Propulsion system study for Small Transport Aircraft Technology (STAT)

Propulsion system technologies applicable to the generation of commuter airline aircraft expected to enter service in the 1990's are identified and evaluated in terms of their impact on aircraft operating economics and fuel consumption. The most promising technologies in the areas of engine, propeller, gearbox, and nacelle design are recommended for future research. Each item under consideration is evaluated relative to a modern baseline engine, the General Electric CT7-5, in a current technology aircraft flying a fixed range and payload. The analysis is presented for two aircraft sizes (30 and 50 passenger), over a range of mission lengths (100 to 1100 km) and fuel costs ($264 to$396 per cu m)

Electronographic polarimetry of reflection nebulae

In the first part of this thesis imaging polarimeter developed at the University of Durham for use in the optical waveband is described, and details are presented of a new computer data reduction system which allows the production of polarisation naps automatically from polarimeter images recorded using a McMullan electronographic camera. New methods arc employed to achieve higher accuracy and reliability than previously possible, particularly at low brightness levels. A method of checking the smoothness and mutual consistency of images is described, and its use in eliminating image defects is illustrated. This technique is also used to investigate the sources of error in electronography and ways are suggested in which these errors can be reduced, In the second part of the thesis, new polarimetric observations of the reflection nebula NGC1999 arc presented and discussed' in the light of previous colour and brightness observations. Theoretical arguments are used to relate important nebular parameters to observational features in reflection, nebulae, and these ideas are applied to produce a numerical model of NGC1999. Complete multiple scattering calculations are performed and the model is shown to be consistent with all available observations of the nebula. Finally, observations of other reflection nebulae are discussed and the experience gained with NGC1999 is used to outline deficiencies in current models of the interstellar extinction law, and it is suggested that a broad spectrum of particle sizes in the interstellar medium may be indicated. The .importance of imaging polarimetry in further investigation of this problem is pointed out

Identifying Student Difficulties with Entropy, Heat Engines, and the Carnot Cycle

We report on several specific student difficulties regarding the Second Law of Thermodynamics in the context of heat engines within upper-division undergraduates thermal physics courses. Data come from ungraded written surveys, graded homework assignments, and videotaped classroom observations of tutorial activities. Written data show that students in these courses do not clearly articulate the connection between the Carnot cycle and the Second Law after lecture instruction. This result is consistent both within and across student populations. Observation data provide evidence for myriad difficulties related to entropy and heat engines, including students' struggles in reasoning about situations that are physically impossible and failures to differentiate between differential and net changes of state properties of a system. Results herein may be seen as the application of previously documented difficulties in the context of heat engines, but others are novel and emphasize the subtle and complex nature of cyclic processes and heat engines, which are central to the teaching and learning of thermodynamics and its applications. Moreover, the sophistication of these difficulties is indicative of the more advanced thinking required of students at the upper division, whose developing knowledge and understanding give rise to questions and struggles that are inaccessible to novices

The Unusual Variability of the Large Magellanic Cloud Planetary Nebula RPJ 053059-683542

We present images and light curves of the bipolar Planetary Nebula RPJ 053059-683542 that was discovered in the Reid-Parker AAO/UKST H-alpha survey of the Large Magellanic Cloud (LMC). The emission from this object appears entirely nebular, with the central star apparently obscured by a central band of absorption that bisects the nebula. The light curves, which were derived from images from the SuperMACHO project at CTIO, showed significant, spatially resolved variability over the period 2002 January through 2005 December. Remarkably, the emission from the two bright lobes of the nebula vary either independently, or similarly but with a phase lag of at least one year. The optical spectra show a low level of nebular excitation, and only modest N enrichment. Infrared photometry from the 2MASS and SAGE surveys indicates the presence of a significant quantity of dust. The available data imply that the central star has a close binary companion, and that the system has undergone some kind of outburst event that caused the nebular emission to first brighten and then fade. Further monitoring, high-resolution imaging, and detailed IR polarimetry and spectroscopy would uncover the nature of this nebula and the unseen ionizing source.Comment: Accepted for ApJ Letters; 6 page

Dynamic Line Management

Talk Talk Technology has an ongoing programme of Dynamic Line Management (DLM), aimed at improving the performance of ADSL broadband connections. Choosing the most appropriate configuration, or "profile", for an individual line allows a balance to be reached between achieving a high line speed and a stable customer experience. Among the objectives of DLM are to determine the likely line speed of new connections and to identify lines that might benefit from an updated profile. Addressing the questions raised by TalkTalk regarding DLM requires three complementary types of modelling: physical modelling of the electrical characteristics of ADSL lines (these are existing copper telephone lines); information modelling of the associated communication channel, taking into account the levels of noise and the coding of ADSL signals; and finally statistical modelling, which enables data gathered from the exchange to be used to construct relationships between key variables and to identify lines that might be faulty or on poor profiles. The work of the Study Group 2010 contributed mainly to developing the statistical modelling. The report summarises the progress that was made and the opportunities for developing these techniques further

The STARLINK software collection

The UK's STARLINK project based at the Rutherford Appleton Laboratory develops and distributes software applicable to a wide range of problems in Astronomy; it covers most wavebands, caters for a variety of instrumentation, and ranges from programming tools and libraries through to large package of applications. The facilities available and gives details of how they may be obtained are summarized. Recent developments and other features of particular interest are highlighted

Hysteresis of spectral evolution in the soft state of black-hole binary LMC X-3

We report the discovery of hysteresis between the x-ray spectrum and luminosity of black-hole binary LMC X-3. Our observations, with the Proportional Counter Array on the Rossi X-ray Timing Explorer, took place entirely within the soft spectral state, dominated by a spectral component that was fitted well with a multicolor disk blackbody. A power-law component was seen only during times when the luminosity of the disk blackbody was declining. The x-ray luminosity at these times was comparable to that seen in transient systems (x-ray novae) when they return to the hard state at the end of an outburst. Our observations may represent partial transitions to the hard state; complete transitions have been seen in this system by Wilms et al. (2001). If they are related to the soft-to-hard transition in transients, then they demonstrate that hysteresis effects can appear without a full state transition. We discuss these observations in the context of earlier observations of hysteresis within the hard state of binaries 1E 1740.7-2942 and GRS 1758-258 and in relation to published explanations of hysteresis in transients.Comment: 14 pages, 6 figures, accepted by The Astrophysical Journa

Multi-axis fields boost SABRE hyperpolarization via new strategies

The inherently low signal-to-noise ratio of NMR and MRI is now being addressed by hyperpolarization methods. For example, iridium-based catalysts that reversibly bind both parahydrogen and ligands in solution can hyperpolarize protons (SABRE) or heteronuclei (X-SABRE) on a wide variety of ligands, using a complex interplay of spin dynamics and chemical exchange processes, with common signal enhancements between $10^3-10^4$. This does not approach obvious theoretical limits, and further enhancement would be valuable in many applications (such as imaging mM concentration species in vivo). Most SABRE/X-SABRE implementations require far lower fields (${\mu}T-mT$) than standard magnetic resonance (>1T), and this gives an additional degree of freedom: the ability to fully modulate fields in three dimensions. However, this has been underexplored because the standard simplifying theoretical assumptions in magnetic resonance need to be revisited. Here we take a different approach, an evolutionary strategy algorithm for numerical optimization, Multi-Axis Computer-aided HEteronuclear Transfer Enhancement for SABRE (MACHETE-SABRE). We find nonintuitive but highly efficient multi-axial pulse sequences which experimentally can produce a 10-fold improvement in polarization over continuous excitation. This approach optimizes polarization differently than traditional methods, thus gaining extra efficiency