TRANSALP—Cross-line recording during the seismic reflection transect in the Eastern Alps     

Karl Millahn  Ewald Lüschen  Helmut Gebrande  TRANSALP Working Group 《Tectonophysics》2006,414(1-4):39

Cross-line recording formed a companion experiment of the TRANSALP seismic reflection transect through the Eastern Alps, conducted by partner institutions from Austria, Germany and Italy in three field campaigns in the period fall 1998 to fall 1999. Besides of the originally expected three-dimensional control for the north–south running main transect, additional information on seismic anisotropy and alternative images of crucial parts of the main transect could be gained.Conventionally processed sections along N–S running common-midpoint (CMP) binning lines confirm and strengthen the predominance of midcrustal reflective structures of the ‘Sub-Tauern-Ramp’ beneath and south of the Tauern Window. Velocity analysis of the first arrivals exhibit about 10% higher velocities in east–west propagating P-waves, compatible with texture-dominated rock anisotropy, recorded on cross-lines at the Tauern Window. Pre-stack depth migration of cross-line recordings shows dominant south dip of the Sub-Tauern-Ramp with easterly dip components and a sub-horizontal root zone of the Sub-Dolomites-Ramp.  相似文献   

Tomographic inversion of local earthquake data from the Gioia Tauro basin (south-western Calabria, Italy)   总被引：1，自引：0，他引：1  

R. Raffaele  H. Langer  S. Gresta  F. Moia 《Geophysical Journal International》2006,165(1):167-179

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Predicting the deforestation-trend under different carbon-prices   总被引：1，自引：0，他引：1  

Georg E Kindermann  Michael Obersteiner  Ewald Rametsteiner  Ian McCallum 《Carbon balance and management》2006,1(1):15-17

Background  

Global carbon stocks in forest biomass are decreasing by 1.1 Gt of carbon annually, owing to continued deforestation and forest degradation. Deforestation emissions are partly offset by forest expansion and increases in growing stock primarily in the extra-tropical north. Innovative financial mechanisms would be required to help reducing deforestation. Using a spatially explicit integrated biophysical and socio-economic land use model we estimated the impact of carbon price incentive schemes and payment modalities on deforestation. One payment modality is adding costs for carbon emission, the other is to pay incentives for keeping the forest carbon stock intact.  相似文献   

A survey of natural aggregate properties and characteristics important in remote sensing and airborne geophysics     

Daniel H. Knepper Jr.  William H. Langer  Susanne Miller 《Natural Resources Research》1995,4(1):99-120

Natural aggregate is vital to the construction industry. Although natural aggregate is a high volume/low value commodity that is abundant, new sources are becoming increasingly difficult to find and develop because of rigid industry specifications, political considerations, development and transportation costs, and environmental concerns. There are two primary sources of natural aggregate: (1) exposed or near-surface bedrock that can be crushed, and (2) deposits of sand and gravel. Remote sensing and airborne geophysics detect surface and near-surface phenomena, and may be useful for detecting and mapping potential aggregate sources; however, before a methodology for applying these techniques can be developed, it is necessary to understand the type, distribution, physical properties, and characteristics of natural aggregate deposits.The distribution of potential aggregate sources is closely tied to local geologic history. Conventional exploration for natural aggregate deposits has been largely a ground-based operation, although aerial photographs and topographic maps have been extensively used to target possible deposits. Today, the exploration process also considers factors such as the availability of the land, space and water supply for processing, political and environmental factors, and distance from the market; exploration and planning cannot be separated.There are many physical properties and characteristics by which to judge aggregate material for specific applications; most of these properties and characteristics pertain only to individual aggregate particles. The application of remote sensing and airborne geophysical measurements to detecting and mapping potential aggregate sources, however, is based on intrinsic bulk physical properties and extrinsic characteristics of the deposits that can be directly measured, mathematically derived from measurement, or interpreted with remote sensing and geophysical data. On the cover: Northward view of alluvial fans along San Luis Valley, southcentral colorado. This image was created in the U.S. Geological Survey (USGS) Remote Sensing laboratory by digitally draping SPOT panchromatic satellite data resampled to 30 meters pixels resolution over the 124,000 USGS DEM of the Bonanza, Whle Hill, Bushnell Peak, Graveyard Guich, Klondike Mine, and Villa Grove quadrangles.  相似文献   

