High‐pressure phase transitions of α‐quartz under nonhydrostatic dynamic conditions: A reconnaissance study at PETRA III          下载免费PDF全文

Eva‐Regine Carl  Ulrich Mansfeld  Hanns‐Peter Liermann  Andreas Danilewsky  Falko Langenhorst  Lars Ehm  Ghislain Trullenque  Thomas Kenkmann 《Meteoritics & planetary science》2017,52(7):1465-1474

Hypervelocity collisions of solid bodies occur frequently in the solar system and affect rocks by shock waves and dynamic loading. A range of shock metamorphic effects and high‐pressure polymorphs in rock‐forming minerals are known from meteorites and terrestrial impact craters. Here, we investigate the formation of high‐pressure polymorphs of α‐quartz under dynamic and nonhydrostatic conditions and compare these disequilibrium states with those predicted by phase diagrams derived from static experiments under equilibrium conditions. We create highly dynamic conditions utilizing a mDAC and study the phase transformations in α‐quartz in situ by synchrotron powder X‐ray diffraction. Phase transitions of α‐quartz are studied at pressures up to 66.1 and different loading rates. At compression rates between 0.14 and 1.96 GPa s^?1, experiments reveal that α‐quartz is amorphized and partially converted to stishovite between 20.7 GPa and 28.0 GPa. Therefore, coesite is not formed as would be expected from equilibrium conditions. With the increasing compression rate, a slight increase in the transition pressure occurs. The experiments show that dynamic compression causes an instantaneous formation of structures consisting only of SiO₆ octahedra rather than the rearrangement of the SiO₄ tetrahedra to form a coesite. Although shock compression rates are orders of magnitude faster, a similar mechanism could operate in impact events.  相似文献   

Coesite in suevite from the Ries impact structure (Germany): From formation to postshock evolution          下载免费PDF全文

Agnese Fazio  Ulrich Mansfeld  Falko Langenhorst 《Meteoritics & planetary science》2017,52(7):1437-1448

Coesite is one of the most common and abundant high‐pressure phases occurring in impactites. The mechanism of formation of coesite and its postshock evolution is revisited in this paper based on Raman microspectroscopy, and scanning and transmission electron microscopy of a coesite‐bearing suevite from the Ries impact structure. Our data indicate that coesite forms through a single process, i.e., by crystallization from high‐pressure silica melt, and that its formation is related to fluid inclusions in precursor quartz. During the postshock phase, coesite aggregates are partially modified by annealing and interactions with fluids. In an early stage of the postshock evolution, coesite is back‐transformed to quartz and the surrounding diaplectic glass devitrifies into β‐cristobalite, which transforms into α‐cristobalite and then into microcrystalline quartz during subsequent stages of the postshock evolution. Altogether these postshock modifications result in a significant volume loss and extensional fracturing. During a late postshock stage, the fractures are filled with clay minerals due to circulation of hydrothermal fluids.  相似文献   

Experimental formation of massive hydrate deposits from accumulation of CH₄ gas bubbles within synthetic and natural sediments     

Megan Elwood Madden  Shannon Ulrich  Phillip Szymcek  Scott McCallum  Tommy Phelps 《Marine and Petroleum Geology》2009

In order for methane to be economically produced from the seafloor, prediction and detection of massive hydrate deposits will be necessary. In many cases, hydrate samples recovered from seafloor sediments appear as veins or nodules, suggesting that there are strong geologic controls on where hydrate is likely to accumulate. Experiments have been conducted examining massive hydrate accumulation from methane gas bubbles within natural and synthetic sediments in a large volume pressure vessel through temperature and pressure data, as well as visual observations. Observations of hydrate growth suggest that accumulation of gas bubbles within void spaces and at sediment interfaces likely results in the formation of massive hydrate deposits. Methane hydrate was first observed as a thin film forming at the gas/water interface of methane bubbles trapped within sediment void spaces. As bubbles accumulated, massive hydrate growth occurred. These experiments suggest that in systems containing free methane gas, bubble pathways and accumulation points likely control the location and habit of massive hydrate deposits.  相似文献   

Shock waves—Phenomenology,experimental, and numerical simulation     

Klaus Thoma  Ulrich Hornemann  Martin Sauer  Eberhard Schneider 《Meteoritics & planetary science》2005,40(9-10):1283-1296

Abstract— The purpose of this paper is to review the results of long‐term cooperation between Dieter Stöffler and the authors in the field of shock wave deformation of minerals and rocks. First, the principal phenomena of shock wave generation and propagation, predominantly in solid media, are presented, and then analytical and numerical mathematical treatment of shock wave processes on the basis of mass, momentum, and energy conservation laws will be described and discussed. Experimental methods of shock wave investigations by means of impact and explosive techniques are summarized, including hypervelocity acceleration facilities and high‐pressure explosive devices. Shock pressure barometry by means of mineralogical evidence of distinct material phase transitions and characteristic shock structures is also discussed.  相似文献   

NOBLE GASES AND THE CLASSIFICATION OF BRACHINA     

Ulrich Ott  Hans-Peter Lhr  Friedrich Begemann 《Meteoritics & planetary science》1985,20(1):69-78

