Infrared extinction of heavy ion irradiated and amorphous olivine,with applications to interstellar dust

A smooth surface layer of highly disordered olivine, (Mg, Fe)₂SiO₄, has been produced by exposure of polished, natural olivine to a dose of 5×10¹⁶ cm^–2 of 1.5 MeV neon ions from a Van de Graaff accelerator. The dielectric functions of the disordered silicate in the wavelength range from 8 to 30 m have been determined from analysis of specular reflectance data, and extinction for Rayleigh particles of such disordered olivine has been calculated. Extinction measurements for amorphous olivine smoke collected on a substrate are also presented. The small particle extinctions of both kinds of structurally disordered olivine are shown to agree well with the main features of the absorption and emission spectra from interstellar grains in the 10 and 20 m region.     

Response of the uppermost mantle to Indo-Eurasian collisional tectonics

The rheological law for the power law creep field of peridotite suggested by Chopra and Paterson (1981, 1984) is combined with theoretically modelled thermal and stress perturbations for continent-continent collisions (Bird et al., 1975; Bird, 1978a) to determine the effect of such collisions on the uppermost mantle below the zone of convergence. The model predicts a change from continental to oceanic geotherms during the oceanic subduction phase, followed by a rapid rise in differential stress during the collisional phase.These perturbations, when combined, cause a cyclical change in the steady state flow of the uppermost mantle ending with a re-equilibration of thermal and stress regimes. The thermal re-equilibration proceeds at a much slower rate, with a suggested total re-equilibration period of about 100 m.y. after collision has ceased. The combination of the flow law with the model predicts that the perturbations in the mantle are limited in depth with no changes in mantle behavior below about 100 km.     

Mossbauer detection of goethite (α-FeOOH) in coal and its potential as an indicator of coal oxidation

Mössbauer spectroscopy of three suites of oxidized coals shows that the transformation of pyrite to FeOOH correlates with other parameters of oxidation. As pyrite is very common in coals and the transformation to FeOOH is sensitive to small degrees of oxidation, the Mössbauer technique shows considerable promise as a means for the detection of coal oxidation.     

Climate change influences on agricultural research productivity

This paper investigates the impacts of climate change on US returns to research investments on agricultural productivity. We examine this using a historical data set in a panel time-series econometric model of state agricultural productivity. The fitted model allows derivation of the rate of return to research investments and the effects of climate change thereon. We find climate change is altering the rate of return to public agricultural research in a spatially heterogeneous manner. Increases in precipitation raise returns to research, while the impact of higher temperatures varies by region, are negative in Southern areas, particularly the Southern Plains, and positive in northern areas. We simulate the impact of projected climate change and find cases where agricultural productivity is reduced, for example in the Southern Plains. Finally, we consider the amount of research investment that is needed to adapt to overcome the impacts of climate change on agricultural productivity. Under the 2100 scenario, a 7–17 % increase in total US research investment is needed to adapt, but effects by region differ greatly—some requiring little changes and the Southern Plain requiring an increase as high as 57 %.     

Optical properties of particulates

Optical properties of small particles of olivine (less than 0.1 μ) have been studied in the ultraviolet as an example of an insulating solid. Very little structure survives in the ultraviolet extinction curves for such small particles. By contrast ‘surface modes’, observed for graphite small particles in the ultraviolet and for olivine particles in the infrared, produce dominant and persistent structure in extinction. The general trend of optical properties of graphite is surprisingly similar to the behavior required to explain all features of the interstellar extinction and albedo curves from near visible to 1000 Å. Measured extinction of small olivine particles in the infrared agrees with calculations based on newly measured optical constants, but dominant sharp structure in the 10μ region still presents a bit of a problem in explaining ‘silicate’ features in astronomical data.     

Single close encounters in the planetary problem

We consider a large massM and two small massesm ₁ andm ₂ (m ₁ m ₂;m ₁,m ₂M). The orbit ofm ₁ is initially circular and the motion ofm ₂ hyperbolic with respect toM. The orbital elements of the small masses are strongly modified after a close, single encounter betweenm ₁ andm ₂.An approximative method, similar to the theory of stellar encounters, is used to determine the probabilities of collisions, hyperbolas, direct and retrograde ellipses, as well as the mean values of the semimajor axes and their root mean square deviation after the encounter.The results are close to those which are obtained if the massm ₂ is negligibly small, (Mm ₁m ₂;m ₂ 0), as should be also expected on general grounds.     

