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1.
2.
Geoffrey Blewitt William C. Hammond Corné Kreemer Hans-Peter Plag Seth Stein Emile Okal 《Journal of Geodesy》2009,83(3-4):335-343
We identify the key design aspects of a GPS-based system (and in the future, GNSS-based systems) that could contribute to real-time earthquake source determination and tsunami warning systems. Our approach is based on models of both transient and permanent displacement of GPS stations caused by large earthquakes, while considering the effect of GPS errors on inverted earthquake source parameters. Our main conclusions are that (1) the spatial pattern, magnitude, and timing of permanent displacement of GPS stations can be inverted for the earthquake source and so predict the 3D displacement field of the ocean bottom, thus providing the initial conditions for tsunami models, and (2) there are no inherently limiting factors arising from real-time orbit and positioning errors, provided sufficient near-field GPS stations are deployed. This signal could be readily exploited by GPS networks currently in place, and will be facilitated by the IGS Real-Time Project as it comes to fruition. 相似文献
3.
Joel Sanchez-Bermudez Florentin Millour Fabien Baron Roy van Boekel Laurent Bourgès Gilles Duvert Paulo J. V. Garcia Nuno Gomes Karl-Heinz Hofmann Thomas Henning Jacob W. Isbell Bruno Lopez Alexis Matter J-Uwe Pott Dieter Schertl Eric Thiébaut Gerd Weigelt John Young 《Experimental Astronomy》2018,46(3):457-473
During the last two decades, the first generation of beam combiners at the Very Large Telescope Interferometer has proved the importance of optical interferometry for high-angular resolution astrophysical studies in the near- and mid-infrared. With the advent of 4-beam combiners at the VLTI, the u ? v coverage per pointing increases significantly, providing an opportunity to use reconstructed images as powerful scientific tools. Therefore, interferometric imaging is already a key feature of the new generation of VLTI instruments, as well as for other interferometric facilities like CHARA and JWST. It is thus imperative to account for the current image reconstruction capabilities and their expected evolutions in the coming years. Here, we present a general overview of the current situation of optical interferometric image reconstruction with a focus on new wavelength-dependent information, highlighting its main advantages and limitations. As an Appendix we include several cookbooks describing the usage and installation of several state-of-the art image reconstruction packages. To illustrate the current capabilities of the software available to the community, we recovered chromatic images, from simulated MATISSE data, using the MCMC software SQUEEZE. With these images, we aim at showing the importance of selecting good regularization functions and their impact on the reconstruction. 相似文献
4.
Dr. Hans-Peter Geis 《International Journal of Earth Sciences》1967,56(1):561-567
Zusammenfassung Die Magnetiterzlager der Insel Andörja/Nordnorwegen liegen in einer Serie mesozonal metamorphisierter Sedimente des Kambro-Silurs der Kaledoniden: Granatglimmerschiefer Hangender Kalkmarmor (max. 5 Horizonte, die bis 9 m mächtig sind) Amphibolitschiefer (83–175 m mächtig, mit marin-sedimentären Magnetiterzen) Liegender Kalkmarmor (0–4 m mächtig) Granatglimmerschiefer, z. T. Quarzit.Diese Gesteinsfolge hat typisch miogeosynklinalen Charakter. Da sie westlich des Verbreitungsgebiets der eugeosynklinalen kaledonischen Sedimente und nahe dem Westrand des Verbreitungsgebiets kambro-silurischer Gesteine überhaupt auftritt, könnte es sich hier um den Westrand der Kaledoniden handeln. Westlich davon auftretende präkaledonische Gesteine könnten dann zur irischen Plattform gehören.
The magnetite layers on the island of Andörja lie in a series of metamorphosed cambro-silurian sediments with the following sequence: garnet mica schist upper marble (max. 5 layers with up to 5 m thickness) amphibolite schist (83–175 m thickness, with marine sedimentary magnetite ore) lower marble (0–4 m thickness) garnet mica schist, partly quartzite.This rock sequence is of typically miogeosynclinal character. As it is situated to the west of the extension of the eugeosynclinal Caledonian rocks and near the western border of the cambro-silurian rocks on the whole, we might have here the western boundary of the caledonian geosyncline. Precaledonian rocks to the west of Andörja might then belong to the Irish platform.
