Sensitivity of tidal marshes as recorders of major megathrust earthquakes: constraints from the 25 December 2016 Mw 7.6 Chiloé earthquake,Chile     

Martin Brader  Ed Garrett  Daniel Melnick  Ian Shennan 《第四纪科学杂志》2021,36(6):991-1002

We present evidence of land-level change resulting from the 2016 M_w 7.6 Chiloé earthquake from tidal wetlands along the southern coastline of Isla de Chiloé, Chile, to test criteria for the detection of low-level, <0.1 m, coseismic land-level change. In order to record coseismic land-level change in tidal wetland sediments, both the creation and preservation thresholds must be exceeded. High-resolution diatom analyses of sediment blocks at two tidal marshes reveal that the 2016 earthquake exceeded the creation threshold and a statistically significant change in diatom assemblage is recorded. In contrast, the preservation threshold was not exceeded and the record of coseismic land-level motion is not preserved at any location visited. After nine months, interseismic and coseismic changes are statistically indistinguishable. The most sensitive part of the tidal wetland is not consistent between research locations, possibly as a result of changes in sedimentation after the earthquake. We compare records of change from great earthquakes in Alaska with the record from the Chiloé earthquake to explore the detection limit. We propose that coastal palaeoseismological records are highly likely to underestimate the frequency of major (M_w 7–8) earthquakes, with important implications for recurrence intervals and assessment of future seismic hazards.  相似文献   

How to survive a Lunar night     

Stephan Ulamec  Jens Biele  Ed Trollope 《Planetary and Space Science》2010,58(14-15):1985-1995

In the frame of the recent worldwide activities of Lunar research, including various studies for surface stations, the aspect of longevity of such stations has been identified as a particular technical challenge. The reason for this lies in the long (about 14 days) and cold Lunar night during which it is non-trivial to keep spacecraft systems alive and sensitive equipment within an acceptable temperature range.The following paper analyzes and compares various concepts to survive Lunar night, both with and without radioisotope heater technology.The latter normally implies the use of highly toxic material (typically plutonium), which is politically problematic and a driver for cost and safety procedures.Concepts without radioisotope heating need to foresee special measures, like extremely efficient thermal insulation or sub-surface positioning of all temperature sensitive components.Special emphasis has been taken on the thermal analysis of a penetrator-type surface station. The relevant issues are discussed and results for day–night cycles are presented, assuming a typical set of engineering parameters. This concept appears to be the easiest to implement from a thermal point of view, if the use of radioisotope heaters has to be avoided.  相似文献   

Pilbara galenas: Precise isotopic assay of the oldest Australian leads; model ages and growth-curve implications     

J. R. Richards  I. R. Fletcher  J. G. Blockley 《Mineralium Deposita》1981,16(1):7-30

Precise Pb isotopic data are reported for 19 galenas and 2 other minerals from the Archaean Pilbara District of Western Australia. Repeated measurements on the Broken Hill Standard Ore show good agreement with published calibrations from two other laboratories, and an overall 95 percent confidence level within ±0.05 percent per mass unit, whether fractionation correction is by the double-spike procedure or by use of a simple mass-dependent factor. Two stratiform deposits yield the most primitive ratios (²⁰⁶Pb/²⁰⁴Pb=11.89; ²⁰⁷Pb/²⁰⁴Pb=13.69; ²⁰⁸Pb/²⁰⁴Pb=31.79) and model ages in good agreement with the 3.45 Ga age on zircons from volcanics correlatable with the host-rocks. Other minor galena occurrences, with quartz-vein association, appear to be younger, with position along the growth curve surprisingly consistent with the age sequence predicted from field observation. The data also extend the time-range of previously-reported trends in apparent U/Pb of the conceptual Pb source, and reveal new features of the corresponding Th/U systematics: a generally-observable trend in the Archaean of Australia, Southern Africa and West Greenland is that the source Th/U seems significantly higher than is allowed for in any of the current Pb-growth models. In detail, the sample-sample variations in indicated source parameters are in many cases correlatable with the nature of the neighbouring rocks and emphasise that, whereas Pb isotope rations in the galenas of huge deposits may well serve as a convenient sampler of overall trends in the Earth's crust, subeconomic occurrences such as these may reveal valuable information about local variations in U-Th-Pb distribution.  相似文献   

Editorial: The Future of Mathematical Geology     

Michael Ed. Hohn 《Mathematical Geology》1998,30(1):1-3

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RXTE spectroscopy of GRS 1915+105     

Jochen Greiner  Ed H. Morgan  Ron A. Remillard 《New Astronomy Reviews》1998,42(9-10)

The galactic superluminal motion source GRS 1915+105 has been extensively observed with the RXTE satellite over the last two years. More than 250 RXTE pointings have been performed until mid-May 1998 with more than 1.5 Msec exposure time on roughly a weekly basis. Here we report on first results of our spectral analysis of a major part of these pointed RXTE observations. We establish the existence of at least 5 spectral components and present the changes of these components over the last two years.  相似文献   

Book reviews     

Michael Ed. Hohn  Melanie A. Wetzel  James R. Carr  W. E. Sharp  C. John Mann 《Mathematical Geosciences》1995,27(2):301-313

