Seasonal variations of diffuse solar radiation at Ilorin (8°32′N,4°46′E), Nigeria

Hourly diffuse solar irradiance (H_d) and the corresponding global irradiance (H) falling on a horizontal surface at Ilorin (8°32N,4°46E), Nigeria has been measured for a period of fifteen months commencing from February, 1993. As expected, each monthly mean diurnal variation of H_d exhibits a mid-day maximum, while that of the ratio H_d/H exhibits a minimum. The month to month variations of these parameters are consequent on the dominant atmospheric conditions observed in the months concerned. The monthly average daily total of diffuse radiation (H_dm) was found to be highest in February, 1994 with a value of (3347 ± 45) Wm^–2day^–1, mainly due to the effects of Harmattan haze and thin clouds, while it was found to be lowest in November, 1993 and January, 1994 with a value of about 2500 Wm^–2day^–1. Similarly, the ratio of the monthly average daily total of diffuse radiation to the monthly average daily total of global radiation (H_dm/H_m) had the lowest value of 0.49 in the relatively clear sky month of November, 1993 and the highest value of 0.74 in the mainly cloudy month of August, 1993. On an annual average, the diffuse component constituted about 60% of the global solar radiation arriving on the ground at Ilorin, Nigeria primarily due to clouds and Harmattan haze which are seasonal, in addition to the constant background of molecular scattering.     

Telescopic investigation of relative spectral reflectivity of mare grounds of lunar surface

A study of the variation of the spectral relative ratios of reflectivity of selected mare lunar grounds between wavelengths 4000 and 8000 Å is given in comparison with lunar craters. The intensities at different wavelengths of each lunar region are corrected for the angles of illumination and viewing, and they are scaled to unity at =5538Å. Distinct variety in the spectral reflectivity values of mare grounds at short wavelengths are confirmed. The Mare Tranquillitatis type grounds (similar to Apollo-11 site), have relative ratio of reflectivity at short wavelength at =4035 Å; larger than or equal to 1.03 in addition to a bigger difference in reflectivity between the short and the long wavelength. The Mare Serenitatis type grounds (similar to Apollo-12) are characterized to give relative ratio of reflectivity less than 1.03 at =4035 Å, and smaller difference in reflectivity between short and long wavelengths. This is due to the variation in the colour of the Mare Tranquillitatis and Mare Serenitatis type ground due to compositional differences. The mare type grounds are generally different in shape than that of lunar craters grounds.Presented at the IAU-COSPAR Julian Schmidt Symposium on 100 Years of Lunar Mapping held at Lagonissi, Greece, 25–27 May, 1978.     

Exospheric perturbations by radiation pressure: II. Solution for orbits in the ecliptic plane

An earlier paper gave solutions for the mean time rates of change of orbital elements of satellite atoms in an exosphere influenced by solar radiation pressure. Each element was assumet to beahve independently. Here the instantaneous rates of change for three elements $\text{(e, ω,}\text{and}\text{θ = ω + Ω)}$ are integrated simultaneously for the case of the inclination i = 0. The results (a) confirm the validity of using mean rates when the orbits are tightly bound to the planet and (b) serve as examples to be reproduced by the complicated numerical solutions required for arbitrary inclination. Strongly bound hydrogen atoms perturbed in Earth orbit by radiation pressure do not seem a likely cause of the geotail extending in the anti-Sun direction. Instead, radiation pressure wil cause those particles' orbits to form a broad fan-shaped tail and to deteriorate into the Earth's atmosphere. Whether loosely bound H atoms are plentiful enough to create the geotail depends on their source function versusr; that question is beyond the scope of this paper.     