Résumé Les couches de magnétite du gisement d'Andörja se trouvent dans une série de sediments cambro-siluriens métamorphiques avec la séquence suivante: marbre supérieur (max. 5 horizons qui ont une épaisseur jusqu'à 9 m) amphibolite (83–175 m d'épaisseur, avec gisements de magnétite) marbre inférieur (0–4 m d'épaisseur) schistes de grenat et mica, en partie quartzites.La séquence est d'un caractère typiquement miogeosynclinal. Parce qu'elle apparaît à l'ouest de l'extension des roches eugéosynclinales calédoniennes et à la bordure des roches cambro-siluriennes en général, on y a probablement la frontière occidentale de la géosynclinale calédonienne. Les roches précalédoniennes plus à l'ouest pourraient alors appartenir à la plateforme d'Irlande.
Andörja ( ), - : (9 ), (83–175 , ), (0–4 ), - , . . , .相似文献
5.
Harald Geiger Ian Barnes Karl H. Becker Birger Bohn Theo Brauers Birgit Donner Hans-Peter Dorn Manfred Elend Carlos M. Freitas Dinis Dirk Grossmann Heinz Hass Holger Hein Axel Hoffmann Lars Hoppe Frank Hülsemann Dieter Kley Björn Klotz Hans G. Libuda Tobias Maurer Djuro Mihelcic Geert K. Moortgat Romeo Olariu Peter Neeb Dirk Poppe Lars Ruppert Claudia G. Sauer Oleg Shestakov Holger Somnitz William R. Stockwell Lars P. Thüner Andreas Wahner Peter Wiesen Friedhelm Zabel Reinhard Zellner Cornelius Zetzsch 《Journal of Atmospheric Chemistry》2002,42(1):323-357
Within the German Tropospheric Research Programme (TFS) numerous kinetic and mechanistic studies on the tropospheric reaction/degradation of the following reactants were carried out: oxygenated VOC, aromatic VOC, biogenic VOC, short-lived intermediates, such as alkoxy and alkylperoxy radicals.At the conception of the projects these selected groups were classes of VOC or intermediates for which the atmospheric oxidation mechanisms were either poorly characterised or totally unknown. The motivation for these studies was the attainment of significant improvements in our understanding of the atmospheric chemical oxidation processes of these compounds, particularly with respect to their involvement in photooxidant formation in the troposphere. In the present paper the types of experimental investigations performed and the results obtained within the various projects are briefly summarised. The major achievements are highlighted and discussed in terms of their contribution to improving our understanding of the chemical processes controlling photosmog formation in the troposphere. 相似文献
6.
Dr. Hans-Peter Geis 《International Journal of Earth Sciences》1966,55(2):414-417
Zusammenfassung In Westnorwegen auftretende Magnetit-Ilmeniterze sind teilweise an intrusive, gabbroide Gesteine und teilweise an wahrscheinlich extrusive Amphibolite gebunden. Das TiO2Fe-Verhältnis der Amphiboliterze beträgt 0,14–0,15 und ist innerhalb der einzelnen Vorkommen konstant. In den Gabbroerzen liegt das Verhältnis zwischen 0,21 und 0,35 und schwankt auch innerhalb der Einzelvorkommen stark.
Magnetite-ilmenite ore in western Norway occurs partly in intrusive, gabbroic rocks, partly in amphibolites which seem to be extrusive. The relation TiO2: Fe in the amphibolite ores is 0.14–0.15 and is constant within every deposit. In the gabbro ores the relation TiO2Fe lies between 0.21 and 0.35 and varies also within every single deposit.
Résumé Dans l'Ouest de la Norvège des gisements de magnétite-ilménite se trouvent en partie dans des roches gabbroïques et intrusives, en partie dans des amphibolites qui sont probablement extrusives. Le rapport TiO2Fe dans les minerais amphibolitiques est de 0,14–0,15 et se montre très constant d'un gisement à l'autre. Dans les minerais gabbroïques, le rapport TiO2Fe varie entre 0,21 et 0,35 et diffère selon le gisement.
. TiO2: Fe .相似文献
7.
A. L. Perchuk M. Burchard H.-P. Schertl W. V. Maresch T. V. Gerya H.-J. Bernhardt O. Vidal 《Contributions to Mineralogy and Petrology》2009,157(5):573-592
We demonstrate the possibility of studying several diffusion couples in a single run, i.e. under almost similar P–T–t– conditions, allowing direct comparison of the diffusion rates in different diffusion couples. Thus the duration of experimental
study and the risk of failure of expensive experimental equipment can be decreased considerably. The diffusion experiments
were carried out in piston-cylinder apparatus. Gem-quality garnets of almandine, spessartine and grossular compositions together
with inclusion-rich eclogitic garnets were embedded in a powder of natural pyrope and annealed together under dry conditions
at P = 1.9–3.2 GPa and T = 1,070–1,400°C. Diffusion profiles were measured by electron microprobe and fitted numerically on the basis of multicomponent
diffusion theory. The datasets derived from different diffusion couples yields parameters of the Arrhenius equation for Ca,
Mg and Fe in natural eclogitic garnets and Mg, Mn and Fe in gem-quality garnets. We have also studied the effect of grain-boundary
diffusion in the sintered pyrope matrix on interdiffusion on the basis of 2D modeling. Under conditions analogous to those
of our experimental runs, we show that observed irregularities in some measured diffusion profiles (not applied for the diffusion
modeling) can be directly related to the superposition of local grain-boundary diffusion on dominant volume diffusion. 相似文献
8.
