186 resultados para Glauconycteris superba


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A new genus is proposed for the strikingly patterned African vespertilionid "Glauconycteris" superba Hayman, 1939 on the basis of cranial and external morphological comparisons. A review of the attributes of a newly collected specimen from South Sudan (a new country record) and other museum specimens of "G." superba suggests that "G." superba is markedly distinct ecomorphologically from other species classified in Glauconycteris and is likely the sister taxon to Glauconycteris sensu stricto. The recent capture of this rarely collected but widespread bat highlights the need for continued research in tropical sub-Saharan Africa and in particular, for more work in western South Sudan, which has received very little scientific attention. New country records for G. cf. poensis (South Sudan) and G. curryae (Gabon) are also reported.

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e. Menura superba is an illuminated, interactive, computational, sculptural work, but in comparison it is much smaller in scale. The work explores the paradox between our fascination with the exotic and our potentially dystopic future devoid of many animal species. The work was selected for inclusion in the Juried Exhibition at the 2009 International Symposium on Electronic Arts held in Belfast.

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The extremely high level of solar radiation on the Qinghai-Tibet Plateau may induce photoinhibition and thus limit leaf carbon gain. To assess the effect of high light, we examined gas exchange and chlorophyll fluorescence for two species differing in light interception: the prostrate Saussurea superba and the erect-leaved Gentiana straminea. In controlled conditions with favorable water and temperature, neither species showed apparent photoinhibition in gas exchange measurements. In natural environment, however, their photosynthetic rate decreased remarkably at high light. Photosynthesis depression was aggravated under high leaf temperature or soil water stress. Relative stomatal limitation was much higher in S. superba than in G. straminea and it remarkably increased in the later species at midday when soil was dry. F-v/F-m as an indicator for photoinhibition was generally higher in S. superba than in the other species. F-v/F-m decreased significantly under high light at midday in both species, even when soil moisture was high. F-0 linearly elevated with the increment of leaf temperature in G. straminea, but remained almost constant in S. superba. Electron transport rate (ETR) increased with photosynthetically active photon flux density (PPFD) in S. superba, but declined when PPFD was high than about 1000 mumol m(-2) s(-1) in G. straminea. Compared to favorable environment, the estimated daily leaf carbon gain at PPFD above 800 mumol m(-2) s(-1) was reduced by 32% in S. superba and by 17% in G. straminea when soil was moist, and by 43% and 53%, respectively, when soil was dry. Our results suggest that the high radiation induces photoinhibition and significantly limits photosynthetic carbon gain, and the limitation may further increase at higher temperature and in dry soil.

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Experiments were conducted in an alpine Kobresia humilis meadow near Haibei Alpine Meadow Ecosystem Research Station (37degrees29'-37degrees45'N, 101degrees12'-101degrees33'E; altitude 3200 m). Effects of enhanced ultraviolet-B (UV-B) radiation on photosynthesis of the alpine plants of Saussurea superba and Gentiana straminea were investigated. Both species were exposed to a UV-B-BE density at 15.80 kJ m(-2) per day, simulating nearly 14% ozone (O-3) reduction during the plant growing season. Neither photosynthetic CO2 uptake rate nor photosynthetic O-2 evolution rate were decreased after a long period of enhanced UV-B radiation treatment. On the contrary, there was a tendency to increase of both parameters in both species. The photosynthetic pigments were also increased, when expressed on a leaf area basis. UV-B absorbing compounds, detected by the absorbance values at 300 mm, had a tendency to increase in both species after enhanced UV-B radiation. After long-term exposure of plants to enhanced UV-B radiation, leaf morphology was also affected. Leaf thickness in both S. superba and G. straminea were increased significantly (P < 0.001). This supports our hypothesis that the increase of leaf thickness in both species after long-term exposure of enhanced UV-B radiation could compensate for the photodestruction of photosynthetic pigments when light passes through the leaf. Therefore, photosynthesis is not reduced in either species when expressed on leaf area basis. (C) 2003 Elsevier B.V. All rights reserved.

