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NASA Scientific and Technical Aerospace Reports

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20040111068 European Space Agency. European Space Research <strong>and</strong> Technology Center, ESTEC, Noordwijk, Netherl<strong>and</strong>s<br />

European Approach to Material Characterization for Plasma Interaction Analysis<br />

VanEesbeek, Marc; Hilgers, Alain; Reulet, Rene; Dirassen, Bernard; Levy, Leon; Montero, Isabel; Galan, Luis; 8th Spacecraft<br />

Charging Technology Conference; March 2004; 10 pp.; In English; See also 20040111031; No Copyright; Avail: CASI; A02,<br />

Hardcopy<br />

The European Space Agency (ESA) has initiated an activity on material characterisation for plasma interaction analysis.<br />

This work is part of a mini-project in the frame of the ESA Technology Research Program, which is also covering two other<br />

main aspects of the research <strong>and</strong> industry community needs, i.e. (1) Spacecraft plasma interaction analysis <strong>and</strong> simulation<br />

software toolkit <strong>and</strong> (2) Guidelines for spacecraft charging <strong>and</strong> plasma interactions. The activities in the three parts will be<br />

harmonized in the framework of SPINE (Spacecraft Plasma Interaction Network in Europe). The main objectives of the<br />

activities described in this paper are: (1) Definition of required material characteristics needed for the different simulation<br />

software, the comparison of different characterisation techniques <strong>and</strong> the available test houses in Europe. (2) Design of a<br />

database for relevant properties on materials used in spacecraft manufacturing; largely concentrated on external surfaces. (3)<br />

Collection <strong>and</strong> integration of existing, <strong>and</strong> verifiable, material property data into an easy accessible database, compatible with<br />

the software under development. (4) Measurement of properties on a set of newly proposed materials.<br />

Author<br />

Plasma Interactions; Computer Programming; Computerized Simulation; Software Development Tools; Spacecraft Charging<br />

20040111083 <strong>NASA</strong> Johnson Space Center, Houston, TX, USA<br />

Specification of ISS Plasma Environment Variability<br />

Minow, Joseph I.; Neergaard, Linda F.; Bui, Them H.; Mikatarian, Ronald R.; Barsamian, H.; Koontz, Steven L.; 8th<br />

Spacecraft Charging Technology Conference; March 2004; 15 pp.; In English; See also 20040111031<br />

Contract(s)/Grant(s): NAS8-00187; No Copyright; Avail: CASI; A03, Hardcopy<br />

Quantifying spacecraft charging risks <strong>and</strong> associated hazards for the International Space Station (ISS) requires a plasma<br />

environment specification for the natural variability of ionospheric temperature (Te) <strong>and</strong> density (Ne). Empirical ionospheric<br />

specification <strong>and</strong> forecast models such as the International Reference Ionosphere (IRI) model typically only provide long term<br />

(seasonal) mean Te <strong>and</strong> Ne values for the low Earth orbit environment. This paper describes a statistical analysis of historical<br />

ionospheric low Earth orbit plasma measurements from the AE-C, AE-D, <strong>and</strong> DE-2 satellites used to derive a model of<br />

deviations of observed data values from IRI-2001 estimates of Ne, Te parameters for each data point to provide a statistical<br />

basis for modeling the deviations of the plasma environment from the IRI model output. Application of the deviation model<br />

with the IRI-2001 output yields a method for estimating extreme environments for the ISS spacecraft charging analysis.<br />

Author<br />

Atmospheric Density; Atmospheric Models; Environment Models; Forecasting; Hazards; Spacecraft Charging; Statistical<br />

Analysis<br />

20040111092 <strong>NASA</strong> Glenn Research Center, Clevel<strong>and</strong>, OH, USA<br />

Solar Array in Simulated LEO Plasma Environment<br />

Vayner, Boris; Galofaro, Joel; Ferguson, Dale; 8th Spacecraft Charging Technology Conference; March 2004; 16 pp.; In<br />

English; See also 20040111031; No Copyright; Avail: CASI; A03, Hardcopy<br />

Six different types of solar arrays have been tested in large vacuum chambers. The low Earth orbit plasma environment<br />

was simulated in plasma vacuum chambers, where the parameters could be controlled precisely. Diagnostic equipment<br />

included spherical Langmuir probes, mass spectrometer, low-noise CCD camera with optical spectrometer, video camera, very<br />

sensitive current probe to measure arc current, <strong>and</strong> a voltage probe to register variations in a conductor potential. All data<br />

(except video) were obtained in digital form that allowed us to study the correlation between external parameters (plasma<br />

density, additional capacitance, bias voltage, etc) <strong>and</strong> arc characteristics (arc rate, arc current pulse width <strong>and</strong> amplitude, gas<br />

species partial pressures, <strong>and</strong> intensities of spectral lines). Arc inception voltages, arc rates, <strong>and</strong> current collections are<br />

measured for samples with different coverglass materials <strong>and</strong> thickness, interconnect designs, <strong>and</strong> cell sizes. It is shown that<br />

the array with wrapthrough interconnects have the highest arc threshold <strong>and</strong> the lowest current collection. Coverglass design<br />

with overhang results in decrease of current collection <strong>and</strong> increase of arc threshold. Doubling coverglass thickness causes the<br />

increase in arc inception voltage. Both arc inception voltage <strong>and</strong> current collection increase significantly with increasing a<br />

sample temperature to 80 C. Sustained discharges are initiated between adjacent cells with potential differences of 40 V for<br />

the sample with 300 m coverglass thickness <strong>and</strong> 60 V for the sample with 150 m coverglass thickness. Installation of cryogenic<br />

pump in large vacuum chamber provided the possibility of considerable outgassing of array surfaces which resulted in<br />

significant decrease of arc rate. Arc sites were determined by employing a video-camera, <strong>and</strong> it is shown that the most probable<br />

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