Report of the Inter-American Tropical Tuna Commission for the year 1952

ENGLISH: The Inter-American Tropical Tuna Commission, established by a Convention between the United States and Costa Rica, has as its purpose the collection and interpretation of information which will facilitate maintaining, at levels of maximum sustained yield, the populations of tropical tunas in the Eastern Pacific and of the bait species used in their capture. To this end, the Commission is directed by the Convention to undertake investigations of the tunas and bait species, and to make recommendations for joint action by the member governments designed to attain the objectives of the Convention. The year 1952 is the second since the initiation of the investigations of the Commission. The Commission was organized in 1950. Its program of investigations ~as outlined and work commenced during 1951. The work during 1952 has been a continuation and logical development of the research commenced the previous year. SPANISH: La Comisión Interamericana del Atún Tropical, establecida por una Convención entra Costa Rica y los Estados Unidos de América, tiene como deberes recolectar e interpretar la información que facilite el mantenimiento, a niveles de una contínua producción máxima, de las poblaciones de las especies tropicales de atún en el Pacífico Oriental y de los peces de carnada que se emplean para su pesca. Con este propósito la Comisión se encarga, en conformidad con los términos de la antes expresada Convención de efectuar investigaciones sobre los atunes y mencionadas especies de carnada, y de hacer recomendaciones a los Gobiernos Miembros a fin de que pueden tomar una acción conjunta que les permita obtener los resultados que el citado Convenio persigue. El año 1952 es el segundo desde la iniciación de las investigaciones de la Comisión. Esta fué organizada en 1950. Durante 1951 se preparó el programa de estudios y se comenzaron los trabajos. La tarea realizada en el año 1952 ha sido una continuación y lógico desarrollo de las investigaciones empezadas en el año anterior. (PDF contains 61 pages.)

Interpretation of lunar topography : impact cratering and surface roughness

This work seeks to understand past and present surface conditions on the Moon using two different but complementary approaches: topographic analysis using high-resolution elevation data from recent spacecraft missions and forward modeling of the dominant agent of lunar surface modification, impact cratering. The first investigation focuses on global surface roughness of the Moon, using a variety of statistical parameters to explore slopes at different scales and their relation to competing geological processes. We find that highlands topography behaves as a nearly self-similar fractal system on scales of order 100 meters, and there is a distinct change in this behavior above and below approximately 1 km. Chapter 2 focuses this analysis on two localized regions: the lunar south pole, including Shackleton crater, and the large mare-filled basins on the nearside of the Moon. In particular, we find that differential slope, a statistical measure of roughness related to the curvature of a topographic profile, is extremely useful in distinguishing between geologic units. Chapter 3 introduces a numerical model that simulates a cratered terrain by emplacing features of characteristic shape geometrically, allowing for tracking of both the topography and surviving rim fragments over time. The power spectral density of cratered terrains is estimated numerically from model results and benchmarked against a 1-dimensional analytic model. The power spectral slope is observed to vary predictably with the size-frequency distribution of craters, as well as the crater shape. The final chapter employs the rim-tracking feature of the cratered terrain model to analyze the evolving size-frequency distribution of craters under different criteria for identifying "visible" craters from surviving rim fragments. A geometric bias exists that systematically over counts large or small craters, depending on the rim fraction required to count a given feature as either visible or erased.

A qualificação do lucro da intervenção:responsabilidade civil ou enriquecimento sem causa?

O presente estudo tem por objetivo demonstrar que, nas hipóteses em que alguém intervém na esfera jurídica alheia e obtém benefícios econômicos sem causar danos ao titular do direito ou, causando danos, o lucro obtido pelo ofensor é superior aos danos causados, as regras da responsabilidade civil, isoladamente, não são suficientes, à luz do ordenamento jurídico brasileiro, enquanto sanção eficaz pela violação de um interesse merecedor de tutela. Isto porque, como a principal função da responsabilidade civil é remover o dano, naquelas hipóteses, não fosse a utilização de um remédio alternativo, o interventor faria seu o lucro da intervenção, no primeiro caso integralmente e, no segundo, no valor equivalente ao saldo entre o lucro obtido e a indenização que tiver que pagar à vítima. A tese pretende demonstrar que o problema do lucro da intervenção não deve ser solucionado por intermédio das regras da responsabilidade civil, devendo, portanto, ser rejeitadas as propostas de solução neste campo, como a interpretação extensiva do parágrafo único, do artigo 944, do Código Civil, as indenizações punitivas e o chamado terceiro método de cálculo da indenização. Como alternativa, propõe-se o enquadramento dogmático do lucro da intervenção no enriquecimento sem causa, outorgando ao titular do direito uma pretensão de restituição do lucro obtido pelo ofensor em razão da indevida ingerência em seus bens ou direitos. Defende-se que a transferência do lucro da intervenção para o titular do direito tem por fundamento a ponderação dos interesses em jogo à luz da Constituição Federal, com especial atenção ao princípio da solidariedade, e da teoria da destinação jurídica dos bens. A tese procura demonstrar, ainda, que o ordenamento jurídico brasileiro não exige um efetivo empobrecimento do titular do direito para a configuração do enriquecimento sem causa e que a regra da subsidiariedade não impede a cumulação de ações, de responsabilidade civil para eliminar o dano (e no limite do dano), e de enriquecimento sem causa, para forçar a restituição do saldo positivo que permanecer no patrimônio do ofensor após o pagamento da indenização, se houver. Finalmente, a tese pretende provocar a discussão acerca da quantificação do objeto da restituição, propondo alguns critérios que deverão orientar o aplicador do direito.

