Contemporary methods for retrieving the integrated atmospheric water-vapor content and the total cloud liquid-water content

A review of contemporary methods for determining integrated parameters of the water content in the atmosphere―atmospheric water-vapor content and cloud liquid-water content―is presented. Fields of these parameters can only be mapped spatially on the basis of using data of satellite measurements. The least errors of the retrieval of atmospheric water-vapor content and cloud liquid-water content is provided by methods based on using measurements of the satellite-borne scanning multichannel microwave radiometers over the ice-free ocean areas in the absence of precipitation. Most methods for retrieving the atmospheric water-vapor content and cloud liquid-water content from the data of microwave radiometers are based on results of numerical simulation of brightness temperatures of the upwelling microwave radiation of the ocean–atmosphere system. The evolution of satellite-borne microwave radiometers and methods for the retrieval of integrated parameters of water content is presented.     

Geomechanical modelling to assess fault integrity at the CO2CRC Otway Project,Australia

This paper presents the first published 3D geomechanical modelling study of the CO2CRC Otway Project, located in the state of Victoria, Australia. The results of this work contribute to one of the main objectives of the CO2CRC, which is to demonstrate the feasibility of CO₂ storage in a depleted gas reservoir. With this aim in mind, a one-way coupled flow and geomechanics model is presented, with the capability of predicting changes to the in situ stress field caused by changes in reservoir pressure owing to CO₂ production and injection. A parametric study investigating the pore pressures required to reactivate key, reservoir-bounding faults has been conducted, and the results from the numerical simulation and analytical analysis are compared. The numerical simulation indicates that the critical pore fluid pressure to cause fault reactivation is 1.15 times the original pressure as opposed to 1.5 times for the comparable analytical model. Possible reasons for the differences between the numerical and analytical models can be ascribed to the higher degree of complexity incorporated in the numerical model. Heterogeneity in terms of lateral variations of hydrological and mechanical parameters, effect of topography, presence of faults and interaction between cells are considered to be the main sources for the different estimation of critical pore pressure. The numerical model, which incorporates this greater complexity, is able then to better describe the state of stress that acts in the subsurface compared with a simple 1D analytical model. Moreover, the reactivation pressures depend mainly on the state of stress described; therefore we suggest that numerical models be performed when possible.     

Refractory metal nuggets within presolar graphite: First condensates from a circumstellar environment

Transmission electron microscope (TEM) investigations have revealed Os, Ru, Mo‐rich refractory metal nuggets within four different presolar graphites, from both the high‐density (HD) Murchison (MUR) and low‐density (LD) Orgueil (ORG) fractions. Microstructural and chemical data suggest that these are direct condensates from the gas, rather than forming later by exsolution. The presolar refractory metal nugget (pRMN) compositions are variable (e.g., from 8 < Os atom% < 77), but follow the same chemical fractionation trends as isolated refractory metal nuggets (mRMNs) previously found in meteorites (Berg et al. 2009). From these compositions one can infer a temperature of last equilibration with the gas of 1405–1810 K (e.g., Berg et al. 2009 at approximately 100 dyne cm^?2 pressure), which implies that the host graphites form over roughly the same range (in agreement with predictions) and that the pRMNs are chemically isolated from the gas when captured by graphite. Further, the pRMN compositions give evidence that HD graphites form at a higher T than LD ones. Chemical and phase similarities with the isolated mRMNs suggest that the mRMNs also condense directly from a gas, although from the early solar nebula rather than a presolar environment. Although the pRMNs themselves are too small for detection of isotopic anomalies, NanoSIMS isotopic measurements of their host graphites confirm a presolar origin for the assemblages. The two pRMN‐containing LD graphites show evidence of a supernova (SN) origin, whereas the stellar origins of the pRMNs in HD graphite are unclear, because only less‐diagnostic ¹²C enrichments are detectable (as is commonly true for HD graphites).     

The Darwin Rise demise: the western Pacific guyot heights trace the trans-Pacific Mendocino fracture zone

