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7/31/2019 Intern Abstract Booklet_10.24.12
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NASA University Research Centers Present a
Virtual Poster Session and SymposiumWelcome to the NASA University Research Centers (URC) Virtual Poster Session and Symposium(VPSS). This is a unique opportunity to meet NASA URC students and learn about their exciting
experiences as summer 2012 interns or co-ops at NASA centers.
Browse the poster presentations below to see a description and visual representation of researchprojects that URC students completed under the guidance of NASA mentors.
You can leave questions or comments for student presenters using accounts on Facebook, Yahoo,Hotmail and AOL. The comment section is at the bottom of each project page.
URC students welcome your feedback during the VPSS. If you are a poster session judge, students
will respond to you within 24 hours of your post.
To learn more about the NASA URC Program,
Please visit us at the following websites:
http://www.nasa.gov/offices/education/programs/national/urc/home/index.html
http://www.facebook,com/NASAURC1
http://www.nasa.gov/offices/education/programs/national/urc/home/index.htmlhttp://www.facebook%2Ccom/NASAURC1http://www.facebook%2Ccom/NASAURC1http://www.nasa.gov/offices/education/programs/national/urc/home/index.html7/31/2019 Intern Abstract Booklet_10.24.12
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Virtual Poster Sessionand Symposium
2012 Summer Intern ParticipantsPage
Raul Acevedo 3
Adeyemi Adegbite 4
Juan M. Barragan 5
Billy Barrios 6
Tara Blakey 7
Harry Burton III 8
Kalind Carpenter 9
Stanford Carter 10Frank Ceballos 11
Vanessa Dorado 12
Robert Ellis 13
Jordan Fuchs 14
Raul Garcia-Sanchez 15
Zenia Garcia 16
Valeria C. Arce Gonzalez 17
Kelly Courtney Gustafson 18
This VPSS is open to the NASA URC community and the public.
The competition and judging portion of the poster session will
run from Oct. 24- 31, 2012.
Winners and runners-up in the three categories listed below will
be announced on Nov. 1, 2012. These individuals will be invited
to give an oral presentation of their research to the NASA URC
community at a Virtual Symposium on Nov. 8, 2012.
For additional details, contact the NASA URC Management Office
via [email protected] [email protected].
Poster Categories: Aeronautics Research (ARMD)
Human Exploration and Operations (HEOMD)
Science (SMD)
PageDaniel H. Hernandez, Jr. 19
Jesus Hinojosa 20
Adrienne Lam 21
Alberto Mata 22
Jose A. McKinnon 23
Hctor Mendez-Colberg 24
Kevin J. Monk II 25
Gregory Morales 26Brandon Norman 27
Ryan OConnor 28
Edwin Ortiz-Quiles 29
Francisco Pena 30
Darian Phillips 31
Zachary Roberts 32
Rigoberto Roche 33
Robert Conrad Rorie 34
Janet Ruedas 35
Kimberlin Schnittaker 36
Christopher St. Julian 37
Eric Thomas 38
Loraine Torres-Castro 39
Viviana Villamizar 40
Michael Joseph Williams 41Jason Ziccardi 42
mailto:[email protected]:[email protected]:[email protected]:[email protected]:[email protected]:[email protected]7/31/2019 Intern Abstract Booklet_10.24.12
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Raul AcevedoUniversity of Puerto Rico, Rio PiedrasMajor: Chemical Physics
Degree Level: Ph.D.
Intern Site: NASA Kennedy Space Center
Mentor: Dr. Luz M. Calle
Electrokinetic deposition of methylmethacrylate is used to mitigate
corrosion in reinforced concrete. The methylmethacrylate (MMA)
monomer deposits in the pores in the concrete where it is converted into
its polymer, polymethylmethacrylate, thus creating a barrier that also
enhances the mechanical properties of the concrete. Previous to the MMA
treatment, an electrokinetic deposition is used to transport calcium,
sodium and potassium hydroxide particles through the capillary pores of
concrete directly to the concrete reinforcement. The intent is to use these
compounds as a sacrificial electrode layer during the electrokinetic
deposition of methylmethacrylate monomer. Cylindrical reinforced
concrete specimens were subjected to electrokinetic treatment and the
specimens were tested to characterize porosity reduction and tensile
splitting strength, showing an increase in the tensile strength. In addition,
nine specimens treated electrokinetically and in long-term atmospheric
exposure testing at NASAs Kennedy Space Centers seaside atmospheric
exposure test site were tested to determine their corrosion rate.
Abstract:
In Situ Electrosynthesis of
Polymethylmethacrylate within
Ceramic Launch Pad Materials
HEOMD
http://www.nasa.gov/centers/kennedy/news/corrosion.htmlhttp://www.nasa.gov/centers/kennedy/news/corrosion.html7/31/2019 Intern Abstract Booklet_10.24.12
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Adeyemi AdegbiteMorgan State University, MarylandMajor: Electrical Engineering
Degree Level: Bachelor of Science
Intern Site: NASA Goddard Space Flight Center
Mentors: Harry Shaw and Darryl Lakins
The Satellite Network (SN) is a data communication system
comprised of a constellation of Tracking and Data Relay
Satellites (TDRS) and several ground terminals. My main
purpose was attaining and organizing all the legal return
service modes of the Narrow Band Modem and mapping them
to each other, with proper documentation. The modes of the
Narrow Band Modems are the different configurations that
are being used during the various tests to check the
functionality requirements. These modems are in use for theUSS-CR project, which will is testing key components that will
replace current subsystems for the TDRS ground terminals at
the White Sand Facility. Using requirement specification
documents and test data, the modes are organized using
Mindjet MindManager, a tool that is helpful for organizational
and presentational purposes. With Mindjet, I successfully
mapped all modes for a S-Band Single Access Return Service.
Abstract:
USS-CR Modem Functional
Configuration Summary
http://www.mindjet.com/http://www.mindjet.com/7/31/2019 Intern Abstract Booklet_10.24.12
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Juan M. BarraganUniversity of El Paso at El Paso, TexasMajor: Mechanical Engineering
Degree Level: Bachelor of Science
Intern Site: NASA Johnson Space Center
Mentor: Eric Hurlbert
Morpheus is a vertical test bed that is currently being used
by the NASA Johnson Space Center to explore and perfect
green propellant propulsion. This vertical lander utilizes
different technologies that allow the test bed to
autonomously land, detect and avoid hazards with the help
of various subsystems. The vehicle at the moment will be
tested at the Kennedy Space Center and a spare vehicle is
needed for backup. My task is to begin the construction of
the spare vehicle propellant storage and propellant deliverysystem in conjunction with the vehicle structure, as well as
supporting any testing and preparation for the KSC test.
Learning from current vehicle testing, components new
vehicles subsystem will be upgraded and modified for
increased performance.
