Polarimetry in the visible and infrared: application to CMB polarimetry

Interstellar polarization from aligned dust grains can be measured both in transmission at visible and near-infrared wavelengths and in emission at far-infrared and sub-mm wavelengths. These observations can help predict the behavior of foreground contamination of CMB polarimetry by dust in the Milky Way. Fractional polarization in emission from aligned dust grains will be at the higher range of currently observed values of 4–10%. Away from the galactic plane, fluctuations in Q and U will be dominated by fluctuations in intensity, and less influenced by fluctuations in fractional polarization and position angle.     

Lunar polarization studies at 3.1mm wavelength

Observations of the distribution of linearly polarized lunar thermal emission were made at a wavelength of 3.1 mm with The University of Texas 4.88 m parabolic reflector (0.042° HPBW). A shadow corrected, rough surface, thermal emission model for a homogeneous Moon was leastsquares-fitted to the polarization data. Results indicate an effective lunar dielectric constant of 1.34 ±0.04 with surface roughness characterized by a standard deviation of 17° ± 5° for surface slopes with a normal probability density, independent of lunar phase. A comparison of these results with published values at other wavelengths suggests that the effective lunar dielectric constant, as obtained by lunar emission measurements, decreases with decreasing wavelength of observation. This wavelength dependence may be interpreted in terms of an inhomogeneous surface and/or a surface that possesses intermediate scale surface roughness.This work was supported in part by NASA Grant NGL 44-012-006.     

The collisio operator and long-time behavior of a perturbed two-body problem

The nature of the collision operator for a classical mechanical system whose dynamics is represented by a probability density satisfying the Liouville equation is illustrated with a soluble example. This example is that of a two-body problem with a particular perturbation. The collision operator is found and the time reversibility of the system is examined utilizing the analysis of Stey. For negative energies, the collision operator is zero in the limitzi0⁺, while for zero energy, the collision operator is different from zero in that limit. This indicates that the system is reversible for negative energy and irreversible for zero energy.     

Stratospheric aerosol sulfuric acid: First direct in situ measurements using a novel balloon-based mass spectrometer apparatus

The first direct in situ measurements of the sulfuric acid contained in stratospheric aerosol particles were made using a novel balloon-based Ion Molecule Reaction Mass Spectrometer instrument (IMRMS) equipped with an aerosol vaporizer. The IMRMS method employed offers direct aerosol sulfuric acid measurements with high spatial resolution. The balloon flight took place on 23 October 1995 in middle latitudes (44°N) and reached a maximum altitude of 24 km. Measured molecular number densities of aerosol sulfuric acid decreased with increasing altitude from about 2.9 × 109 cm-3 at 15km altitude to about 2.4 × 108 cm-3 at 21 km. Corresponding mass mixing ratios are 2.5 and 0.6 ppbm, respectively. Calculated sulfuric acid mixing ratios from aerosol volumes inferred from aerosol size distribution measurements on the same balloon agree well with the IMRMS data using standard assumption aerosol composition.     

Molecular gas in the Perseus cooling flow galaxy, NGC 1275

The central arcminute of the Perseus cooling flow galaxy, NGC 1275, has been mapped with the JCMT in ¹²CO(2–1) at 21-arcsec resolution, with detections out to at least 36 arcsec (12 kpc). Within the limits of the resolution and coverage, the distribution of gas appears to be roughly east–west, consistent with previous observations of CO, X-ray, Hα and dust emission. The total detected molecular hydrogen mass is ∼ 1.6 × 10¹⁰ M_⊙, using a Galactic conversion factor. The inner central rotating disc is apparent in the data, but the overall distribution is not one of rotation. Rather, the line profiles are bluewards-asymmetric, consistent with previous observations in H  i and [O  iii ]. We suggest that the blueshift may be due to an acquired mean velocity of ∼ 150 km s⁻¹ imparted by the radio jet in the advancing direction. Within the uncertainties of the analysis, the available radio energy appears to be sufficient, and the interpretation is consistent with that of Bo¨hringer et al. for displaced X-ray emission. We have also made the first observations of ¹³CO(2–1) and ¹²CO(3–2) emission from the central 21-arcsec region of NGC 1275 and combined these data with IRAM data supplied by Reuter et al. to form line ratios over equivalent, well-sampled regions. An LVG radiative transfer analysis indicates that the line ratios are not well reproduced by single values of kinetic temperature, molecular hydrogen density and abundance per unit velocity gradient. At least two temperatures are suggested by a simple two-component LVG model, possibly reflecting a temperature gradient in this region.     

Asymptotic Expansions for the Calculation of the Transient Electromagnetic Fields Induced by a Vertical Magnetic Dipole Source Above a Conductive Halfspace

We have derived asymptotic expansions that can be used to estimate the impulse response of a conductive halfspace when excited by an airborne electromagnetic system. Two expressions are required to calculate the response, one is applicable in the late-time regime and a second is used for the early-time regime. Fortunately, there is a small overlap in the late- and early-time regimes. Asymptotic expansions are commonly used for interpreting ground EM data, but our expressions are the first ones applicable to the airborne situation. The expansions are simple to program, can be calculated extremely rapidly and will be useful for understanding and interpreting airborne electromagnetic data. As an example of the use of the expressions, we have calculated the response of seawater and compared this with the airborne electromagnetic response measured off the coast of Perth, Western Australia.     