Single crystal absorption spectra of synthetic Ti,Fe-substituted pyropes     

V. M. Khomenko  K. Langer  M. Andrut  M. Koch-Müller  A. A. Vishnevsky 《Physics and Chemistry of Minerals》1994,21(7):434-440

Synthetic pyrope crystals up to 0.5 mm in diameter, substituted by titanium or by titanium plus iron, were grown under defined conditions of P, T, $f_{O_2 }$ in the presence of water using a piston-cylinder device. The crystals were characterized by X-ray and microprobe techniques. Their single-crystal optical absorption spectra were measured by means of a microscope-spectrometer. Two absorption bands at 16100 and 22300 cm{cm-1} in the spectra of pale-blue Fe-free Ti-bearing pyropes, grown under reduced conditions, were identified as originating from spin-allowed transitions, derived from ² T _2g → ² E _g of octahedral Ti³⁺ ions. The splitting value of the excited ²E _g state, 6200 cm^-1, and the crystal field parameter of Ti³⁺ in pyrope Δ ₀ = 19 200 cm^-1 are both in agreement with literature data. In spectra of brown Fe, Ti-bearing garnets, a broad band at 23000 cm^-1 was interpreted as a Fe^2+[8] → Ti^4+[6] charge-transfer band. The spectral position and width of this band agree with those observed for a FeTi charge transfer band in natural garnets. Fe, Ti-containing garnets synthesized at relatively high oxygen fugacity (10^-11,0 atm), which permits a fraction of Fe³⁺ to enter the garnet, show an additional Fe^2+[8] → Fe^3+[6] charge transfer band at 19800 cm^-1.  相似文献   

Electronic absorption spectra of chromium-bearing sapphirine     

K. Langer  A. N. Platonov  S. S. Matsuk  M. Andrut 《Physics and Chemistry of Minerals》1994,21(1-2):29-35

Violet, non-pleochroic and greenish-blue, pleochroic chromium-substituted sapphirines were found in corundum-bearing spinel-websterite xenolites from the Yakutian kimberlite pipes Noyabrskaya (N) and Sludyanka (Sl), respectively. The crystallochemical formulae of sapphirine crystals from such xenolites were determined by EMP to be (Mg_3.40Fe_0.23Al_3.25Cr_0.16)^[6] Al _1.00 ^[6] [O₂/Al_4.53Si_1.47O₁₈] (N) and (Mg_2.53Fe_0.55 Mn_0.04Ti _0.03 ⁴⁺ Al_3.55Cr _0.08 ³⁺ )^[6]Al _1.00 ^[16] [O₂/Al_4.28Si_1.73O₁₈] (Sl). Single crystal spectra in the range 35000–6000 cm^1- showed a slightly polarization dependent absorption edge near 3200 cm^1- (N) or 30000 cm^1- (Sl) and unpolarized bands at 25300 and 17300 cm^1-, typical of spin-allowed transitions, derived from ⁴A_2g→⁴T_1g and ⁴A_2g→⁴T_2g, of Cr³⁺ in octahedral sites, with point symmetry C₁, of the structure. Another weak band at 23000 cm^?1 in the sapphirine-N spectra is attributed to low symmetry splitting of the excited ⁴T₁ (F)-State of Cr³⁺. These assignments lead to crystal field parameters Dq=1730cm^?1 and B= 685cm^?1 of Cr³⁺ in sapphirine. Crystallochemical and spectroscopic arguments suggest that Cr³⁺ subsitutes for Al in the M(1) or M(8) sites of the sapphirine structure. In addition to Cr³⁺-transitions, spectra of Sl exhibit weak dd-bands of Fe²⁺ at 10000 and 7700 cm^1-, which are unpolarized in consistency with the C₁ site symmetry of the octahedra in the structure. Spectra of Sl show also prominent, broad bands (Δv_1/2～-5000 cm^1-) at 15000 and 11000 cm^1-, which occur in E//Y(//b) and E//Z(//_c=12°) only and exhibit an intensity ratio α_Y∶α_z close to 1∶3. This result, the large half width, as well as band energy — MM distance considerations suggest that these bands originate from Fe^2+[6]-Fe^3+[6] charge-transfer transitions in wall octahedra M(1)M(2), M(6)M(7) etc., forming MM vectors of 30° with the c-axis. The lack of Fe²⁺-Fe³⁺ charge-transfer bands in sapphirine N might indicate a lower oxygen fugacity during the formation of the websterite from the Noyabrskaya pipe compared to that from the Sludyanka pipe.  相似文献   

