Conceptual Designs for NLC Ubitrons with Permanent-Magnet Wigglers
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Engineering topics
Publications and source records attributed to Phillips, R..
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Silicon carbide fiber reinforced silicon carbide (SiC/SiC) composites are candidate materials for various high temperature turbine engine applications because of their high specific strength and good creep resistance at temperatures of 1400 C (2552 F) and higher. Chemical vapor infiltration (CVI) SiC/SiC ceramic matrix composites (CMC) incorporating Sylramic-iBN SiC fiber were evaluated via fast fracture tensile tests (acoustic emission damage characterization to assess cracking behavior), tensile creep testing, and microscopy. The results of this testing and observed material behavior degradation mechanisms are reviewed.
A spacecraft Attitude Control and Determination Subsystem (ACDS) is heavily dependent upon simulation throughout its entire development, implementation and ground test cycle. Engineering simulation tools are typically developed to design and analyze control systems to validate the design and software simulation tools are required to qualify the flight software. However, the need for simulation does not end here. Operating the ACDS of a spacecraft on the ground requires the simulation of spacecraft dynamics, disturbance modeling and celestial body motion. Sensor data must also be simulated and substituted for actual sensor data on the ground so that the spacecraft will respond by sending commands to the actuators as they will on orbit. And finally, the simulators is the primary training tool and test-bed for the Flight Operations Team. In this paper various ACDS simulation, developed for or used by the Landsat 7 project will be described. The paper will include a description of each tool, its unique attributes, and its role in the overall development and testing of the ACDS. Finally, a section is included which discusses how the coordinated use of these simulation tools can maximize the probability of uncovering software, hardware and operations errors during the ground test process.
A planet orbiting a rado-emitting star can be indirectly detected by high-precision Very Long Baseline Interferometry (VLBI) astrometry through the reflex orbit of the star.
We present a comparison of VLBI and Hipparcos astrometric parameters of several optically bright radio-emitting stars.
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A diamond film made of (100)-oriented diamond crystallites has relatively flat surfaces in parallel with the silicon surface. This is desirable because it provides a smoother surface of the diamond film. The difficulty in retaining the (100)-oriented diamond crystallites is strongly influenced by the growth temperature. This paper reports the results from a study on the surface morphologies of diamond films deposited in a hot filament reactor at reduced substrate temperature compared to that deposited at higher temperature.
The IR absorption in polycrystalline diamond films deposited in oxygen-acetylene flames is characterized using FTIR. The one-phonon absorption coefficient in the region from 7 to 12 microns that is related to extrinsic defects in the diamond films shows a strong dependence on the flame conditions as well as the substrate temperature. A high degree of diamond crystalline perfection, as judged from the undetectable one-phonon absorption, is achieved under the optimized deposition conditions for our flame setup. This is further supported by the sharp Raman peak at 1332/cm as well as the high purity in crystal orientation according to the X-ray diffraction pattern measured for the high quality diamond films.
Apollo 11 lunar igneous rocks mineralogical, chemical and petrological features by optical and electron microscopy and X ray spectrometry