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51.
Direct measurements of plasma motions in the photosphere are limited to the line-of-sight component of the velocity. Several algorithms have therefore been developed to reconstruct the transverse components from observed continuum images or magnetograms. We compare the space and time averages of horizontal velocity fields in the photosphere inferred from pairs of consecutive intensitygrams by the LCT, FLCT, and CST methods and the DeepVel neural network in order to identify the method that is best suited for generating synthetic observations to be used for data assimilation. The Stein and Nordlund (Astrophys. J. Lett.753, L13, 2012) magnetoconvection simulation is used to generate synthetic SDO/HMI intensitygrams and reference flows to train DeepVel. Inferred velocity fields show that DeepVel performs best at subgranular and granular scales and is second only to FLCT at mesogranular and supergranular scales. 相似文献
52.
Light curve modeling for the newly discovered super contact low-mass WUMa system 1SWASPJ092328.76+435044 was carried out by using a new BVR complete light curves. A spotted model was applied to treat the asymmetry of the light curves. The output model was obtained by means of Wilson–Devinney code, which reveals that the massive component is hotter than the less massive one with about ΔT ~ 40 K. A total of six new times of minima were estimated. The evolutionary state of the system components was investigated based on the estimated physical parameters. 相似文献
53.
54.
Discontinuous Galerkin numerical simulations of single phase flow problem are described in this paper. The simulations show the advantages of using discontinuous approximation spaces. hp convergence results are obtained for smooth solutions. Unstructured meshes and unsmooth solutions are also considered. 相似文献
55.
Márton Pécsi 《GeoJournal》1995,36(2-3):117-131
In the process of loessification, the development of loess fabric, the role of zonal, regional and partly of local environmental factors is regarded decisive. In the loess sequences various genetic types of loess pockets and paleosols occur and reflect different climatic and paleogeographical conditions.As a consequence, even within a single profile the colour, grain size and mineral composition, CaCO3 content, degree of weathering and fabric of loess may vary. Zonal, regional or even local variations in such loess properties may equally derive from syngenetic or postgenetic processes. For similar reasons, spatially and temporally different forms, types and subtypes of paleosol also developed.This way, loess and soil formation resulted in various spatial types in the same glacial, interstadial or interglacial phase in the various geographical zones and regions. Although there exist major loess regions where the interglacial soils (eg brown forest soils) are markedly distinct from interstadial steppe soils or from other types of humic soils, continental loess areas can also be observed where the paleosols developed under interglacial and interstadial conditions (eg steppe or forest steppe soils) cannot be referred into different genetic types. In such cases the changes in paleoenvironments are difficult and uncertain to reconstruct.The interregional correlation of paleosols is occasionally hindered by the various terminologies applied to denote them. In addition, there are uncertainties concerning the dating and identification of paleoenvironments of polygenetic soils and of soil complexes consisting of paleosol units: how many soil formation phases they represent and how long erosional gaps can be reckoned with between these phases. 相似文献
56.
Due to its physical and chemical properties, areas with a loess mantle of proper thickness favour arable farming. Loess as a parent material promotes the formation of soils of good structure, nutrient supply and water budget. The ongoing land evaluation project places particular emphasis on the consideration of parent material in its scoring system as soil and climatic parameters are assessed in conjunction with the grain size composition of subsurface material and soil texture.A test area most suitable for the presentation of the method seems to be a sandy alluvial fan with loess mantle and this circumstance allows the contrasting of the agroecological potentials of soils developed on the two parent materials of different nature.The favourable water storage properties of loess make this deposit particularly valuable under the conditions of climatic aridification. The geographical information system applied here is capable of simulating the agroecological potential changes caused by reduced precipitation, increased evaporation and dropping groundwater levels.The research for this paper was carried out as part of the MEDALUS II (Mediterranean Desertification and Land Use) collaborative research project. MEDALUS II was funded by the EC under its Environment Progamme, contract no. EV5V 0128/0166. A grant was also provided by the OTKA (Hungarian National Science Foundation), project no 1278. The support is gratefully acknowledged. 相似文献
57.
