Provisional specification for satellite time in a geomagnetic environment

Satellites in geosynchronous orbit were experiencing operational anomalies. These anomalies are believed to be due to the environment charging the spacecraft surfaces to a point where discharges occur. In designing future satellites for long term operation at geosynchronous altitude, it is important that designers have a specification that will give the total time per year, the particle flux density and particle energies that their satellites can be expected to encounter in these substorm environmental conditions. The limited data currently available on the environmental conditions are used to generate the provisional specification given in this report

Provisional specification for satellite time in a geomagnetic substorm environment

Satellites in geosynchronous orbit have been experiencing operational anomalies. These anomalies are believed to be due to the environment charging the spacecraft surfaces to a point where discharges occur. In designing future satellites for long term operation at geosynchronous altitude, it is important that designers have a specification that will give the total time per year, the particle flux density, and particle energies that their satellites can be expected to encounter in these substorm environmental conditions. The limited data currently available on the environmental conditions was used to generate the provisional specification given

Manufacturing Multiple View Constraints

In this paper we present an algorithm for the generation of the multiple view constraints for arbitrary configurations of cameras and image features correspondences. Multiple view constraints are an important commodity in computer vision since they facilitate in determining camera locations using only the correspondences between common features observed in sets of uncalibrated images. We show that by a series of counting arguments and a systematic application of the principles of antisymmetric algebra it is possible to generate arbitrary multiple view constraints in a completely automated fashion. The algorithm has already been utilized to discover new sets of multiple view constraints for surfaces

Understanding HMM Training For Video Gesture Recognition

When developing a video gesture recognition system to recognise letters of the alphabet based on hidden Markov Model (HMM) pattern recognition, we observed that by carefully selecting the model structure we could obtain greatly improved recognition performance. This led us to the questions: Why do some HMMs work so well for pattern recognition? Which factors affect the HMM training process? In an attempt to answer these fundamental questions of learning, we used simple triangle and square video gestures where good HMM structure can be deduced analytically from knowledge of the physical process. We then compared these analytic models to models estimated from Baum-Welch training on the video gestures. This paper shows that with appropriate constraints on model structure, Baum-Welch reestimation leads to good HMMs which are very similar to those obtained analytically. These results corroborate earlier work where we show that the LR banded HMM structure is remarkably effective in recognising video gestures when compared to fully-connected (ergodic) or LR HMM structures

PMN J1632-0033: A new gravitationally lensed quasar

We report the discovery of a gravitationally lensed quasar resulting from our survey for lenses in the southern sky. Radio images of PMN J1632-0033 with the VLA and ATCA exhibit two compact, flat-spectrum components with separation 1.47" and flux density ratio 13.2. Images with the HST reveal the optical counterparts to the radio components and also the lens galaxy. An optical spectrum of the bright component, obtained with the first Magellan telescope, reveals quasar emission lines at redshift 3.42. Deeper radio images with MERLIN and the VLBA reveal a faint third radio component located near the center of the lens galaxy, which is either a third image of the background quasar or faint emission from the lens galaxy.Comment: 21 pp., including 4 figures; thoroughly revised in light of new MERLIN/HST data; accepted for publication in A

Residential Perceptions of Environmental Exposures and Associated Health Effects in the Fresno, Texas Community

Background: Environmental contaminants are often located in areas heavily populated by African Americans, Hispanics/Latinos, and the poor. In many communities, the discovery of environmental hazards occurs following concern and investigation by its constituents. The residents of Fresno, Texas, which is a predominantly minority community located near Houston, Texas, have long-standing undocumented concerns related to potential environmental exposures and associated health effects. To begin to document the concerns of the members of the Fresno community, we used focus group methodology to examine the resident’s perceptions of the environment in the Fresno community, potential routes and sources of environmental exposures, and how Fresno residents perceived that these environmental hazards could affect their health. Methods: Focus group methodology was used to assess the Fresno communities’ perceptions of environmental exposure, perceived routes of exposure, and perceived adverse health affects. Nineteen Fresno residents took part in four focus group discussions that were recorded, transcribed, and analyzed using content analysis. Results: The residential participants overwhelmingly described poor water quality in the Fresno community. While some residents perceived that the air quality was good or clear, others described the air as poor or potentially dangerous. Some residents identified the local chemical companies, a landfill, chlorination, and a lack of public water supply as potential sources of contamination in the Fresno community. The residents perceived that environmental exposures could potentially affect their health status, in particular the drinking water. Conclusions: The findings of our study convey the concerns of the members of the Fresno community. Potential environmental exposures were identified along with sources of environmental hazards. Although there were differing perceptions of air quality, the perceptions of water quality and sources of contamination were consistent. These findings should be used in developing a larger-scale environmental health assessment in the Fresno community to examine self-reported health status and measure contaminant levels in the residential drinking water

