Fission track dating obsidians in Central and Northern Anatolia

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.     

Interpretation of magnetic anomalies of dikes using correlation factors

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.     

Evolution of a tertiary volcanogenic trough in SW Turkey — The Alakaya basins of the Lycien belt

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.

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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.

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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.

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Intermediate-term periodicities in the green corona brightness of the Sun

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.     

The solar niobium abundance

The solar Nb abundance is derived from five Nb i and ten Nb ii lines in the photospheric spectrum. Equivalent widths are obtained from measurements on spectra recorded at Kitt Peak National Observatory. Synthetic spectrum calculations gave abundances of 2.23 and 2.08 from neutral and ionized lines respectively in the logarithmic A _H = 12.00 scale. This gives an average abundance value of A _Nb = 2.13 ± 0.10.     

A reply to Richard Greenberg's review of interplanetary encounters: Close range gravitational interactions

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.     

The missing planet

Ovenden's hypothesis suggesting former existence of a planet of 90 Earth masses which supposedly filled the Titius-Bode gap in the asteroid belt and then suddenly disappeared 16 million years ago, is critically examined by the morphological method. It is shown that an explosive removal, however improbable, could have led to the formation of the asteroids from a non-explosive core (the nuclear charge being placed outside of it), but that life on Earth would have been completely destroyed by three successive blasts-one from the direct impact of the ejecta of the planet, another from the increased radiation suddenly emitted by the Sun when hit by the ejecta, and a third one (arriving, however, first) from the radiation emitted by the nuclear explosion. The geological record of the continuity of Life on Earth for the past 10⁹ years definitely excludes the possibility of such an explosion in the late Tertiary.The other mode of removal of the planet-in a gravitational encounter with an intruder either from interstellar space or from the unexplored outskirts of the solar system, under the condition of not having disturbed the existing regularity of planetary orbits-is not only extremely improbable, to be expected once during 100 million times the age of the solar system; but it would leave no asteroids behind, all of the previously existing primaeval asteroids having been rapidly eliminated in encounters with the hypothetical planet.Whatever the merits of Ovenden's long-range calculations of the secular perturbations of coplanar circularized planetary orbits, the hypothesis of a massive planet to have existed in the asteroidal region and then recently to have suddenly disappeared, belongs to the realm of the impossible. After such a hypothetical event, either we would not be here on Earth, or there would be no asteroids in their present place between Jupiter and Mars.Paper dedicated to Professor Hannes Alfvén on the occasion of his 70th birthday, 30 May 1978.     

Detecting of Lithological Units by Using Terrestrial Spectral Data and Remote Sensing Image

The objective of the study was to carry out an automatic classification of the lithological units of interest using the integration of remote sensing image, in which various objects are spread on, and terrestrial spectral measurement data. Only endmembers of interest are classified using spectral classification methods such as Spectral Angle Mapper. Following the identification of the types of rock and minerals, integration of remote sensing images and spectral measurement data enable spectral classification. In this study, Short Wave Infrared detector images of Advanced Spaceborne Thermal Emission and Reflection Radiometer satellite and spectroradiometer measurements were used. The study area, Gölova with its geological diversity is located in the Kelkit Valley section of the North Anatolian Fault Zone in Northeast of Turkey. Seventeen rock samples were collected and their coordinates were recorded. The samples were categorized via spectral measurements on their thin sections through petrographic analyses. Marble and Meta lava with different lithological were selected as endmembers. SAM was used as the classification method that enables the analysis of the endmember with the threshold value of 0.009 radian for marble and 0.010 radian for metalava. SAM analysis was compared by visual analysis to principle component analysis, decorrelation stretch, band ratio (R: 4/7, G: 4/1, B (2/3) x (4/3)) and band combination analysis (R: 9, G: 4 and B: 5). This study demonstrates that the SAM method can be successfully used in both the integration of remote sensing image and terrestrial spectral measurement data in lithological classification. Both the endmembers of metalava and marbles were detected in the SAM results at the GPS coordinates noted down whilst collecting the rock samples for accuracy assessment.     

VGDI – Advancing the Concept: Volunteered Geo‐Dynamic Information and its Benefits for Population Dynamics Modeling

The concept of Volunteered Geographic Information (VGI) has progressed from being an exotic prospect to making a profound impact on GIScience and geography in general, as initially anticipated. However, while massive and manifold data is continuously produced voluntarily and applications are built for information and knowledge extraction, the initially introduced concept of VGI lacks certain methodological perspectives in this regard which have not been fully elaborated. In this article we highlight and discuss an important gap in this concept, i.e. the lack of formal acknowledgment of temporal aspects. By coining the proposed advanced framework ‘Volunteered Geo‐Dynamic Information’ (VGDI), we attempt to lay the ground for full conceptual and applied spatio‐temporal integration. To illustrate that integrative approach of VGDI and its benefits, we describe the potential impact on the field of dynamic population distribution modeling. While traditional approaches in that domain rely on survey‐based data and statistics as well as static geographic information, the use of VGDI enables a dynamic setup. Foursquare venue and user check‐in data are presented for a test site in Lisbon, Portugal. Two core modules of spatio‐temporal population assessment are thereby addressed, namely time use profiling and target zone characterization, motivated by the potential integration in existing population dynamics frameworks such as the DynaPop model.