P. Schmidt-Thomé 《International Journal of Earth Sciences》1954,42(2):172-187
Zusammenfassung Klufttektonische Untersuchungen in den Alpen sind spärlich. Nur die Arbeiten aus den bayerischen Kalkalpen lohnen eine vergleichende Betrachtung. Die in nichtalpinen Gebirgen zu Beginn der Faltung auftretenden kubischen Zerrungs-Kluftsysteme lassen sich in den nördlichen Kalkalpen nicht erkennen. Dort treten statt dessen Scherkluftsysteme auf, teils als gekreuzte Systeme, teils als Begleitklüfte streichender Störungen. Unbeeinflußt ziehen sie über Falten- und Deckenstrukturen hinweg, sind also jünger als diese. Das Diagonalkluftsystem geht auf seitliche Spannungen infolge Horizontalbeanspruchung zurück, die gegen Norden gerichtet war. Die Schernatur kommt in der vorwiegend horizontalen Striemung zum Ausdruck. Ein Vergleich mit den offenbar aus Scherklüften hervorgegangenen Diagonalstörungen, die mit den Klüften annähernd gleich alt sind, macht es wahrscheinlich, daß in Südbayern die Einbeziehung der Molasse in den Faltenbau jünger ist als die Diagonalstörungen. Scherkluftsystem und Diagonal-Blattverschiebungen sind für die nördlichen Kalkalpen mit ihrem flachen, nordvergenten Deckenbau besonders bezeichnend und scheinen in zentralen oder westlicheren Alpengebieten zurückzutreten oder ganz zu fehlen. 相似文献
58.
Different diagenetic transformations and their relative chronological sequence are studied in the meteoric diagenetic zone from the Upper Oligocene limestone at the North of the Aquitaine Basin (France), by combining high-resolution cathodoluminescence spectroscopy and electron-microprobe analyses. More than 128 spot analyses by electron microprobe and 60 analyses by cathodoluminescence spectroscopy are done on different meteoric cements firstly identified by classic optical microscopy. Three cement types are identified according to the relative intensity of the bands of their respective cathodoluminescence spectra (350, 380, 430, 500, and 620 nm). From these investigations, we could identify for each meteoric cement different phases of crystalline growth and crystalline dissolution. As a result, a better and more realistic meteoric diagenetic model is proposed. It illustrates the cyclic transformations from vadose zone (unsaturated) to meteoric zone (saturated). To cite this article: R. Chapoulie et al., C. R. Geoscience 337 (2005). 相似文献
59.
Pierre Strzerzynski Stéphane Guillot Gabriel Courrioux Patrick Ledru 《Comptes Rendus Geoscience》2005,337(14):1284-1292
The structural analysis and the 3D modelling of Stephanian granites of the Pelvoux Massif characterize an emplacement along sinistral NW–SE- and dextral NE–SW-trending shear zones in the Pelvoux and in the Aiguilles Rouges–Mont Blanc Massifs, respectively. This Carboniferous shear system is consistent with a north–south extension direction known in the whole Variscan belt at this time. To cite this article: P. Strzerzynski et al., C. R. Geoscience 337 (2005). 相似文献
60.
Cosmogenic nuclides in extraterrestrial matter provide a wealth of information on the exposure and collision histories of
small objects in space and on the history of the solar and galactic cosmic radiation. The interpretation of the observed abundances
of cosmogenic nuclides requires detailed and accurate knowledge of their production rates. Accelerator experiments provide
a quantitative basis and the ground truth for modeling cosmogenic nuclide production by measurements of the relevant cross
sections and by realistic simulations of the interaction of galactic protons with meteoroids under completely controlled conditions,
respectively. We review the establishment of physical model calculations of cosmogenic nuclide production in extraterrestrial
matter on the basis of such accelerator experiments and exemplify this approach by presenting new experimental and theoretical
results for the cosmogenic nuclide44Ti. The model calculations describe all aspects of cosmogenic nuclide production and allow the determination of long-term
solar and galactic cosmic ray spectra and a consistent interpretation of cosmogenic nuclides in extraterrestrial matter. 相似文献