Abstract:
Morpheus Supportand
Secondary Vehicle Development
http://morpheuslander.jsc.nasa.gov/http://morpheuslander.jsc.nasa.gov/7/31/2019 Intern Abstract Booklet_10.24.12
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The Neutron Star Interior Composition ExploreR (NICER) will be a NASA Explorer Mission of
Opportunity, dedicated to the study of neutron stars, the only places in the universe
where all four fundamental forces of nature are simultaneously important. Answering the
long-standing astrophysics question How big is a neutron star?, NICER will confront
nuclear physics theory with unique observation constraints, exploring the exotic states of
matter within neutron stars, and revealing their interior and surface compositions through
rotation-resolved X-ray spectroscopy. NICER will feature 56 co-aligned X-ray concentrators
and matching detectors with a 2,000 cm2 effective area. Each optic is roughly 6 inches in
height and 4 inches in diameter, featuring 24 concentric aluminum foils which are
individually coated with gold. The detectors which are , located at the focal length of 1.085
meters behind the optics, each have a 2mm aperture. NICER will be the first X-Ray
telescope utilizing mirrors in a full cylindrical configuration, along with new
manufacturing techniques on such a small scale. We began characterizing the
effectiveness of the first assembled optics or engineering testing units (ETUs) bydetermining the point-spread function. The optics were placed inside a vacuum, where
they received approximately parallel X-ray photons. The data is then picked up by the
detector and analyzed with software. We find a 1.84 mm half-flux radius and a 3.49 mm
80% flux radius for the fully populated optic, and a 0.72 mm half-flux radius and a 1.64 mm
80 % flux radius for the sparsely populated optic. From these results we conclude that the
optics are performing relatively well, and should meet design requirements with
improvements in the manufacturing methods. (This project was co-authored by Billy
Barrios, Steve Lentine, and Ceili Burdhimo).
Goddard intern Billy
Barrios performs an
optical check on oneof the NICER Optics
mirrors. Image
Credit: URC.
Abstract:
NICER X-Ray Optics
Assembly and Testing
Billy BarriosCalifornia State University, Los Angeles, California
Major: Mechanical Engineering/Physics
Degree Level: Bachelor of Science
Intern Site: NASA Goddard Space Flight Center
Mentor: Dr. Keith C. Gendreau
SMD
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Leishmaniases are among the most important emerging and resurging
vector-borne diseases, second only to malaria in terms of the number ofaffected people. Leishmaniases are endemic in 88 countries worldwide
and threaten about 350 million people (WHO, 2007). Since the first
reported case of zoonotic cutaneous leishmaniasis (ZCL) in Saida, Algeria,
in 1991, 1,275 cases have been recorded (Makhlouf & Houti, 2010), with
the vast majority of study-area cases (99%) reported between the years
of 2000 and 2009. An investigation of potential climatic indicators for the
apparent shift in disease prevalence was conducted by comparing
anomalies in the climate data specific to the local pathogen cycle. It was
determined that long-term climate trends have resulted in conditions
that promote the prevalence of ZCL. Increased precipitation haveresulted in greater vegetation and promoted host and vector population
growth through a trophic cascade. Increased minimum temperatures
have lengthened the annual duration of sandfly activity. Short-term
variations in maximum temperatures, however. show a correlation with
disease suppression in the subsequent years. These findings indicate a
potential to forecast the risk of ZCL infection through models of the
trophic cascade and sandfly population growth.
Abstract:
Incidence ofVector-borne Disease and Climate
Change: A Case Study in Semi-Arid Algeria
Tara BlakeyFlorida International University
Major: HydrogeologyDegree Level: Ph.D.
Intern Site: NASA Goddard Space Flight Center
Mentor: Dr. Lahouri Bounoua
SMD
http://www.ncbi.nlm.nih.gov/pubmedhealth/PMH0002362/http://www.ncbi.nlm.nih.gov/pubmedhealth/PMH0002362/7/31/2019 Intern Abstract Booklet_10.24.12
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Quantum Cascade Lasers (QCLs) can be designed to operate anywhere from
the Mid-IR to THz spectrum, and with their small size, tunable frequencies,and high energy output makes them an excellent choice for Trace Gas
Detection. During the course of this internship, our job was to construct a
laser system capable of producing low enough beat frequencies that could be
detected via a spectrum analyzer. After the internship, the QCL would then
undergo experimentation into detecting various molecules. Research and
experimentation into QCLs will allow them to be used in both Earth science
and future planetary NASA missions. QCLs are relatively new within the field
of spectroscopy and operate on a principle different from that of common p-
n junction diode lasers. In a diode laser, conduction band electrons jump into
a valence band hole and emit a photon whose wavelength is determined by
the band gap energy of the semiconductor, known as an interband transition.With QCLs, a conduction band electron can make a series of jumps in a
staircase-like potential existing in the conduction band, emitting an identical
photon in each transition. Here, a single electron emits a cascade of photons
leading to the formation of a high-power laser. Transitions within a QCL take
place from subband-to-subband inside a quantum well, continuing into the
next quantum well, and so on. Thus, these are referred to as intersubband
transitions.
Abstract:
Quantum Cascade Laser Frequency
Modulation for Trace Gas Detection
Harry Burton IIIDelaware State University
Major: Applied OpticsDegree Level: Master of Science
Intern Site: NASA Goddard Space Flight Center
Mentor: Eduard Luzhanskiy
SMD
7/31/2019 Intern Abstract Booklet_10.24.12
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Design, model, fabricate, setup, conduct and analyze thermal and
cryogenic test results for several current JPL projects.
Ultra Compact Imaging Spectroscopy (UCIS):
Quantify the effective thermal conductance of a data cable to enable
optimization of tactical cryocooler use in future systems.
Airborne scanning MultiSPectral Infrared instrument (AirMSPI):
Set up and run a test to determine whether normal operating thermal
stresses on a silica filter will result in epoxy failure and
delamination of the layers within the silica filter.
Mars Atmospheric Trace Molecule Occultation Spectrometer (MATMOS):
Created interface parts in Solidworks for the physical connection
between the radiator, thermal strap and load; and created a LabVIEW
data acquisition graphical user interface for the test data
characterizing the cooling system thermal performance.
Mechanical engineering
researcher Kalind Carpenter
assembles the SOLO TREC
Power generation
subsystem test rig. Image
Credit: URC.
Abstract:
Thermal and Cryogenic
Testing Systems Development
Kalind CarpenterCalifornia State University, Los Angeles, California
Major: Mechanical EngineeringDegree Level: Master of Science
Intern Site: NASA Jet Propulsion Laboratory
Mentor: Dr. Eugenio Urquiza
SMD
7/31/2019 Intern Abstract Booklet_10.24.12
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Hygroscopic growth is one of the most fundamental properties of atmospheric aerosols.
By absorbing or evaporating water, an aerosol particle changes its size, morphology,
phase, chemical composition and reactivity, and other parameters such as its refractive
index. Because of this, extensive research is being done on aerosol particle hygroscopic
growth at NASA. This research is important to the understanding of aerosol effects on
climate change. Currently, the operation of radiosondes is the most common technique
used to characterize vertical profiles of temperature, water vapor mixing ratio and
relative humidity. However, radiosondes are launched only two to three times a day
because of the high cost of each one. The attempted solution to this problem is utilizing a
Microwave Radiometer (MWR). Microwave radiometry allows for continuous retrievals
of temperature profiles by measuring brightness and sky temperature at different zenith
elevations. The focus of this study is the sensitivity of Relative Humidity Profiles obtained
from both instruments. This will be accomplished by using temperature profiles from the
MWR and radiosonde. The result of these comparisons will allow for the study of thesensitivity of the Relative Humidity profile obtained by radiosonde and those combining
temperature profiles from the MWR and the Water Vapor mixing ratio from the
radiosonde. These Relative Humidity profiles will then be compared to Relative Humidity
profiles from the radiosonde. The data used in this study was acquired from the Howard
University Beltsville Campus during the Discover AQ campaign in the summer of 2011.
The result of this project will be used as a baseline for evaluating uncertainties in the
retrieval of aerosol hygroscopic growth by means of Lidar measurement.
Stanford Carter reviews
data captured on the HURLRaman Lidar at the Howard
University Beltsville Center
for Climate System
Observation. Image Credit:
URC.