Complex refractive index of Martian dust: Wavelength dependence and composition

Mariner 9 ultraviolet spectra of the 1971 dust clouds were analyzed to obtain the phase function times single scattering albedo of the dust particles. The phase functions were matched with Mie scattering calculations for size distributions of spheres of homogeneous and isotropic material. The absorption index of the dust particles was found to increase with decreasing wavelenght from 350 nm down to about 210 nm, and drop off shortward of this wavelength. A structural shoulder occurs in the absorption spectrum between 240 and 250 nm. Titanium dioxide (anatase) has the correct transitions at 210 and 250 nm to match the absorption curve of Martian dust, and is proposed as a candidate constituent in Martian surface material. The spectral neutrality of TiO₂ between 0.5 and 4 μm is consistent with visible and infrared observations of Mars. The high refractive index of TiO₂ can explain the large refringence of Martian dust. The titanium dioxide content of the dust particles is estimated to be a few percent or less. Uncertainties in the results due to limitations in the model and data are discussed.     

Boundary-layer parameterizations for applied dispersion modeling over urban areas

Many applied dispersion models require the knowledge of boundary-layer parameters such as sensible heat flux,Q _H , friction velocity,u _*, and turbulent energy components, _w and _v . Formulas are suggested for calculating these parameters over a wide variety of types of ground surfaces, based on simple observations of wind speed near the ground and fractional cloud cover, and specification of constants such as roughness length, albedo, and soil moisture availability. Observations ofu _*,Q _H , _w , and _v during field experiments in St. Louis and Indianapolis are used to test the formulas for urban sites. Relative errors of about ±20% in the predictions are seen to occur whenu _*,Q _H , _w , and _v are large. However, when these quantities are small (e.g.,u _* < 0.2 m/s), the errors in the predictions are as large as the mean value of the quantity itself.In addition, it is concluded from studies of available field data and theories that the magnitude of _w is not well-known at elevations above about 100m during the late afternoon and night. Some simple parameterizations for _w . are suggested that are consistent with the observed steady decrease in ground-level concentration in the afternoon and the sudden increase in concentration that can occur a few hours after sunset due to wind shears associated with a low-level jet, for continuous plumes emitted from moderate to tall stacks.     

Chemical study of tectonically controlled hydrothermal dolomitization: an example from the Lessini mountains,Italy

In the Central Southern Alps (Feltre, Verona — Italy), a 750 m thick interval of Jurassic and Cretaceous pelagic limestones shows post-depositional partial brecciation and dolomitization. The overlying 500 m thick Tertiary sedimentary sequence is unaffected. Through the Paleogene, mostly submarine, mafic volcanism has been documented in the area. Small-scale extensional features were observed in the limestone near the contact with the dolomitized breccias. Their orientations measured in the field correspond to the tectonic framework of the area and give evidence for the contemporaneousness of the volcanic activity and the brecciation. The distribution and petrologic characteristics of the basalts, combined with the orientation of the extensional features observed in the field, allow a paleotectonic reconstruction. This tectonic scenario can be viewed as a back-arc extension, an eastward prolongation of the spreading that divided Southern France from the Sardinia-Corsica-Calabria block, generating the Ligurian-balearic basin in the Late Oligocene.The dolomite is fine-grained to sucrosic, with a microamygdaloidal porosity, partially filled with ankerite and calcite. The matrix shows a homogeneous, orange-red cathodoluminescence, indicating a single phase of iron-poor dolomite. The carbonate fraction consists of more than 90% dolomite. The dolomite is almost stoichiometric (Ca_0.6Mg_0.4 to Ca_0.5Mg_0.5). The ¹³C values of the dolomite are less than 1%. more negative than the unaffected limestone. The ¹⁸O values are between –5%. to –13%., with a depletion of 2–11%. relative to the undolomitized limestone. The depleted oxygen isotope ratios in the dolomitized rock can be derived either from fluids impoverished in the heavy isotopes (e.g. meteoric water) or high temperatures. The unvaried carbon isotopic ratios make the second interpretation the most acceptable. As the⁸⁷Sr/⁸⁶Sr values increase from a mean of 0.7077 in the unaffected limestones to 0.7085 in the dolomitized limestones, a derivation of the dolomitizing fluids from the volcanic rocks can be excluded. Comparing the obtained data with the Phanerozoic seawater isotope curve, however, the radiogenic Sr may be derived from marine waters of Late Oligocene-Early Miocene age. Microthermometric analyses of the fluid inclusions in the dolomite crystals from the bulk rocks and from the veins suggest a trapping temperature ranging from a minimum of 70°C (dolomite rock) to a maximum of 120°C (dolomite in veins). The solution contained in the inclusions is water with NaCl and MgCl₂ with salinities of 46%. (dolomite bulk rock) and 17%. (dolomite in veins). The pressure correction calculated from the fluid inclusion data is about 250 bars, which roughly correspond to the lithostatic pressure over the Mesozoic limestones in the Early Miocene.These results point to a hydrothermal origin of the dolomitization during the Late Oligocene-Early Miocene, as ascertained from the strontium isotope and fluid inclusion data. The circulation of hot marine water through the brecciated limestones in convective cells, triggered by the geothermal gradient related to the volcanic activity, is the proposed hydrodynamic model. Hydrologie considerations demonstrate that the proposed model is feasible.