The Darwin Rise has been proposed so many times and in so many forms and places that the time has come to make a more comprehensive examination of the region. Lying on the NW Pacific Plate between the Geisha Guyots, the Mid-Pacific Mountains, the equator, and the trenches, the region is roughly bounded by magnetic anomaly M20 (147 Ma). It was subjected to a massive outpouring of lava about 105 to 120 Ma, which created the guyots and seamounts in that region. Guyots are excellent tools for studying events of long ago because they eroded in the same lowstand in the Cretaceous and guyot relief, therefore, is a surrogate for paleo-sealevel. The relief is derived by subtracting the break depth of the summit plateau of a guyot from the regional depth. Guyot relief would necessarily be less in the center than to the periphery if the feature formed on a pre-existing rise, as has been postulated. The existence of a paleo-Darwin Rise would give concentric contours for the region in question. Of the sixty guyots used in this study, thirty-seven of these guyots were surveyed using SASS multibeam in the Marcus-Wake seamount group. Twenty-three guyots were surveyed using random track single-beam sonar surveys. An entirely different scenario is shown. Data revealed a major fracture passing through the area coevally or after the guyots formed. Because the depths to the summit are not the same now, vertical tectonics occurred after subaerial erosion. This means the fracture formed during and after the erosion (roughly 105 Ma) and influenced the normal sequence of events in guyot formation. Depending on how one deciphers trends through the Hess Rise morass, SASS bathymetry shows a continuation of the Surveyor/Mendocino fracture zone swarm inside the M20 region to the NE of these data. The fracture swarm continues to the western Pacific trench system. Based on this information, if the Darwin Rise ever existed, it had to have done so elsewhere.     

Klimatologische Untersuchung über die geographische Verteilung der Globalstrahlung und der diffusen Himmelsstrahlung

Zusammenfassung Die vorliegende strahlungsklimatologische Studie verfolgt den Zweck, ausschließlich auf Grund von Meßergebnissen anhand ausgewählter Beispiele gegensätzlicher Großaumklimate zunächst die typischen Eigenschaften des Jahresganges der Globalstrahlung (T) und der diffusen Himmelsstrahlung (D) zu untersuchen. In Ergänzung hierzu werden häufigkeitsstatistische Betrachtungen über die Eigenheiten im Verhalten dieser Strahlungselemente im Bereich verschieden beschaffener geographischer Räume angestellt. Dabei zeigt sich, daß neben dem jahreszeitlichen Ablauf auch die Häufigkeitsverteilungen vonT undD sich zur Klimatypisierung heranziehen lassen. Ein besonderes Interesse beansprucht der jahreszeitliche Verlauf des VerhältnissesD/T in den Hauptklimazonen der Erde. Ferner wird die Breitenabhängigkeit der Globalstrahlung (T), der diffusen Himmelsstrahlung (D) und des VerhältnissesD/T behandelt. Hinsichtlich der Höhenabhängigkeit ergibt sich auf Grund des Verhaltens vonT undD für die gemäßigten Breiten eine Abnahme des QuotientenD/T. Den Abschluß bilden strahlungsklimatologische Überlegungen zur Frage der Abhängigkeit des VerhältnissesD/T von der Sonnenscheindauer im Bereich charakteristischer Klimazonen der Erde.

---

Summary The present study of radiation climatology, exclusively basing on results of measurements, presents selected examples of contrary large-scale climatic conditions and examines the typical features of the annual variation of global radiation (T) and diffuse sky radiation (D). Supplementary considerations on frequency statistics refer to the peculiarities in the behaviour of these two radiation elements in different geographical areas. It results that beside the seasonal variation frequency distributions ofT andD can be used for a characterization of radiation climates. The seasonal variation of the characteristic ratioD/T in the main climatic zones of the earth is of particular interest. Furthermore, the latitudinal dependency of global radiation (T), diffuse sky radiation (D) and of the ratioD/T is discussed. As to the dependence on altitude the ratioD/T shows a decrease in temperate latitudes on account of the behaviour ofD andT. Finally climatological reflections on the dependence of the ratioD/T on the duration of sunshine in characteristic climatic regions of the earth are discussed.

---

Résumé La présente étude de la climatologie du rayonnement a pour but de déterminer les propriétés typiques de l'évolution annuelle du rayonnement global (T) et du rayonnement diffus du ciel (D) et cela exclusivement sur la base de mesures faites et d'exemples choisis parmi des climats très différenciés. En complément, on prend en considération des statistiques de la fréquence des particularités de ces deux éléments à l'intérieur d'aires géographiques de climats divers. On en déduit que, à côté de l'évolution annuelle, la répartition des fréquences deT et deD permettent d'établir le type du climat. L'évolution saisonnière du rapportD/T est tout spécialement intéressant dans les principales zones climatiques de la terre. On considère ensuite la dépendance du rayonnement global (T), du rayonnement diffus du ciel (D) et du rapportD/T de la latitude du lieu. Dans les zones tempérées, le quotientD/T diminue avec l'altitude. L'auteur termine par des réflexions concernant la climatologie du rayonnement en relation avec la dépendance du rapportD/T de la durée d'insolation dans des zones climatiques caractéristiques de notre planète.