Abstract:
Study ofMicrowave Radiometer Temperature
Profiles for Use in Calculating Relative Humidity
Stanford CarterHoward University, Washington, D.C.
Major: PhysicsDegree Level: Bachelor of Science
Intern Site: NASA Goddard Space Flight Center
Mentor: Dr. Daniel Ramirez
SMD
http://meiyu.atmphys.howard.edu/beltsville/inde3.htmlhttp://meiyu.atmphys.howard.edu/beltsville/inde3.htmlhttp://meiyu.atmphys.howard.edu/beltsville/inde3.htmlhttp://meiyu.atmphys.howard.edu/beltsville/inde3.html7/31/2019 Intern Abstract Booklet_10.24.12
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The Laser Interferometer Gravitational-Wave Observatory (LIGO) is a large-scale
Michelson interferometer which aims to directly detect gravitational waves
predicted by Albert Einstein in 1916. The gravitational waves sources that LIGO
expects to detect consist of the merging of two neutron stars or a neutron and
black hole at cosmic distances. It is anticipated that the coalescence of these
compact objects may also produce a short -lived gamma ray burst (GRB).
Unfortunately, LIGO is not accurate in localizing the points in the sky where the
gravitational sources are to be found. The best that LIGO can do is to constrain a
gravitational wave source in an area of approximately 100 square degrees,
where literally millions of electromagnetic sources can be observed. So it seems
that the simultaneous detection of gravitational and electromagnetic wavescoming from a source is highly unlikely. To facilitate the task of searching for
electromagnetic counterparts coming from gravitational waves, a list of galaxies
within 100 Mpc has been compiledthe gravitational waves galaxy catalog
(GWGC). LIGO is now being designed to improve its sensitivity by a factor of 10,
which means that it would be able to observe neutron star/ neutron star
coalescence to distances of 300 Mpc and neutron star/ black hole coalescence
up to 650 Mpc. Therefore, GWGC must be updated to contain galaxies at these
distances. We present the results of the updates made to GWGC.
Physics student Frank
Ceballos discovers that
work at NASA Goddard can
be challenging, yet fun.
Image Credit: URC.
Abstract:
Update: Gravitational Wave Galaxy Catalogue
for the Rapid Search of Electromagnetic
Counterparts from Gravitational Waves
Frank CeballosUniversity of Texas at Brownsville, Texas
Major: Physics
Degree Level: Bachelor of Science
Intern Site: NASA Glenn Research Center
Mentor: Jonah Kanner
SMD
http://www.ligo.caltech.edu/http://www.ligo.caltech.edu/7/31/2019 Intern Abstract Booklet_10.24.12
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Vanessa DoradoUniversity of Texas at El Paso, TexasMajor: Mechanical Engineering
Degree Level: Master of Science
Intern Site: NASA Marshall Space Flight Center
Mentor: Kevin Pedersen
Historically, spacecraft reaction control systems have primarily used cold gas
thrusters because of their inherent simplicity and reliability. However, cold gas
thrusters typically have a low specific impulse. It has been determined that a
higher specific impulse can be achieved by passing a monopropellant fluid
mixture through a catalyst bed prior to expulsion through the thruster nozzle.
This research analyzes the potential efficiency improvements from using tri-
gas: a mixture of hydrogen, oxygen, and an inert gas, in this case helium.
Passing tri-gas through a platinum catalyst causes the hydrogen and oxygen to
become reactive, ultimately heating the exiting fluid and generating a higher
specific impulse. The goal of this project was to optimize the thrusterperformance by characterizing the effects of several system components. The
performance effects were examined by varying catalyst types, catalyst lengths,
and initial catalyst temperatures. Additional testing would utilize a hydrogen
rich tri-gas mixture or characterize the performance effects of firing in a
vacuum chamber for future applications and advancement in the field of green
propellants
Abstract:
Characterization of a
Tri-Gas Thruster
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7/31/2019 Intern Abstract Booklet_10.24.12
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Jordan FuchsPrairie View A&M University, TexasMajor: Electrical Engineering
Degree Level: Bachelor of Science
Intern Site: NASA Johnson Space Center
Mentor: Robert Hirsh
My project involved improving upon existing software and
developing new software for the Project Morpheus Team.
Specifically, I created and updated Integrated Test and
Operations Software (ITOS) user interfaces for on-board
interaction with the vehicle during archive playback as well
as live streaming data. These interfaces are an integral part
of the testing and operations for the Morpheus vehicle,
providing any and all information to evaluate instrumentsand ensure coherence and control during Morpheus
missions. I also developed a bridge program for interfacing
live CCSDS (telemetry) data to the Engineering DOUG
Graphics Engine (EDGE) display for a graphical (stand-alone
or VR dome) view of live Morpheus flights or archive replays.
Abstract:
ITOS to EDGE Bridge Software for the
Morpheus Lunar/Martian Vehicle
http://morpheuslander.jsc.nasa.gov/http://morpheuslander.jsc.nasa.gov/7/31/2019 Intern Abstract Booklet_10.24.12
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Raul Garcia-SanchezHoward University, Washington, D.C.Major: Physics
Degree Level: Ph.D.
Intern Site: NASA Goddard Space Flight Center
Mentor: Dr. Paul Mahaffy
The organic contaminants library was developed as part of the contamination control plan for the Mars
Science Laboratory rover mission. Work to normalize the data taken from Sample Analysis at Mars (SAM)
to match standardized organic compound databases such as the National Institute of Standards and
Technology (NIST) is needed in order to increase its availability to other potential users. To do this, we
analyzed a standard fragmentation pattern, in this case Perfluorotributyl amine (PFTBA), using the SAM
GCMS settings that will be used for the actual mission and then calculated the ratio differences between
the SAM PFTBA data and the NIST standard for PFTBA. This library is submitted as a New Technology
Report, and will be readily available in the future. Carrying out a correction of the SAM spectral
response, developing and providing an algorithm that makes these corrections to match with more
standard libraries like NIST, will allow general users to use this library and correct SAM data for their
work. The data is processed by correcting for instrumental calibration, and other specific instrumental
behaviors. The processing is documented in a linked location related to the data directories. This works
for a large number of the continuing satellite missions. The lower level data is primarily available from
the mission operations groups. Although this work is intensive in terms of the GCMS Spectral library, the
changes to the spreadsheets that contain entries supplementing the contaminants library should be
minimal, and only needed when the normalization changes the spectra enough to change the chemical
formula (in those cases the compound is properly identified by the library). With the expected data for
the Mars Science Laboratory (MSL) Curiosity Mars landing being August 6, continued support of the
mission via further library improvements will be needed.
Raul Garcia-Sanchez and Dr. Prabhakar Misra with a model of
the Sample Analysis at Mars (SAM) instrument for the Mars
Science Laboratory (MSL) mission. Image Credit: URC. Abstract:
Normalization of the
SAM Spectra Using PFTBA
http://marsprogram.jpl.nasa.gov/msl/http://marsprogram.jpl.nasa.gov/msl/http://marsprogram.jpl.nasa.gov/msl/http://marsprogram.jpl.nasa.gov/msl/7/31/2019 Intern Abstract Booklet_10.24.12
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Serving another term as a cooperative program student at
Marshall Space Flight Center, my tasks were largely varied
within the EV32 Structural and Mechanical Design Branch.
Within the branch, I helped provide structural and
mechanical design support including: specialized engineering,
technical assistance, program support, model and CAD
packages for structural/mechanical component systems
design, and development for spacecraft and vehicle systems.
