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Information
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UPCOMING SEMINARS: Presenter: Date/time: Location: Title: Abstract: |
| PREVIOUS SEMINARS: |
| Presenter: | Troy D. Altus, Graduate Research Scholar Assistant |
| Date/time: | Wednesday, January 30, 2002 at 1:00 p.m. |
| Location: | NASA Langley Research Center, Hampton, VA
227 Hunting Avenue, Bldg. 647, Rm. 307 |
| Title: | "A Response Surface Methodology For Bi-Level Integrated System Synthesis (BLISS)" |
| Abstract: | BLISS (Bi-Level Integrated System Synthesis) is a decomposition
optimization method for engineering systems. The method is characterized
by the separate optimization of a relatively few system-level variables
and the optimization of potentially numerous local variables. Subsystem
optimizations are autonomous and may be conducted concurrently (i.e. on
a multiple processor computer). In previous versions of BLISS, optimum
sensitivity analysis and system sensitivity data were used to link the
subsystem optimization data to the system optimization. The current
work replaces both the optimum sensitivity analysis and the system sensitivity
equations by the quadratic response surface representations using subsystem
optimization results.
The response surface methodology for BLISS achieves the desired improvements while retaining key attributes of previous versions of BLISS: the autonomy of the black box optimizations and the clear separation of the system variables from the potentially numerous local variables. The response surface formulation of BLISS was successfully demonstrated on a simplified conceptual design of a supersonic business jet (1995 AIAA graduate team aircraft design topic). In addition to changes in the overall optimization methods of BLISS, subsystem fidelity was enhanced, accompanied by the necessary modifications to the data flow between subsystem analyses. Documentation of these modifications that have not as yet been tested is included as a reference for future research. This research was conducted in partial satisfaction of the requirements for the degree of Master of Science with The George Washington University. Professor Robert R. Sandusky (ext. 41982) is coordinating this presentation which is expected to last approximately 1 hour. |
| Presenter: | Craig A. Hunter, Aerospace Engineer |
| Date/time: | Monday, January 7, 2002 at 9:30 a.m. |
| Location: | NASA Langley Research Center, Hampton, VA
227 Hunting Avenue, Bldg. 647, Rm. 307 |
| Title: | "An Approximate Jet Noise Prediction Method Based on Reynolds-Averaged Navier-Stokes Computational Fluid Dynamics Simulation" |
| Abstract: | The work conducted in this investigation represents the
first key steps towards developing a state of the art jet noise prediction
and analysis package capable of dealing with advanced nozzle concepts and
complex three-dimensional turbulent flows. The jet noise prediction
theory developed here has been implemented into the computational code
"Jet3D", which is based on Lighthill¹s Acoustic Analogy and uses Reynolds-averaged
Navier-Stokes (RANS) computational fluid dynamics (CFD) simulations from
the NASA Langley flow solver PAB3D.
Implementation of the Lighthill theory in Jet3D centers on the modeling of two-point space-time correlations. Mean flow correlations for velocity and density are modeled using a Taylor series expansion, written in terms of local mean flow gradients. Turbulent velocity correlations are separated into space and time factors, and modeled using a combination of Gaussian-type exponential functions and quadratic functions. The proposed model satisfies basic correlation requirements and scales with characteristic turbulence length and time scales. Two cases were used to validate and test Jet3D, based on the experimental jet noise and flow field data Yamamoto et al. obtained for a supersonic axisymmetric nozzle. In each case, Jet3D noise predictions were in very good agreement with experimental data for observer angles from 50° to 140°, but diverged from experimental data at shallow angles to the jet axis, overpredicting the OASPL by 812 dB at an observer angle of 20°. 