Comparative Study of the Three-Dimensional Thermodynamical Structure of the Inner Corona of Solar Minimum Carrington Rotations 1915 and 2081

Using differential emission measure tomography (DEMT) based on time series of EUV images, we carry out a quantitative comparative analysis of the three-dimensional (3D) structure of the electron density and temperature of the inner corona (\(r<1.25\,\mathrm{R}_{\odot}\)) between two specific rotations selected from the last two solar minima, namely Carrington Rotations (CR)1915 and CR-2081. The analysis places error bars on the results because of the systematic uncertainty of the sources. While the results for CR-2081 are characterized by a remarkable north–south symmetry, the southern hemisphere for CR-1915 exhibits higher densities and temperatures than the northern hemisphere. The core region of the streamer belt in both rotations is found to be populated by structures whose temperature decreases with height (called “down loops” in our previous articles). They are characterized by plasma \(\beta\gtrsim1\), and may be the result of the efficient dissipation of Alfvén waves at low coronal heights. The comparative analysis reveals that the low latitudes of the equatorial streamer belt of CR-1915 exhibit higher densities than for CR-2081. This cannot be explained by the systematic uncertainties. In addition, the southern hemisphere of the streamer belt of CR-1915 is characterized by higher temperatures and density scale heights than for CR-2081. On the other hand, the coronal hole region of CR-1915 shows lower temperatures than for CR-2081. The reported differences are in the range \({\approx}\,10\,\mbox{--}\,25\%\), depending on the specific physical quantity and region that is compared, as fully detailed in the analysis. For other regions and/or physical quantities, the uncertainties do not allow assessing the thermodynamical differences between the two rotations. Future investigation will involve a DEMT analysis of other Carrington rotations selected from both epochs, and also a comparison of their tomographic reconstructions with magnetohydrodynamical simulations of the inner corona.     

Balancing deformation in NW Borneo: Quantifying plate-scale vs. gravitational tectonics in a delta and deepwater fold-thrust belt system

Recent GPS measurements demonstrate that NW Borneo undergoes 4–6 mm of plate-scale shortening a year, which is not accommodated by plate-scale structures. The only geological structure in NW Borneo described to accommodate on-going shortening is the Baram Delta System located on the outer shelf to basin floor. Delta toe fold-thrust belts are commonly thought to be caused by margin-normal compressional stresses generated by margin-parallel upslope gravitational extension.     

Understanding marine ecosystem based management: A literature review

Ecosystem based management takes into account the interconnectedness and interdependent nature of ecosystem components and emphasizes the importance of ecosystem structures and functions which provide a range of services. The concept has now been adopted by many international agreements and national governments and is in the process of being implemented. This paper seeks to review the literature and to analyze the understanding of the subject. The term is defined and its implementation in fisheries and for all marine uses is analyzed. It has been concluded that to understand marine ecosystem based management one must consider ecosystems as complex adaptive systems which can show changes at higher levels from actions and processes occurring at lower levels. Recognizing that humans are part of these complex adaptive systems is vital in that their actions along with other processes can lead to transformations in ecosystem functioning. This recognition is also important to show how society can sustainably exploit these resources and that the inclusion of all stakeholders in the management process is necessary to legitimize the process. The uses of the precautionary principle along with adaptive management are seen to be useful tools in implementing these insights into the management of natural resources. Finally, the need for reducing consumption of fish is considered.     

Modal metasomatism in the Kaapvaal craton lithosphere: constraints on timing and genesis from U–Pb zircon dating of metasomatized peridotites and MARID-type xenoliths

