Isotope ratios of basalts from ODP Leg 115 holes (Table 1)

Strontium, neodymium, and lead isotope ratios are reported for 13 Leg 115 basalts as well as 3 basalts from Texaco drill hole SM-1 on the Mascarene Plateau. The 87Sr/86Sr ratios and eNd range from 0.70330 to 0.70439 and 5.5 to 7.4, respectively, although 87Sr/86Sr ratios higher than 0.70383 are found only in SM-1 basalts. The high 87Sr/86Sr values are thought to reflect seawater Sr in secondary phases, although all samples were strongly leached in HC1 before analysis. 206Pb/204Pb ratios range from 18.53 to 18.80, and sho high 207Pb/204Pb and 208Pb/204Pb ratios relative to 206Pb/204Pb ratios, typical of Indian Ocean mid-ocean ridge (MORB) and oceanic-island basalts (OIB). Isotopic compositions of Leg 115 basalts generally fall between fields for MORB and Reunion Island basalts, consistent with the conclusion drawn from geochronological studies that Deccan flood basalt volcanism, the Chagos-Laccadive Ridge, and the Mascarene Plateau are all products of the Reunion mantle plume. Isotopic compositions of magmas produced by this plume have varied systematically with time in the direction of less "depleted," less MORB-like isotopic signatures. This compositional change has been accompanied by a decrease in eruption rate. We interpret Deccan volcanism as the voluminous beginning of the plume. Reduced entrainment of asthenosphere following melting of the plume head resulted in less MORB-like isotope ratios in magmas and a decrease in eruptive activity with time.

Primary mineralogy of ODP Leg 115 basalts

Basement rocks were recovered at four sites on Leg 115 along the Reunion hotspot track in the western Indian Ocean. Plate tectonic reconstructions indicate that the drilled structures formed in three different volcanic environments. Sites 706 and 713 from the eastern side of the Saya de Malha Bank and the northern end of the Chagos Bank, respectively, are on a large volcanic platform analogous to Iceland on the Mid-Atlantic Ridge. Lavas at Site 707 on the northwestern side of the Saya de Malha Bank erupted during the early stages of rifting of the Seychelles from India. Basalts from Site 715 were erupted onto an isolated oceanic island that was distant from ocean ridges and continents much as Reunion Island is today. Many of the rocks were examined in thin section and found to be primarily augite-plagioclase basalts with minor olivine and rare opaque oxides. Site 715 is unusual in that it contains a variety of basalts including olivine-rich and aphyric Fe-Ti basalts. At each of the four sites the rocks were grouped into chemical types (units) on the basis of ship- board bulk-rock analyses and at least one thin section from each chemical unit was analyzed by electron microprobe. The plagioclase and augite chemistry reflects the bulk-rock chemistry and, in general, these minerals were in equilibrium with their host magmas at the time the basalts were quenched. Olivine was rarely preserved, but where it is still present it also appears to have crystallized in equilibrium with the host magma. At three of the drill sites plagioclase phenocrysts or megacrysts that crystallized from a primitive magma are also present. The one site (715) that does not contain these primitive plagioclase phenocrysts is also the site that appears to have been influenced the least by ocean- ridge or Deccan-type magmas. Site 715, furthermore, has a mineralogy that is dominated by olivine as compared with the plagioclase-rich lavas of the other sites.

Paleomagnetism of ODP Leg 115 sediments

Ocean Drilling Program Leg 115 was designed to study Neogene sedimentation history in the western Indian Ocean Basin as well as the Cenozoic evolution of the Reunion hotspot. We describe the paleomagnetic analysis of the sediments recovered on this leg, focusing on the sites that provided the most readily interpretable data: Sites 706, 709, 710, and 711. Sediments from Site 706 show no reversals but appear to give a reliable reversed polarity primary direction, judged on the basis of the demagnetization behavior of individual samples as well as from the results of a fold test formulated by comparing the two holes drilled at this site. Magnetic polarity stratigraphy in sediments from Site 709 can be deduced in two limited sections of Pliocene-Pleistocene and Oligocene-Miocene age. Sediments recovered at Site 710 (and, to a lesser extent, Site 711) render a relatively continuous magnetic polarity stratigraphy that spans most of the Neogene and adds significantly to the body of data available to address problems in Miocene geochronology. In addition to these magnetostratigraphic results, the paleomagnetism of these sediments can be used to determine paleolatitude. Using the most reliable inclination measurements from Sites 706, 710, and 711, we compared paleomagnetic estimates of paleolatitude with estimates derived from a hotspot-based absolute plate motion model. Our data, which covers the interval since 33 Ma, shows that paleolatitudes calculated with the geocentric axial dipole assumption are in general accord with the hotspot predictions. However, a correction for the long-term nondipole field brings the paleomagnetic results into even better agreement with plate motions that are based on the fixity of African hotspots.