During this time I worked on efforts and projects that areproprietary and data sensitive and therefore not listed in
detail here. Aside from these activities, I was being prepared
for follow-on work and had to take course training and
Preliminary Development Flight Instrumentation modeling as
listed.
University of Texas at El
Paso Mechanical
Engineering major Zenia
Garcia. Image Credit:
URC.
Abstract:
Principles in Avoiding Design Errors and
Facets ofEngineering a Total System
Zenia GarciaUniversity of Texas at El Paso, TexasMajor: Mechanical Engineering
Degree Level: Master of Science
Intern Site: NASA Marshall Space Flight Center
Mentor: Kevin Pedersen
SMD
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Valeria C. Arce GonzlezUniversity of Puerto Rico, MayaguezMajor: Chemical Engineering
Degree Level: Bachelor of Science
Intern Site: NASA Glenn Research Center
Mentor: Dr. Marisabel Lebrn-Coln
Todays helicopter gearboxes are limited by their poor structural design and
lack of capability to correlate changes in transmission and gearbox noise levels
with expected changes in cabin noise levels. This research focuses on the
development of multifunctional nanocomposite materials that possess high
strength, good thermal conductivity and high-performance abilities in vibration
and noise control. The project seeks to demonstrate improvement in the
vibration damping properties of polymeric materials by the addition of carbon
nanotubes. Carbon nanotubes are commonly used to improve the stiffness,
durability, performance and damping properties of materials. Because of their
adjustable elasticity and ability to act as springs, they can dissipate energy much
more efficiently, becoming a key component in noise-reduction applications.
Some of the greater benefits and payoffs of this research include quieter cabinsand the development of lightweight materials that carry no weight penalties.
These materials have many other applications, especially in the automotive and
aerospace industries where manufacturers require vibration-absorbing
materials that are cost-effective for the production of next-generation vehicles.
This research project involves the synthesis of epoxy nanocomposite materials,
dispersion and organic functionalization of carbon nanotubes, and the
processing and characterization of polymeric samples.
Valeria C. Arce
Gonzlez analyzes
the dispersion of
carbon nanotubes in
an epoxy resin
sample. Image
Credit: URC
Abstract:
Effects ofCarbon Nanotubes Addition on
Vibration Damping Behavior ofEpoxy Resins
SMD
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Climate variability in Australia is largely driven by an atmospheric phenomenon called the Southern
Oscillation (SO), which involves a see-saw like behavior between low and high pressure systems within the
equatorial Pacific regions. The interaction of SO with abnormally high sea surface temperatures (SSTs) El
Nio and abnormally low SSTsLa Nia (anti-El Nio) creates extreme drought or extreme flooding,
respectively, throughout Australia. El Nio-Southern Oscillation (ENSO) events have significant impacts on
Australias landscape, ecosystems, agriculture production, and, as this report shows, human health. During
La Nia years, when ENSO events involve increased rainfall and consequential flooding, Australias tropical,
warm climate and an associated increase in vegetation growth from the rainfall creates an ideal habitat for
mosquito population increases. Certain species of mosquitoes (Culux annulirostris) are carriers of Murray
Valley Encephalitis (MVE) virus, a rare but potentially fatal infection that attacks neurological and muscular
functioning. We hypothesized that a widespread increase in vegetation indicates an expansion of ideal
mosquito production habitats and will translate to an increased risk of MVE contraction. Our objective is to
show if a correlation exists between the ENSO-driven climate and consequential ecosystem changes and
MVE outbreaks throughout Australia. This study makes use of the Moderate Resolution ImagingSpectroradiometer (MODIS) sensor operating on NASAs Terra satellite to obtain monthly Normalized
Difference Vegetation Index (NDVI) data. It is assumed in this research that an anomalous increase in NDVI
values indicative of vegetation growth occurs due to increased rainfall, which, in tandem with
Australias tropical climate, allows for NDVI to be an adequate proxy for the combined influence of rainfall
and temperature on mosquito ecology. Our results showed a general temporal and spatial correlation
between MVE outbreaks and a greening period, suggestive of ideal mosquito breeding habitats and
assumed population increases. (This project was co-authored by K.Cortney Gustafson, Mouhamad Diabate,
and Dr. Assaf Anyamba).
Kelly Gustafson marvels
at the advance of
technology while
encountering archives ofresearch and equipment
from ages past. Image
Credit: URC.
Abstract:
Australia: Climate-Ecosystem
Varability and Impacts on Diseases
Kelly Courtney Gustafson
Florida International UniversityMajor: Environmental Studies
Degree Level: Master of Science
Intern Site: NASA Goddard Space Flight Center
Mentor: Dr. Assaf Anyamba
SMD
http://en.wikipedia.org/wiki/Southern_oscillationhttp://en.wikipedia.org/wiki/Southern_oscillationhttp://en.wikipedia.org/wiki/Southern_oscillationhttp://en.wikipedia.org/wiki/Southern_oscillation7/31/2019 Intern Abstract Booklet_10.24.12
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Daniel H. Hernandez, Jr.University of Texas at El Paso, TexasMajor: Mechanical Engineering
Degree Level: Bachelor of Science
Intern Site: NASA Marshall Space Flight Center
Mentor: Shane Brooke, Jon Street and Carolyn Russell
Friction Stir Welding is a process in which different factors such as travel speed, rotational
speed (RPM), and plunge force play a key role in creating a successful weld. Friction is
created between two panels by a shoulder and pin. This friction causes the material at the
abutting edge of two panels to plasticize (plastically deformed 70 percent of melting
point- taffy consistency), allowing for the material to be stirred and welded. This project
will consist of two separate but equally important tasks. First, is to analyze the nugget
shape and material flow characteristics of conventionally friction stir welded (C-FSW)
panels with different pin tool designs. Analyzing the nugget shape and stirring of the weld
through optical microscopy will aid in understanding how these flats will affect a weld.
There are six different pin tool designs for this project: a standard C-FSW pin without
machined flat edges (baseline), and five others with flats ranging from 1 to 5. The panels tobe welded are aluminum 2219 to aluminum 2219. This project will aid in understanding the
differences and similarities between each of the pins. This work will ultimately aid in
determining which pin design provides the optimum weld schedule and characteristics.
Second, is to support fixture design, stress analysis (FEA), and procurement for the Multi-
purpose Crew Vehicle Stage Adapter (MSA) pathfinder cone to adapter ring weld for the
Space Launch System (SLS). (The research was co-authored by Daniel H. Hernandez Jr. and
Elvis Boves).
Abstract:
Stress Analysis, Fixture Design for
MAS Pathfinder and Pin Tool Analysis
Using Conventional Friction Stir Welding
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Jesus HinojosaUniversity of Texas at Brownsville, TexasMajor: Physics
Degree Level: Bachelor of Science
Intern Site: NASA Goddard Space Flight Center
Mentor: Dr. Ronald Oliversen
At the beginning of my internship, I operated the McMath-Pierce
Solar Telescope at Kitt Peak National Observatory. There we
observed the moon and received high-resolution spectral data of
lunar exospheric sodium emissions for four nights. The overall data
measured sodium emission from the lunar limb out to two lunar
radii from the limb for lunar latitudes from the equator to the pole
over lunar phases from the first to third quarter. Here at GSFC I
have started gaining experience in CCD data reductions, line profile
fitting, and IDL software programming. The expected outcome ofmy internship is to advance the understanding of the interaction
between the solar wind and lunar surface via line profile
measurements, yielding exospheric sodium atom temperatures and
velocities.