New detections of HC5N towards hot cores associated with 6.7 GHz methanol masers

We present new detections of cyanodiacetylene (HC5N) towards hot molecular cores, observed with the Tidbinbilla 34 m radio telescope (DSS–34). In a sample of 79 hot molecular cores, HC5N was detected towards 35. These results are counter to the expectation that long chain cyanopolyynes, such as HC5N, are not typically found in hot molecular cores, unlike their shorter chain counterpart HC3N. However, it is consistent with recent models which suggest HC5N may exist for a limited period during the evolution of hot molecular cores

Earth Radiation Budget Experiment (ERBE) scanner instrument anomaly investigation

The results of an ad-hoc committee investigation of in-Earth orbit operational anomalies noted on two identical Earth Radiation Budget Experiment (ERBE) Scanner instruments on two different spacecraft busses is presented. The anomalies are attributed to the bearings and the lubrication scheme for the bearings. A detailed discussion of the pertinent instrument operations, the approach of the investigation team and the current status of the instruments now in Earth orbit is included. The team considered operational changes for these instruments, rework possibilities for the one instrument which is waiting to be launched, and preferable lubrication considerations for specific space operational requirements similar to those for the ERBE scanner bearings

PMN J1838-3427: A new gravitationally lensed quasar

We report the discovery of a new double-image quasar that was found during a search for gravitational lenses in the southern sky. Radio source PMN J1838-3427 is composed of two flat-spectrum components with separation 1", flux density ratio 14:1 and matching spectral indices, in VLA and VLBA images. Ground-based BRI images show the optical counterpart (total I=18.6) is also double with the same separation and position angle as the radio components. An HST/WFPC2 image reveals the lens galaxy. The optical flux ratio (27:1) is higher than the radio value probably due to differential extinction of the components by the lens galaxy. An optical spectrum of the bright component contains quasar emission lines at z=2.78 and several absorption features, including prominent Ly-alpha absorption. The lens galaxy redshift could not be measured but is estimated to be z=0.36 +/- 0.08. The image configuration is consistent with the simplest plausible models for the lens potential. The flat radio spectrum and observed variability of PMN J1838-3427 suggest the time delay between flux variations of the components is measurable, and could thus provide an independent measurement of H_0.Comment: 23 pages, incl. 6 figures, to appear in A.J.; replaced with accepted version; minor changes to text, improved figure

Optimizing countershading camouflage

Countershading, the widespread tendency of animals to be darker on the side that receives strongest illumination, has classically been explained as an adaptation for camouflage: obliterating cues to 3D shape and enhancing background matching. However, there have only been two quantitative tests of whether the patterns observed in different species match the optimal shading to obliterate 3D cues, and no tests of whether optimal countershading actually improves concealment or survival. We use a mathematical model of the light field to predict the optimal countershading for concealment that is specific to the light environment and then test this prediction with correspondingly patterned model “caterpillars” exposed to avian predation in the field. We show that the optimal countershading is strongly illumination-dependent. A relatively sharp transition in surface patterning from dark to light is only optimal under direct solar illumination; if there is diffuse illumination from cloudy skies or shade, the pattern provides no advantage over homogeneous background-matching coloration. Conversely, a smoother gradation between dark and light is optimal under cloudy skies or shade. The demonstration of these illumination-dependent effects of different countershading patterns on predation risk strongly supports the comparative evidence showing that the type of countershading varies with light environment