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Zusammenfassung In den zentralen Südalpen (Feltre, Verona — Italien) findet sich eine etwa 750 m dicke Abfolge jurassischer und kretazischer pelagischer Kalke, die nach der Ablagerung zum Teil breckziert und dolomitisiert wurde, während die darüberliegenden 500 m mächtigen tertiären Sedimente keine Dolomitisierung zeigen. Im Paläogen ist im Gebiet ein mafischer, überwiegend mariner Vulkanismus dokumentiert. Kleinmaßstäbliche listrische Brüche in Kalken am Kontakt mit der dolomitisierten Breckzie entsprechen geometrisch einem großräumigen extensiven Regime im Paläogen. Sie beweisen die Gleichzeitigkeit der vulkanischen Aktivität und der Breckzierung. Die Verteilung und petrographischen Eigenschaften der Basalte, mit der Geometrie der Extensionsstrukturen, erlauben eine paläotektonische Rekonstruktion. Diese tektonische Situation entspricht einem Back-arc-basin und stellt die östliche Verlängerung des ligurisch-balearischen Beckens dar, das Südfrankreich vom Sardisch-Korsisch-Kalabrischen-Block im späten Oligozän getrennt hat.Die ¹³C Werte der Dolomite sind weniger als 1%. negativer als die entsprechender nicht dolomitisierter Kalke. Die ¹⁸O-Werte (relativ zum PDB Standard) variieren zwischen –5%. und –13%., das ist 2 bis 11%. negativer als die nicht dolomitisierter Kalke. Dies wird auf erhöhte Bildungstemperaturen zurückgeführt. Ein Anstieg der⁸⁷Sr/⁸⁶Sr-Signaturen im Mittel von 0.7077 in den nicht dolomitisierten Kalken auf 0.7085 in den dolomitisierten Kalken schließt eine Herkunft der dolomitisierenden Fluide von den vulkanischen Gesteinen aus. Beim Vergleich der Isotopensignaturen mit der phanerozoischen Meerwasser-Isotopenkurve, könnte aber das radiogene Strontium von spät oligozänem — früh miozänem Meerwasser kommen. Mikrothermometrische Analysen flüssiger Einschlüsse in Dolomitkristallen im Gestein und in Adern deutet auf eine Einschlußtemperatur von 70°C (Dolomitgestein) bzw. 120°C (Dolomit in Adern) hin. Die Lösung in den Einschlüssen ist Wasser mit NaCl und MgCl₂, mit einer Salinität von 46%. (Dolomitgestein) bzw. 17%. (Adern). Die aus den Einschlüssen berechnete Druckkorrektur ist etwa 250 bar. Dies entspricht ungefähr der früh miozänen Gesteinssäule über den mesozoischen Kalken.Aufgrund dieser Daten wird eine hydrothermale Bildung der Dolomite im späten Oligozän - frühen Miozän postuliert. Es wird ein hydrodynamisches Modell vorgeschlagen, in dem aufgeheiztes Meerwasser konvektiv durch die breckzierte mesozoische Abfolge zirkuliert. Als Motor wirkt ein vulkanischer geothermischer Gradient. Dieses Modell läßt sich mit hydrologischen Betrachtungen testen und stützen.