Abstract:
Lunar Exospheric Sodium and
Potassium Emissions
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The Deep Space Network (DSN) is an international antenna network funded by NASA which
provides communications and support for various space missions. A 34-meter beam
waveguide antenna is under construction in Canberra, Australia, and requires a new downlink
channel and telemetry processors. This project focuses on testing of new telemetry decoders
which are implemented on Field-Programmable Gate Array (FPGA) boards. These are also
intended to replace legacy telemetry processors in the future to improve ease of maintenance
and sustainability. The intended functionality and performance of the decoders must be the
same as those which they are replacing. The new decoders are tested using different code
rates, coding schemes and modulation schemes standard to the DSN. The testing process
utilizes equipment similar to those at DSN ground stations, along with a signal generator to
provide equivalent RF signals. The Python scripting language is used to verify the integrity ofdecoded data and can handle large sets. These tools are used to obtain characteristics of
performance such as symbol error rate (SER), bit error rate (BER), and signal-to-noise-ratio
(SNR). Throughout the course of the internship, the encoding scheme that was of primary
focus was Turbo Code using code rates and modulation schemes seen on the actual DSN.
Discrepancies in decoder performance were encountered during testing, with several sources
identified. Various parameters were added to the output to isolate different sections of the
test setup for identifying those sources of error.
Adrienne Lam with the
telemetry processor and
Unix computer. Image
Credit: URC.Abstract:
Testing ofFPGA Telemetry Decoders for the
New 35 m Beam Waveguide Antenna
Adrienne Lam
California State University, Los Angeles, CaliforniaMajor: Electrical Engineering
Degree Level: Master of Science
Intern Site: NASA Jet Propulsion Laboratory
Mentor: Dr. Chau M. Buu
SMD
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Alberto MataUniversity of Texas at Brownsville, TexasMajor: Physics
Degree Level: Bachelor of Science
Intern Site: NASA Goddard Space Flight Center
Mentor: Dr. Avi Mandell
Using Interactive Data Language (IDL), an established data visualization
software, I analyze infrared spectroscopic observations of protoplanetary
disks. The observations are taken with the Very Large Telescope (VLT) in
the Atacama Desert of Chile using the Cryogenic Infrared Echelle
Spectrograph (CRIRES). Observing protoplanetary disks, or the gas and
dust around early stars, gives us insight as to what material surrounds
early stars, and since planets form in the protoplanetary disk of the star,
investigating the chemical composition of protoplanetary disks allows us
to probe the material that will eventually make up the planets around a
certain star. Planets whose origins and compositions we would like to
better understand include the recent discoveries of "super-Earths."
Observing these super-Earths gives us minimal information as to what
they are composed of, but observing protoplanetary disks can help us
better understand the origins of the atmospheres and interiors of these
planets.
Brandon Norman (left) and University of Texas at Brownsville, TX student,
Alberto Mata at the NASA Goddard Intern Poster Session. Image Credit: URC.
Abstract:
Investigating the Gas Chemistry of
Protoplanetary Disks
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Jose A. McKinnonUniversity of Texas at Brownsville, TexasMajor: Physics
Degree Level: Master of Science
Intern Site: NASA Goddard Space Flight Center
Mentor: Dr. John Baker and Dr. Jeffrey Livas
Gravitational wave detectors in the mHz band (such as the Laser
Interferometer Space Antenna, or LISA) will observe thousands of compact
binaries in the galaxy which can be used to better understand the structure
of the Milky Way. To test the effectiveness of LISA to measure the
distribution of the galaxy, we simulated the Close White Dwarf Binary
(CWDB) gravitational wave sky using different models for the Milky Way. To
do so, we have developed a galaxy density distribution modeling code based
on the Markov Chain Monte Carlo method. The code uses different
distributions to construct realizations of the galaxy. We then use the FisherInformation Matrix to estimate the variance and covariance of the recovered
parameters for each detected CWDB. This is the first step toward
characterizing the capabilities of space-based gravitational wave detectors to
constrain models for galactic structure, such as the size and orientation of
the bar in the center of the Milky Way.
Master of Science
student Jose A.
McKinnon.. Image
Credit: URC.
Abstract:
Mapping the Milky Way Galaxy
with LISA
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In the last decade, there has been an
increased interest in using palladium (Pd)
nanostructures for hydrogen (H2) sensing
devices. Nanostructured based sensors
promise shorter response times and higher
sensitivity due to their high surface-to-
volume ratio. With this in mind, an anodic
alumina membrane (AAM) Pd
nanostructured based sensor has beendeveloped and tested. The Solid State
Reduction method used formed a
combination of a thin film and nanowires
in the AAM. The fabrication method and
preliminary test results are discussed here.
Chemical engineeringdoctoral candidate
Hctor Mendez-Colberg
catches a rare moment
of rest during his
internship at NASA
Glenn Research Center.
Image Credit: URC.
Abstract:
Development of Chemical
Sensors for Hydrogen Detection
Hctor Mendez-ColbergUniversity of Puerto Rico, Mayaguez
Major: Chemical Engineering
Degree Level: Ph.D.
Intern Site: NASA Glenn Research Center
Mentor: Dr. Gary W. Hunter
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The Advanced Multimission Operations System (AMMOS) offers missions operationstools and services to deep space missions that are reliable and cost-effective. The
Instrument Operations Subsystem (IOS) of AMMOS deals with the processing of data
from space, and provides tools to orbiters and observatories for tactical operations
related to image processing and instrument design. Currently, up to 189
measurements from Mars' surface (such as wind speed, temperature, and
atmospheric pressure) are available to observers in the form of raw data. However,
this data is recorded every two seconds, making the amount of data enormous and
more difficult to sift through for specific information. Using Javascript/jQuery, a more
aesthetically pleasing way of viewing this information was developed and
demonstrated to make it easier for scientists to dissect. Tools such as the Mars Image
Viewer (MIV) are required from low-volume, relatively simple missions to high-volume, complex missions. Primary users of the MIV were observed in their workspace
and surveyed. Secondary users were also queried on their interest in and the usability
of the tool. The interaction between the MIV and its current/potential users were
analyzed in order to define requirements and ensure that it adequately fit the needs
of the users in ways that enable them to reach their goals with optimal efficiency.
Recommendations were provided for the MIV users manual to further cater to the
standpoint of the novice user.
Kevin J. Monk II at
California State
University, Long Beach.
Image Credit: URC.
Abstract:
Mars Image Viewer:
User Needs Analysis
Kevin J. Monk IICalifornia State University, Long Beach, California
Major: Human Factors Psychology
Degree Level: Master of Science
Intern Site: NASA Jet Propulsion Laboratory
Mentor: Elias Sayfi
SMD
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Gregory MoralesCalifornia State University, Long Beach, California
Major: Human Factors Psychology
Degree Level: Master of Science
Intern Site: NASA Dryden Flight Research Center
Mentor: Mark Pestana
As part of the Federal Aviation Administration (FAA)
Reauthorization Act, the FAA is tasked to develop regulations
testing and licensing unmanned aircraft systems (UAS) to be
integrated in the National Airspace System. Lead by NASAs
Dryden Flight Research Center, a project is under way to address
safety and operational challenges for UAS integration. The
Research Ground Control Station is being developed as a test
bed and database to provide data and proof of concept for a
Ground Control Station. This research supports the developmentof standards and practices with consideration to human factors
issues for the Ground Control Station. The project includes:
developing and evaluation of display and control formats,
command and control schemes, ergonomics, procedures for the
UAS pilot, and other human system integration features.