Plankton distribution associated with frontal zones in the vicinity of the Pribilof Islands

We studied the effect of four types of fronts, the coastal front, the middle front, the shelf partition front and the shelf break front on the quantitative distribution and the composition of plankton communities in the Pribilof area of the eastern Bering Sea shelf in late spring and summer of 1993 and 1994. The coastal fronts near St. Paul and St. George Islands and the coastal domains encircled by the fronts featured specific taxonomic composition of planktonic algae, high abundance and production of phytoplankton, as well as large numbers of heterotrophic nanoplankton. The coastal fronts also were characterized by high values of total mesozooplankton biomass, high concentrations of Calanus marshallae, as well as relatively high abundances of Parasagitta setosa and Euphausiacea compared to surrounding shelf waters. We hypothesize that wind-induced erosion of a weak thermocline in the inner part of the coastal front as well as transfrontal water exchange in subthermocline layers result in nutrient enrichment of the euphotic layer in the coastal fronts and coastal domains in summer time. This leads to prolonged high primary production and high phytoplankton biomass. In this paper a new type of front—the shelf partition front located 45–55 km to the north-east off St. Paul Island—is described, which is assumed to be formed by the flux of oceanic domain waters onto the shelf. This front features a high abundance of phytoplankton and a high level of primary production compared to the adjacent middle shelf. Near the southwestern periphery of the front a mesozooplankton peak occurred, composed of C. marshallae, with biomass in the subthermocline layer, reaching values typical for the shelf break front and the highest for the area. High abundance of phyto- and zooplankton as well as heterotrophic nanoplankton and elevated primary production were most often observed in the area adjacent to the shelf break front at its oceanic side. The phyto- and mesozooplankton peaks here were formed by oceanic community species. The summer levels of phytoplankton numbers, biomass and primary production in the shelf break frontal area were similar to those reported for the outer and middle shelf during the spring bloom and the coastal domains and coastal fronts in summer. In the environment with a narrow shelf to the south of St. George Island, the mesozooplankton peak was observed at the inner side of the shelf break front as close as 20 km from the island shore and was comprised of a “mixed” community of shelf and oceanic species. The biomass in the peak reached the highest values for the Pribilof area at 2.5 g mean wet weight m⁻³ in the 0–100 m layer. Details of the taxonomic composition and the numbers and production of phytoplankton hint at the similarity of processes that affect the phytoplankton summer community in the coastal domains of the islands, at the coastal fronts, and at the oceanic side of the shelf break front. The middle front was the only one that had no effect on plankton composition or its quantitative characteristics in June and July. Location of a variety of frontal productive areas within 100 km of the Pribilof Islands creates favorable foraging habitat for higher trophic level organisms, including sea birds and marine mammals, populating the islands.     

Role of lipid/water partitioning and membrane composition in the uptake of organochlorine pesticides into a freshwater mussel

The aim of this investigation is to understand the factors influencing uptake of persistent organochlorine pesticides into a freshwater mussel (Sphaerium corneum). Previous work has shown that although a substantial proportion of dieldrin is bound to particulates in the river system, uptake is from the dieldrin in solution. This suggests partitioning of the hydrophobic xenobiotics into membranes as the major route of entry. Membrane composition was established using lipid fractionation into neutral lipids and phospholipids followed by derivatisation to fatty acid methyl esters and estimation using GC/FID. Membrane composition varied with acclimation temperature over the range 5–20°C. Dieldrin concentrations in the mussel at equilibrium with 2000 ng dieldrin/litre water burden were studied at one temperature under laboratory conditions using animals acclimated to different temperatures. Any differences may be explicable in terms of effects of membrane composition on partitioning or other physiological adaptations. To establish which of these factors is most significant a membrane fragment partition system has been analysed in vitro. Preliminary results indicate that although water/lipid partitioning may be important in entry (and exit) of non-polar xenobiotics, significant differences could not be found using current methods. The role of membrane composition and therefore temperature history of the organism may still be significant. The implications of this for attempted correlations between bioaccumulation factors and simple octanol/water partition coefficients are discussed.     

Indigenous peoples and food entitlement losses under the impact of externally-induced change

Three issues related to hunger, famine and food security are highlighted by the problems faced by indigenous peoples in many parts of the world. They affect not only the indigenous groups themselves, but also the potential for improved and increased food availability for the rest of humankind. First, indigenous peoples themselves continue to be subjected to the shock impact of outsiders in ways that remove their traditional access to land and other resources, especially those that provide customary sources of foods. The shock is therefore very negative in nutritional as well as the better-known cultural and health terms. Second, the destruction and disruption of many indigenous peoples is reducing the pool of knowledge (ethnoschience) available concerning the biosphere and natural resources, which is of widespread value to humanity. Thirdly, this compounds the already well-known shock impact of the invaders on those natural resources through environmental destruction and habitat alteration. These issues have a potential impact on global sustainability that is far greater than might be suggested by the small numbers of indigenous peoples involved. The paper argues for priority to be given to the links between hunger and food problems, the human rights of indigenous peoples, and environmental destruction.An earlier verison of this paper was published in Hans-Georg Bohle (ed.).World of Pain and Hunger: geographical perspectives on famine and food security. Saarbrücken/Fort Lauderdale: Breitenbach Publishers, Freiburg Series in Development Studies, 1 (1994)I would like to acknowledge the support of the ESRC (UK), the IGU, the University of Greenwich, and the Henry R. Luce Food Programme at Hampshire College (USA) for enabling me to attend the IGU Workshop at which this was presented. This paper has benefitted from the helpful criticisms of members of that workshop, and of other colleagues in Britain and The Netherlands; I remain responsible for its opinions and any errors.     

IBC arrays: Present and future prospects

The development of arrays which operate at wavelengths longer than 8 m has opened up new possibilities for imaging and spectroscopy but offers challenges not present at shorter wavelengths. Impurity Band Conduction (IBC) or Blocked-Impurity-Band (BIB) detectors can meet these challenges and offer numerous advantages over standard photoconductors. We review some of the general operating principles of these devices and discuss the current state of technology. We then discuss the requirements placed on mid-infrared arrays by groundbased, airborne and spacebased astronomy.