Lithologic correlation of ODP Leg 115 holes

Whole-core (WC) measurements of low-field magnetic susceptibility (MS) provide an extremely simple, rapid, and nondestructive technique for high-resolution core logging and lithostratigraphic correlation between subsidiary holes at Ocean Drilling Program (ODP) sites. This is particularly useful for reconstructing composite, stratigraphically continuous sequences for individual ODP sites by splicing the uninterrupted records obtained from subsections of offset cores recovered from adjacent holes. Correlation between the WCMS profiles of holes drilled at different sites is also possible in some instances, especially when lithologic variations at each site are controlled by regional paleoceanographic or global (i.e., orbitally forced) paleoclimatic changes. In such circumstances, WCMS may also be used as a proxy paleoclimatic indicator, duly assisting climatostratigraphic zonation of the recovered sequence by more conventional microfossil and isotopic techniques. High-resolution WCMS profiles are also useful in detecting intervals of the recovered sequence affected by drilling disturbance, in the form of contamination by pipe rust or similar metallic artifacts as well as discontinuities related to repenetration of the corer or loss of material between successively cored intervals. Stratigraphic intervals that have been affected by early (suboxic) diagenesis resulting from a high initial organic matter content of the sediment are also readily identified by WCMS logging. The MS signal of horizons affected by suboxic diagensis is typically degraded in proportion to the duration and intensity (related to initial Corg concentration) of organic matter remineralization. The lowering of MS values during suboxic diagenesis results from "dissolution" (bacterially mediated ionic dissociation) of magnetic iron and manganese oxides and oxyhydroxides in the sediment. It is to be hoped that, on future ODP (or similar) cruises, WCMS logging will cease to be regarded as a mere adjunct to paleomagnetic measurements, but rather as a simple, yet powerful, lithostratigraphic tool, directly analogous to downhole geophysical logging tools, and complimentary to shipboard techniques for whole-core measurements of physical properties (e.g., P-wave logging, GRAPE, etc.).

Eocene-Oligocene diatoms in the western Indian Ocean

The occurrence of diatom species in the Eocene-Oligocene sections of Ocean Drilling Program (ODP) Leg 115 sites and Deep Sea Drilling Project (DSDP) Sites 219 and 236 in the low-latitude Indian Ocean are investigated. Diatoms are generally rare and poorly preserved in the Paleogene sequences we studied. The best-preserved assemblages are found close to ash layers in early Oligocene sediments. The low-latitude diatom zonation established for the Atlantic region by Fenner in 1984 is fully applicable to the Paleogene sequences of the western Indian Ocean. Correlation of the diatom zones to the calcareous nannofossil stratigraphy of the sites places the Coscinodiscus excavatus Zone of Fenner within calcareous nannofossil Subzone CP16b. For the Mascarene Plateau and the Chagos Ridge, the times when the sites studied, together with the areas upslope from them, subsided to below the euphotic zone are deduced from changes in the relative abundance between the group of benthic, shallow-water species and Grammatophora spp. vs. the group of fully planktonic diatom species. The Eocene section of Site 707, on the Mascarene Plateau, is characterized by the occurrence of benthic diatoms (approximately 10% of the diatom assemblage). These allochthonous diatoms must have originated from shallow-water environments around volcanic islands that existed upslope from ODP Site 707 in Eocene times. In Oligocene and younger sediments of Sites 707 and 706, occurrences of benthic diatoms are rare and sporadic and interpreted as reworked from older sediments. This indicates that the area upslope from these two Mascarene Plateau sites had subsided below the euphotic zone by the early Oligocene. Only Grammatophora spp., for which a neritic but not benthic habitat is assumed, continues to be abundant throughout the Oligocene sequences. The area of the Madingley Rise sites (Sites 709-710) and nearby shallower areas subsided below the euphotic zone already in middle Eocene times, as benthic diatoms are almost absent from these Eocene sections. Only sites located on abyssal plains, and which intermittently received turbidite sediments (e.g., Sites 708 and 711), contain occasionally single, benthic diatoms of Oligocene age. The occurrence of the freshwater diatom Aulacosira granulata in a few samples of late early Oligocene and late Oligocene age at Sites 707, 709, and 714 is interpreted as windblown. Their presence indicates at least seasonally arid conditions for these periods in the source areas of eastern Africa and India. Three new species and two new combinations are defined: Chaetoceros asymmetricus Fenner sp. nov.; Hemiaulus gracilis Fenner, sp. nov.; Kozloviella meniscosa Fenner, sp. nov.; Cestodiscus demergitus (Fenner) Fenner comb, nov.; and Rocella princeps (Jouse) Fenner comb. nov.

