Almacenamiento refrigerado de cerezas : efecto de madurez y atmósfera modificada

Se estudió el efecto de cosechar cerezas en dos estados de madurez: rojo pálido y rojo maduro y la utilización de atmósferas modificadas, empleando PBD de 11 y 40 m, sobre la calidad de fruta almacenada a 0 °C y después de 3 días a temperatura ambiente. La calidad fue evaluada en términos de pérdida de peso (%), color (ángulo hue), firmeza, contenido de sólidos solubles, aspecto de los pedicelos y presencia de podredumbres. La fruta cosechada más madura presentó color, sólidos solubles y firmeza adecuados durante 21 días a 0 °C pero el almacenamiento prolongado estuvo limitado por la deshidratación de los pedicelos, que mantuvieron aspecto comercial sólo durante una semana. Para ambos estados de madurez se registró importante pérdida de peso; disminución del valor de °hue y aumentos de sólidos solubles y de firmeza. Durante la simulación comercial la fruta experimentó ablandamiento, pérdida de peso, oscurecimiento de la piel y deshidratación de los pedicelos. Con el uso del PBD no se detectaron cambios significativos para ninguno de los parámetros estudiados, permitiendo además reducir la deshidratación y mantener el aspecto comercial de los pedicelos, independientemente del espesor de la película.

Influencia de la intercepción lumínica en el desarrollo vegetativo y productivo de durazneros cv. Elegant Lady

El presente ensayo fue establecido en el Alto Valle del Río Negro, Argentina (38°55´ Sur), sobre durazneros cv. Elegant Lady conducidos en vaso, de 5 m de altura, con un distanciamiento de 4 m entre plantas y 4,8 m entre filas. Se realizaron tres tratamientos en un diseño totalmente aleatorizado, simulando diferentes intensidades de luz: restricción lumínica con mallas de sombreo del 80%, poda en verde y un control sin intervención. En cada una de las plantas se diferenciaron 4 sectores orientados hacia los 4 puntos cardinales y 3 alturas distintas de la copa del árbol. La radiación fotosintéticamente activa (RFA) fue medida en cada sector 25, 15 y 6 días antes de la cosecha. La RFA interceptada estuvo influenciada por la restricción lumínica y por la altura. Las variables vegetativas y de producción se relacionaron entre sí linealmente, y ambas dependieron principalmente de la RFA interceptada. Los modelos que explican el comportamiento entre la RFA y las variables de calidad son de tipo asintóticos. A partir de los 25 días anteriores a la cosecha, la RFA necesaria para alcanzar frutos con un peso y color adecuados para su comercialización debe ser del 30%. En el rango de 0 a 15% de RFA interceptada, pequeñas variaciones de RFA dan como resultado grandes cambios en las variables de peso, color de cobertura e intensidad de color del fruto.

Desarrollo de estándares de calidad para uvas Vitis vinifera L. cv. Malbec y Syrah