Esa Microgravity Research Activities In The Field Of Physical Sciences And Applications     

Minster  Olivier  Kufner  Ewald  Vago  Jorge  Jarvis  David 《Earth, Moon, and Planets》1999,87(3):127-147

During the eighties, microgravity research focussed predominantly on the investigation of fundamental phenomena, often with limited industrial support. Although this approach led to some rather impressive breakthroughs in terms of new theoretical insights and microgravity experimentation, the need for increased co-ordination and interest from industry became increasingly apparent. In this decade, a user-driven research strategy has been instigated by ESA to promote microgravity research. The objective is to coordinate ESA, national activities and industry into an overall European strategy, which will allow valuable application-oriented microgravity research to be performed aboard the International Space Station (ISS). On this basis, it is expected that scientific progress will evolve even more rapidly due to the easier planning, regular access and longer experiment-durations associated with the ISS. This paper highlights the wealth of microgravity research being co-ordinated by ESA in the field of physical sciences. A number of key areas of research under microgravity conditions are currently being explored such as alloy solidification, crystal growth,measurement of thermophysical properties, combustion mechanisms, fluid flow, cold atom physics and complex plasmas, to name but a few. The following sections will provide background information relating to the various ESA research programmes, as well as emphasising their microgravity relevance. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

The Global Earthquake Vulnerability Estimation System (GEVES): an approach for earthquake risk assessment for insurance applications   总被引：4，自引：0，他引：4  

Robin Spence  Emily So  Sarah Jenny  Hervé Castella  Michael Ewald  Edmund Booth 《Bulletin of Earthquake Engineering》2008,6(3):463-483

For the insurance and reinsurance industries, earthquake loss estimation is crucial not only to adequately price its product but also to manage the accumulation risk in the face of the ever-increasing exposure in highly seismic regions. Changes in the built environment and a continuously evolving earthquake science make it a necessity for the industry to constantly refine earthquake loss estimation models. In particular, it has been recognized for a long time that the vulnerability of buildings to ground shaking is a key parameter in any earthquake risk model. Current methods tend either to rely on the limited historical damage and loss data or on the numerical simulation of the response of individual buildings to the ground-shaking produced by earthquakes. Although both methods have their advantages and pitfalls, we are proposing here a simple solution, using transparent input data, that can be realistically used for the needs of the insurance and reinsurance industry, whether detailed information about the insured structures is available or not. The resulting product is known as GEVES (Global Earthquake Vulnerability Estimation System). It is primarily intended for evaluating the mean damage ratio (MDR) suffered by a portfolio of buildings classified by use, under the action of a given earthquake scenario (i.e. an earthquake of given size at a given distance from the portfolio of buildings). A key assumption was that macroseismic intensity rather than spectral displacement would be the basis of loss estimation. The paper describes the model with emphasis on its structure and the justification for the assumptions made. In addition to a new set of earthquake vulnerability functions, the paper also provides recommendations on some aspects of the earthquake hazard, in particular about how to define macroseismic intensity at the site of interest, for a given earthquake scenario. This paper also discusses validation of the GEVES model against calculated vulnerability approaches, and the treatment of uncertainty within the model.  相似文献   

