Leo Fabisinski
Marshall Space Flight Center
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Featured researches published by Leo Fabisinski.
Proceedings of SPIE | 2010
Paul S. Ray; Deepto Chakrabarty; C. Wilson-Hodge; Bernard F. Phlips; Ronald A. Remillard; Alan M. Levine; Kent S. Wood; Michael T. Wolff; Chul Gwon; Tod E. Strohmayer; Michael Baysinger; M. S. Briggs; Peter Capizzo; Leo Fabisinski; Randall C. Hopkins; Linda S. Hornsby; Les Johnson; C. Dauphne Maples; Janie Miernik; Dan Thomas; Gianluigi De Geronimo
The Advanced X-ray Timing Array (AXTAR) is a mission concept for X-ray timing of compact objects that combines very large collecting area, broadband spectral coverage, high time resolution, highly flexible scheduling, and an ability to respond promptly to time-critical targets of opportunity. It is optimized for submillisecond timing of bright Galactic X-ray sources in order to study phenomena at the natural time scales of neutron star surfaces and black hole event horizons, thus probing the physics of ultradense matter, strongly curved spacetimes, and intense magnetic fields. AXTARs main instrument, the Large Area Timing Array (LATA) is a collimated instrument with 2-50 keV coverage and over 3 square meters effective area. The LATA is made up of an array of supermodules that house 2-mm thick silicon pixel detectors. AXTAR will provide a significant improvement in effective area (a factor of 7 at 4 keV and a factor of 36 at 30 keV) over the RXTE PCA. AXTAR will also carry a sensitive Sky Monitor (SM) that acts as a trigger for pointed observations of X-ray transients in addition to providing high duty cycle monitoring of the X-ray sky. We review the science goals and technical concept for AXTAR and present results from a preliminary mission design study.
49th AIAA Aerospace Sciences Meeting including the New Horizons Forum and Aerospace Exposition | 2011
Tara Polsgrove; Sharon Fincher; Robert B. Adams; George C. Marshall; Jason Cassibry; Ross Cortez; Matthew Turner; C. Daphne Maples; Janie N. Miernik; Geoffrey Statham; Leo Fabisinski; John Santarius; Tom Percy
Z-pinch and Dense Plasma Focus (DPF) are two promising techniques for bringing fusion power to the field of in-space propulsion. A design team comprising of engineers and scientists from UAHuntsville, NASAs George C. Marshall Space Flight Center and the University of Wisconsin developed concept vehicles for a crewed round trip mission to Mars and an interstellar precursor mission. Outlined in this paper are vehicle concepts, complete with conceptual analysis of the mission profile, operations, structural and thermal analysis and power/avionics design. Additionally engineering design of the thruster itself is included. The design efforts adds greatly to the fidelity of estimates for power density (alpha) and overall performance for these thruster concepts
photovoltaic specialists conference | 2015
Tiffany Lockett; Armando Martinez; Darren Boyd; Michael P. SanSoucie; Brandon Farmer; Todd A. Schneider; Greg Laue; Leo Fabisinski; Les Johnson; John A. Carr
This paper describes recent advancements of the Lightweight Integrated Solar Array and Transceiver (LISA-T) currently being developed at NASAs Marshall Space Flight Center. The LISA-T array comprises a launch stowed, orbit deployed structure on which thin-film photovoltaic (PV) and antenna devices are embedded. The system provides significant electrical power generation at low weights, high stowage efficiency, and without the need for solar tracking. Leveraging high-volume terrestrial-market PVs also gives the potential for lower array costs. LISA-T is addressing the power starvation epidemic currently seen by many small-scale satellites while also enabling the application of deployable antenna arrays. Herein, an overview of the system and its applications are presented alongside sub-system development progress and environmental testing plans.
13th International Energy Conversion Engineering Conference | 2015
Les Johnson; John A. Carr; Leo Fabisinski; Tiffany Russell-Lockett
Affordable and convenient access to electrical power is essential for all spacecraft and is a critical design driver for the next generation of smallsats, including cubesats, which are currently extremely power limited. The Lightweight Innovative Solar Array (LISA), a concept designed, prototyped, and tested at the NASA Marshall Space Flight Center (MSFC) in Huntsville, Alabama provides an affordable, lightweight, scalable, and easily manufactured approach for power generation in space. This flexible technology has many wideranging applications from serving small satellites to providing abundant power to large spacecraft in GEO and beyond. By using very thin, ultraflexible solar arrays adhered to an inflatable structure, a large area (and thus large amount of power) can be folded and packaged into a relatively small volume. The LISA array comprises a launchstowed, orbitdeployed structure on which lightweight photovoltaic devices and, potentially, transceiver elements are embedded. The system will provide a 2.5 to 5 fold increase in specific power generation (Watts/kilogram) coupled with a >2x enhancement of stowed volume (Watts/cubicmeter) and a decrease in cost (dollars/Watt) when compared to stateoftheart solar arrays.
AIAA SPACE 2010 Conference & Exposition | 2010
Leo Fabisinski; Charlotte Dauphne Maples
Typically, the most important decisions in the design of a spacecraft are made in the earliest stages of its conceptual design – the Pre-Phase A stages. It is in these stages that the greatest number of design alternatives is considered, and the greatest number of alternatives is rejected. The focus of Pre-Phase A conceptual development is on the evaluation and comparison of whole concepts and the larger-scale systems comprising those concepts. This comparison typically uses general Figures of Merit (FOMs) to quantify the comparative benefits of designs and alternative design features. Along with mass, performance, and cost, risk should be one of the major FOMs in evaluating design decisions during the conceptual design phases. However, risk is often given inadequate consideration in conceptual design practice. The reasons frequently given for this lack of attention to risk include: inadequate mission definition, lack of rigorous design requirements in early concept phases, lack of fidelity in risk assessment methods, and undervaluation of risk as a viable FOM for design evaluation. In this paper, the role of risk evaluation in early conceptual design is discussed. The various requirements of a viable risk evaluation tool at the Pre-Phase A level are considered in light of the needs of a typical spacecraft design study. A technique for risk identification and evaluation is presented. The application of the risk identification and evaluation approach to the conceptual design process is discussed. Finally, a computational tool for risk profiling is presented and applied to assess the risk for an existing Pre-Phase A proposal. The resulting profile is compared to the risks identified for the proposal by other means.
Archive | 2012
David Smitherman; Tiffany E. Russell; Mike Baysinger; Pete Capizzo; Leo Fabisinski; Brand N. Griffin; Linda S. Hornsby; Dauphne Maples; Janie Miernik
Archive | 2012
Les Johnson; Leslie Alexander; Leo Fabisinski; Andy Heaton; Janie Miernik; Rob Stough; Roosevelt Wright; Roy Young
INCOSE International Symposium | 2012
John A. Mulqueen; C. Dauphne Maples; Leo Fabisinski
Archive | 2010
Tara Polsgrove; Robert B. Adams; Leo Fabisinski; Sharon Fincher; C. Dauphne Maples; Janie Miernik; Tom Percy; Geoff Statham; Matt Turner; Jason Cassibry; Ross Cortez; John Santarius
Archive | 2011
Janie Miernik; Geoffrey Statham; Robert B. Adams; Tara Polsgrove; Sharon Fincher; Leo Fabisinski; C. Dauphne Maples; Thomas K. Percy; Ross Cortez; Jason Cassibry