1/3 octave band frequency spectrum SPL results were in good agreement with experimental data at forward and sideline observer angles, but diverged away from experimental data for observer angles less than about 70°. As the observer point approached the jet axis, Jet3D overpredicted SPL levels and the SPL spectra were biased (or shifted) to higher frequencies than the experimental data. The disparity between Jet3D predictions and experimental data at rearward observer angles is likely due to sound-flow interaction effects (not modeled in Jet3D). Simple ray acoustics analysis suggests that mean flow convection and refraction affects the sound radiated to observer angles less than about 73-75°, which falls in line with the observed region in which experimental data and the Jet3D prediction differ. This research was conducted in partial satisfaction of the requirements for the degree of Doctor of Science with The George Washington University. Dr. John L. Whitesides (ext. 41982) is coordinating this presentation which is expected to last approximately 1 hour. |
| Presenter: | Stephen J. Alter, Aerospace Technologist |
| Date/time: | Friday, December 21, 2001 at 1:00 p.m. |
| Location: | NASA Langley Research Center, Hampton, VA
227 Hunting Avenue, Bldg. 647, Rm. 307 |
| Title: | "The Generation of High Fidelity Structured Volume Grids For Computational Science Applications Using a System of Elliptic Partial Differential Equations" |
| Abstract: | This thesis presents new techniques that improve the
capabilities of a volume grid smoother to produce high fidelity structured
grids about arbitrary bodies while reducing the time required to iteratively
solve elliptic partial differential equations (PDEs). Elliptic PDEs
with non-zero source terms used for controlling grid line incidence and
cell size at a boundary are notoriously difficult to solve because of the
stiffness produced by the source terms. The source terms are computed
based on the application of boundary conditions to the elliptic PDEs at
the defining boundaries of a volumetric domain, and propagated onto the
volume interior using a blending function. Traditionally, the blending
scheme chosen made no use of the dependency between the bounding faces
of the volume. The current work offers an alternative that accommodates
a dependency for grid line angle controls from all faces of the bounded
volume while decoupling the dependency on cell size control. Using
the dependency for angle control, and no dependency for cell size reduces
the conflicting conditions of the boundary conditions as they are propagated
onto the interior. The reduction of the conflicting conditions or
over specification of the problem in the interior coupled with the non-dependent
controls of cell size significantly reduces the stiffness associated with
the elliptic PDEs system. The reduced stiffness inherently permits
the convergence of the PDEs to an equilibrium state faster than through
the use of the traditional blending schemes. This structured grid
generation tool offers numerous advantages over the various unstructured
grid technologies including the minimization of overhead associated with
computations, and ease of boundary condition application. However,
structured grid generation remains a time intensive task. The new
technique for structured grid generation also offers a viable alternative
to over-set grid technology by providing volume grids as quickly as those
obtained through the solution of hyperbolic and parabolic PDEs. This
new tool enables the use of the existing experience with structured grid
solvers which has been acquired over the past 40 years.
This research was conducted in partial satisfaction of the requirements for the degree of Master of Science with The George Washington University. Dr. John L. Whitesides (ext. 41982) is coordinating this presentation which is expected to last approximately 1 hour. |
| Presenter: | Govinda B. Haines, Graduate Research Scholar Assistant |
| Date/time: | Thursday, October 4, 2001 at 1:00 p.m. |
| Location: | NASA Langley Research Center, Hampton, VA
227 Hunting Avenue, Bldg. 647, Rm. 307 |
| Title: | "Optimization of a Solar Powered High Altitude Long Endurance Aircraft with a Stirling Heat Engine" |
| Abstract: | There is an ongoing challenge to develop a vehicle capable
of loitering for weeks at altitudes above the tropopause to potentially
perform high altitude missions at lower cost than current solutions.
Given the central role propulsion plays in this objective, there is a need
to continue exploration of unconventional power sources. Current
solar-powered vehicle synthesis capability has primarily been developed
for photovoltaic (PV) cell solutions.