El objetivo del trabajo fue desarrollar estándares de calidad de uva basados en atributos físicos y químicos, capaces de predecir la calidad del vino. Se instaló una red de ensayos en Mendoza (Norte, Este y Valle de Uco), San Juan (Valle de Zonda), La Rioja (Chilecito), Catamarca y Salta (Valles Calchaquíes) (Argentina). Se ensayaron niveles de carga de uva (desbrote 30 y 50%, raleo 30 y 50% y testigo) en Malbec y Syrah. En la cosecha, las uvas fueron analizadas (tamaño baya, concentración azucarina, pH, antocianos, catequinas, taninos, fenoles totales) y vinificadas. Los vinos fueron analizados (alcohol, extracto seco, intensidad colorante, matiz, antocianos, catequinas, taninos, fenoles totales, color polimérico) y evaluados por un panel de degustadores. Empleando todos las variables de los vinos, mediante un análisis de componentes principales, se generaron dos índices que resumieron los atributos con mayor peso explicativo de la variabilidad observada (80%); ellos fueron: Riqueza Fenólica (RF, asociado a antocianos, taninos, catequinas, fenoles totales y concentración) y Peligro Oxidativo (PO, asociado a pH, matiz y tonalidad percibida). No existieron diferencias en cuanto a RF entre variedades ni entre niveles de producción de uva. Los vinos con RF mayor y PO menor se consideraron de mayor calidad. Las uvas cultivadas en zonas más frías tuvieron una mayor RF. En Malbec, las zonas frías y los bajos niveles productivos generaron un PO menor. Para cada variedad se desarrollaron predictores para RF y PO del vino. Se usó la regresión múltiple lineal paso a paso, seleccionando las variables de la uva con mayor poder predictivo. Se definieron las funciones de ajuste RFpred (Malbec R2 = 80%; Syrah R2 = 62%) y POpred (Malbec R2 = 80%; Syrah R2 = 62%). Los índices se tradujeron en estándares de calidad que mostraron concordancia entre uvas y vinos. La metodología puede ser válida para otras variedades tintas, pero debe ajustarse para cada caso. Los estándares permitirían asociar un precio a cada calidad y aumentar la transparencia del mercado.

Variación agromorfológica y cambios biofísicos poscosecha en frutos de tomate (Solanum lycopersicum L.)

Se evaluó la variación fenotípica agromorfológica y cambios biofísicos de frutos después de 10 días de almacenamiento a temperatura ambiente, en una colección de tomate de Oaxaca, México. La colección de 57 colectas fue sembrada y caracterizada bajo invernadero. En poscosecha se evaluó pH, grados Brix, pérdida de peso y parámetros de color (L*, a*, b*, cromaticidad y ángulo Hue) a 0 y 10 días después de la cosecha. Las colectas mostraron diferencias significativas (P < 0,01) en todos los caracteres agromorfológicos y también hubo diferencias significativas entre acervos genéticos preclasificados como cultivados, ruderales e intermedios entre cultivados y ruderales. Nueve grupos de diversidad fenotípica fueron conformados. Se determinaron diferencias significativas entre tiempos de almacenamiento (0 y 10 días) para todas las características biofísicas. Después de 10 días de almacenamiento a temperatura ambiente (20,6±5°C y 34±10% HR), se incrementaron los °Brix de 4,1 a 4,6 y pH de 3,7 a 4,3. Entre grupos fenotípicos e interacción tiempo de almacenamiento-grupos, se determinaron diferencias significativas en °Brix, coordenadas de color L* y b*, y ángulo Hue. Los cambios diferenciales poscosecha indican divergencias fenotípicas entre y dentro de acervos genéticos que pueden explotarse en programas de mejoramiento con objetivos regionales.

Documentation of sediment cores during SONNE Expedition SO228 from the western tropical Pacific

The core descriptions (chapter 7) summarize the most important results of the analysis of each sediment core following procedures applied during ODP/IODP expeditions. All cores were opened, described, and color-scanned. In the core descriptions the first column displays the lithological data that are based on visual analysis of the core and are supplemented by information from binocular and smear slide analyses. The sediment classification largely follows ODP/IODP convention. Lithological names consist of a principal name based on composition, degree of lithification, and/or texture as determined from visual description and microscopic observations. In the structure column the intensity of bioturbation together with individual or special features (turbidites, volcanic ash layers, plant debris, shell fragments, etc.) is shown. The hue and chroma attributes of color were determined by comparison with the Munsell soil color charts and are given in the color column in the Munsell notation. A GretagMacbethTM Spectrolino spectrophotometer was used to measure percent reflectance values of sediment color at 36 wavelength channels over the visible light range (380-730 nm) on all of the cores. The digital reflectance data of the spectrophotometer readings were routinely obtained from the surface (measured in 1 cm steps) of the split cores (archive half). The Spectrolino is equipped with a measuring aperture with folding mechanism allowing an exact positioning on the split core and is connected to a portable computer. The data are directly displayed within the software package Excel and can be controlled simultaneously. From all the color measurements, for each core the red/blue ratio (700 nm/450 nm) and the lightness are shown together with the visual core description. The reflectance of individual wavelengths is often significantly affected by the presence of minor amounts of oxyhydroxides or sulphides. To eliminate these effects, we used the red/blue ratio and lightness.