---

---

Mit 12 Textabbildungen     

A Nd- and O-isotope study of the REE-rich peralkaline Strange Lake granite: implications for Mesoproterozoic A-type magmatism in the Core Zone (NE-Canada)

It is well established that A-type granites enriched in high field strength elements, such as Zr, Nb and the REE, form in anorogenic tectonic settings. The sources of these elements and the processes controlling their unusual enrichment, however, are still debated. They are addressed here using neodymium and oxygen isotope analyses of samples from the 1.24 Ga Strange Lake pluton in the Paleoproterozoic Core Zone of Québec-Labrador, an A-type granitic body characterized by hyper-enrichment in the REE, Zr, and Nb. Age-corrected εNd values for bulk rock samples and sodic amphiboles (mainly arfvedsonite) from the pluton range from ?0.6 to ?5.7, and ?0.3 to ?5.3, respectively. The εNd values for the Napeu Kainiut quartz monzonite, which hosts the pluton, range from ?4.8 to ?8.1. The ¹⁴⁷Sm/¹⁴⁴Nd ratios of the suite and the host quartz monzonite range from 0.0967 to 0.1659, large variations that can be explained by in situ fractionation of early LREE-minerals (Strange Lake), and late hydrothermal HREE remobilization. Oxygen isotope analyses of quartz of both Strange Lake and the host yielded δ¹⁸O values between +8.2 and +9.1, which are considerably higher than the mantle value of 5.7 ± 0.2‰. Bulk rock oxygen isotope analyses of biotite-gneisses in the vicinity of the Strange Lake pluton yielded δ¹⁸O values of 6.3, 8.6 and 9.6‰. The negative εNd values and positive δ¹⁸O values of the Strange Lake and Napeu Kainiut samples indicate that both magmas experienced considerable crustal contamination. The extent of this contamination was estimated, assuming that the contaminants were sedimentary-derived rocks from the underlying Archean Mistinibi (para-) gneiss complex, which is characterized by low εNd and high δ¹⁸O values. Mixing of 5–15% of a gneiss, having an εNd value of ?15 and a δ¹⁸O value of +11, with a moderately enriched mantle source (εNd = +0.9, δ¹⁸O = +6.3) would produce values similar to those obtained for the Strange Lake granites. Based on analogies between the Nain Plutonic Suite and the Gardar alkaline igneous province (SW-Greenland), we conclude that the Strange Lake pluton and associated REE-mineralized anorogenic bodies formed from a combination of subduction-induced fertilization of the sublithospheric mantle, crustal extension and in situ magma evolution.     

On the transport of small river run off by an alongshore baroclinic sea current

A numerical simulation has been undertaken to study the process of the transport of small river runoff by alongshore baroclinic sea currents. The study is based on the implementation of the Princeton Ocean Model (POM) under the conditions of a circular stratified basin whose surface is exposed to a transient tangential wind stress to form an alongshore baroclinic current. A baroclinic current of the downwelling type (in the Northern Hemisphere directed to the left to a sea-viewing observer) was shown to provide the carrying out of the river discharge from estuary’s vicinity more effectively than that of the upwelling type (in the Northern Hemisphere directed to the right to a sea-viewing observer).     

Main results of recent investigations into the physical mechanisms of the interaction of tropical cyclones and the ionosphere

Izvestiya, Atmospheric and Oceanic Physics - International investigations into the correlation between tropical cyclones (TCs) and the ionosphere are associated with great difficulties in proving...     

The multiple chronological techniques applied to the Lake Suigetsu SG06 sediment core,central Japan

The varved sediment of Lake Suigetsu (central Japan) provides a valuable opportunity to obtain high‐resolution, multi‐proxy palaeoenvironmental data across the last glacial/interglacial cycle. In order to maximize the potential of this archive, a well‐constrained chronology is required. This paper outlines the multiple geochronological techniques being applied – namely varve counting, radiocarbon dating, tephrochronology (including argon–argon dating) and optically stimulated luminescence (OSL) – and the approaches by which these techniques are being integrated to form a single, coherent, robust chronology. Importantly, we also describe here the linkage of the floating Lake Suigetsu (SG06) varve chronology and the absolute (IntCal09 tree‐ring) time scale, as derived using radiocarbon data from the uppermost (non‐varved) portion of the core. This tie‐point, defined as a distinct (flood) marker horizon in SG06 (event layer B‐07–08 at 1397.4 cm composite depth), is thus derived to be 11 255 to 11 222 IntCal09 cal. years BP (68.2% probability range).