This thesis presents a method to size a solar concentrator-Stirling engine system for a conceptual High Altitude Long Endurance (HALE) aircraft and to determine the power available. Concentrated solar energy is input to the hot side of a Stirling Engine and a radiator rejects heat to the environment. The development of an optimization approach incorporating the existing AirCraft SYNThesis program, ACSYNT, is explained with emphasis on concentrator-Stirling engine integration. The new Propulsion/Energy Storage module and modifications to the existing Weights and Aerodynamics modules are all incorporated within the ACSYNT program to permit analysis of all input parameters for the lowest weight aircraft. To test the method, a design study is performed for an example HALE Unmanned Aerial Vehicle (UAV) having a payload of 9.0 kilograms and an endurance of 30 days at 32 degrees N latitude and 17,000 - 21,000 meters altitude. Both, a Stirling-powered baseline vehicle and a PV cell-powered baseline vehicle are developed. The PV cell-powered baseline is used to validate sections of the methodology and serve as a reference for comparison. Sensitivity studies are presented for key independent design parameters. This research was conducted in partial satisfaction of the requirements for the degree of Master of Science with The George Washington University. Professor Robert Sandusky (ext. 41982) is coordinating this presentation which is expected to last approximately 1 hour. |
| Presenter: | Jason P. Hundley, Graduate Research Scholar Assistant |
| Date/time: | Friday, September 21, 2001 at 1:00 p.m. |
| Location: | NASA Langley Research Center, Hampton, VA
227 Hunting Avenue, Bldg. 647, Rm. 307 |
| Title: | "A Thermography System for Imaging Reusable Launch Vehicles" |
| Abstract: | The use of non-intrusive measurements in aerospace systems
has always played a critical role in the development of aeronautics and
astronautics. This work describes the development of a new quantitative,
global, non-intrusive surface temperature measurement technique using the
principles of ratio intensity thermography. The work presented discusses
the theoretical development of a ratio intensity thermography system, calibration
of the temperature measurement system, verification of the calibration
technique, and identification of a data analysis procedure that eliminates
many of the possible errors associated with processing raw infrared image
data. This Ratio Intensity Thermography System (RITS) is used in
conjunction with an independently controlled high speed tracking telescope
mount to create a new High Altitude / Re-entry Vehicle Infrared Imaging
(HARVII) system. The HARVII instrument has the capability of
tracking a vehicle at a slant range of over 250,000 feet regardless of
flight plan or known trajectory information. By using the RITS, the
HARVII system can determine surface temperatures on a flight vehicle from
800K – 1400K. Using conventional optics, the HARVII can determine
a vehicle’s surface temperature independent of the material emissivity,
background sky, or atmospheric conditions with greater accuracy and less
cost than other current systems.
This research was conducted in partial satisfaction of the requirements for the degree of Master of Science with The George Washington University. Dr. Michael K. Myers (ext. 41982) is coordinating this presentation which is expected to last approximately 1 hour. |
| Presenter: | Byron R. Monzon, Graduate Research Scholar Assistant |
| Date/time: | Wednesday, September 19, 2001 at 1:00 p.m. |
| Location: | NASA Langley Research Center, Hampton, VA
227 Hunting Avenue, Bldg. 647, Rm. 307 |
| Title: | "Non-Linear Simulation Development For A Sub-Scale Research Airplane" |
| Abstract: | The FASER (Free Flying Aircraft for Sub-scale Experimental
Research) program was established at the NASA Langley Research Center to
provide the center with an affordable, easy-to-modify testbed to conduct
research in the areas of stability and control in high-alpha regimes, spin
recovery, and system identification. Because the rapid high angle-of-attack
and high angle-of-sideslip flight maneuvers that will be executed with
this remote control airplane might jeopardize the airplane, it was desired
to have a simulation of the aircraft so the pilots can practice the maneuvers
beforehand. Also, the simulation can be used for control law testing
and development.
The simulation consists of a MATLAB program of the mathematical model that describes the dynamics of the FASER aircraft using the rigid body equations of motion in standard form. The main body of work performed for this thesis was obtaining the FASER characteristics necessary to develop the non-linear simulation, which included measuring the moments of inertia accurately and calculating the aerodynamic characteristics through theoretical methods. To calculate the aerodynamic coefficients, a MATLAB program that uses theoretical methods to estimate the stability and control derivatives and the propulsion effects based on the geometry of the aircraft was created. The simulation performs as expected and it received a positive response from the people that tested it at the Langley Research Center. This research was conducted in partial satisfaction of the requirements for the degree of Master of Science with The George Washington University. Dr. V. Klein (ext. 41982) is coordinating this presentation which is expected to last approximately 1 hour. |