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Résumé Dans la partie sud des Alpes Centrales (Feltre, Verone: Italie) il existe une succession, épaisse de 750 m, de calcaires pélagiques jurassiques et crétacés, qui ont subi après leur sédimentation une bréchification et une dolomitisation partielles. Les sédiments tertiaires surincombants, épais de 500 m, ne sont pas affectés par ces phénomènes. Un volcanisme paléogène mafique, essentiellement sousmarin, a été reconnu dans la région. Dans les calcaires, au contact de la brèche dolomitisée, existent des cassures listriques de petite échelle dont la géométrie témoigne d'un régime extensif général au Paléogène. Leurs orientations, mesurées sur le terrain, indiquent la contemporanéité de l'activité volcanique et de la bréchification. La distribution et les caractères pétrologiques des basaltes, combinés à la géometrie des structures extensives, permet une reconstitution paléotectonique. Celle-ci montre une extension dans un bassin d'arrière-arc, prolongement oriental de l'expansion qui, à l'Oligocène supérieur, a séparé du sud de la France le bloc corsico-sardo-calabrais en créant le bassin liguro-baléare.La dolomie, finement grenue à saccharoïde, possède une porosité à vides micro-amygdaloïdes, partiellement occupés par de l'ankérite et de la calcite. La matrice présente une cathodoluminescence homogène rouge-orange, indiquant la présence d'une seule phase constituée de dolomite pauvre en Fe. La fraction carbonatée consiste en dolomite pour plus de 90%. Cette dolomite est à peu près stoechiométrique (Ca_0,6Mg_0,4 à Ca_0,5Mg_0,5). Les rapports ¹³C de la dolomie sont inférieurs de moins de 1%. à ceux du calcaire intact. Les rapports ¹⁸O sont compris entre –5%. et –13%., soit 2 à 11%. inférieurs à ceux du calcaire non dolomitisé. Cette baisse du rapport isotopique peut provenir soit de fluides appauvris en isotopes lourds (p. ex. l'eau météorique), soit d'une température élevée; la constance des rapports isotopiques du C rend cette deuxième explication la plus plausible. Le rapport⁸⁷Sr/⁸⁶Sr passe d'une valeur moyenne de 0,7077 dans les calcaires non affectés à 0,7085 dans les calcaires dolomitisés; cet accroissement exclut une origine volcanique pour les fluides dolomitisants. En comparant ces valeurs à la courbe isotopique du Sr de l'eau de mer au Phanérozoïque, on peut déduire que le Sr radiogénique est dérivé d'eaux marines d'âge oligocène tardif à miocène inférieur. L'analyse microthermométrique des inclusions fluides contenues dans les cristaux de dolomite suggère une température de formation qui va de 70°C (dans la roche) à 120° (dans les veines). Le contenu de ces inclusions est une solution aqueuse de NaCl et MgCl₂ avec une salinité de 44%. (dans la roche) et de 17%. (dans les veines). La correction de pression calculée à partir des inclusions fluides est d'environ 250 bars, ce qui correspond grosso modo à la pression lithostatique qui s'exerçait au Miocène inférieur sur les calcaires mésozoïques.Sur la base de ces données, on conclut à une origine hydrothermale de la dolomie au cours de l'Oligocène supérieur - Miocène inférieur. Le modèle hydrodynamique proposé fait appel à la circulation convective, à travers le calcaire bréchié, d'eau marine échauffée grâce au gradient géothermique élevé dû à l'activité volcanique. Ce modèle est en accord avec des considérations hydrologiques.

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(, — ) , 750 , , , , 500 , . , . , . , . . - , - . ¹³ , 1%. ¹⁸, PDB –5 –13%, .. 2 11% . , , . ⁸⁷Sr/⁸⁶Sr 0.7077 0,7085 . , - . 70° , 120° . , , 44%, 17%. , , 250 . - . , - . , . , . .

