OGO-6 gas-surface energy transfer experiment

The kinetic energy flux of the upper atmosphere was analyzed using OGO-6 data. Energy transfer between 10 microwatts/sq cm and 0.1 W/sq cm was measured by short-term frequency changes of temperature-sensitive quartz crystals used in the energy transfer probe. The condition of the surfaces was continuously monitored by a quartz crystal microbalance to determine the effect surface contamination had on energy accommodation. Results are given on the computer analysis and laboratory tests performed to optimize the operation of the energy transfer probe. Data are also given on the bombardment of OGO-6 surfaces by high energy particles. The thermoelectrically-cooled quartz crystal microbalance is described in terms of its development and applications

Localization of Interaction using Fibre-Optic Shape Sensing in Soft-Robotic Surgery Tools

Minimally invasive surgery requires real-time tool tracking to guide the surgeon where depth perception and visual occlusion present navigational challenges. Although vision-based and external sensor-based tracking methods exist, fibre-optic sensing can overcome their limitations as they can be integrated directly into the device, are biocompatible, small, robust and geometrically versatile. In this paper, we integrate a fibre Bragg grating-based shape sensor into a soft robotic device. The soft robot is the pneumatically attachable flexible (PAF) rail designed to act as a soft interface between manipulation tools and intra-operative imaging devices. We demonstrate that the shape sensing fibre can detect the location of the tools paired with the PAF rail, by exploiting the change in curvature sensed by the fibre when a strain is applied to it. We then validate this with a series of grasping tasks and continuous US swipes, using the system to detect in real-time the location of the tools interacting with the PAF rail. The overall location-sensing accuracy of the system is 64.6%, with a margin of error between predicted location and actual location of 3.75 mm

Far Ultraviolet Absolute Flux of alpha Virginis

We present the far ultraviolet spectrum of alpha Virginis taken with EURD spectrograph on-board MINISAT-01. The spectral range covered is from ~900 to 1080 A with 5 A spectral resolution. We have fitted Kurucz models to IUE spectra of alpha Vir and compared the extension of the model to our wavelengths with EURD data. This comparison shows that EURD fluxes are consistent with the prediction of the model within 20-30%, depending on the reddening assumed. EURD fluxes are consistent with Voyager observations but are ~60% higher than most previous rocket observations of alpha Vir.Comment: 13 pages, 4 figures. Submitted to The Astrophysical Journa

Unveiling the Active Nucleus of Centaurus A

We report new HST WFPC2 and NICMOS observations of the center of the nearest radio galaxy Centaurus A (NGC 5128) and discuss their implications for our understanding of the active nucleus and jet. We detect the active nucleus in the near-IR (K and H) and, for the first time, in the optical (I and V), deriving the spectral energy distribution of the nucleus from the radio to X-rays. The optical and part of the near-IR emission can be explained by the extrapolation of the X-ray power law reddened by A_V~14mag, a value consistent with other independent estimates. The 20pc-scale nuclear disk discovered by Schreier et al. (1998) is detected in the [FeII] 1.64mic line and presents a morphology similar to that observed in Pa alpha with a [FeII]/Pa alpha ratio typical of low ionization Seyfert galaxies and LINERs. NICMOS 3 Pa alpha observations in a 50"x50" circumnuclear region suggest enhanced star formation (~0.3Msun/yr) at the edges of the putative bar seen with ISO, perhaps due to shocks driven into the gas. The light profile, reconstructed from V, H and K observations, shows that Centaurus A has a core profile with a resolved break at ~4" and suggests a black--hole mass of ~10^9 Msun. A linear blue structure aligned with the radio/X-ray jet may indicate a channel of relatively low reddening in which dust has been swept away by the jet.Comment: 19 pages, 13 figures, Astrophysical Journal, in press. High quality figures available at http://www.arcetri.astro.it/~marconi/colpic.htm

