First data on U-Pb SHRIMP-II isotopic dating based on zircons of ash sediments from Cenozoic depressions in Southwest of Primorie

U-Pb (SHRIMP-II) isotopic dating has been conducted for zircons of the ash sediments of the Ust’-Suifun Suite, which was the final stage of Late Cenozoic explosive volcanism in Southwest Primorskii krai. These pyroclastic units are widespread within sediments that fill in Cenozoic depressions including large coalfields. The concordant dates (23.7–24.6 Ma) are in line with the results of the K-Ar determinations for volcanic tephra (23.6–27.1 Ma) and correspond to the beginning of the active phase of spreading and taphrogenesis in the neighboring Trench of the Sea of Japan. These processes started as early as the Eocene and are reflected in the continental vicinity with the formation of riftogenic depressions and the occurrence of a peculiar gas volcanism.     

The British Tertiary igneous province: palaeomagnetism of the dyke swarm along the Sleat coast of Skye

Summary. A palaeomagnetic investigation has been made of a swarm of more than 400 dykes along the south coast of Skye, Scotland, by the Sound of Sleat.
Seven red lamprophyre dykes have palaeomagnetic directions inconsistent with Tertiary age, and not inconsistent with their previously held Caledonian age. The remaining 409 dykes have palaeomagnetic directions that are consistent with a Lower Tertiary age. We present evidence suggesting that the Tertiary dykes might have been emplaced during a short time, over which the geomagnetic polarity occupied as few as three polarity intervals (NRN or RNR).
Certain 'intermediate' directions of magnetization have also been found, and are presented here.     

Campanian stage of granite formation in the south of the Sredinnyi Range in Kamchatka: New U-Pb SHRIMP Data

This article gives an account of the results of the U-Pb-SHRIMP study of zircons derived from gneissoid and equigranular granitoids of the Malka Uplift of the Sredynnyi Range in Kamchatka. It was established that intrusion and crystallization of granitoids occurred in the time interval from 76.2 ± 1.5 to 83.1 ± 2.0 Ma. The texture of zircon crystals suggests their magmatic origin. The obtained data reliably confirm that granite formation and emplacement of the recently formed continental crust in Kamchatka took place in the Late Cretaceous (Campanian).     

Relevance of Pentane- and Hexane-Utilizing Bacterial Indicators for Finding Hydrocarbon Microseepage: A Study from Jamnagar Sub-basin, Saurashtra, Gujarat, India

Mesozoic sediments are source rocks for nearly half the world’s hydrocarbon reserves. Hence, there is great interest in the oil industry to know the trap and sub-trappean sediment thickness and their extent in the trap covered regions of Jamnagar study area. The microbial prospecting method is applied in the Jamnagar sub-basin, Gujarat for evaluating the prospects for hydrocarbon exploration by investigating the anomalous abundance of n-pentane- and n-hexane-oxidizing bacteria of this area. A total of 150 near-surface soil samples were collected in Jamnagar sub-basin, Gujarat for the evaluation of hydrocarbon resource potential of the basin. In this study, bacterial counts for n-pentane-utilizing bacteria range between 1.09 × 10² and 9.89 × 10⁵ cfu/g and n-hexane-utilizing bacteria range between 1.09 × 10² and 9.29 × 10⁵ cfu/g. The adsorbed hydrocarbon gases consisting of ethane plus hydrocarbons (ΣC₂₊) of 1–977 ppb and n-pentane (nC₅) of 1–23 ppb. The integrated geomicrobial and adsorbed soil gas studies showed the anomalous hydrocarbon zones nearby Khandera, Haripur, and Laloi areas which could probably aid to assess the true potential of the basin. Integrated geophysical studies have shown that Jamnagar sub-basin of Saurashtra has significant sediment thickness below the Deccan Traps and can be considered for future hydrocarbon exploration.     

AIDS to geographic research afforded by the office of naval research

The following is a preliminary program, with some positions as yet unfilled. The final and complete program will he distributed at the meetings.     

FluBiDi – a model to estimate flood based on runoff: validation using extreme and natural basin conditions

FluBiDi is a two-dimensional model created to simulate real events that can take days and months, as well as short events (minutes or hours) and inclusive laboratory tests. To verify the robustness of FluBiDi, it was tested using a previous study with both designed and real digital elevation models. The results highlight good agreement between the models (i.e. Mike Flood, SOBEK, ISIS 2D, and others) tested and FluBiDi (around 90% for a specific instant and 95% for the complete time simulation). In the simulated hydrographs, the discharge peak value, time to peak, and water level results were accurate, reproducing them with an error of less than 5%. The velocity differences observed in a couple of tests in FluBiDi were associated with very short periods of time (seconds). However, FluBiDi is highly accurate for simulating floods under real topographical conditions with differences of around 2 cm when water depth is around 150 cm. The average water depth and velocities are precise, and the model describes with high accuracy the pattern and extent of floods. FluBiDi has the capability to be adjusted to different types of events and only requires limited input data.     