     

Basement-controlled faulting of Paleozoic strata in southern Ontario, Canada: new evidence from geophysical lineament mapping

Basement fault reactivation is now recognized as an important control on sedimentation and fault propagation in intracratonic basins. In southern Ontario, the basement consists of complexly structured mid-Proterozoic (ca. 1.2 Ga) crystalline rocks and metasedimentary rocks that are overlain by up to 1500 m of Paleozoic sedimentary strata. Reactivation of basement structures is suspected to control the location of Paleozoic fault and fracture systems, but evaluation has been hindered by a limited understanding of the regional structural characteristics of the buried basement. New aeromagnetic- and gravimetric-lineament mapping presented in this paper better resolves the location of basement discontinuities and provides further evidence for basement controls on the distribution of Paleozoic fault and fracture systems. Lineament mapping was facilitated by reprocessing and digital image enhancement (micro-levelling, regional residual separation, derivative filtering) of existing regional gravity and aeromagnetic datasets. Reprocessed images identify new details of the structural fabric of the basement below southern Ontario and delineate several previously unrecognized aeromagnetic and gravity lineaments and linear zones. Linear zones parallel the projected trends of mid-Proterozoic terrane boundaries identified by field mapping on the exposed shield to the north of the study area, and are interpreted as zones of shearing and basement faulting. Mapped aeromagnetic and gravity lineaments show similar trends to Paleozoic faults and fracture networks and broad zones of seismicity in southern Ontario. These new data support an ‘inheritance model’ for Paleozoic faulting, involving repeated reactivation and upward propagation of basement faults and fractures into overlying cover strata.     

The chemistry of lava-seawater interactions II: the elemental signature

The flow of lava into the ocean at the shoreline of Kilauea Volcano during the ongoing Pu’u O’o eruption has allowed a detailed study of the geochemical interaction between lava and seawater. This paper focuses on the chemistry of the major and minor elements in the fluids that resulted from this interaction. The elemental enrichments in these fluids are dominated by three processes: (1) evaporation of water from seawater, which creates solutions enriched in the major elements found in seawater, (2) congruent dissolution of the basalt glass matrix, which is limited by the solubility of some of the elements in seawater, and (3) removal of volatile phases from the lava on contact with seawater.Using a simple model of volatile emanation (using published emanation coefficients) and congruent dissolution, we are able to explain the concentrations observed for the majority of elements in precipitation from the steam plume at the shoreline lava entry and in water allowed to interact with molten lava in controlled experiments. Fe, Al, Ti, and some of the rare earth elements (REEs) in precipitation samples from the steam plume at the lava entry were > 10,000-times enriched over their ambient seawater concentrations, suggesting that these elements may be useful for identifying submarine eruptions. The flux of elements from the Kilauea ocean lava entry is greater than that from a typical midocean ridge hydrothermal vent field for Al, Cd, Co, and the REEs, whereas the opposite is true for the remainder of the elements studied.     

Determining the trophic guilds of fishes and macroinvertebrates in a seagrass food web

We established trophic guilds of macroinvertebrate and fish taxa using correspondence analysis and a hierarchical clustering strategy for a seagrass food web in winter in the northeastern Gulf of Mexico. To create the diet matrix, we characterized the trophic linkages of macroinvertebrate and fish taxa present inHalodule wrightii seagrass habitat areas within the St. Marks National Wildlife Refuge (Florida) using binary data, combining dietary links obtained from relevant literature for macroinvertebrates with stomach analysis of common fishes collected during January and February of 1994. Heirarchical average-linkage cluster analysis of the 73 taxa of fishes and macroinvertebrates in the diet matrix yielded 14 clusters with diet similarity ≥ 0.60. We then used correspondence analysis with three factors to jointly plot the coordinates of the consumers (identified by cluster membership) and of the 33 food sources. Correspondence analysis served as a visualization tool for assigning each taxon to one of eight trophic guilds: herbivores, detritivores, suspension feeders, omnivores, molluscivores, meiobenthos consumers, macrobenthos consumers and piscivores. These trophic groups, corss-classified with major taxonomic groups, were further used to develop consumer compartments in a network analysis model of carbon flow in this seagrass ecosystem. The method presented here should greatly improve the development of future network models of food webs by providing an objective procedure for aggregating trophic groups.