Shyh‐Lung Hwang Pouyan Shen Hao‐Tsu Chu Tzen‐Fu Yui Yoshiyuki Iizuka Hans‐Peter Schertl 《Journal of Metamorphic Geology》2019,37(8):1079-1098
Metamorphic garnet commonly contains needle‐like rutile inclusions as well as equant rutile inclusions that surround quartz inclusions and range in size from submicrometer to nanometer. Although the origin of these equant rutile inclusions, that is, exsolution or non‐exsolution, has important implications for petrological and tectonic processes, the crystallographic characteristics of these inclusions have rarely been studied because of the small sizes and analytical difficulties involved. Here, we report the crystallographic characteristics pertinent to the genetic origin of minute equant rutile inclusions in cloudy, nearly spherically shaped garnet domains with Ti‐depleted compositions surrounding quartz inclusions in ultrahigh‐pressure garnet from several diamondiferous Erzgebirge quartzofeldspathic gneissic rock samples. TEM analyses show that the equant rutile crystals in cloudy garnet domains are partially bounded by the low‐energy {100}rt ± {110}rt ± {101}rt facets and have rather random crystallographic orientation relationships (CORs) with the garnet host, with preferential alignment of low‐energy lattice planes, for example, {100}rt//{112}grt, for some rutile crystals. Although the rather random CORs are unlikely to be attributed to solid‐state exsolution subjected to the stringent topotactic garnet lattice constraints, the characteristic subhedral {100}rt ± {110}rt ± {101}rt crystal forms of rutile can be rationalized by a metasomatic dissolution‐reprecipitation mechanism via a fluid phase. In this scenario, the quartz+fluid inclusions in garnet were first subjected to decompression microcracking during rock exhumation, followed by dissolution of Ti‐bearing garnet matrix at the crack tips or along the crack surfaces and subsequent reprecipitation of rutile, apatite, gahnite, akdalaite, and Ti‐depleted garnet. The rapid coalescence between rutile and garnet crystals in fluid or direct attachment of rutile crystals onto the dissolving crack surfaces would then yield the rather random CORs as reported here. These results, along with previous work on rutile needles, indicate rather diverse genesis of rutile inclusions in various crystal forms, thus shedding light on the controversial exsolution origin for other inclusion suite/microstructure in minerals. 相似文献
9.
Stefan?R?sel Anna?Rych?a Christian?Wurzbacher Hans-Peter?GrossartEmail author 《Aquatic Sciences - Research Across Boundaries》2012,74(1):87-99
Nutrient fluxes across terrestrial-aquatic boundaries and their subsequent integration into lake nutrient cycles are currently
a major topic of aquatic research. Although pollen represents a good substrate for microorganisms, it has been neglected as
a terrestrial source of organic matter in lakes. In laboratory experiments, we incubated pollen grains of Pinus sylvestris in water of lakes with different trophy and pH to estimate effects of pollen input and its subsequent microbial degradation
on nutrient dynamics. In this ex situ experiment, we measured concentrations of organic carbon, phosphorus and nitrogen in the surrounding water as well as microbial
dynamics (bacteria and fungal sporangia) at well-controlled conditions. Besides leaching, chemical and microbial decomposition
of pollen was strongest within the first week of incubation. This led to a marked increase of soluble reactive phosphorus
and total dissolved nitrogen (up to 0.04 and 1.5 mg L−1, respectively, after 5 days of incubation) in the ambient water. In parallel, pollen grains were rapidly colonized by heterotrophic
bacteria and aquatic fungi. Leaching and microbial degradation of pollen accounted for ≥80, ≥40, ≥50% for organic C, N and
P, respectively, and did not significantly differ among water samples from the studied lakes. Thus, pollen introduces high
amounts of bio-available terrestrial organic matter and nutrients into surface waters within a short time. A rough calculation
on P input into oligotrophic Lake Stechlin indicates that pollen plays an important ecological role in nutrient cycling of
temperate lakes. This requires further attention in aquatic ecology. 相似文献
10.
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 Xef (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