Effects of turbulence on average refraction angles in occultations by planetary atmospheres

Four separable effects of atmospheric turbulence on average refraction angles in occultation experiments are derived from a simplified analysis, and related to more general formulations by B.S. Haugstad. The major contributors are shown to be due to gradients in height of the strength of the turbulence, and the sense of the resulting changes in refraction angles is explained in terms of Fermat's principle. Because the results of analyses of such gradient effects by W. B. Hubbard and J. R. Jokipii are expressed in other ways, a special effort is made to compare all of the predictions on a common basis. We conclude that there are fundamental differences, and use arguments based on energy conservation and Fermat's principle to help characterize the discrepancies.     

Valley winds in the mount Rainier area

Summary Four summer seasons of field work near Mt. Rainier have shown that a well-developed valley wind system tends to have the following features: Airflow within a valley is up the valley during the day and down it at night and is compensated by a return flow (anti-wind) at a higher level. The layers occupied by the two flows are of approximately equal thickness, and the boundary between them is generally at, or somewhat below, ridgeheight. Above the anti-wind, the flow depends on the large-scale synoptic situation.Horizontal wind speed in these two layers is greatest slightly below the center of each layer. Speeds reach a maximum in early afternoon and just beforce sunrise. The reversal between day and nighttime flows is almost simultaneous everywhere in the valley, about an hour after sunnet and sunrise.Vertical transport of air between the two layers appears to be localized, mainly in the neighborhood of the ridges. Slope winds apparently feed the vertical currents. Speed fluctuations, having a period of about 20 minutes, were observed in drainage winds near the surface at night.When a well-developed wind system occured in one valley, well-developed systems tended to occur in other valleys in the same area.

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Zusammenfassung Beobachtungen im Verlaufe von vier Sommern im Mount-Rainier-Gebiet zeigten ein gutentwickletes Talwind-System mit folgenden Eigenschaften: Die Luft im Tale bewegt sich tags talaufwärts und nachts talabwärts; diese Strömung wird kompensiert durch ein Gegenwind-System in größerer Höhe. Die vertikale Erstreckung der übereinander liegenden Strömungen ist etwa gleich, und ihre Grenzfläche liegt, im allgemeinen, in oder etwas unter der Höhe der Bergkämme. Oberhalb des Gegenwindes beherrscht die weiträumige synoptische Situation die Strömung.Die Horizontalgeschwindigkeit ist für beide Windsysteme am größten etwas unter dem Zentrum der betreffenden Schicht. Geschwindigkeitsmaxima werden am frühen Nachmittag und kurz vor Sonnenaufgang erreicht. Der Umschlag von Tag- zu Nachtströmungen erfolgt nahezu gleichzeitig in allen Teilen des Tales, und zwar je etwa eine Stunde nach Sonnenaufgang bzw. Sonnenuntergang.Der vertikale Luftmassenaustausch zwischen beiden Schichten erfolgt im wesentlichen oberhalb der Bergkämme. Dieser vertikale Kammwind wird von unten durch den Hangwind ernährt. Im nächtlichen Fallwind wurden Geschwindigkeits-Variationen mit einer Periode von etwa 20 Minuten beobachtet.Wenn gut entwickelte Wind-Systeme in einem Tal vorkommen, kann man auch in anderen Tälern gut entwickelte Systeme erwarten.

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Résumé Des observations faites durant quatre étés dans la région du Mount Rainier ont montré la présence d'un système bien développé de brises de vallée et de montagne. Ce système a les particularités suivants: Le courant est dirigé vers l'amont durant la journée, vers l'aval durant la nuit. Ces courants sont compensés par un système de vents contraires à grande altitude. Le développement vertical des deux courants est à peu près identique et la surface qui les sépare est située, en général, à l'altitude des crêtes ou légèrement au-dessous. Le courant situé au-dessus du ven contraire est déterminé par la situation synoptique générale.La vitesse horizontale du vent est maximum pour les deux systèmes un peu au-dessous du centre de la couche correspondante. Les plus grandes vitesses se mesurent au début de l'après-midi et peu avent le lever du soleil. Le passage de la brise de vallée à la brise de montagne ou vice versa s'opère presque simultanément en tous les points de la vallée et cela approximativement une heure après le lever, respectivement le coucher du soleil.L'échange vertical des masses d'air entre les deux couches se fait principalement au-dessus des crêtes. Ce vent vertical de crêtes est alimenté d'en bas par le courant remontant les pentes. Dans le cas du vent nocturne descendant, on a observé des variations de vitesse ayant une périodicité de 20 minutes environ.Si l'on observe dans une vallée déterminée un système bien développé de brises de vallée et de montagne, on peut s'attendre à ce que des systèmes semblables se retrouvent également dans d'autres vallées de la même région.

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With 9 Figures

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Contribution No. 97, department of Atmospheric Sciences, University of Washington, Seattle, USA.

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This research was aided by the U.S. Air Force Cambridge Research Laboratories under AF Contract 19 (604)-7201, Project 7655, Task 7655.     