Abstract:
Human Factors in
Unmanned Aircraft Systems
ARMD
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This project involved Total Ionizing Dose (TID) tests at the
GSFC radiation chamber. The tests were performed using
a TLE2022 Bipolar Op Amp as the Device Under Test
(DUT).
The DUT was subject to a Cobalt 60 source at a Low Dose
Rate (LDR). The main values observed were the input bias
current, supply current, voltage offset, and current offset.
The implication from the results support that the device
has characteristics of radiation hardened.
Intern BrandonNorman tests
the op amp after
taking it out of
the radiation
chamber of the
Keithley 4200
and HP test
fixture. Image
Credit: URC.
Abstract:
Low Dose Rate TID Testof
Commercial Bipolar Op Amp
Brandon NormanPrairie View A&M University, TexasMajor: Electrical Engineering
Degree Level: Bachelor of Science
Intern Site: NASA Goddard Space Flight Center
Mentor: Jonathan Pellish
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Ryan OConnorCalifornia State University, Long Beach, California
Major: Human Factors Psychology
Degree Level: Master of Science
Intern Site: NASA Ames Research Center
Mentor: Dr. Walter Johnson
The number of crew members in commercial flights has steadily
decreased to two members, down from five members 50 years
ago. The next step is to reduce the crew to one pilot, and
eventually fully automate commercial aircraft, with one ground
pilot managing numerous UAS. This reduction in crew will
reduce costs for major airliners. Consistent development of new
aeronautic technologies has enabled this drastic shift to be
possible. The (FDRL) at NASA Ames is getting involved in theresearch efforts for the upcoming changes. My task as an intern
was to develop a cognitive walkthrough and work directly with a
commercial pilot to create testing scenarios and flowcharts for
the experimental testing on single-pilot operations.
Intern Ryan OConnor (left) with fellow California State
University, Long Beach, graduate student Zack Roberts.
Image Credit: URC.
Abstract:
Cognitive Walkthrough with a
Commercial Pilotfor Preliminary
Single-Pilot Operations Experiment
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Edwin Ortiz-QuilesUniversity of Puerto Rico, Rio Piedras
Major: Chemistry
Degree Level: Ph.D.
Intern Site: NASA Jet Propulsion Laboratory
Mentor: Dr. William C. West
Lithium ion batteries using Li2MnO3/LiMO2 (M = Mn, Co, Ni) as the cathode had
been extensively studied. Under 0 C, batteries with this composite oxide present
efficiency issues. This can be explained by a diffusion process with the lithium as
consequences of the poor layer organization. LiCl salts can help improve this
organization by resupplying the intercalated lithium to a molten mixture. Sensitivity
studies directed to understand the effects of LiCl on the cathode material
controlling variables as the synthesis time, and LiCl concentration will be
accomplished. Electrochemical experiments using galvanostatic charge/dischargeprocesses at C/5 and C/10 and impedances at different temperatures provide direct
information of the diffusion and the dynamics of the batteries prepared with
Li2MnO3/LiMO2. Tap density analysis will be completed to have a better
understanding of the behavior of the cathode after being packed in the batteries
and an AlPO4 coating. Results show an improvement in the capacity of the cathode
after the LiCl flux.
Abstract:
Molten Salt Flux Synthesis to Reduce
Cation Disorder in Cathodes for Lithium
Ion Batteries
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Francisco PenaCalifornia State University, Los Angeles, California
Major: Mechanical Engineering
Degree Level: Master of Science
Intern Site: NASA Dryden Flight Research Center
Mentor: Dr. Lance Richards
The Dryden Aero-Elastic Lab located at the AERO Institute is developing
cutting-edge research in fiber optic strain sensing. The innovative fiber
optics systems are capable of monitoring mechanical and thermal strains,
which allow engineers to monitor real-time deformation of a structure.
Utilizing the NASA University Research Center (S.P.A.C.E.) Uninhabited
Air Vehicle (Odyssey) as a test bed for the fiber optics strain sensors,
engineers will validate the capabilities of the Fiber Bragg Grating sensors.
The use of finite element modeling will aid in the further development of
embedded Fiber Bragg Grating sensors for Uninhabited Air Vehicles.
With real-time, deformation-shape prediction, it will be possible toaccurately measure mode-shape deformations of aircraft wings due to
aero-elastic effects on the aircraft during flight. Structural deformation
data can be sent to a feedback control system to mitigate the aero-
elastic effects on the airframe. Methods developed by NASA's Dryden
Flight Research Center for real-time deformation-shape prediction of
lightweight unmanned flying aerospace structures can potentially reduce
the risk of in-flight breakups, such as that of the Helios Wing..
Abstract:
Analysis and Experimental Validation of
Lightweight Structures for
Uninhabited Aerial Vehicles
ARMD
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I have been working on the USS-CR (User Service
Subsystem Component Replacement) Project that deals
with the replacement of key components that process user
signals within the TDRS (Tracking Data Relay Satellite)
ground terminals at the White Sands Complex in New
Mexico. New modems, Frequency Converters, Switch Gear,
and a Monitor and Control System (MCS) are being
provided to update Space Ground Link Terminals (SGLT)
currently in use at White Sands. The main goal of USS-CR is
to modernize equipment that is currently active and thenprovide backups so that hardware can stay functional until
the SGSS (Space Network Ground Segment Sustainment)
project is complete around the year 2017. In particular, my
research involves learning various Systems Engineering
techniques so that I can model a SSAF (S-band Singe Access
Forward) service.
Morgan State
electrical
engineering
student DarianPhillips. Image
Credit: URC.
Abstract:
Modeling a SSAF Service
Darian PhillipsMorgan State University, Maryland
Major: Electrical EngineeringDegree Level: Bachelor of Science
Intern Site: NASA Goddard Space Flight Center
Mentor: Harry Shaw
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Zachary RobertsCalifornia State University, Long Beach, CaliforniaMajor: Human Factors Psychology
Degree Level: Master of Science
Intern Site: NASA Ames Research Center
Mentor: Dr. Walter Johnson
Using a simulated air traffic environment, this study
measured the response time, execution time, and
general behavior of unmanned aerial vehicle (UAV)
pilots in response to direct commands from air traffic
controllers. Data was collected from eight participant
UAV pilots who were asked to respond to and execute
ATC commands as quickly as possible. Quick
responses to ATC commands are one factor essential
for UAVs to operate safely with manned aircraft andthis measured response data contributes to the
knowledge base necessary to fully integrate
unmanned aerial systems into the national airspace
in the near future. (This project was co-authored by
Zachary Roberts and Jason Ziccardi).
Abstract:
Measured Response to
UAS Pilot Commands
ARMD
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An experimental study was conducted on the Mid-Atlantic region to investigate the rainfallvariability within the instantaneous field of view of the microwave sensor-based satellite rainfall
estimate. The study was conducted through 30 rain gauges that were deployed at 11 sites, where
eight sites had triple and remaining sites had dual gauges. The gauges were tipping bucket at 0.01
inches resolution. The time of the t ip was recorded to a data logger which is powered by lithium
battery. A continuous gauge record was obtained at every gauge site from May 2005 to September
2010. The gauges sites were distributed from Ocean City, Maryland, to Kiptopeke, Virginia, at a
maximum separation of 150 km and at a minimum separation of 1 km between the two sites at
Wallops Island, Virginia. This study focuses on the variability of rainfall at different climatological
periods. The observations were divided into 20 seasons, 10 cold/warm periods, and five years. A
stretched exponential model was applied to the correlations of paired gauge rainfall at 30-minute
integration period. Two tips (0.5 mm) were considered as the threshold for rain events. The
correlations fell below 50 % at a 10 km distance most of the time in an observational period, whilethey were below 20% at 40 km distance. The variability was more noticeable between the seasons
than between the warm/cold periods and between the years. This could, in part, be related to the
sample size, partly to differences in rainfall characteristics. Additionally, the remnants of tropical
cyclones bring abundant rainfall to the Mid-Atlantic region but they may not be observed at a given
year. The nugget parameter was mainly above 0.95, while the shape parameter was mainly
between 0.4 and 1.0. The correlation distances remained mostly less than 50 km at a given
observational period.
