(Table 1) Stratigraphic datums from ODP Site 130-806

A 2 m.y. oxygen isotope record of Globigerinoides sacculifer from the Ontong Java Plateau, based on cores from Ocean Drilling Program Leg 130, is dated by matching variations to an orbital template. The procedure allows us to present the most complete Quaternary record available for the western equatorial Pacific. The template-generating algorithm describes a balance between growth and melting of ice. Following basic Milankovitch theory, ice growth is taken as constant, while melting is taken to depend on summer insolation, current ice mass, and average past ice mass. Template settings must be changed once, between 1 and 1.2 Ma, to reflect a major shift in climate. Template fits are strikingly good over much of the record and can be used to detect and fill gaps from core breaks and other disturbances. One result of template dating is an exact age for the Brunhes-Matuyama magnetic reversal boundary, at 790+/-5 ka, as well as several other precise dates (900 ka for the middle Pleistocene climate shift; 1070, 1240, and 1450 ka for isotope stages 31, 37, and 47, respectively). Sedimentation rates fluctuate between 18 and 28 m/m.y., a ca. 400 ka cycle being the most prominent. Major anomalies arise within the transitional regime (1.2 to 1 Ma). The origin of the cycles is unknown; we propose productivity variations in the western equatorial Pacific.

Evaluación de un sistema de energía solar térmica basado en colectores de tubos de vacío para suministro de agua a alta temperatura

