Redistriution of Major Elements in the Alteration of Some Basic Lavas during Burial Metamorphism

An Ordovician geanticlinal marine sequence is exposed in theCentral West of New South Wales, Australia. The sequence containingbasic lavas, labile sedimentary, and proclastic rocks, has undergoneextensive adjustment during regional burial metamorphism. Thebasic lavas have a patchy coloration due to the formation ofalternation minerals of the prehnite-pumpellyite facies whichapperar to have formed during the metamorphism. The hererogeneousappearance of the basic lavas reflects a pronouced chemicaland mineralogical departure from the original composition. Twodiverging trends result. One leads to the production of a Ca-enrichedlithology, the other, which by far dominates in area at eachouterop, leads to a ‘spilitic’ lithology. The alterationdomains in many cases cross–cut all primary textural featureand their chemical variation does not correspond to likely variationsin the original lava composition.     

THE COMPUTATION OF SINGLE STRIPS IN PLAN

This paper discusses a simple method of computing independent strips under certain reasonable approximations. It is shown that, if the method is regarded as if it were computation by polynomials, the order of the polynomial is decided by the nature of the control provided and not by the number of controlled models. This conclusion should throw some light on the vexed (and perennial) problem of the choice of orders for polynomials.     

Variations in exospheric density at heights near 1100km, derived from satellite orbits

In an earlier paper, values of exospheric density were obtained from the orbit of Echo 2 for the years 1964–1965. The results indicated a semi-annual variation in density by a factor of between 2 and 3, considerably larger than predicted by existing atmospheric models.

These studies have now been extended to the beginning of 1967, using both Echo 2 and Calsphere 1, to show how the density is responding to increasing solar activity. Variations in density during 1964 have been analysed in more detail. The long-term variation associated with the solar cycle and the short-term variations associated with magnetic and solar disturbances agree with the variations expected on the basis of current models. The semi-annual variation is persisting to higher levels of solar activity, and although its amplitude is diminishing the factor of variation was still 1.6 in 1966.     

Measurements of radio noise at 0.700 mc and 2.200 mc from a high-altitude rocket probe

Radio noise observations at frequencies of 0·700 Mc and 2·200 Mc were made at altitudes between 3000 and 11,000 km from a Blue Scout Jr. high-altitude rocket probe on 30 July 1963. A steady background flux of (7·5₋₃⁺⁶) × 10⁻¹⁹ W m⁻²)(c/s)⁻¹ at 0·700 Mc and (1·8^+1.0_−0.5 × 10⁻¹⁹ W m⁻² (c/s)⁻¹ at 2·200 Mc was observed. Assuming a galactic origin of the observed fluxes at both frequencies, the averaged sky brightnesses are b(0·700 Mc) = (6₋₃⁺⁵) × 10⁻²⁰ W m⁻² (c/s)⁻¹ sr⁻¹b(2·200 Mc) = (1.4^+1.0_−0.5 × 10⁻²⁰ W m⁻² (c/s)⁻¹ sr⁻¹ The observed brightness at 2·200 Mc is in reasonable agreement with the results of other observers. The apparent brightness at 0·700 Mc is, however, greater than was expected from previous observations. An alternative source of the 0·700 Mc flux in the terrestrial exosphere, as well as characteristics of several noise bursts observed during the flight, is briefly discussed.     

Equivalent thickness of the outer ionosphere obtained by evaluation of Faraday records

With an appropriate system of higher order approximations the Faraday-effect is calculated for instantaneous ionospheric models the data of which are derived from the results of vertical soundings. Only one parameter which corresponds to the thickness of the outer ionosphere is left open; it is determined by global comparison with simultaneous Faraday-observations of satellite emissions. The thickness parameter shows various forms of variation with latitude; an increase towards north is the rule for quiet daytime conditions. Comparison with local methods shows considerable differences due to the indetermination of the absolute number of rotations.     

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