Rigoberto Roche makes
changes to improve
output statistics and
provide high quality
graphical represen-
tations of the analyzed
data produced during
his internship at NASA
Goddard Space Flight
Center. Image Credit:NASA/Dr. Ali Tokay.
Abstract:
An Experimental Study of the
Small-Scale Variability of Rainfall
Rigoberto RocheFlorida International University
Major: Biomedical Engineering, Mechanical Engineering
Degree Level: Master of Science
Intern Site: NASA Goddard Space Flight Center
Mentor: Ali Tokay
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Robert Conrad RorieCalifornia State University, Long Beach, CaliforniaMajor: Human Factors Psychology
Degree Level: Master of Science
Intern Site: NASA Ames Research Center
Mentor: Dr. Walter Johnson
This study examined the effect of force feedback on target
acquisition in a simulated task, using a computer mouse
and the Novint Falcon, with and without force-feedback
information. Participants were asked to select targets that
varied in size, distance, and angular direction from the
start location. Results showed significant differences
between the movement times for the various input
devices. Movement times with the mouse and the Falcon
with force feedback were significantly faster than the
Falcon without force feedback. Force feedback was foundto reduce the effect of target size, but not the effect of
target distance. Force feedback also produced faster
movement times when the direction of movement was in
two dimensions. The findings suggest that force feedback
may be a useful method for assisting pilots in future CDTIs.
Abstract:
EffectofForce Feedbackon an
Aimed Movement Task
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Janet RuedasPrairie View A&M University, TexasMajor: General Engineering, Emphasis on Chemical Engineering
Degree Level: Master of Science
Intern Site: NASA Johnson Space Center
Mentor: Dr. Ramona Gaza
When charged particles pass through CR-39 detectors, they lose
energy and break the molecular bonds of the CR-39 polymer to form
paths of high chemical reactive sites along their trajectories. These
trajectories can be revealed as etched cones on the surfaces of CR-39
detectors by chemical etch for a CE-39 plate. Chemical etching for
plastic nuclear track detectors (CR-39) and thermoluminescence
measurements were performed per established techniques currently
used by the Space Radiation Analysis Group (SRAG) at NASA/JSC.
Work objectives included: working with the sodium hydroxide (NaOH)
etching solution, etching the plastic nuclear track detectors,measuring the detectors pre- and post-etch. The goal was to
calculate the bulk etch and prepare the detectors for storage for
future analysis. Over 150 CR-39s were etched successfully and the
bulk etch values were analyzed for accuracy using the standard errors
and error propagation..
Prairie View A&M
University
researcher Janet
Ruedas engraves
CR-39 detectors foretching. Image
Credit: URC.
Abstract:
Chemical Etching ofPlastic
Nuclear Track Detectors
ARMD
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The sustainability of aviation directly depends on the availability ofenvironmentally responsible fuel. With the growing gap between petroleum
production and demand, increasing prices, carbon emissions, mounting
environmental regulations, and the limited concentration of known fuel
reserves in politically unstable regions, biofuels are considered a viable
alternative to securing the future of aviation. Biofuels are a renewable
energy source, which could be customized to meet specific fuel needs.
NASA GRC developed the GreenLab Research Facility to study two principal
sources of biofuels: arid land halophytes (salt-tolerant plants) and sea water
algae. Through a Life Cycle Assessment (LCA) of the GreenLab, we
investigated the benefits and contributions to motivating the nextgeneration in STEM-related fields that the facility and its research offer
outweighs the cost of running the program every year. We also looked into
the optimization of Chaetomorpha sp. macro-algae by studying its growth
under four different conditions. Results showed that a direct light source
and some dirt accumulation lead to more successful growth of
Chaetomorpha sp. macro-algae
Kimberlin Schnittakercleans and monitors the
six ecosystems for
optimal growth of
halophytes (salt-tolerant
plants) used for the
creation of biofuels.
Image Credit: NASA
Glenn/Tamaera
McDowell.
Abstract:
A Life Cycle Assessmentof a Self-Sustainable
Renewable Energy Ecosystem
Kimberlin SchnittakerUniversity of Texas at El Paso, Texas
Major: Metallurgical and Materials Engineering
Degree Level: Master of Science
Intern Site: NASA Glenn Research Center
Mentor: Dr. Bilal Mark McDowell Bomani
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Christopher St. JulianPrairie View A&M University, Texas
Major: Electrical Engineering
Degree Level: Bachelor of Science
Intern Site: NASA Johnson Space Center
Mentor: Chatwin Lansdowne and Brandon Sherman
The aim of this project is to demonstrate techniques for effectively penetrating
a radio-shielded enclosure using Ethernet cable (CAT-6). This process requires
that we measure the shielding performance by means of testing and data
orchestration to collect and analyze our data, and then present observations
with different test cases. Each test case would represent a different penetration
strategy that utilizes distinctive wire coupling and characteristics (i.e., the type
of bulkhead link, the twist of each CAT-6 cable, the shielding type of each CAT-6
cable, and the length of the cable). As the different cable setups are fabricated,
a prototype evaluation of setup is conducted to measure the signal integrity of
the testing configuration. Our signal integrity is measured through the analysisof different parameters found in the prototype evaluation such as RF leakage,
impedance mismatch, and decay rate. As data values are effectively collected
and analyzed, the most effective cable setup is selected based upon its ability to
penetrate the shielded enclosure. The testing data are compared in conjunction
with the cost of the manufacturing of the prototype wire penetration.
Abstract:
Evaluate Techniques for Penetrating a
Radio-Shielded Enclosure
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When irradiating an Advanced Micro Device(AMD) Processor that is connected to the
motherboard within a chamber, it is
important to shield the motherboard from
the gamma rays. In doing so I constructed a
collimator with lead (Pb) bricks so that only
the AMD processor is open to the gamma
rays. While the motherboard was powered,
the AMD processor experienced radiation.The results examined the effects that
radiation had on an AMD processor and
whether or not the processor could survive
in the harmful space radiation environment.
Eric Thomas, is a
mechanical engineering
major at Prairie ViewA&M University. Image
Credit: URC
Abstract:
Radiation Testing on Biased
Commercial AMD Microprocessor
Eric ThomasPrairie View A&M University, Texas
Major: Mechanical Engineering
Degree Level: Bachelor of Science
Intern Site: NASA Goddard Space Flight Center
Mentor: Jonathan Pellish
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Lithium-ion batteries are among the most energetic rechargeable batteries available,
making them very popular for various applications. A lithium-ion rechargeablebattery provides high energy density, requiring less weight and smaller size
compared to other rechargeable systems. The battery manufacturer ABSL selected
the Sony Lithium 18650 HC cell in the late 1990s to make its space-qualified cells.