Esta tesis pretende contribuir al fomento y utilización de la energía solar como alternativa para la producción de agua caliente en el sector agroindustrial. La demanda de agua caliente es un aspecto clave en un gran número de agroindustrias y explotaciones agrarias. Esta demanda presenta una gran variabilidad, tanto en los horarios en que se solicita como en la temperatura del agua del depósito requerida (TADr), difiriendo del perfil de demanda habitual para uso doméstico. Existe una necesidad de profundizar en la influencia que tiene la variación de la TADr en la eficiencia y viabilidad de estos sistemas. El objetivo principal de esta tesis es caracterizar el funcionamiento de un sistema solar térmico (SST) con captador de tubos de vacío (CTV) para producir agua a temperaturas superiores a las habituales en estos sistemas. Se pretende determinar la influencia que la TADr tiene sobre la eficiencia energética del sistema, cuantificar el volumen de agua caliente que es capaz de suministrar en función de la TADr y determinar la rentabilidad del SST como sistema complementario de suministro. Para ello, se ha diseñado, instalado y puesto a punto un sistema experimental de calentamiento de agua, monitorizando su funcionamiento a diferentes TADr bajo condiciones ambientales reales. Los resultados cuantifican cómo el aumento de la TADr provoca una disminución de la energía suministrada al depósito, pudiendo superar diferencias de 1000 Wh m-2 d-1 entre 40 ºC y 80 ºC, para valores de irradiación solar próximos a 8000 Wh m-2 d-1 (la eficiencia del sistema oscila entre 73% y 56%). Esta reducción es consecuencia de la disminución de la eficiencia del captador y del aumento de las pérdidas de calor en las tuberías del circuito. En cuanto al agua suministrada, cuanto mayor es la TADr, mayor es la irradiación solar requerida para que tenga lugar la primera descarga de agua, aumentando el tiempo entre descargas y disminuyendo el número de éstas a lo largo del día. A medida que se incrementa la TADr, se produce una reducción del volumen de agua suministrado a la TADr, por factores como la pérdida de eficiencia del captador, las pérdidas en las tuberías, la energía acumulada en el agua que no alcanza la TADr y la mayor energía extraída del sistema en el agua producida. Para una TADr de 80 ºC, una parte importante de la energía permanece acumulada en el depósito sin alcanzar la TADr al final del día. Para aprovechar esta energía sería necesario disponer de un sistema complementario de suministro, ya que las pérdidas de calor nocturnas en el depósito pueden reducir considerablemente la energía útil disponible al día siguiente. La utilización del sistema solar como sistema único de suministro es inviable en la mayoría de los casos, especialmente a TADr elevadas, al no ajustarse la demanda de agua caliente a la estacionalidad de la producción del sistema solar, y al existir muchos días sin producción de agua caliente por la ausencia de irradiación mínima. Por el contrario, la inversión del sistema solar como sistema complementario para suministrar parte de la demanda térmica de una instalación es altamente recomendable. La energía útil anual del sistema solar estimada oscila entre 1322 kWh m-2 y 1084 kWh m-2. La mayor rentabilidad se obtendría suponiendo la existencia de una caldera eléctrica, donde la inversión se recuperaría en pocos años -entre 5.7 años a 40 ºC y 7.2 años a 80 ºC -. La rentabilidad también es elevada suponiendo la existencia de una caldera de gasóleo, con periodos de recuperación inferiores a 10 años. En una industria ficticia con demanda de 100 kWh d-1 y caldera de gasóleo existente, la inversión en una instalación solar optimizada sería rentable a cualquier TADr, con valores de VAN cercanos a la inversión realizada -12000 € a 80 ºC y 15000€ a 40 ºC- y un plazo de recuperación de la inversión entre 8 y 10 años. Los resultados de este estudio pueden ser de gran utilidad a la hora de determinar la viabilidad de utilización de sistemas similares para suministrar la demanda de agua caliente de agroindustrias y explotaciones agropecuarias, o para otras aplicaciones en las que se demande agua a temperaturas distintas de la habitual en uso doméstico (60 ºC). En cada caso, los rendimientos y la rentabilidad vendrán determinados por la irradiación de la zona, la temperatura del agua requerida y la curva de demanda de los procesos específicos. ABSTRACT The aim of this thesis is to contribute to the development and use of solar energy as an alternative for producing hot water in the agribusiness sector. Hot water supply is a key issue for a great many agribusinesses and agricultural holdings. Both hot water demand times and required tank water temperature (rTWT) are highly variable, where the demand profile tends to differ from domestic use. Further research is needed on how differences in rTWT influence the performance and feasibility of these systems. The main objective of this thesis is to characterize the performance and test the feasibility of an evacuated tube collector (ETC) solar water heating (SWH) system providing water at a higher temperature than is usual for such systems. The aim is to determine what influence the rTWT has on the system’s energy efficiency, quantify the volume of hot water that the system is capable of supplying at the respective rTWT and establish whether SWH is feasible as a booster supply system for the different analysed rTWTs. To do this, a prototype water heating system has been designed, installed and commissioned and its performance monitored at different rTWTs under real operating conditions. The quantitative results show that a higher rTWT results in a lower energy supply to the tank, where the differences may be greater than 1000 Wh m-2 d-1 from 40 ºC to 80 ºC for insolation values of around 8000 Wh m-2 d-1 (system efficiency ranges from 73% to 56%). The drop in supply is due to lower collector efficiency and greater heat losses from the pipe system. As regards water supplied at the rTWT, the insolation required for the first withdrawal of water to take place is greater at higher rTWTs, where the time between withdrawals increases and the number of withdrawals decreases throughout the day. As rTWT increases, the volume of water supplied at the rTWT decreases due to factors such as lower collector efficiency, pipe system heat losses, energy stored in the water at below the rTWT and more energy being extracted from the system by water heating. For a rTWT of 80 ºC, much of the energy is stored in the tank at below the rTWT at the end of the day. A booster supply system would be required to take advantage of this energy, as overnight tank heat losses may significantly reduce the usable energy available on the following day. It is often not feasible to use the solar system as a single supply system, especially at high rTWTs, as, unlike the supply from the solar heating system which does not produce hot water on many days of the year because insolation is below the required minimum, hot water demand is not seasonal. On the other hand, investment in a solar system as a booster system to meet part of a plant’s heat energy demand is highly recommended. The solar system’s estimated annual usable energy ranges from 1322 kWh m-2 to 1084 kWh m-2. Cost efficiency would be greatest if there were an existing electric boiler, where the payback period would be just a few years —from 5.7 years at 40 ºC to 7.2 years at 80 ºC—. Cost efficiency is also high if there is an existing diesel boiler with payback periods of under 10 years. In a fictitious industry with a demand of 100 kWh day-1 and an existing diesel boiler, the investment in the solar plant would be highly recommended at any rTWT, with a net present value similar to investment costs —12000 € at 80 ºC and 15000 € at 40 ºC— and a payback period of 10 years. The results of this study are potentially very useful for determining the feasibility of using similar systems for meeting the hot water demand of agribusinesses and arable and livestock farms or for other applications demanding water at temperatures not typical of domestic demand (60ºC). Performance and cost efficiency will be determined by the regional insolation, the required water temperature and the demand curve of the specific processes in each case.