Multitemporal terrestrial laser scanning point clouds for thaw subsidence observation at Arctic permafrost monitoring sites     

Katharina Anders  Sabrina Marx  Julia Boike  Benjamin Herfort  Evan James Wilcox  Moritz Langer  Philip Marsh  Bernhard Höfle 《地球表面变化过程与地形》2020,45(7):1589-1600

This paper investigates different methods for quantifying thaw subsidence using terrestrial laser scanning (TLS) point clouds. Thaw subsidence is a slow (millimetre to centimetre per year) vertical displacement of the ground surface common in ice-rich permafrost-underlain landscapes. It is difficult to quantify thaw subsidence in tundra areas as they often lack stable reference frames. Also, there is no solid ground surface to serve as a basis for elevation measurements, due to a continuous moss–lichen cover. We investigate how an expert-driven method improves the accuracy of benchmark measurements at discrete locations within two sites using multitemporal TLS data of a 1-year period. Our method aggregates multiple experts’ determination of the ground surface in 3D point clouds, collected in a web-based tool. We then compare this to the performance of a fully automated ground surface determination method. Lastly, we quantify ground surface displacement by directly computing multitemporal point cloud distances, thereby extending thaw subsidence observation to an area-based assessment. Using the expert-driven quantification as reference, we validate the other methods, including in-situ benchmark measurements from a conventional field survey. This study demonstrates that quantifying the ground surface using 3D point clouds is more accurate than the field survey method. The expert-driven method achieves an accuracy of 0.1 ± 0.1 cm. Compared to this, in-situ benchmark measurements by single surveyors yield an accuracy of 0.4 ± 1.5 cm. This difference between the two methods is important, considering an observed displacement of 1.4 cm at the sites. Thaw subsidence quantification with the fully automatic benchmark-based method achieves an accuracy of 0.2 ± 0.5 cm and direct point cloud distance computation an accuracy of 0.2 ± 0.9 cm. The range in accuracy is largely influenced by properties of vegetation structure at locations within the sites. The developed methods enable a link of automated quantification and expert judgement for transparent long-term monitoring of permafrost subsidence. © 2020 The Authors. Earth Surface Processes and Landforms published by John Wiley & Sons Ltd  相似文献   

Total particulate mass in Enceladus plumes and mass of Saturn’s E ring inferred from Cassini ISS images     

Andrew P. Ingersoll  Shawn P. Ewald 《Icarus》2011,216(2):492-506

The eclipse mosaic (PIA08329) of the Saturn system, taken on September 15, 2006 when Cassini was in Saturn’s shadow, contains numerous color images of the Enceladus plume and the E ring at phase angles ranging from 173° to 179°. These forward-scattering observations sample the diffraction peak for particle radii in the 1–5 μm range. The phase angle dependence and total brightness are sensitive indicators of the total mass of solid material in the plume. We fit the data with a variety of particle shapes and size distributions, and find that the median radius of the equivalent-volume sphere is 3.1 μm, with an uncertainty of ±0.5 μm. The total mass of particles in the plume is (1.45 ± 0.5) × 10⁵ kg. We have not considered variations with altitude in the particle size and shape distribution, and we leave that for another paper. We find that the brightness of the E ring varies with position in the orbit, not only because of the viewing geometry, e.g., variations in phase angle, but also because of some unknown intrinsic variability. The total mass of solid material in the E ring is (12 ± 5.5) × 10⁸ kg. For the plume, the production rate of particles – the mass per unit time leaving the vents is 51 ± 18 kg s⁻¹. We estimate that 9% of these particles are escaping from Enceladus, implying lifetimes of ∼8 years for the E ring particles. Based on three comparisons with vapor amounts from ultraviolet spectroscopy, the ice/vapor ratio is in the range 0.35–0.70. This high ratio poses a problem for theories in which particles form by condensation from the gas phase, and could indicate that particles are formed as spray from a liquid reservoir.  相似文献