Noble-gas systematics show that Brachino is not a member of the SNC-group of meteorites. The whole-rock K-Ar gas retention age is (3.11 ± 0.07) AE as compared to the 1.3 AE solidification ages of SNCs; the content of radiogenic¹²⁹ Xe* of (3.47 ±. 15) × 10^?10 cm³ STP/g is about two orders of magnitude higher, and the¹²⁹ Xe/¹³² Xe ratio (11.0), the ratio of radiogenic¹²⁹ Xe* to fissiogenic¹³⁶ Xe_f (300), and the ratio³⁶ Ar/¹³² Xe in the trapped gases are about one order of magnitude higher than observed for SNCs. The same evidence argues strongly against any simple genetic relationship with eucrites. The noble-gas abundance pattern resembles closely that in silicate inclusions from the iron meteorites Campo del Cielo and Udei Station. Abundances of cosmic-ray produced³ He and²¹ Ne (5.7 and. 99 × 10^?8 cm³ STP/g, resp.) indicate an exposure age of ～ 2.4 Ma. Irradiation conditions appear to have been perfectly normal except for an unaccountably low content of spallogenic ³⁸Ar. Losses by diffusion of radiogenic⁴ He are severe; they must have occurred at or before the onset of the exposure of the meteoroid to the cosmic radiation.  相似文献   

Future impacts of global warming and reforestation on drought patterns over West Africa     

Ulrich?DiassoEmail authorView author&#;s OrcID profile  Babatunde?J?Abiodun 《Theoretical and Applied Climatology》2018,133(3-4):647-662

This study investigates how a large-scale reforestation in Savanna (8–12°N, 20°W–20°E) could affect drought patterns over West Africa in the future (2031–2060) under the RCP4.5 scenario. Simulations from two regional climate models (RegCM4 and WRF) were analyzed for the study. The study first evaluated the performance of both RCMs in simulating the present-day climate and then applied the models to investigate the future impacts of global warming and reforestation on the drought patterns. The simulated and observed droughts were characterized with the Standardized Precipitation and Evapotranspiration Index (SPEI), and the drought patterns were classified using a Self-organizing Map (SOM) technique. The models capture essential features in the seasonal rainfall and temperature fields (including the Saharan Heat Low), but struggle to reproduce the onset and retreat of the West African Monsoon as observed. Both RCMs project a warmer climate (about 1–2 °C) over West Africa in the future. They do not reach a consensus on future change in rainfall, but they agree on a future increase in frequency of severe droughts (by about 2 to 9 events per decade) over the region. They show that reforestation over the Savanna could reduce the future warming by 0.1 to 0.8 °C and increase the precipitation by 0.8 to 1.2 mm per day. However, the impact of reforestation on the frequency of severe droughts is twofold. While reforestation decreases the droughts frequency (by about 1–2 events per decade) over the Savanna and Guinea coast, it increases droughts frequency (by 1 event per decade) over the Sahel, especially in July to September. The results of this study have application in using reforestation to mitigate impacts of climate change in West Africa.  相似文献   

ON THE PHYSICS OF FLOW-DRIVEN SEDIMENTS (BED-LOAD)     

Ulrich C. E. ZANKE Prof  Institute of Hydraulic Engineering  University of Technology  Darmstadt  Germany 《国际泥沙研究》2001,16(1)

l PROBLEMS AND AlMSSediments may be transported close to the bed, rolling and sliding, as we1l as susPended in the flow. Forvarious reasons the theoretical treatment of the bed-load problem has been exceptionally difficult. Noanalytical solution had been fOund uP to now, beginning with Du Buat (l786), Huebbe (l86l) and DuBoys (I 879). Since the aPProach of Du Boys numerous new attemPts have been catried out, mostly of anempirical nature. Consequently they are not generally valid an…  相似文献   

Visualization of tectonic structures in shallow-depth high-resolution ground-penetrating radar (GPR) profiles   总被引：3，自引：0，他引：3  

Martin Meschede  Ulrich Asprion  & Klaus Reicherter 《地学学报》1997,9(4):167-170

Ground-penetrating radar (GPR) is applied to detect subsurface tectonic structures and to map the geometry of faulted blocks. Tectonic interpretations from a profile crossing the graben fault and a grid in a second-order graben structure providing a 3D data set are correlated to the structural inventory of the outcrop. Folded layers of the roll-over anticline are identified by continuous curved reflectors and an increasing dip towards the main graben fault. Faults are indicated by arrays of reflector terminations. Variations in the water and clay content caused by karstification and brecciation on fault planes are displayed by changing amplitudes of the detected signal. The 3D visualization of the second-order graben structure with a grid of GPR profiles illustrates the local stress pattern which coincides with structural observations in the outcrop and photo lineations.  相似文献   

Access and Assimilation: Pivotal environmental information challenges     

Benking Heiner  Kampffmeyer  B. Ulrich 《GeoJournal》1992,26(3):323-334

The world-wide environmental exchange of information is hampered by difficulties bridging terminologies and languages so that trans-cultural, cross-sectoral, and multi-dimensional information can be made available in a usable form at low cost. The alternative concepts and elements described are planned to contribute to HEMIS, UNEP-HEMs world-wide information and reference system. The potential content includes: environmentally relevant organizations, activities, systems, methods, data sources, qualities, and access methods. The key design element is a multi-lingual thesaurus which has harmonization effect resulting from the structuring and strategic access to information. Documentation and retrieval is another concern beside the provision of tools to ease identification, dissemination, and validation of information. The maintenance of validated source data and documents will reduce the volumes of requested information and thereby counteract the present information overkill.  相似文献   

Mapping mountains: Vegetation in the Himalaya     

Ulrich Schweinfurth 《GeoJournal》1992,27(1):73-83

The author deals with the vegetation of the Himalayas taking his 1957 map as basis of the presentation. This map by way of vegetation first opened insigh into the hitherto unknown landscape structure of the mountain system, thereby revealing, for instance, the phenomeon of the inner valleys and the climatically dry valleys, in particular as well as the areas vegetationwise still unknown. Progress in our knowledge of the vegetation in the Himalayas since publication of the 1957 map is carefully recorded showing, above all, the advancement of our knowledge in Nepal since. In contrast to expectations, research was unable to concentrate on all the gaps in our knowledge as demonstrated on the 1957 map owing to political conditions prevailing.  相似文献