Initiation of clement surface conditions on the earliest Earth

In the beginning the surface of the Earth was extremely hot, because the Earth as we know it is the product of a collision between two planets, a collision that also created the Moon. Most of the heat within the very young Earth was lost quickly to space while the surface was still quite hot. As it cooled, the Earth's surface passed monotonically through every temperature regime between silicate vapor to liquid water and perhaps even to ice, eventually reaching an equilibrium with sunlight. Inevitably the surface passed through a time when the temperature was around 100°C at which modern thermophile organisms live. How long this warm epoch lasted depends on how long a thick greenhouse atmosphere can be maintained by heat flow from the Earth's interior, either directly as a supplement to insolation, or indirectly through its influence on the nascent carbonate cycle. In both cases, the duration of the warm epoch would have been controlled by processes within the Earth's interior where buffering by surface conditions played little part. A potentially evolutionarily significant warm period of between 105 and 107 years seems likely, which nonetheless was brief compared to the vast expanse of geological time.

A long marine history of carbon cycle modulation by orbital-climatic changes

Pacing of the marine carbon cycle by orbital forcing during the Pliocene and Pleistocene Ice Ages [past 2.5 million years (Myr)] is well known. As older deep-sea sediment records are being studied at greater temporal resolution, it is becoming clear that similar fluctuations in the marine carbon system have occurred throughout the late Mesozoic and Tertiary, despite the absence of large continental ice sheets over much of this time. Variations in both the organic and the calcium carbonate components of the marine carbon system seem to have varied cyclically in response to climate forcing, and carbon and carbonate time series appear to accurately characterize the frequency spectrum of ancient climatic change. For the past 35 Myr, much of the variance in carbonate content carries the “polar” signal of obliquity [41,000 years (41 kyr)] forcing. Over the past 125 Myr, there is evidence from marine sediments of the continued role of precessional (≈21 kyr) climatic cycles. Repeat patterns of sedimentation at about 100, 400, and 2,400 kyr, the modulation periods of precession, persistently enter into marine carbon cycle records as well. These patterns suggest a nonlinear response of climate and/or the sedimentation of organic carbon and carbonates to precessional orbital perturbations. Nonlinear responses of the carbon system may help to amplify relatively weak orbital insolation anomalies into more significant climatic perturbations through positive feedback effects. Nonlinearities in the carbon cycle may have transformed orbital-climatic cycles into long-wavelength features on time scales comparable to the residence times of carbon and nutrient elements in the ocean.

Climate simulation for 125 kyr BP with a coupled ocean-atmosphere general circulation model

The ECHAM-1 T21/LSG coupled ocean-atmosphere general circulation model (GCM) is used to simulate climatic conditions at the last interglacial maximum (Eemian. 125 kyr BP). The results reflect thc expected surface temperature changes (with respect to the control run) due to the amplification (reduction) of the seasonal cycle of insolation in the Northern (Southern) Hemisphere. A number of simulated features agree with previous results from atmospheric GCM simulations e.g. intensified summer southwest monsoons) except in the Northern Hemisphere poleward of 30 degrees N. where dynamical feedback, in the North Atlantic and North Pacific increase zonal temperatures about 1 degrees C above what would be predicted from simple energy balance considerations. As this is the same area where most of the terrestrial geological data originate, this result suggests that previous estimates of Eemian global average temperature might have been biased by sample distribution. This conclusion is supported by the fact that the estimated global temperature increase of only 0.3 degrees C greater than the control run ha, been previously shown to be consistent a with CLIMAP sea surface temperature estimates. Although the Northern Hemisphere summer monsoon is intensified. globally averaged precipitation over land is within about 1% of the present, contravening some geological inferences bur not the deep-sea delta(13)C estimates of terrestrial carbon storage changes. Winter circulation changes in the northern Arabian Sea. driven by strong cooling on land, are as large as summer circulation changes that are the usual focus of interest, suggesting that interpreting variations in the Arabian Sea. sedimentary record solely in terms of the summer monsoon response could sometimes lead to errors. A small monsoonal response over northern South America suggests that interglacial paleotrends in this region were not just due to El Nino variations.