Ein Beitrag zur Struktur des Windes über Wien

Zusammenfassung Nach zweijährigen Parallelregistrierungen der Windgeschwindigkeit und Windrichtung in Wien-Hohe Warte am Rande der Stadt Wien und an einer Meßstelle in der Stadtmitte wird gezeigt, daß ein merklicher und jahreszeitlich veränderlicher Umgebungseinfluß gerade am Stadtrand auf die Windgeschwindigkeit einwirkt. Während der Vegetationsperiode ist die Bodenrauhigkeit erhöht, die Windgeschwindigkeit in den unteren Stufenwerten bis etwa 35 km/h wird verringert. Während der vegetationslosen Zeit ist die Bodenrauhigkeit viel geringer, die Häufigkeitsverteilung der Windgeschwindigkeit im Winter daher viel normaler. Es besteht ein scharfer Gegensatz zwischen den Sommer-und Wintermonaten ohne langsame Übergänge. Das Ergebnis dieses zunächst lokalen Vergleiches ist von allgemeiner Bedeutung für Windbeobachtungen in den gemäßigten Breiten mit Vegetationswechsel.

---

Summary Based on two year's parallel observations of velocity and direction of wind at two stations, viz. the secular station Wien-Hohe Warte at the periphery and a station in the town-centre, it is shown that there exists a considerable and seasonally variable effect of local influences on the wind velocity, especially at the periphery of the town. During the vegetation period the roughness of the ground is increased and up to about 35 km/h the wind velocity is reduced. Out of the vegetation period the roughness of the ground is much smaller, the frequency distribution of wind velocity during the winter, therefore, shows more the normal features. There is a marked difference between the summer and winter months, and there exists no graduate change. The result of this local comparison seems to be of general interest to the climatology of wind in temperate latitudes with their seasonal change of vegetation.

---

Résumé Pendant deux ans on a enregistré les vitesses et les directions des vents dans le cadre d'observations faites simultanément à la périphérie de la ville de Vienne (station météorologique «Hohe Warte») et à une station située au centre de cette ville. Les résultats démontrent que c'est précisément à la périphérie de la ville que l'aspect du sol exerce une influence très nette, la vitesse des vents, qui varie selon les saisons. Pendant la saison de végétation la «rugosité» du terrain étant plus grande, les vents moins forts (jusqu'à 35 km/h) sont affaiblis. En hiver, quand il n'y a pas de végétation, la rugosité du sol est moindre, et par conséquent les fréquences respectives des vents d'intensités diverses offrent un tableau mieux équilibré. Entre les mois d'hiver et les mois d'été, le contraste est très brusque; il n'y a pas de période de lente transition. Le résultat de ces essais, effectués seulement sur un plan local jusqu'à présent, est d'importance générale pour l'étude des vents dans les régions de climat tempéré, avec une végétation changeante.

---

---

Mit 1 Textabbildung

---

Herrn Prof. Dr.H. Ficker zum 75. Geburtstag gewidmet.     

Alteration processes in the CV chondrite parent body based on analysis of NWA 2086 meteorite

Analysis of the NWA 2086 CV3 chondrite showed a matrix/chondrule ratio of 52%, similar to Bali, Mokoia, and Grosanaja. Nearly twice as many chondrule fragments as intact ones demonstrate that an early fragmentation phase occurred prior to final accretion. After this event, no substantial mechanical change or redeposition is evident. Rims with double‐layered structures were identified around some chondrules, which, in at least one case, is attributed to an accretionary origin. The rim's outer parts with a diffuse appearance were formed by in situ chemical alteration. During this later process, Mg content decreased, Fe content increased, and olivine composition was homogenized, producing a rim composition close to that of the matrix. This alteration occasionally happened along fractures and at confined locations, and was probably produced by fluid interactions. Iron oxides are the best candidate for a small grain‐sized alteration product; however, technical limitations in the available equipment did not allow exact phase identification. These results suggest that NWA 2086 came from a location (possible more deeply buried) in the CV parent body than Mokoia or Bali, and suffered less impact effects—although there is no evidence of sustained thermal alteration. This meteorite may represent a sample of the CV parent asteroid interior and provide a useful basis for comparison with other CV meteorites in the future.