Bücher- und Zeitschriftenschau

Ohne Zusammenfassung     

Experiments with scale models of oil collectors for subsea well blowouts — Part II

A previous paper of the same title indicated the feasibility of the collection of oil by an open bottom collector above a blowout with a marine riser above the collector; the whole collection system being driven by gas lift from the blowout gas. That paper was based on small-scale laboratory experiments and it identified the salient dimensionless parameters governing those experiments. This paper describes laboratory experiments on a refinement of the collection system and also describes the results of intermediate scale experiments. The length scale of these experiments was about four times greater than laboratory scale and about one-fourth of full scale. Generally, the intermediate scale results are consistent with the laboratory predictions. Furthermore, two scale-dependent parameters have been identified. The effects of these have been included in an analysis of the results.     

Environmental responses to Lateglacial climatic fluctuations recorded in the sediments of pre‐Alpine Lake Mondsee (northeastern Alps)

Investigation of the sedimentary record of pre‐Alpine Lake Mondsee (Upper Austria) focused on the environmental reaction to rapid Lateglacial climatic changes. Results of this study reveal complex proxy responses that are variable in time and influenced by the long‐term evolution of the lake and its catchment. A new field sampling approach facilitated continuous and precisely controlled parallel sampling at decadal to sub‐annual resolution for µ‐XRF element scanning, carbon geochemistry, stable isotope measurements on ostracods, pollen analyses and large‐scale thin sections for microfacies analysis. The Holocene chronology is established through microscopic varve counting and supported by accelerator mass spectrometry ¹⁴C dating of terrestrial plant macrofossils, whereas the Lateglacial age model is based on δ¹⁸O wiggle matching with the Greenland NGRIP record, using the GICC05 chronology. Microfacies analysis enables the detection of subtle sedimentological changes, proving that depositional processes even in rather large lake systems are highly sensitive to climate forcing. Comparing periods of major warming at the onset of the Lateglacial and Holocene and of major cooling at the onset of the Younger Dryas reveals differences in proxy responses, reflecting threshold effects and ecosystem inertia. Temperature increase, vegetation recovery, decrease of detrital flux and intensification of biochemical calcite precipitation at the onset of the Holocene took place with only decadal leads and lags over a ca. 100 a period, whereas the spread of woodlands and the reduction of detrital flux lagged the warming at the onset of the Lateglacial Interstadial by ca. 500–750 a. Cooling at the onset of the Younger Dryas is reflected by the simultaneous reaction of δ¹⁸O and vegetation, but sedimentological changes (reduction of endogenic calcite content, increase in detrital flux) were delayed by about 150–300 a. Three short‐term Lateglacial cold intervals, corresponding to Greenland isotope substages GI‐1d, GI‐1c2 and GI‐1b, also show complex proxy responses that vary in time. Copyright © 2011 John Wiley & Sons, Ltd.     

Sources and distribution of organic matter in northern Patagonia fjords,Chile (∼44–47°S): A multi-tracer approach for carbon cycling assessment

We investigated the provenance of organic matter in the inner fjord area of northern Patagonia, Chile (～44–47°S), by studying the elemental (organic carbon, total nitrogen), isotopic (δ¹³C, δ¹⁵N), and biomarker (n-alkanoic acids from vascular plant waxes) composition of surface sediments as well as local marine and terrestrial organic matter. Average end-member values of N/C, δ¹³C, and δ¹⁵N from organic matter were 0.127±0.010, ?19.8±0.3‰, and 9.9±0.5‰ for autochthonous (marine) sources and 0.040±0.018, ?29.3±2.1‰, and 0.2±3.0‰ for allochthonous (terrestrial) sources. Using a mixing equation based on these two end-members, we calculated the relative contribution of marine and terrestrial organic carbon from the open ocean to the heads of fjords close to river outlets. The input of marine-derived organic carbon varied widely and accounted for 13–96% (average 61%) of the organic carbon pool of surface sediments. Integrated regional calculations for the inner fjord system of northern Patagonia covered in this study, which encompasses an area of ～4280 km², suggest that carbon accumulation may account for between 2.3 and 7.8×10⁴ ton C yr^?1. This represents a storage capacity of marine-derived carbon between 1.8 and 6.2×10⁴ ton yr^?1, which corresponds to an assimilation rate of CO₂ by marine photosynthesis between 0.06 and 0.23×10⁶ ton yr^?1. This rate suggests that the entire fjord system of Patagonia, which covers an area of ～240,000 km², may represent a potentially important region for the global burial of marine organic matter and the sequestration of atmospheric CO₂.     

Jurassic granitoid magmatism in the Dinaride Neotethys: geochronological constraints from detrital minerals

Three independent single‐grain geochronometers applied to detrital minerals from Central Dinaride sediments constrain the timing of felsic magmatism that associated the Jurassic evolution of the Neotethys. The Lower Cretaceous clastic wedge of the Bosnian Flysch, sourced from the Dinaride ophiolitic thrust complex, yields magmatic monazite and zircon grains with dominant age components of 164 ± 3 and 152 ± 10 Ma respectively. A unique tephra horizon within the Adriatic Carbonate Platform was dated at 148 ± 11 Ma by apatite fission track analysis. These consistent results suggest that leucocractic melt generation in the Central Dinaride segment of the Neotethys culminated in Middle to Late Jurassic times, coeval with and slightly post‐dating subophiolitic sole metamorphism. Growth of magmatic monazite and explosive volcanism call for supra‐subduction‐zone processes at the convergent Neotethyan margin. New compilation of geochronological data demonstrates that such Jurassic felsic rocks are widespread in the entire Dinaride–Hellenide orogen.