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Describe las operaciones Perú Antar I, II y III que se ejecutaron entre los meses de enero y febrero de 1988, 1989 y 1991, respectivamente, a bordo del BIC Humboldt en el estrecho de Bransfield, ampliandose el área de estudio, en Antar III, a los alrededores de la isla Elefante. Se presenta la distribución horizontal y vertical así como los estimados de biomasa del krill (Euphausia superba) determinados en el área de estudio en tales expediciones. En todos los casos se emplearon los mismos equipos y similares metodologías. Se incluye una revisión de los antecedentes de evaluación acústica del krill tendientes al cálculo de su biomasa en la zona del Estrecho de Bransfield e Isla Elefante. Los estimados de biomasa fueron los siguientes: ANTAR I, 17.0x106 t (±29,41%) con una densidad de 536,05 g/m2; en ANTAR II, 5,67 x 106 t (±16,66%) con una densidad de 176,66 g/m2 ; en ANTAR III, 8,43 x 106 t (±12,0%) con una densidad de 200,93 g/m2 . Las principales zonas de concentración del krill se observaron entre la Isla Rey Jorge e Isla Elefante en ANTAR I; entre las Islas Bravante y Livingstone en ANTAR II; y, entre las Islas Decepción y Trinidad, y al norte de la Isla Elefante, en ANTAR III.

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Se realizaron mediciones de la Fuerza de Blanco (TS) del krill (Euphausia superba) durante los 29 lances efectuados en el Crucero de Evaluación Hidroacústica utilizando la ecosonda SIMRAD EK 500 a bordo del BIC Humboldt entre los días 12 y 24 de enero de 1998 a lo largo del Estrecho de Bransfield y alrededores de la Isla Elefante. Se derivaron los valores de b20 a partir de le ecuación de TS de FOOTE (1990), de las longitudes promedios de los individuos capturados durante cada uno de los lances y de las tablas de TS generadas por la ecosonda, determinándose una ecuación de TS para el krill en un rango de longitud comprendido entre 2,1 y 5,3 cm de la siguiente forma: TS = 20 log L - 89,26. Se discute el posible sesgo de la ecuación debido, entre otros aspectos a que no se consideraron los estadíos sexuales del krill.

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Con el objetivo de evaluar la biomasa y distribución del krill se llevó a cabo un Crucero de Evaluación Hidroacústica a bordo del BIC Humboldt entre los días 12 y 24 de enero de 1998, a largo del Estrecho de Bransfield y alrededores de la Isla Elefante. Previamente se efectuaron calibraciones de la ecosonda SIMRAD EK 500 utilizando blanco estándar. El trayecto utilizado para el muestreo acústico fue sistemático, paralelo con separaciones de 15 y 12 mn (Estrecho Bransfield e Isla Elefante, respectivamente). Se utilizaron frecuencias de 38 y 120 kHz; la frecuencia de 120 kHz se determinó para la detección entre 2 y 150 mn de profundidad y la de 38 kHz entre 150 - 400 m. Para obtener el área de distribución del krill se utilizó un software de interpolación de datos; y para estimados de biomasa, la metodología de estratificación por cuadrantes de 0,5 - de latitud 1,0 - de longitud. Los resultados obtenidos indican que el krill se encontró en gran parte del área evaluada, con las mayores concentraciones cerca de la Isla D 'Urville, al este de la Isla Rey Jorge, sur de la Isla Robert y en áreas cercanas a la Isla Elefante, distribuidas principalmente entre 50 y 100 m de profundidad.

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Se ha determinado, mediante un análisis preliminar, que el krill (Euphausia superba) se distribuyó en aguas provenientes del Mar de Wedell y en aquellas procedentes del Paso Drake a lo largo del Estrecho de Bransfield y al sur de la Isla Elefante. En cuanto a sus parámetros preferenciales de distribución se ha determinado que esta especie se distribuyó en aguas con relativamente baja temperatura, pero con altos contenidos de salinidad y oxígeno.