(Table 1) Color, Fe-C-S chemistry and carbonate content from ODP Sites 172-1062 and 172-1063

Reflectance spectra collected during ODP Leg 172 were used in concert with solid phase iron chemistry, carbonate content, and organic carbon content measurements to evaluate the agents responsible for setting the color in sediments. Factor analysis has proved a valuable and rapid technique to detect the local and regional primary factors that influence sediment color. On the western North Atlantic drifts, sediment color is the result of primary mineralogy as well as diagenetic changes. Sediment lightness is controlled by the carbonate content while the hue is primarily due to the presence of hematite and Fe2+/Fe3+ changes in clay minerals. Hematite, most likely derived from the Permo-Carboniferous red beds of the Canadian Maritimes, is differentially preserved at various sites due to differences in reductive diagenesis and dilution by other sedimentary components. Various intensities for diagenesis result from changes in organic carbon content, sedimentation rates, and H2S production via anaerobic methane oxidation. Iron monosulfides occur extensively at all high sedimentation sites especially in glacial periods suggesting increased high terrigenous flux and/or increased reactive iron flux in glacials.

Mineralogical and isotopic compositions of ODP Hole 107-650A

Red-brown dolomitic claystones overlay the Marsili Basin basaltic basement at ODP Site 650. Sequential leaching experiments reveal that most of the elements considered to have a hydrothermal or hydrogenous origin in a marine environment, such as Fe, Cu, Zn, Pb, Co, Ni, are present mainly in the aluminosilicate fraction of the dolomitic claystones. Their vertical distribution, content and partitioning chemistry of trace elements, and REE patterns suggest enhanced terrigenous input during dolomite formation, but no significant hydrothermal influence from the underlying basaltic basement. Positive correlations in the C and O isotopes in the dolomites reflect complex conditions during the dolomitization. The stable isotopes can be controlled in part by temperature variations during the dolomitization. Majority of the samples, however, form a trend that is steeper than expected for only temperature control on the C and O isotopes. The latter indicates possible isotopic heterogeneity in the proto-carbonate that can be related to arid climatic conditions during the formation of the basal dolomitic claystones. In addition, the dolostones stable isotopic characteristics can be influenced by diagenetic release of heavier delta18O from clay dehydration and/or alteration of siliciclastic material. Strontium and Pb isotopic data reveal that the non-carbonate fraction, the "dye" of the dolomitic claystones, is controlled by Saharan dust (75%-80%) and by material with isotopic characteristics similar to the Aeolian Arc volcanoes (20%-25%). The non-carbonate fraction of the calcareous ooze overlying the dolomitic claystones has a Sr and Pb isotopic composition identical to that of the dolomitic claystones, indicating that no change in the input sources to the sedimentary basin occurred during and after the dolomitization event. Combination of climato-tectonic factors most probably resulted in suitable conditions for dolomitization in the Marsili and the nearby Vavilov Basins. The basal dolomitic claystone sequence was formed at the initiation of the opening of the Marsili Basin (~2 Ma), which coincided with the consecutive glacial stage. The glaciation caused arid climate and enhanced evaporation that possibly contributed to the stable isotope variations in the proto-carbonate. The conductive cooling of the young lithosphere produced high heat flow in the region, causing low-temperature passive convection of pore waters in the basal calcareous sediment. We suggest that this pumping process was the major dolomitization mechanism since it is capable of driving large volumes of seawater (the source of Mg2+) through the sediment. The red-brown hue of the dolomitic claystones is terrigenous contribution of the glacially induced high eolian influx and was not hydrothermally derived from the underlying basaltic basement. The detailed geochemical investigation of the basal dolomitic sequence indicates that the dolomitization was most probably related to complex tectono-climatic conditions set by the initial opening stages of the Marsili Basin and glaciation.

