Jarred Alexander Young September 18, 2013. Beam Analysis Performed scans with RPA perpendicular to...
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Transcript of Jarred Alexander Young September 18, 2013. Beam Analysis Performed scans with RPA perpendicular to...
High Energy Plume Impingement on Spacecraft Systems
AFOSR Telecon
Jarred Alexander YoungSeptember 18, 2013
Current Events
Beam Analysis Performed scans with RPA perpendicular
to beam to look at possible CEX behavior
Material Experiments Completed second round of experiments
with Aluminum samples
CEX Beam Data Beam Data from
recent experiments shows that CEX energy distribution peak increases in energy and probability with axial distance
Tests performed with a background pressure ~3-5E-4 torr 10 12 14 16 18 20 22 24
-5.00E-10
0.00E+00
5.00E-10
1.00E-09
1.50E-09
2.00E-09
2.50E-09
Energy Distribution Comparisons
Particle Energy (eV)
Curr
ent
Spec
tral
Den
sity
(A/
V)
CEX Beam Data Most papers indicate that CEX energy levels are
heavily influenced by facility environment High background pressures lead to higher densities of
CEX ions Papers indicate that CEX environment found in lab
testing is usually not indicative of space conditions
Electron temperature plays a great part in CEX ion energy distribution Higher Te leads to higher CEX energy peaks Paper: Far Field Modeling of the Plasma Plume of a
Hall Thruster, Boyd and Dressler, 2002
CEX Beam Data
Possible plan of attack: analyze electron temperature of ion beam Set up and use an array of langmuir
probes to gather plasma characteristics of the beam and facility environment for clues to CEX energy trends
Previous data sent to Burak for implementation to simulation
Samples, Pre-Beam
Sample 1, 150 eV Sample 2, 150 eV Sample 3, 150 eV
Sample 4, 150 eV Sample 5, 150 eV Sample 6, 150 eV
Samples, Post-Beam
Sample 1, 150 eV Sample 2, 150 eV Sample 3, 150 eV
Sample 4, 150 eV Sample 5, 150 eV Sample 6, 150 eV
Sample Comparison
SAMPLE 1, PRE-BEAM SAMPLE 1, POST-BEAM
Comparison of EDS Results Pre & Post-Sample 1 (whole surface)
PRE BEAM POST BEAM
Spots on SEM Images
Heavier elements in SEM show up as bright-colored Spots are made up
of lighter elements Concentrated
amounts of Mg, Si, C, and O appear in majority of “dark” areas
Summary of Sample Results
All samples show signs of all major elements represented in Al 6061-T4 Copper retroactively found in samples
scanned last week Two samples showed traces of Rhodium
in small amounts (which may also be in Al 6061-T4)
Samples appear polished and no sign of material removal
Implications of Sample Results
Different types of ion impingement Backstreaming ions low energy▪ Interested in sheath potentials of spacecraft in
LEO-GEO High energy ion plume (> 300 eV)▪ Find suitable power supply solution
Expanding tests to other materials Looking into solar cell cover glass Mylar
Future Work
Work on electron temperature gathering for PSU group Data will be included into plasma
simulation
Work on next phase of material testing Develop power supply solution for high
energy beam testing Determine energies for low energy
testing