Producción de biomasa y concentración de nutrientes en el pasto cubano (Pennisetum purpureum x P. tiphoides) CV CT - 115. Finca la Tigra, Cárdenas, Rivas, Nicaragua

Con el propósito de determinar la producción de la biomasa forrajera y la concentración de nutrientes del pasto cubano CT - 115, se realizó un estudio en la Finca la Tigra, Cárdenas, Rivas, para ello se utilizó un área de 48 m2, subdividida en tres parcelas de 16 m2, donde se realizaron cortes a los 15, 30, 45, 60 y 75 días. Se evaluaron las variables altura de la planta, producción de biomasa fresca y seca por hectárea, en cada muestreo se tomaron muestras de plantas de 1,000 g, las que fueron remitidas al laboratorio de suelo y planta de la UNA, donde se hicieron las determinaciones de contenido de materia seca, % de nitrógeno, % fósforo, % potasio, % calcio, % magnesio, hierro (ppm), manganeso (ppm) y zinc (ppm). Se realizarón análisis de correlación usando el programa SAS (Sistema de Análisis Estadístico) versión 9. para los elementos de la composición nutritiva de la planta y las variables rendimiento de biomasa y altura, a través del programa CVEXPT (Experto de Curvas) versión 1.4, se determinaron las curvas de mejor ajustes para dichas relaciones. Encontrándose que a medida que aumentaba la edad de corte, la producción de biomasa fresca y seca así como la altura tendían a incrementar, inversamente a ello los niveles de nutrientes en las plantas, las ecuaciones de mejor ajustes para la producción de biomasa fresca, seca y altura fueron el Lineal, Logístico y Rotacional, con r2 de 94, 98 y 99% respectivamente, para el caso de los nutrientes las ecuaciones de mejor ajuste fueron: los modelos de función Rotacional, Logístico, Polinomial y Harris también con r2 de 92 a 99%, evidenciándose con esto que las tendencias de los incrementos de la biomasa seca, altura, y la concentración de nutrientes no presentan comportamiento lineal. Únicamente para el caso de la biomasa fresca se presentó una tendencia lineal.

Productividad y concentración de nutrientes del Taiwán Cubano (Pennisetum purpureum X Pennisetum tiphoides), CT 115, en época lluviosa, 2010 en la Fincas Santa Rosa

Con el objetivo de evaluar la Productividad y concentración de nutrientes del pasto cubano (Pennisetum purpureum x Pennisetum typhoides) cv CT – 115, se llevó a cabo la presente investigación en la finca Santa Rosa propiedad de la Universidad Nacional Agraria (UNA) Managua, Nicaragua. Localizada geográficamente a los 12° 08´ 33"de latitud norte y, 86° 10´ 31" de longitud oeste (INETER, 2006). Para ello se utilizó un área total de 33 m2 la cual se subdividió en tres parcelas de 10 m2 cada una donde se realizaron cortes cada 15 días hasta llegar a los 75 días. Se evaluaron las variables : altura, (cm) biomasa fresca (kg ha-1), Materia Seca (%), Biomasa seca (kg ha-1), Nitrógeno (%), Fósforo (%), Potasio (%),Calcio (%), Magnesio (%), Hierro (ppm), Manganeso (ppm), Zinc (ppm). Para la determinación de la producción de biomasa verde y seca (kg ha-1), se utilizó la metodología propuesta por la Red Internacional de evaluación de Pasturas Tropicales (CIAT, 1982). Para determinar los parámetros MS (%) se utilizó la metodología del análisis de Weende o análisis proximal (AOAC. 1990). Para el análisis de correlación se utilizo el programa SAS VERSION 9 para cada uno de las variables evaluadas, para la determinación de las curvas de mejor ajuste se utilizó el programa CVXP32. Durante el ensayo no se aplico ningún tipo de tratamiento agronómico (fertilización, riego). Los resultados obtenidos fueron: Altura 220 cm Biomasa fresca 31,764 kg ha-1 Materia seca 24% Biomasa seca 7529 kg ha-1. Las mayores concentraciones de nutrientes en la planta fueron: N 3.21% P 0.38% K 4.94% Ca 0.24% Mg 0.18% Fe 105.0ppm Mn 53.33ppm Zn 50ppm. Los modelos de mejor ajuste son: Modelo Múltiple Multiplicativo, Modelo Richards, Modelo Harris, Función Rotacional, Tercer Grado Polinomial y Asociación Exponencial.

Sapientia, 1975, Vol. XXX, nº 115 (número completo)

Contenido: Retorno a Santo Tomás : el documento de Paulo VI sobre Santo Tomás: Lumen Ecclesiae / Octavio N. Derisi – Los dos planos de la metafísica y la fenomenología / Teófilo Urdánoz O. P. – Antropología tomista y antropología actual / Victorino Rodríguez O. P. – Notas y comentarios -- Bibliografía