The Coronae of AR Lac

We observed the coronally active eclipsing binary, AR Lac, with the High Energy Transmission Grating on Chandra for a total of 97 ks, spaced over five orbits, at quadratures and conjunctions. Contemporaneous and simultaneous EUV spectra and photometry were also obtained with the Extreme Ultraviolet Explorer. Significant variability in both X-ray and EUV fluxes were observed, dominated by at least one X-ray flare and one EUV flare. We saw no evidence of primary or secondary eclipses. X-ray flux modulation was largest at high temperature, indicative of flare heating of coronal plasma. Line widths interpreted in terms of Doppler broadening suggest that both binary stellar components are active. From line fluxes obtained from total integrated spectra, we have modeled the emission measure and abundance distributions. A strong maximum was found in the differential emission measure, characterized by peaks at log T = 6.9 and 7.4, together with a weak but significant cooler maximum near log T=6.2, and a moderately strong hot tail from log T= 7.6-8.2. Coronal abundances have a broad distribution and show no simple correlation with first ionization potential. While the resulting model spectrum generally agrees very well with the observed spectrum, there are some significant discrepancies, especially among the many Fe L-lines. Both the emission measure and abundance distributions are qualitatively similar to prior determinations from other X-ray and ultraviolet spectra, indicating some long-term stability in the overall coronal structure.Comment: 31 pages, 8 figures, 3 tables; Accepted for publication in the Astrophysical Journal (tentatively October 1, 2003

Diet and Habitat of Mountain Woodland Caribou Inferred from Dung Preserved in 5000-year-old Alpine Ice in the Selwyn Mountains, Northwest Territories, Canada

Alpine ice patches are unique repositories of cryogenically preserved archaeological artefacts and biological specimens. Recent melting of ice in the Selwyn Mountains, Northwest Territories, Canada, has exposed layers of dung accumulated during seasonal use of ice patches by mountain woodland caribou of the ancestral Redstone population over the past ca. 5250 years. Although attempts to isolate the DNA of known caribou parasites were unsuccessful, the dung has yielded numerous well-preserved and diverse plant remains and palynomorphs. Plant remains preserved in dung suggest that the ancestral Redstone caribou population foraged on a variety of lichens (30%), bryophytes and lycopods (26.7%), shrubs (21.6%), grasses (10.5%), sedges (7.8%), and forbs (3.4%) during summer use of alpine ice. Dung palynomorph assemblages depict a mosaic of plant communities growing in the caribou’s summer habitat, including downslope boreal components and upslope floristically diverse herbaceous communities. Pollen and spore content of dung is only broadly similar to late Holocene assemblages preserved in lake sediments and peat in the study region, and differences are likely due to the influence of local vegetation and animal forage behaviour. The 5000-year legacy of summer use of alpine ice patches by mountain woodland caribou suggests that these small, long-lived features may be important for the health of caribou populations in the Selwyn/Mackenzie Mountain range.Les névés des régions alpines constituent des réserves uniques d’artefacts archéologiques et de spécimens biologiques préservés cryogéniquement. La fonte récente des glaces de la chaîne de Selwyn, dans les Territoires du Nord-Ouest, au Canada, a mis au jour des couches de déjections animales qui ont été accumulées lors de l’usage saisonnier des névés par le caribou des bois des montagnes de la population ancestrale de Redstone au cours des quelques 5 250 dernières années. Bien que les tentatives visant à isoler l’ADN des parasites connus du caribou aient échoué, les déjections ont permis de repérer de nombreux restes et palynomorphes de végétaux bien préservés et variés. Les restes de végétaux qui ont été conservés dans les déjections animales laissent croire que la population de caribou ancestrale de Redstone s’alimentait d’une variété de lichens (30 %), de bryophytes et de lycopodes (26,7 %), d’arbrisseaux (21,6 %), de graminées (10,5 %), de foin plat (7,8 %) et de plantes herbacées non graminoïdes (3,4 %) lorsqu’ils utilisaient la glace alpine pendant l’été. Les assemblages de palynomorphes provenant des déjections laissent entrevoir la croissance d’une mosaïque de peuplements végétaux au sein de l’habitat d’été du caribou, ce qui comprend des composantes boréales en pentes descendantes et des peuplements végétaux herbacés floristiquement variés en pentes ascendantes. La teneur en pollen et en spores des déjections animales est seulement largement similaire aux assemblages de l’Holocène tardif préservés dans les sédiments lacustres et dans la tourbe de la région visée par l’étude. Les différences sont vraisemblablement attribuables à l’influence de la végétation locale et au comportement alimentaire des animaux. L’utilisation estivale des névés des régions alpines par le caribou des bois des montagnes ces 5 000 dernières années laisse entrevoir que ces petites caractéristiques longévives pourraient revêtir de l’importance pour la santé des populations de caribou de la chaîne de Selwyn et des monts Mackenzie