Physical properties of four profiles from the Triassic in Germany

The Norian Steinmergel-Keuper (SMK) represents a low-latitude cyclically-bedded playa system of the Mid-German Basin. We investigated a drilling site (core Morsleben) and sections from marginal positions. Dolomite/red mudstone beds form rhythmic alternations that were associated with varying monsoon activity. Hence, low K/Al ratios of dolomite beds suggest increased chemical weathering of the crystalline hinterland and therefore increased monsoonal rainfall. High K/Al ratios in red mudstone beds reflect increased physical weathering of the hinterlands during dryer periods. Dolomite layers reflect the lake stage (maximum monsoon) while red mudstones indicate the dry phase (minimum monsoon) of the playa cycle. We distinguished five major types of cyclic facies alternations, representing specific facies zones in the playa system. We have implemented spectrophotometry as a tool for high-resolution cyclostratigraphy. The dense sampling increment (up to 1 cm) allows for the recognition of all orbital frequencies. Sediment colour profiles reveal striking hierarchical cycles from semi-precession (SP, 99 kyr) over precession (P, 19.8 kyr) and obliquity (O, 36 kyr) to eccentricity (E1-2 109 kyr; E3, 413 kyr). A significant about 2 Myr-signal is attributed to the longer-term eccentricity E4. One monsoonal (precession) cycle includes two carbonate precipitation events. We propose that stratified mudstone and red mudstone are associated with maximum and minimum monsoon during the transition of the solstices in perihelion and aphelion, respectively. The two carbonate precipitation events were most likely created when equinoxes were in perihelion and aphelion, respectively. A sedimentary semi-precession response cycle is a novel finding for the Norian strata. The obliquity signal is attributed to incoming atmospheric moisture from the northeast of the SMK basin. The E4 cycle controls lake-level changes over long times. Apparently, E4 is responsible whether or not a threshold value is crossed. Bundles of 109 kyr and 413 kyr in red mudstones suggest a dry system with reduced monsoonal activity. In contrast, humid periods reveal thick layers of dolomite beds, indicating that during those intervals the monsoonal activity was strong enough to prevent the playa system from drying out completely.

Sediment composition in NE Greenland Fjords, Shelf, and Slope

In order to document changes in Holocene glacier extent and activity in NE Greenland (~73° N) we study marine sediment records that extend from the fjords (PS2631 and PS2640), across the shelf (PS2623 and PS2641), to the Greenland Sea (JM07-174GC). The primary bedrock geology of the source areas is the Caledonian sediment outcrop, including Devonian red beds, plus early Neoproterozoic gneisses and early Tertiary volcanics. We examine the variations in colour (CIE*), grain size, and bulk mineralogy (from X-ray diffraction of the <2 mm sediment fraction). Fjord core PS2640 in Sofia Sund, with a marked red hue, is distinct in grain size, colour and mineralogy from the other fjord and shelf cores. Five distinct grain-size modes are distinguished of which only one is associated with a coarse ice-rafting signal - this mode is rare in the mid- and late Holocene. A sediment unmixing program (SedUnMixMC) is used to characterize down-core changes in sediment composition based on the upper late Holocene sediments from cores PS2640 (Sofia Sund), PS2631 (Kaiser Franz Joseph Fjord) and PS2623 (south of Shannon Is), and surface samples from the Kara Sea (as an indicator of transport from the Russian Arctic shelves). Major changes in mineral composition are noted in all cores with possible coeval shifts centred c. 2.5, 4.5 and 7.5 cal. ka BP (±0.5 ka) but are rarely linked with changes in the grain-size spectra. Coarse IRD (>2 mm) and IRD-grain-size spectra are rare in the last 9-10 cal. ka BP and, in contrast with areas farther south (~68° N), there is no distinct IRD signal at the onset of neoglaciation. Our paper demonstrates the importance of the quantitative analysis of sediment properties in clarifying source to sink changes in glacial marine environments.