An investigation of techniques for the measurement and interpretation of cosmic ray isotopic abundances

An instrument, the Caltech High Energy Isotope Spectrometer Telescope (HEIST), has been developed to measure isotopic abundances of cosmic ray nuclei in the charge range 3 ≤ Z ≤ 28 and the energy range between 30 and 800 MeV/nuc by employing an energy loss -- residual energy technique. Measurements of particle trajectories and energy losses are made using a multiwire proportional counter hodoscope and a stack of CsI(TI) crystal scintillators, respectively. A detailed analysis has been made of the mass resolution capabilities of this instrument.

Landau fluctuations set a fundamental limit on the attainable mass resolution, which for this instrument ranges between ~.07 AMU for z~3 and ~.2 AMU for z~2b. Contributions to the mass resolution due to uncertainties in measuring the path-length and energy losses of the detected particles are shown to degrade the overall mass resolution to between ~.1 AMU (z~3) and ~.3 AMU (z~2b).

A formalism, based on the leaky box model of cosmic ray propagation, is developed for obtaining isotopic abundance ratios at the cosmic ray sources from abundances measured in local interstellar space for elements having three or more stable isotopes, one of which is believed to be absent at the cosmic ray sources. This purely secondary isotope is used as a tracer of secondary production during propagation. This technique is illustrated for the isotopes of the elements O, Ne, S, Ar and Ca.

The uncertainties in the derived source ratios due to errors in fragmentation and total inelastic cross sections, in observed spectral shapes, and in measured abundances are evaluated. It is shown that the dominant sources of uncertainty are uncorrelated errors in the fragmentation cross sections and statistical uncertainties in measuring local interstellar abundances.

These results are applied to estimate the extent to which uncertainties must be reduced in order to distinguish between cosmic ray production in a solar-like environment and in various environments with greater neutron enrichments.

Constraining the interpretation of 2-methylhopanoids through genetic and phylogenetic methods

Hopanoids are a class of sterol-like lipids produced by select bacteria. Their preservation in the rock record for billions of years as fossilized hopanes lends them geological significance. Much of the structural diversity present in this class of molecules, which likely underpins important biological functions, is lost during fossilization. Yet, one type of modification that persists during preservation is methylation at C-2. The resulting 2-methylhopanoids are prominent molecular fossils and have an intriguing pattern over time, exhibiting increases in abundance associated with Ocean Anoxic Events during the Phanerozoic. This thesis uses diverse methods to address what the presence of 2-methylhopanes tells us about the microbial life and environmental conditions of their ancient depositional settings. Through an environmental survey of hpnP, the gene encoding the C-2 hopanoid methylase, we found that many different taxa are capable of producing 2-methylhopanoids in more diverse modern environments than expected. This study also revealed that hpnP is significantly overrepresented in organisms that are plant symbionts, in environments associated with plants, and with metabolisms that support plant-microbe interactions; collectively, these correlations provide a clue about the biological importance of 2-methylhopanoids. Phylogenetic reconstruction of the evolutionary history of hpnP revealed that 2-methylhopanoid production arose in the Alphaproteobacteria, indicating that the origin of these molecules is younger than originally thought. Additionally, we took genetic approach to understand the role of 2-methylhopanoids in Cyanobacteria using the filamentous symbiotic Nostoc punctiforme. We found that hopanoids likely aid in rigidifying the cell membrane but do not appear to provide resistance to osmotic or outer membrane stressors, as has been shown in other organisms. The work presented in this thesis supports previous findings that 2-methylhopanoids are not biomarkers for oxygenic photosynthesis and provides new insights by defining their distribution in modern environments, identifying their evolutionary origin, and investigating their role in Cyanobacteria. These efforts in modern settings aid the formation of a robust interpretation of 2-methylhopanes in the rock record.