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排序方式: 共有481条查询结果,搜索用时 78 毫秒
191.
Andrew C. Poje Angelique C. Haza Tamay M. Özgökmen Marcello G. Magaldi Zulema D. Garraffo 《Ocean Modelling》2010,31(1-2):36-50
In order to determine the effect of Eulerian spatial resolution on the two particle statistics of synthetic drifter trajectories, we examine a hierarchy of ocean models, starting from 2D turbulence simulations, progressing to idealized simulations of a buoyant coastal jet with ROMS, and finally to realistic HYCOM simulations of the Gulf Stream. In each case, particle dispersion at large time and space scales is found to be controlled by energetic meso-scale features of the flow that are relatively insensitive to the resolution of finer scale motions. In all cases, time-distance graphs given in terms of computed Finite Scale Lyapunov Exponents show an expected increase in the extent of exponential scaling with increasing spatial smoothing of the velocity field. The limiting value of the FSLE at small separation distances is found to scale remarkably well with the resolution of Eulerian velocity gradients as given by the average of positive Okubo–Weiss parameter values. 相似文献
192.
Öivind Hauge 《Solar physics》1970,11(1):17-21
Europium has two stable isotopes, Eu 151 and Eu 153. The high isotope shift and the different hyperfine splitting of the energy levels of the two isotopes make it possible to study the isotope ratio by an analysis of the spectral line profiles. From five spectral lines the solar isotope ratio is found to be equal to the terrestrial ratio within an error limit of about 10 %. 相似文献
193.
194.
Yngve Öhman 《Solar physics》1983,85(1):53-63
From a study of the chromospheric lines listed by Pierce (1968, 1973) indications have been found that first-order plasma satellites appear sometimes as a pair of faint chromospheric emission lines in such places where forbidden lines, mainly of metals, should be located. Second-order satellites are indicated sometimes by an asymmetry in the emission wings of stronger lines, either with respect to intensity or with respect to distance from the line centre and, if so, with the remote wing of diffuse shape. Finally diffuse faint lines, appearing in somewhat greater distances from strong chromospheric lines, suggest the appearance sometimes of fourth-order plasma satellites. All the three types of satellites give electron densities of the order of 1012 cm?3. Traces of possible absorption satellites are found also for some of the lines in the solar spectrum. In this connection special attention is drawn to a few faint solar lines located near the wavelengths of corona emission lines. The observational evidence is discussed on the bases of recent theoretical research by Drawin and Truong-Bach (1982a, b). 相似文献
195.
Giulio Bigazzi Zehra Yegingil Tuncay Ercan Massimo Oddone Mehmet Özdogan 《Bulletin of Volcanology》1993,55(8):588-595
Twenty obsidian samples from Central and North Anatolia were dated by the fission track method. Split samples analyzed in two different laboratories give consistent results. Data presented refer to three volcanic fields and are summarized as follows: Orta-Sakaeli (Northern Anatolia) obsidians with ages from 21–23 Ma; Göllü Dagi dome complex near Çiftlik (Central anatolia) has given ages between 1.33–0.98 Ma; Acigöl caldera (Central Anatolia) shows three age groups: (1) Eruptions of precaldera (Bogazköy) obsidians with ages 0.18–0.15 Ma; (2) Formation of the large intracaldera dome Kocadag-Taskesiktepe at about 0.08 Ma (uncorrected apparent age of 0.075 Ma); and (3) Acigöl peripheral obsidian domes with plateau ages of 0.020 and 0.019 Ma, and an additional uncorrected age of 0.018 Ma form a distinct age group. This fission track parameters discriminate between the various obsidian sources of prehistoric obsidian artifacts. 相似文献
196.
The magnetic anomaly due to a buried dike consists of the sum of two easily separated elementary functions. These functions, which have simple symmetry, are called even and odd functions. The correlation factors (r
0,1 for the even andr
0,2 for the odd function) between least-squares residual anomalies from even and odd functions are computed. Correlation values are used to determine the depth to the top and the half-width of the dike. The method also includes the determination of the index parameter and the amplitude coefficient. The validity of the method is tested against a theoretical and a field example where the parameters of the latter were determined by other investigators in comparing the results. 相似文献
197.
Ismail Özkaya 《International Journal of Earth Sciences》1991,80(3):657-668
Field study of several stratigraphic sections from allochthonous thrust fault slices of SW Turkey reveal that a deeply subsiding volcanogenic trough, the Alakaya basin existed during Paleocene-Middle Eocene times along the Lycian belt. The Alakaya basin was located along a tectonically active zone of weakness between two relatively stable tectonic terrains, the Menderes massif to the northwest and the Beydaglari continental platform to the southeast. The basin was underlain by continental substratum. All known outcrops of the Alakaya sediments overlie platform carbonates of Cretaceous age that correlate with the Beydaglari shelf sediments. The generation of the volcanogenic Alakaya basin reflects a tensional period that culminated in Middle Eocene when basic volcanic activity took place. The tensional stage was replaced by a compressional regime in Late Eocene and large scale overthrust faulting took place. The Alakaya basin was closed when the Tefenni nappe from the north was emplaced on its sediments in Late Eocene. The Alakaya sediments overlying the Tefenni nappe and underlying the Cretaceous platform carbonates moved southeastward over a hundred kilometers onto the autochthonous sediments of the Beydaglari terrain in Miocene time. The Alakaya basin is analogous to the Maden basin of SE Turkey thrust fault belt. Both basins were located along tectonically active belts. The main stage of basin subsidence and volcanism was in Middle Eocene. Closure of both basins by large scale thrust faulting was in Late Eocene. The creation and destruction of the volcanogenic Alakaya basin may be related to the regional adjustments in plate motions in Paleocene-Eocene times.