Characterizing the severe turbulence environments associated with commercial aviation accidents. A real-time turbulence model (RTTM) designed for the operational prediction of hazardous aviation turbulence environments

Summary In this paper, we will focus on the real-time prediction of environments that are predisposed to producing moderate-severe (hazardous) aviation turbulence. We will describe the numerical model and its postprocessing system that is designed for said prediction of environments predisposed to severe aviation turbulence as well as presenting numerous examples of its utility. The purpose of this paper is to demonstrate that simple hydrostatic precursor circulations organize regions of preferred wave breaking and turbulence at the nonhydrostatic scales of motion. This will be demonstrated with a hydrostatic numerical modeling system, which can be run in real time on a very inexpensive university computer workstation employing simple forecast indices. The forecast system is designed to efficiently support forecasters who are directing research aircraft to measure the environment immediately surrounding turbulence. The numerical model is MASS version 5.13, which is integrated over three different grid matrices in real-time on a university workstation in support of NASA-Langley’s B-757 turbulence research flight missions. The model horizontal resolutions are 60, 30, and 15 km and the grids are centered over the region of operational NASA-Langley B-757 turbulence flight missions. The postprocessing system includes several turbulence-related products including four turbulence forecasting indices, winds, streamlines, turbulence kinetic energy, and Richardson numbers. Additionally there are convective products including precipitation, cloud height, cloud mass fluxes, lifted index, and K-index. Furthermore, soundings, sounding parameters, and Froude number plots are also provided. The horizontal cross section plot products are provided from 16,000–46,000 feet in 2,000 feet intervals. Products are available every three hours at the 60 and 30 km grid interval and every 1.5 hours at the 15 km grid interval. The model is initialized from the NWS ETA analyses and integrated two times a day.     

The effects of suspended sediment on brown trout (Salmo trutta) feeding and respiration after macrophyte control

Sediment resuspension during and after mechanical excavation of macrophytes may have a significant impact on resident fish populations. Unfortunately, little is known about the influence of this sediment on the respiratory performance and feeding abilities of fishes in New Zealand waterways. We examined the effects of suspended sediment (SS) concentrations previously observed after a large-scale macrophyte removal operation on oxygen consumption (MO₂) and feeding rates of brown trout (Salmo trutta). MO₂ at 0 mg L^?1, 150 mg L^?1, 300 mg L^?1, 450 mg L^?1 and 600 mg L^?1 of SS was measured using semi-closed respirometry. Feeding rates at the same SS concentrations were also measured using laboratory tank experiments. Results suggest that SS concentrations up to 600 mg L^?1 have no effect on MO₂. Conversely, feeding rates were significantly reduced at 450 mg L^?1 (22% reduction) and 600 mg L^?1 (31% reduction), indicating that sediment concentrations above 450 mg L^?1 may negatively affect brown trout populations.     

An archeomagnetic analysis of burnt grain bin floors from ca. 1200 to 1250 AD Iron-Age South Africa

Recognition of the rapid decay of Earth’s magnetic field over the last 150 years, chronicled in magnetic observatory and satellite data, highlights the need for a higher resolution record of geomagnetic field behavior over the past millennium. Such a record would help us better understand the nature of the recent dramatic changes. A limitation of the existing database is undersampling of the Southern Hemisphere. Here we investigate the potential of obtaining archeomagnetic data from Iron-Age burnt grain bins from southern Africa. These structures preserve oriented material that can record both paleodirections and paleointensity information. Directional data collected from three sites (ca. 1200–1250 AD) fall 9–22° to the East of predictions. Thellier–Coe and Shaw paleointensity results differ from model values by ～15%. The consistency of results between the three sites suggests that further investigations of these materials with different ages could markedly improve the current spatial distribution of the archeomagnetic database.     

Observations on low-temperature oxidation of minerals in bituminous coals

Mineral matter in three naturally weathered coals from Pennsylvania strip mines and in two laboratory-oxidized coals has been characterized by ⁵⁷Fe Mössbauer spectroscopy, scanning electron microscopy and other techniques to determine mineralogical trasnformations that occur in coals during weathering. Pyrite was found to be the most readily oxidized mineral, forming a variety of iron sulfates initially and geethite eventually. The iron sulfates formed were different in the two laboratory-oxidized coals, despite identical oxidation treatments. Calcite disappeared from one calcite-rich coal with increasing oxidation, but was not replaced by an equivalent amount of gypsum. A severely weathered strip-mine coal was enriched in calcium, which was dispersed through the oxidized macerals. Extended X-ray absorption fine-structure spectroscopy indicated that this dispersed calcium was most likely present as salts of carboxylic acids. Siderite was suprisingly resistant to oxidation at room temperature. Less direct evidence indicates that clay minerals also take part in the alteration to some extent.The coals oxidized in the laboratory showed alteration behavior that differed in a number of respects from that of the strip-mine coals. For example, iron sulfates were much less common in the latter coals; also, the formation of geothite appeared to be controlled to a large extent by the pyrite particle size in the strip-mine coals, but not in the laboratory-oxidized coals.The oxidation of an individual pyrite grain is not only a function of general conditions (temperature, humidity, oxygen partial pressure), but also the immediate local (< 1 mm) chemistry, as a variety of iron sulfates were observed in the coals, often in close proximity. Also, assemblages of gypsum and goethite were observed in otherwise slightly oxidized coal, which indicates that the alteration of pyrite and calcite, when in close contact, proceeds most rapidly.