NASA Goddard Space Flight Center has flown ABSL batteries built from Sony 18650
HC cells on ST-5, SDO and LRO missions. Recently, Sony made modifications to these
cells due to failures in terrestrial applications. The addition of a mandrel tube is
supposed to "improve the vent path within cell to the safety vent" (Troutman, Joe,
2011) without causing any changes in the performance of the cell and the built-in
safety features. The aim of my project was to establish the baseline characterization
of the life-test batteries, which the contractors at the Naval Surface Warfare Center
at Crane, Indiana, will use to compare later performance tests of the Sony 18650 HC
and Sony 18650 HC mandrel cells. The study consisted in the creation of a test planthat allows researchers to know the capacity of the battery and its behavior in
different environments. The test plan was conducted in the Battery Laboratory at
NASA Goddard Space Flight Center. The project exposed me to Integration and
Testing (I&T) in a Class 10,000 clean room, visits to contractors and vendors (SAFT,
ABSL), and the opportunity to travel to the Naval Surface Warfare Center at Crane,
Indiana. (This project was co-authored by Loraine Torres-Castro, Leonine S. Lee,
Thomas Y. Yi and Ram S. Katiyar).
Ph. D. candidate Loraine Torres-Castro tests the batteries for the Global PrecipitationMeasurement mission. Image Credit: URC.
Abstract:
Global Precipitation Measurement Mission Project
Life-Test Support/Life Test Battery Characterization
Loraine Torres-CastroUniversity of Puerto Rico, Rio Piedras
Major: Physical Chemistry
Degree Level: Ph.D.
Intern Site: NASA Goddard Space Flight Center
Mentor: Amri Hernndez-Pellerano
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The overall objective is to assess the potential of satellite Lidar to retrieve thesurface of the coastal tides during normal (non-surge) conditions. Specific
objectives are to assess the capability of the GLAS sensor on board the ICESat
satellite platform to retrieve the spatial water surface profile during a March 2006
transect over the Chesapeake Bay, using the 1064 wavelength; validate the
retrieved water levels using a calibrated, high resolution 2D hydrodynamic model;
and provide insight on future altimetry observations of coastal regions using Lidar.
The present study focuses specifically on the capability to retrieve water surface
elevations of the Chesapeake Bay during a single ICESat transect in March 2006.
Validation is achieved using water surface elevations with a calibrated 2D, high-
resolution hydrodynamic model. This is because ICESat observations do not fall
exactly over available in situ tidal gages. Thus, it is necessary to first calibrate themodel using tide gages. Then, one can compare the ICES at elevations to those grid
elements over which the satellite observations occur. Future Lidar altimeters, that
will provide higher vertical precision and spatial coverage, should be of significant
benefit not only to hydrodynamic modelers, but also to a wide range of
applications including water resources planning, weather forecasting, ecosystem
monitoring, and disaster prevention and management.
Florida International
University
Environmental
Engineering major
Viviana Villamizar.
Image Credit: URCAbstract:
Assessment of ICESat Altimetry and Tidal
Gage Water Elevations with Hydrodynamic
Model Predictions for the Chesapeake Bay
Viviana VillamizarFlorida International University
Major: Environmental Engineering
Degree Level: Master of Science
Intern Site: NASA Goddard Space Flight Center
Mentor: Dr. Michael F. Jasinski
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Geiger-mode avalanche photodiodes (APDs) canconvert the arrival of a single photon into a
digital logic pulse. Arrays of APDs can be directly
interfaced to arrays of per-pixel digital
electronics fabricated in silicon CMOS, providing
the capability to time the arrival of photons in
each pixel. These arrays are of interest for
"flash" LADAR systems, where multiple target
pixels are simultaneously illuminated by the
laser during a single laser pulse, and the
imaging array is used to measure range to each
of the illuminated pixels. This summer I planned
to integrate the GM-APD camera with a Yb:YAG
laser for experimental test of LIDAR and
distance-imaging.
Michael Joseph Williamsreceived the Award of
Excellence for his
research poster at the
2012 NASA Summer
Intern Symposium.
Image Credit: URC.
Abstract:
Geiger Mode APD 1-Kilopixel Camera
for 3-D Topographic Mapping
Michael Joseph Williams
Delaware State UniversityMajor: Optics
Degree Level: Ph.D.
Intern Site: NASA Goddard Space Flight Center
Mentor: Dr. Anthony Yu
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Jason ZiccardiCalifornia State University, Long Beach, CaliforniaMajor: Human Factors Psychology
Degree Level: Master of Science
Intern Site: NASA Ames Research Center
Mentor: Dr. Walter Johnson
Using a simulated air traffic environment, this study
measured the response time, execution time, and
general behavior of unmanned aerial vehicle (UAV)
pilots in response to direct commands from air
traffic controllers. Data was collected from eight
participant UAV pilots who were asked to respond to
and execute ATC commands as quickly as possible.
Quick responses to ATC commands are one factor
essential for UAVs to operate safely with mannedaircraft and this measured response data
contributes to the knowledge base necessary to fully
integrate unmanned aerial systems into the national
airspace in the near future. (Jason Ziccardi and
Zachary Roberts, co-authors)
California State
University student
Jason Ziccardi.
Image Credit: URC.
Abstract:
Measured Response to
UAS Pilot Commands
ARMD
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With sincere appreciation, the National Aeronautics and Space Administration
acknowledges the talent, hard work and dedication to excellence of those whose
contributions have resulted in the success of the NASA University Research
Centers Virtual Poster Session and Symposium.
NASA Summer MentorsDr. Assaf Anyamba, Dr. John Baker, Dr. WilliamBluethmann
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Acknowledgements (Continued)
University Research Center Faculty and Staff
California State University, Long Beach
Dr. Thomas Strybel, Project Director
Dr. Kim-Phuong Vu
Diandra Porter
California State University, Los Angeles
Dr. Helen Ryaciotaki-Boussalis, Project Director
Dr. Darrell GuillaumeDr. Charles Liu
Daisy Lui
Delaware State University
Dr. Noureddine Melikechi, Project Director
Teresa Curto
Jacquelyn Jones
Dr. Renu Tripathi
Florida International University
Dr. Fernando Miralles-Wilhelm, Project Director
Juan Rodriguez
Howard University
Dr. Everette Joseph, Project Director
Katherine Cooke-Mundle
Teria Powell
Dr. Demetrius Venable
Morgan State UniversityDr. Carl White, Project Director
Albert Sweets
North Carolina A&T State University
Dr. Kunigal Shivakumar, Project Director
Latoya Best
Dr. Vinayak Kabadi
North Carolina Central University
Dr. Branislav Vlahovic, Project Director
Sergei Shendrick
Dr. Marvin Wu
Prairie View A&M University
Dr. Richard Wilkins, Project Director
Frank (Pat) Craddock
Dr. Kirby Kelvin
Carolyn Wedeking
University of Texas at Brownsville
Dr. Mario Diaz, Project Director
Leslie GomezMaribel Gonzalez
Robert Stone
Texas Southern University
Dr. Adebayo Oyekan, Project Director
Brandi Butler
University of Puerto Rico, Rio Piedras
Dr. Carlos Cabrera, Project DirectorDr. Ana-Rita Mayol
Omayra Rivera
University of Texas at El Paso
Dr. Ahsan Choudhuri
Laura Barnum
Nathaniel Robinson
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Acknowledgements (Continued)
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Chief, Office of Education
NASA Dryden Flight Research Center
University Research Centers National Project
Manager
Debra Weathers
University Research Centers Project
Administrator
Tyra Wheeler-Zubia
University Research Centers Project
Associate for Evaluations/Communications
Daesha Roberts
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Kaitlin Wright
University Research Centers Summer Intern
Judges Event PlanningCommittee and
Support Staff
For more information regarding the University Research Centers, please visit our website at
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Frank (Pat) Craddock
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