The FX/90: A proposal in response to a low Reynolds Number station keeping mission

The FX/90 is a remotely piloted vehicle designed to fly at Reynolds numbers below 2 x 10 to the 5th power. Several applications exist for this type of flight, such as low altitude flight of very small aircraft. The design presented here allows investigation into the unique problems involved in low Reynolds number flight, which will, in turn, further understanding of this flight regime. The aircraft will operate in a steady flight environment, free from significant atmospheric turbulence and weather effects. The F-90 has a 39 in. fuselage which is constructed of balsa and plywood. The landing gear for the aircraft is a detachable carriage on which the aircraft rests. The aerodynamic planform is a rectangular wing (no taper or sweep) with a chord of 9 in., a wingspan of 72 in., and is constructed entirely out of styrofoam. The propulsion system is a puller configuration mounted on the front of the fuselage. It consists of an Astro 05 engine and a 10-6 two bladed propeller. Control of the aircraft is accomplished through the use of two movable control surfaces: elevators for pitch control, and a rudder for yaw control. The aircraft is soundly constructed, highly maneuverable, and adequately powered. Furthermore, the investigation into alternative technologies, most notably the styrofoam wing and the detachable landing gear, holds promise to improve the performance of the aircraft

Light, Scenography and the Choreography of Space

This submission for PhD by publication is primarily concerned with the scenographic role of light, especially in relation to; historiography and dramaturgy, embodiment and the use of projected digital light in performance. There is an emphasis on the ability of light to make meaning, its impact on the experience of audiences and its role in the choreography of space. The research encompasses writings on contemporary and historical uses of light in performance and practice-led, collaborative research with digital light that was part funded through the Arts and Humanities Research Council (AHRC). The research also embraces associated concerns relating to collaborative design processes and the creative use of technology within the performance domain. The title of this submission reflects both the nature and scope of the research of a series of outputs created over the decade 2004-2014 and published between 2005 and 2015. The monograph Light: Readings in Theatre Practice (Palgrave Macmillan, 2013) forms a significant, central core since it focuses on the ways in which light is used as a fundamental aspect of dramatic presentation and provides a range of new insights in thinking about lighting as a creative performance practice

Probing the Gamma-Ray Burst Rate with Trigger Simulations of the Swift Burst Alert Telescope

The long gamma-ray burst (GRB) rate is essential for revealing the connection between GRBs, supernovae and stellar evolution. Additionally, the GRB rate at high redshift provides a strong probe of star formation history in the early universe. While hundreds of GRBs are observed by Swift, it remains difficult to determine the intrinsic GRB rate due to the complex trigger algorithm of Swift. Current studies usually approximate the Swift trigger algorithm by a single detection threshold. However, unlike the previously flown GRB instruments, Swift has over 500 trigger criteria based on photon count rate and additional image threshold for localization. To investigate possible systematic biases and explore the intrinsic GRB properties, we developed a program that is capable of simulating all the rate trigger criteria and mimicking the image trigger threshold. We use this program to search for the intrinsic GRB rate. Our simulations show that adopting the complex trigger algorithm of Swift increases the detection rate of dim bursts. As a result, we find that either the GRB rate is much higher than previously expected at large redshift, or the luminosity evolution is non-negligible. We will discuss the best results of the GRB rate in our search, and their impact on the star-formation history.Comment: 6 pages, 3 figures, 7th Huntsville Gamma-Ray Burst Symposium, GRB 2013: paper 35 in eConf Proceedings C130414

Probing the Cosmic Gamma-Ray Burst Rate with Trigger Simulations of the Swift Burst Alert Telescope

The gamma-ray burst (GRB) rate is essential for revealing the connection between GRBs, supernovae and stellar evolution. Additionally, the GRB rate at high redshift provides a strong probe of star formation history in the early universe. While hundreds of GRBs are observed by Swift, it remains difficult to determine the intrinsic GRB rate due to the complex trigger algorithm of Swift. Current studies of the GRB rate usually approximate the Swift trigger algorithm by a single detection threshold. However, unlike the previously flown GRB instruments, Swift has over 500 trigger criteria based on photon count rate and additional image threshold for localization. To investigate possible systematic biases and explore the intrinsic GRB properties, we develop a program that is capable of simulating all the rate trigger criteria and mimicking the image threshold. Our simulations show that adopting the complex trigger algorithm of Swift increases the detection rate of dim bursts. As a result, our simulations suggest bursts need to be dimmer than previously expected to avoid over-producing the number of detections and to match with Swift observations. Moreover, our results indicate that these dim bursts are more likely to be high redshift events than low-luminosity GRBs. This would imply an even higher cosmic GRB rate at large redshifts than previous expectations based on star-formation rate measurements, unless other factors, such as the luminosity evolution, are taken into account. The GRB rate from our best result gives a total number of 4571^{+829}_{-1584} GRBs per year that are beamed toward us in the whole universe. SPECIAL NOTE (2015.05.16): This new version incorporates an erratum. All the GRB rate normalizations ($R_{\rm GRB}(z=0)$) should be a factor of 2 smaller than previously reported. Please refer to the Appendix for more details. We sincerely apologize for the mistake.Comment: 52 pages, 17 figures, published in ApJ 783, 24L (2014). An erratum is included. A typo in Eq. 8 is fixed in this versio

Peru’s Shining Path: Recent Dynamics and Future Prospects

Although soundly defeated in the early to mid-1990s, Shining Path (Sendero Luminoso) did not disappear. Over the past five years, it has reemerged in a substantially different form, with both a military and a political component. The organization, once again coordinated by jailed leader Abimael Guzmán Reynoso, has eschewed shorter-term military objectives in favor of a longer-term strategy of slowly rebuilding popular support and establishing a party within the Peruvian political system. In so doing, it has also moved from extreme Maoist ideological rigidity to a more pragmatic, though perhaps only tactical, approach. Financial support is derived once again from cocaine production and trafficking in the Upper Huallaga Valley (UHV). Although there may be some individual exceptions, Shining Path is not a narcoterrorist organization. At the same time, Sendero is still very small, in no way a threat to the Peruvian state, and divided. The Lima-based political organization and the military wing in the UHV continue to follow Guzmán‟s leadership, while the Apurímac-Ene Valleys (VRAE) group remains committed to the armed struggle. The Government of Peru (GOP) response to date, both military and civilian, has been inadequate. VRAE military operations are hampered by poor leadership, ill-trained troops, and an outdated strategy. VRAE development resources have been cut, and the long-promised paved road remains in the planning stage. Without significant GOP adjustments, Shining Path is likely to continue to grow