Zusammenfassung Geländestudien einiger stratigraphischer Profile von allochthonen Überschiebungspaketen in der SW Türkei zeigen, daß ein tief abgesunkener vulkanogener Trog, das Alakaya Becken, während des Paläozäns und Mittel Eozäns entlang der Lyzischen Zone bestand. Das Alakaya Becken lag innerhalb einer tektonisch aktiven Schwächezone zwischen zwei relativ stabilen tektonischen Terrains, dem Menderes Massiv im NW und der Beydaglari Kontinentalplattform im SE. Das Becken besaß eine kontinentale Unterlage. Alle bekannten Aufschlüsse mit Alakaya Sedimenten lagern über kretazischen Plattformkarbonaten, die sich mit den Beydaglaria Schelfsedimenten korrelieren lassen. Die Entwicklung des vulkanogenen Alakaya Bekkens spiegelt eine Spannungsperiode wieder, die im Mittel Eozän mit basischem Vulkanismus kulminierte. Diese Periode der Zugspannung wurde im späten Eozän von einer kompressiven Beanspruchung abgelöst, welche zu großmaßstäblichen Überschiebungen führte. Das Alakaya Becken wurde geschlossen, als auf Grund der späteozänen Platznahme die aus dem Norden stammende Tefenni Decke auf deren Sedimenten zu liegen kam. Die Alakaya Sedimente zusammen mit der überlagernden Tefenni Decke und den unterlagernden kretazischen Plattformkarbonaten wurden während des Miozäns über einhundert Kilometer südostwärts auf die autochthonen Sedimente des Beydaglari Terrains überschoben. Das Alakaya Becken ist ein Analogon zu dem Maden Becken der SE Türkischen Überschiebungszone. Beide Becken lagen entlang tektonisch aktiver Zonen. Während des Mittel Miozäns war das Hauptstadium der Beckensubsidenz und des Vulkanismus. Das Schließen der Becken mittels großmaßstäblicher Überschiebung fand in beiden Fällen im späten Eozän statt. Die Bildung und der Zerfall des vulkanogenen Alakaya Beckens scheint mit den regionalen Anpassungen an die Plattenbewegung während des Paläozäns und Eozäns verbunden zu sein.
Résumé L'étude de terrain de plusieurs coupes stratigraphiques dans les lames charriées de l'allochtone du sud-ouest de la Turquie révèle l'existence, du Paléocène à l'Eocène moyen, d'une fosse volcanogénique fortement subsidente: le bassin d'Alakaya, situé le long de la chaîne lycienne. Ce bassin d'Alakaya s'est localisé le long d'une zone de faiblesse tectoniquement active, entre deux blocs relativement stables: le massif de Menderes au nord-ouest et la plate-forme continentale de Beydaglari au sud-est. Le bassin repose sur un substratum continental. Dans tous les affleurements connus, les sédiments d'Alakaya surmontent des carbonates de plateforme d'âge Crétacé, corrélables aux sédiments de shelf de Beydaglari. La genèse du bassin volcanogène d'Alakaya reflète une période d'extension dont le maximum se situe à l'Eocène moyen, lors de l'apparition d'une activité volcanique basique. A la phase distensive a succédé, à l'Eocène supérieur, un régime compressif marqué par des charriages de grande échelle. Le bassin d'Alakaya était fermé au moment où la nappe de Tefenni, venant du nord, s'est mise en place sur ses sédiments, à l'Eocène supérieur. Au Miocène, l'ensemble formé par la plate-forme carbonatée crétacée sous-jacente, les sédiments dAlakaya et la nappe de Tefenni surincombante a été transporté d'une centaine de km vers le sud-est sur les sédiments autochtones de Beydaglari. Le bassin d'Alakaya est analogue au bassin de Maden de la ceinture charriée du sud-est de la Turquie. Tous deux se sont localisés le long de zônes tectoniques actives. Leur phase culminante de subsidence et de volcanisme se situe à l'Eocène moyen. Dans les deux cas, les bassins ont été formés à l'Eocène supérieur par un charriage à grande échelle. La formation et la destruction du bassin d'Alakaya semblent pouvoir être rattachées aux ajustements régionaux dans les mouvements des plaques au Paléocène-Eocène.
- , , , Lyzi. deres - Beydaglari -. . , Beydaglari. , . , . , Tefenni . , 100 - .. Beydaglari. Maden - . . , . . , .相似文献
198.
Atila Özgüç 《Astrophysics and Space Science》1992,187(2):197-207
We have analysed intermediate-term periodicities in the green corona by dividing 10° latitudinal belts for the solar cycles 18, 19, and 20 (1947–1976). Discrete Fourier transform technique was used and three noticeable periodicities (3.48, 2.57, and 2.27 years) were found. The physical origin of these periods is not known, but evidence in our results exclude the possibility that the observed periods are a harmonic due to the method of analyse. The period of 3.48-year is the strongest one. 17.6-month periodicity was found only on around +40° belt while 155-day periodicity was not found in our analysis. 相似文献
199.
200.
The large-scale dynamics of the Martian winter atmosphere are analyzed and discussed. Results obtained from a baroclinic instability analysis, including a Newtonian radiational damping term, are compared with the Mariner 9 data. The beta plane baroclinic poleward heat fluxes are contrasted with those produced using spherical geometry, from the stationary orographically forced long waves. 相似文献