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Wet deposition of ammonium in Europe   总被引：2，自引：0，他引：2  

Ed Buijsman  Jan-Willem Erisman 《Journal of Atmospheric Chemistry》1988,6(3):265-280

Ammonium concentration data in precipitation have been compiled to derive a concentration and deposition field for ammonium in Europe. Measurements referring to a total number of 218 measuring sites have been considered. Because of changes in the ammonium concentrations due to the use of improper sampling procedures, a correction procedure is proposed. This makes allowance for the type of sampler used, the length of the sampling period, and whether or not light-protected sample bottles are used. Dependent on the specific sampling procedure used correction factors range from 0.75 to 1.20. According to our calculations, the total wet deposition flux of ammonium in Europe in the early 1980s amounts to 2.4 Mt NH₄ ⁺y^-1. However, for some parts of Europe the flux cannot be estimated very reliably because of the low number or even the absence of measuring sites. Compared to earlier estimates for around 1960, the ammonium wet deposition flux has increased by approximately 25% during the period 1960–1980.  相似文献   

Conditions and timing of high-pressure Variscan metamorphism in the South Carpathians, Romania   总被引：2，自引：0，他引：2  

Gordon Medaris Jr.  Mihai Ducea  Ed Ghent  Viorica Iancu 《Lithos》2003,70(3-4):141-161

High-pressure (HP) metamorphic rocks, including garnet peridotite, eclogite, HP granulite, and HP amphibolite, are important constituents of several tectonostratigraphic units in the pre-Alpine nappe stack of the Getic–Supragetic (GS) basement in the South Carpathians. A Variscan age for HP metamorphism is firmly established by Sm–Nd mineral–whole-rock isochrons for garnet amphibolite, 358±10 Ma, two samples of eclogite, 341±8 and 344±7 Ma, and garnet peridotite, 316±4 Ma.

A prograde history for many HP metamorphic rocks is documented by the presence of lower pressure mineral inclusions and compositional zoning in garnet. Application of commonly accepted thermobarometers to eclogite (grt+cpx±ky±phn±pg±zo) yields a range in “peak” pressures and temperatures of 10.8–22.3 kbar and 545–745 °C, depending on tectonostratigraphic unit and locality. Zoisite equilibria indicate that activity of H₂O in some samples was substantially reduced, ca. 0.1–0.4. HP granulite (grt+cpx+hb+pl) and HP amphibolite (grt+hbl+pl) may have formed by retrogression of eclogites during high-temperature decompression. Two types of garnet peridotite have been recognized, one forming from spinel peridotite at ca. 1150–1300 °C, 25.8–29.0 kbar, and another from plagioclase peridotite at 560 °C, 16.1 kbar.

The Variscan evolution of the pre-Mesozoic basement in the South Carpathians is similar to that in other segments of the European Variscides, including widespread HP metamorphism, in which P–T–t characteristics are specific to individual tectonostratigraphic units, the presence of diverse types of garnet peridotite, diachronous subduction and accretion, nappe assembly in pre-Westphalian time due to collision of Laurussia, Gondwana, and amalgamated terranes, and finally, rapid exhumation, cooling, and deposition of eroded debris in Westphalian to Permian sedimentary basins.  相似文献   

Rough seas and time-lapse seismic     

Robert Laws  Ed Kragh 《Geophysical Prospecting》2002,50(2):195-208

Time‐lapse seismic surveying has become an accepted tool for reservoir monitoring applications, thus placing a high premium on data repeatability. One factor affecting data repeatability is the influence of the rough sea‐surface on the ghost reflection and the resulting seismic wavelets of the sources and receivers. During data analysis, the sea‐surface is normally assumed to be stationary and, indeed, to be flat. The non‐flatness of the sea‐surface introduces amplitude and phase perturbations to the source and receiver responses and these can affect the time‐lapse image. We simulated the influence of rough sea‐surfaces on seismic data acquisition. For a typical seismic line with a 48‐fold stack, a 2‐m significant‐wave‐height sea introduces RMS errors of about 5–10% into the stacked data. This level of error is probably not important for structural imaging but could be significant for time‐lapse surveying when the expected difference anomaly is small. The errors are distributed differently for sources and receivers because of the different ways they are towed. Furthermore, the source wavelet is determined by the sea shape at the moment the shot is fired, whereas the receiver wavelet is time‐varying because the sea moves significantly during the seismic record.  相似文献   

Precise geodesy with the Very Long Baseline Array   总被引：2，自引：2，他引：0  

Leonid Petrov  David Gordon  John Gipson  Dan MacMillan  Chopo Ma  Ed Fomalont  R. Craig Walker  Claudia Carabajal 《Journal of Geodesy》2009,83(9):859-876

We report on a program of geodetic measurements between 1994 and 2007 which used the Very Long Baseline Array (VLBA) and up to ten globally distributed antennas. One of the goals of this program was to monitor positions of the array at a 1 mm level of accuracy and to tie the VLBA into the international terrestrial reference frame. We describe the analysis of these data and report several interesting geophysical results including measured station displacements due to crustal motion, earthquakes, and antenna tilt. In terms of both formal errors and observed scatter, these sessions are among the very best geodetic very long baseline interferometry experiments.  相似文献