisses, a thick series of blastomylonites and a supposed para-autochthonous or allochthonous metamorphic pre-Devonian to Devonian cover. Their broad direction is NNE-SSW. 40Ar-39Ar radiometric measurements allow three main groups of ages to be defined. (1) 300–310 Ma, represented in the Keprník and Desná domes. This age is interpretated following the constraints on the age of the metamorphism, which is linked with the extensional process occurring during the Westphalian. (2) 320–340 Ma, represented mainly in the Snieznik Dome, but not in the Keprnfk Massif. The nappe structure of Orlik-Vysoká hole, in the northern area of the Desna Dome, also exhibits this age, which is interpretated as reflecting the period of the major Variscan Barrowian metamorphism, which accompanied the compressional process. It is only represented in the zones where the extensional process was not strong enough to result in a complete overprinting. (3) 340–440 Ma, corresponding to a very strictly defined area in the eastern rim of the Desná Dome occupied by ultramylonites and mylonites. These ages, obtained on muscovites, result from an incomplete resetting of the minerals developed during the cooling of a granitic protolith and mylonitized during the extensional process. A laser probe analysis confirms the extreme inhomogeneity of the ages of the muscovites and their different resetting from one grain to another. The Late Alpine overprinting is more discrete, but can be deciphered through the low extraction temperatures with ages between 80 and 120 Ma. These ages can be compared with Alpine ages in the close Western Carpathians. 相似文献
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19.
Jan Svoren Marek Husarik Jaroslav Ambroz Jiri Drbohlav Jaroslav Medek 《Earth, Moon, and Planets》2009,105(2-4):361-365
A semi-automated photometric telescope built at the Skalnate Pleso Observatory is described. In December 2000, the 0.3-m f/5 Zeiss astrograph was replaced by a 0.61-m f/4.3 mirror telescope equipped with a CCD camera. The observing programme is created to conform to the photometry of asteroids which are suspected to be of binary nature; photometry of NEAs and MBAs; a long-term photometry for theoretical modelling of the shape of asteroids; and photometry and astrometry of active comets and asteroids. Some results concerning the binary character of the asteroids are described in the paper. 相似文献
20.
Jeremie Vaubaillon Pavel Koten Anastasios Margonis Juraj Toth Regina Rudawska Maria Gritsevich Joe Zender Jonathan McAuliffe Pierre-Dominique Pautet Peter Jenniskens Detlef Koschny Francois Colas Sylvain Bouley Lucie Maquet Arnaud Leroy Jean Lecacheux Jiri Borovicka Junichi Watanabe Jürgen Oberst 《Earth, Moon, and Planets》2015,114(3-4):137-157