On the evaluation of natural illumination from radiometric measurements of solar radiation

Summary A new method is described for deriving values of the natural illumination of direct solar radiation from measurements of the latter, integrally with regard to wavelength and, simultaneously, in well-defined spectral regions. The basic equations are presented and graphical comparisons between data so computed and observed analyzed. The degree of prediction of individual short-period values of direct illumination flux (e. g. half-hourly intervals), established for wide ranges of solar height and turbidity, is of the same order as the accuracy generally expected in such series of carefully conducted measurement programs. This technique of employing radiometric rather than photometric measurements is thus shown to have a general application.

---

Zusammenfassung Es wird eine neue Methode zur Berechnung von Werten der natürlichen Beleuchtungsst?rke durch die direkte Sonnenstrahlung aus Messungen der letzteren abgeleitet, und zwar gleichzeitig für das gesamte Spektrum und für genau abgegrenzte Spektralbereiche. Es werden die Grundgleichungen angegeben und graphische Vergleiche zwischen den so berechneten und den beobachteten Werten durchgeführt. Einzelwerte des direkten Lichtstromes über kurze Zeiten (z. B. Halbstundenintervalle), die für gro?e Bereiche von Sonnenh?he und Trübung berechnet wurden, haben denselben Genauigkeitsgrad, wie man ihn bei sorgf?ltig ausgeführten Me?programmen gew?hnlich erwartet. Damit ist erwiesen, da? die Methode, Strahlungsmessungen statt Lichtmessungen zu verwenden, allgemein angewendet werden kann.

---

Résumé Les auteurs exposent ici une nouvelle méthode permettant de calculer l'intensité lumineuse naturelle du rayonnement solaire direct au moyen de la mesure de ce dernier. Cette méthode permet le calcul aussi bien pour la totalité du spectre que pour certaines bandes délimitées. Les auteurs indiquent les équations de base et donnent des comparaisons graphiques entre des valeurs observeés et calculées de cette manière. Les valeurs isolées du flux lumineux direct regu en des laps de temps brefs (par exemple dúne demie-heure), valeurs calculées pour de grands intervalles aussi bien de la hauteur du soleil que du trouble atmosphérique, donnent le même degré déxactitude que celui quón peut attendre de mesures directés effectées soigneusement. On a ainsi démontré que la méthode qui consiste à utiliser des mesures du rayonnement au lieu de la luminosité peut être utilisée de fa?on trés g&&ale.

---

---

With 3 Figures

---

Dedicated to Dr.W. M?rikofer on the occasion of his 70th birthday.     

Clastic sediments associated with radiolarites (Tauglboden—Schichten, Upper Jurassic, Eastern Alps)

During the early Upper Jurassic, widespread deep-sea radiolarites were deposited in most parts of the Northern Limestone Alps. In the formation described (Tauglboden-Schichten), these pelagic sediments interfinger with local-source clastic material. Depending on the topography and the kind of material, either slides and slumps, mudflows, grain flows or turbidity currents operated and formed slump-folded beds, mud-flow breccias, fluxoturbidites or turbidites. A breccia had been traced over an area of 20 km². Its variation is described in terms of lithological columns, bed thicknesses, maximum grain sizes and grain orientations. It forms a tongue-shaped body, which was probably a part of a submarine fan. The fluxoturbidites of the proximal area grade distally on three sides into turbidites within 3–5 km. The clastic material consists of marls and limestones of Rhaetian and Jurassic age. It was probably derived from a tectonically uplifted palaeo-high by an interplay of tectonics and gravity. The clastics were deposited on submarine fans bordering this high. In its lithology the formation closely resembles certain marginal facies of flysch troughs.     

From Discrete Gravity Survey Data to a High-resolution Gravity Field Representation in the Nordic-Baltic Region

The deduction of a regularly spaced gravity anomaly grid from scattered survey data is studied, addressing mainly two aspects: reduction of gravity to anomalies and subsequent interpolation by various methods. The problem is illustrated in a heterogeneous study area and contrasting test areas including mountains, low terrains, and a marine area. Provided with realistic error estimates, Least Squares Collocation interpolation of Residual Terrain Model anomalies yields the highest quality gravity grid. In most cases, the Bouguer reduction and other interpolation methods tested are equally viable. However, spline-based interpolation should be avoided in marine areas with trackwise survey data.     