Reconstituição da paleoprecipitação no sul do Nordeste Brasileiro durante os dois últimos ciclos glaciais a partir da aplicação de registros isotópicos de oxigênio de estalagmites da Chapada Diamantina, Bahia.

Registros isotópicos de oxigênio obtidos em alta resolução das estalagmites CL2 e MAG das cavernas Calixto e Marota, região da Chapada Diamantina (CD) (12ºS), Estado da Bahia, sul do Nordeste brasileiro (sNEB), permitiram reconstituir as mudanças passadas da precipitação entre 165-128 e 59-39 mil anos A.P. Para a reconstituição paleoclimática considerou-se resultados de um estudo de calibração realizado em duas cavernas da CD o qual demonstrou uma relação entre composição isotópica da água meteórica e de gotejamento e sugeriu um ambiente adequado para a deposição do espeleotema em condições equilíbrio e/ou próximas com a água de gotejamento. A interpretação da paleoprecipitação através dos registros isotópicos \'\'delta\' POT.18\'O das estalagmites também foi baseada na relação entre composição isotópica da água da precipitação e a quantidade de chuva obtidos em estações da IAEA-GNIP no Brasil e de simulações das variações do \'\'delta\' POT.18\'O da chuva através do modelo climático ECHAM-4. Esses dados indicaram o efeito quantidade (amount effect) como fator preponderante de controle isotópico da água da chuva que formam os espeleotemas na CD, significando que a diminuição dos valores de \'\'delta\' POT.18\'O está associada ao aumento do volume de chuvas e vice-versa. Os registros de \'\'delta\' POT.18\'O dos espeleotemas permitiram reconstituir a variação da paleoprecipitação na escala orbital e milenar durante o penúltimo glacial bem como correlacionar mudanças na paleoprecipitação no sNEB com eventos milenares registrados na Groelândia no último glacial. Os registros da CD indicaram um aumento (diminuição) da paleoprecipitação na Bahia relacionado a diminuição (aumento) da insolação austral de verão a 10ºS durante o penúltimo glacial, similar ao observado no último ciclo precessional. Na escala orbital os registros da CD estiveram em antifase com os paleoindicadores isotópicos do Sudeste brasileiro e em fase com os valores de\'\'delta\' POT.18\'O dos espeleotemas do leste da China. Esse padrão de precipitação é similar ao observado na última glaciação e sugere que a variação na insolação de verão afetou as monções sul-americanas (MSA) promovendo mudanças na precipitação no sNEB no penúltimo glacial. Condições áridas no sNEB durante o aumento da insolação de verão estariam provavelmente associadas ao aprofundamento da subsidência de ar provocado pelo fortalecimento da circulação leste-oeste da MSA devido ao aumento das atividades convectivas na Amazônia o que teria, favorecido um posicionamento mais a sul da Zona de Convergência do Atlântico Sul (ZCAS). O oposto também ocorreria durante as fases de baixa insolação de verão quando a MSA estaria provavelmente mais desintensificada. Durante o penúltimo glacial (Terminação Glacial II) abruptas oscilações nos registros da CD para valores mais baixos de \'\'delta\' POT.18\'O indicaram um profundo aumento da precipitação coincidente com o evento Heinrich (H11). Nesse período a paleoprecipitação no sNEB esteve correlacionada negativamente com as mudanças climáticas na China e no oeste amazônico (Peru) e positivamente com o Sudeste brasileiro. Interpretou-se que as anomalias positivas da precipitação no sNEB podem ter estado relacionadas ao deslocamento para sul da Zona de Convergência Intertropical (ZCIT) bem como com a intensificação da MSA e ZCAS nesse período. Finalmente, oscilações isotópicas abruptas para valores mais altos observadas durante o estágio marinho isotópico 3 coincidentes com os eventos quentes registrados na Groelândia, denominados de eventos Dansgaard-Oeschger (DO), foram interpretados como a ocorrência de eventos muito secos no sNEB. Essas variações da precipitação na escala milenar, que estão em fase com os registros no Peru, podem ter estado relacionadas ao deslocamento para norte da ZCIT o que teria promovido uma profunda desintensificação da MSA.