Modal metasomatism in the Kaapvaal craton lithosphere is well documented in upper mantle xenoliths sampled by both group I (mainly late Cretaceous) and group II (mainly early Cretaceous to late Jurassic) kimberlites in the Kimberley area. The metasomatic style is characterized by introduction of K, H and large ion lithophile/high field strength (LIL/HFS) elements into the lithospheric mantle leading to the crystallization of hydrous potassic phases such as phlogopite and/or K-amphibole. Textures indicate that the hydrous phases either replace pre-existing assemblages in peridotites, forming the metasomatized peridotite suite (phlogopite–K-richterite–peridotites: PKPs) or crystallize from K-rich melts, forming the mica–amphibole–rutile–ilmenite–diopside (MARID) suite of xenoliths. These K-rich assemblages become potential low melting source components for alkaline incompatible trace element enriched magmas. The timing of metasomatism and its temporal and possible genetic relation to kimberlite magmatism is poorly constrained because of the rarity of phases in the metasomatic assemblages suitable for precise dating. Here we present precise sensitive high resolution ion microprobe (SHRIMP) U–Pb formation ages of 88 ± 2 (1σ=1 standard deviation) and 82 ± 3 Ma data for zircons from a K-richterite–phlogopite-bearing metasomatized peridotite (PKP) and a MARID xenolith respectively, sampled by a group I kimberlite. Both average PKP and MARID zircon ages are indistinguishable from emplacement ages of group I kimberlites in the Kimberley area dated at 83 ± 4 (2σ) and 84 ± 0.9 Ma. One exceptionally old age spot of 102 ± 5 Ma from a PKP zircon provides evidence for modal metasomatism predating group I kimberlite emplacement by several millions of years with minor resetting of the U–Pb isotopic system of most analyzed PKP zircons to a group I emplacement age. Detailed textural and mineral chemical analysis, including high energy X-ray mapping and analysis of fluid inclusion daughter crystals, indicates a complex reaction history for both PKPs and MARIDs. U–Pb zircon ages from this study combined with literature data and experimentally derived models for MARID formation are used to suggest that MARID-formation is concurrent and genetically related to both group I and II kimberlite magmatism in the Kimberley area. MARID and PKP zircon ages are also consistent with the idea first proposed by Dawson and Smith (Geochim Cosmochim Acta 41: 309–323, 1977) that metasomatized peridotites may form from interaction of hydrous fluids expelled by solidifying MARID-type melts with peridotitic wall rocks. Received: 13 December 1999 / Accepted: 13 April 2000     

Calorimetry of silicate melts at 1773 K: measurement of enthalpies of fusion and of mixing in the systems diopside-anorthite-albite and anorthite-forsterite

Transposed-temperature-drop calorimetry, using a Setaram HT 1500 calorimeter, was used to study directly the melting at 1773 K of mixtures of crystalline albite, anorthite, and diopside and of anorthite and forsterite. The enthalpy of albite at 1000–1773 K, starting with both crystalline and glassy samples, was also measured. The results confirm previously measured enthalpies of fusion of albite, diopside and anorthite (Stebbins et al. 1982, 1983; Richet and Bottinga 1984,1986). The new results use thermochemical cycles which completely avoid the glassy state by transforming crystals directly to melts. The enthalpy of fusion of forsterite is estimated to be 89±12 kJ/mol at 1773 K and 114±20 kJ/mol at its melting point of 2163 K. The data allow semiquantitative evaluation of heats of mixing in the molten silicates. Along the Ab-An join, enthalpies of mixing in the liquid at 773 K are the same or somewhat more negative than those in the glass at 986 K, whereas along Ab-Di and An-Di, enthalpies of mixing in the liquid are distinctly more positive than in the glass. These differences correlate with excess heat capacities in the liquids suggested by Stebbins et al. (1984).     

Puu Hou littoral cones,Hawaii

The Puu Hou littoral cones, on the south shoreline of Hawaii, were built in 5 days by steam explosions from two narrow lava streams of the 1868 Mauna Loa lava flows as they entered the sea. Explosions occurred in localized areas of both streams, from foci that migrated seaward as the flow built jetties into the sea. Debris, radially ejected from the migrating explosion centers, fell partly on land and partly at sea, and thus formed crescent shaped rims (half-cones) on land which overlap one another. The half-cones are breached through their centers by debris-free basalt corridors, because fragments that fell onto the flowing lava were carried seaward beyond the accumulating rims.Gray and red clastic layers are draped smoothly over the rim areas; thus the rims resemble anticlinal arches in cross section. Some beds can be traced from clastic layers on the ridges into irregular agglomeratic masses interbedded with basalt units of the source lava near the foci. The lower layers in the clastic sequence contain less olivine than those high in the sequence, which corresponds in time to an increasing olivine content during the 5 day flow, as recognized in the source lava.Fragments are angular to subangular blocks, lapilli and ash of crystalline basalt mixed with more abundant quickly chilled cognate material of similar sizes. The ash is mostly sideromelane in angular particles and rounded droplets (5–95%), tachylite (2–70%), crystalline basalt (1–40%), and broken olivine phenocrysts (1–9%). In some samples, the sideromelane droplets are partly oxidized on their surfaces, and internally are dark brown (R. I.=1.610–1.616), possibly due to dehydration and/or oxidation during the explosions. Samples with externally oxidized glass also contain etched olivine crystals and some iddingsite. Unaltered sideromelane droplets are pale yellowish-brown with R. I.=1.592–1.600, and are associated with unaltered, angular to subangular olivine crystals. The refractive index of the unaltered sideromelane droplets is the same as sideromelane crusts of pahoehoe on the lava flow farther inland, suggesting that the droplets are not hydrated or highly oxidized. None of the sideromelane fragments are palagonitized, presumably because little or no hydration has taken place since 1868.