A low-scattering approximation for the hydrodynamic interactions of small wave-power devices

This paper concerns mathematical modelling of the hydrodynamic interaction forces between small vertically axisymmetric wave-power devices. The model takes into account small-body approximations for the first order scattered waves but neglects multiple scattering. Further, the local wave fields are neglected, making the model inapplicable for very closely spaced bodies.The model, which is called the low-scattering approximation, comprises analytical formulae for the forces in any of the translation modes surge, sway and heave. It requires, however, that the following isolated-body parameters are known or externally supplied: the added mass and the force coefficients for both heave and surge motion.Comparison with accurate numerical results of a two-buoy system indicates that the present approach is fairly good even when the buoy diameter is as large as 1/6 of the wavelength and the buoy spacing is as small as 5 buoy radii.     

Methane-derived high-Mg calcite submarine cement in Holocene nodules from the Fraser Delta, British Columbia, Canada

Carbonate nodules and slabs in late Holocene shelly terrigenous deposits of the modern Fraser River delta (～49°N) are formed close to the seafloor by precipitation from saline pore waters of mainly fibrous to bladed crystals of high-Mg (～ 10–20 mol% MgCO₃) calcite cement as coalescing isopachous crusts on grains. Previous reports that the cement is low-Mg calcite are not supported by this study. Highly negative δ¹³C values of ? 7 to ? 59‰ for the cements indicate that the bulk of their carbonate carbon was derived from the microbiological degradation of organic matter in the deltaic deposits during shallow burial. In particular, the production of biogenic methane (CH₄) by anaerobic bacterial fermentation, its upward migration, chemical or biological oxidation to CO₂ and neutralization in the near-surface sediment, and diffusion to microenvironments relatively enriched in organic components, are a possible set of conditions influencing the process and sites of carbonate cementation. Methane-derived Mg-calcite appears also to be the major submarine cement in several other modern occurrences of lithified shallow-water terrigenous sands and muds at non-tropical latitudes.     

TEMPERATURE EFFECT ON PRECIPITATION OF CALCIUM CARBONATE FROM CALCIUM BICARBONATE SOLUTIONS AND ITS APPLICATION TO CAVERN ENVIRONMENTS

Solutions of calcium bicarbonate were allowed to lose carbon dioxide and evaporate to dryness under controlled temperature conditions. With filtered solutions prepared from spar calcite, precipitates were 100% calcite in the 2° to 100°C temperature range. When, in analogous experiments, coralline aragonite was the starting material, the precipitates were 100% calcite. Essentially the same was true when carbonate rocks from karst areas were used to prepare the experimental solutions. An artificially prepared mixture (maximum crystal size of about 7 u) of 70% aragonite and 30% calcite was also used in the study. The precipitates from this starting material were apparently affected by seed nuclei which passed through the filter. The stability of calcium carbonate seed nuclei appears to vary with temperature. Natural calcium bicarbonate solutions from caves yielded only calcite at 25°C. Calcite should be the dominant or only polymorph of CaCO₃ formed by the loss of carbon dioxide and evaporation of natural calcium bicarbonate solutions if temperature is the controlling factor. Since appreciable amounts of aragonite are found in many cave deposits, factors other than temperature must influence the polymorphs formed. POBEGUIN (1955) proposed that rapid evaporation and slow diffusion of solutions favor aragonite. If so, layers of aragonite and calcite in speleothems may reprsent alternate wet and dry paleoclimates. During these periods, rate of introduction of solution and rate of evaporation would change markedly.     

OPERATION IRAQI FREEDOM: A MILITARY GEOGRAPHICAL PERSPECTIVE*

ABSTRACT. The war in Iraq has spanned the full spectrum of military operations: intense combat, stability‐and‐support operations, and peacetime activities. Regardless of their nature and relative intensity, military operations are shaped by the characteristics of the military operating environment. Consequently, the scale, tempo, and complexity of any type of military endeavor are linked to the physical and cultural landscapes of the region in which it is conducted. Military geographers use geographical information, tools, and techniques to examine those links. Iraq's operating environment is studied to identify the relevant components of its physical and human geography. This military geographical examination of Iraq tells us a great deal about how the physical and cultural environment have influenced the war, as well as how the complexity of its human landscape continues to affect the postwar rebuilding of the country.     

Optical and magnetic pulsations

Based on data from the PULSAUR-rocket (1980) and ground observations, a correlation study between optical and magnetic pulsations has been carried out. By use of All-Sky TV along with the measured flux of electrons we have also simulated the ground magnetic field. The simulation is based on a model of pulsating currents caused by conductivity changes in the ionosphere. Our simulated field well represents the observed field. The time delay between the optical and magnetic signal is discussed in relation to our model, and so is the lack of correlation between the high frequency component of the two types of pulsations.