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Zusammenfassung Die littoralen Spratzkegel von Puu Hou an der Südküste von Hawaii sind innerhalb von 5 Tagen durch Dampfexplosionen in zwei naheliegenden Lavaströmen des Mauna Loa-Ausbruches im Jahre 1868 entstanden, als diese das Meer erreichten. Die Explosionen traten in eng begrenzten Bereichen beider Ströme auf; die Explosionsherde wanderten mit den Lavaströmen seewärts, wobei sich Landzungen in den Ozean bauten. Aus den seewärts wandernden Explosionsherden wurden Fragmente ausgeworfen, die teilweise auf das Land und in den Ozean fielen; es formten sich dabei halbkreisartige Ränder (Halbkegel), die sich am Land überlappen. Die Halbkegel sind in der Mitte von Basaltkorridoren durchbrochen, die frei von Explosionsfragmenten sind, da diese in die strömende Lava fielen und seewärts abtransportiert wurden.Graue und rote pyro-klastische Sedimentlagen legen sich über die Randzonen der Halbkegel, so daß sie im Querschnitt wie Antiklinalstrukturen aussehen. Einige dieser Schichten können mit klastischen Lagen vom randlichen Saum bis zu irregulären Agglomeratmassen verfolgt werden, die zwischen die Basalte nahe der Explosionsherde eingeschaltet sind. Die tieferen Lagen der klastischen Sedimente enthalten weniger Olivin als die höher liegenden. Dieses entspricht einem sich zeitlich vermehrenden Olivingehalt während der fünftägigen Ausbruchszeit, wie er auch in der Originallava erkannt werden kann.Die Bruchstücke bestehen aus angularen bis subangularen Blöcken, Lapilli und Kristallaschen, die mit rasch erkalteten Lavafetzen ähnlicher Korngröße vermischt sind. Die Asche enthält hauptsächlich Sideromelan in eckigen Bruchstücken und gefundeten Tröpfchen (5–95%), Tachylyt (2–70%), Kristallbasalt (1–40%) und zerbrochene Olivineinsprenglinge (1-9%).In einigen Proben sind die Sideromelantröpfchen teilweise auf ihren Oberflächen oxydiert und im Inneren möglicherweise durch Dehydrierung und/oder Oxydation während der Explosionen dunkelbraun gefärbt (R. I.=1.610-1.616).Proben mit äußerlich oxydiertem Glas enthalten auch angeätzte Olivinkristalle und einigen Iddingsit. Unveränderte Sideromelantröpfchen sind blaß gelblichbraun gefärbt (R. I.=1.592–1.600) und mit unveränderten, eckigen bis subangolaren Olivinkristallen vergesellschaftet. Der Brechungsindex der unveränderten Sideromelantröpfchen ist derselbe wie von Sideromelankrusten auf den Lavaströmen Pahoehoes. Daraus kann gefolgert werden, daß die Tröpfchen nicht hydratisiert oder stark oxydiert sind. Die Sideromelanbruchstücke enthalten keinen Palagonit, weil seit 1868 wahrscheinlich wenig oder gar keine Hydratisierung mehr stattgefunden hat.

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Résumé Les cônes littoraux Puu Hou, sur la côte sud d'Hawai' ont été créés en cinq jours par les explosions de vapeur de deux branches étroites de la coulée de lave de Mauna Loa en 1868 lorsqu'elle entrait en contact avec la mer. Les explosions se sont produites dans des points localisés des deux branches de la coulée à partir du centre avançant en direction de la mer à mesure que la lave y construisait des jetées. Les débris projetés à la ronde depuis les centres d'explosion mobiles tombèrement en partie sur terre et en partie en mer formant ainsi sur le sol des bourrelets en forme de croissants (demi-cônes) qui s'entrecoupent. Les demi-cônes sont traversés dans leur centre par des couloirs de basalte dépourvus de débris, les fragments tombés dans la coulée de lave ayant été entraînés vers la mer au delà des bourrelets d'accumulation.Les couches élastiques grises et rouges sont drapées d'une manière égale au-dessus de la zone des bourrelets. Elle ressemble ainsi à des arches anticlinales en coupe. Certains lits peuvent être retracés à partir des couches élastiques sur les crêtes jusqu'à des masses agglomérées irrégulières mélangées à des éléments de basalte de la lave mère. Les couches inférieures de la séquence élastique contiennent moins d'olivine que les couches supérieures ce qui correspond à un accroissement de la proportion d'olivine pendant les 5 jours ue coulée, comme le lit de lave indique.Les fragments sont des blocs angulaires à sous-angulaires, des lapilli et de la cendre de basalte cristallin, mêlés à des matériaux apparentés de taille semblable, plus abondants et rapidement refroidis. La cendre est composée principalement de sidéromélane en particules anguleuses ou en gouttelettes rondes (5–95%), de tachylite (2–70%), de basalte cristallin (1–40%) et d'olivine phénocristale brisée (1–9%). Dans quelques échantillons, les gouttelettes de sidéromélane sont en partie oxydées à la surface et brun-foncé à l'intérieur (R. I.=1.610–1.616), peut-être par suite de déshydratation e/ou oxydation pendant l'explosion. Les échantillons comportant extérieurement du verre oxydé contiennent des cristaux d'olivine attaqués et une certaine proportion d'iddingsite. Les gouttelettes de sidéromélane intactes, sont d'un jaune-brun pâle, R. I.=1.592-1.600, et sont associées à des cristaux d'olivine non-attaquées, angulaires à sous-angulaires. L'indice de réfraction des gouttelettes intactes de sidéromélane est le même que celui de la croûte de sidéromélane du pahoehoe dans la coulée de lave plus à l'intérieur de l'île, suggérant que les gouttelettes ne sont pas hydratées ou très oxydées. Aucun des fragments de sidéromélane n'est palagonisé, sans doute parce que depuis 1868 il n'y a eu que peu ou pas d'hydratation.

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, 1868 Puu Hou . Ha , .

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Dedicated to Professor Dr. A.Rittmann on the occasion of his 75. birthday     

Covariance structure and morphometric analysis—A contribution to paleogenetics

A method of analysis of covariance structure proposed by A. P. Dempster complements, in some respects, a recently suggested procedure by the author. The method is based on the comparison of ratios of generalized statistical distances and distancelike quantities. An analysis of septivariate data on the foraminiferTextilina mexicana (Cushman) shows general differences in covariance structure in which the sample rest linear discriminators also differ. This difference in covariance structure is thought to be genetic in origin. Two species of Middle Devonian brachiopods,Martinia inflata (Schnur) andUncites gryphus von Schlotheim), also show differences in covariance structure—the former slightly, the latter strongly. This is further analyzed forUncites by the author's methods and good agreement between the two approaches obtained.     

New experimental data for the system CaO-MgO-SiO2-H2O and a synthesis of inferred phase relations

Subsolidus and vapor-saturated liquidus phase relations for a portion of the system CaO-MgO-SiO₂-H₂O, as inferred from experimental data for the composition regions CaMgSi₂O₆-Mg₂SiO₄-SiO₂-H₂O and CaMgSi₂O₆-Mg₂SiO₄-Ca₃MgSi₂O₈ (merwinite)-H₂O, are presented in pressure-temperature projection. Sixteen invariant points and 39 univariant reactions are defined on the basis of the 1 atm and 10 kbar (vapor-saturated) liquidus diagrams. Lack of experimental control over many of the reactions makes the depicted relations schematic in part.An invariant point involving orthoenstatite, protoenstatite, pigeonite, and diopside (all solid solutions) occurs at low pressure (probably between 1 and 2 kbar). At pressures below this invariant point, orthoenstatite breaks down at high temperature to the assemblage diopside + protoenstatite; with increasing temperature, the latter assemblage reacts to form pigeonite. At pressures above the invariant point, pigeonite forms according to the reaction diopside + orthoenstatite = pigeonite, and the assemblage diopside + protoenstatite is not stable. At 1 atm, both pigeonite and protoenstatite occur as primary liquidus phases, but at pressures above 6–7 kbar orthoenstatite is the only Ca-poor pyroxene polymorph which appears on the vapor-saturated liquidus surface.At pressures above approximately 10.8 kbar, only diopside, forsterite, and merwinite occur as primary liquidus phases in the system CaMgSi₂O₆-Mg₂SiO₄-Ca₃MgSi₂O₈-H₂O, in the presence of an aqueous vapor phase. At pressures between 1 atm and 10.2 kbar, both akermanite and monticellite also occur as primary liquidus phases. Comparison of the 1 atm and 10 kbar vapor-saturated liquidus diagrams suggests that melilite basalt bears a low pressure, or shallow depth, relationship to monticellite-bearing ultrabasites.