NASA Scientific and Technical Aerospace Reports
NASA Scientific and Technical Aerospace Reports
NASA Scientific and Technical Aerospace Reports
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wavelengths is not readily available, the constants can be estimated from the atomic refractivities of carbon <strong>and</strong> fluorine. In<br />
order to verify this estimation, a two-beam interferometer was used to experimentally determine the specific refractivities of<br />
CF4 <strong>and</strong> C2F6. This data was required for holographic interferometric measurements made at the Langley Hypersonic CF4<br />
Tunnel. A Twyman-Green interferometer with a He-Ne laser light source of vacuum wavelength lambda equal to 633 nm was<br />
used to measure the constants. One beam of the two-beam interferometer passed through an optical cell of known inside length<br />
l which could be evacuated <strong>and</strong> slowly filled with the test gas to a density of 7.2 kg/cu m for CF4 or 5.7 kg/cu m for C2F6.<br />
If the refractive index (<strong>and</strong> hence density) is constant along the optical path through the cell, the fringe shift M <strong>and</strong> density<br />
change Delta rho are related M = 2Kl Delta rho/lambda for the double pass interferometer. Thus K can be determined by<br />
measuring the fringe shift as the density is changed. The output of a photodiode used to detect the fringe shift was recorded<br />
on a strip chart recorder. The rate of pressure increase of the test gas in the cell was controlled such that the fringes shifted<br />
at a rate of 0.5 to 1 fringe per sec. The pressure in the test cell was measured with a high accuracy quartz crystal pressure<br />
transducer <strong>and</strong> recorded approximately every 20 fringe peaks. The temperature of the cell was measured with a thermocouple<br />
<strong>and</strong> recorded at the start, midpoint, <strong>and</strong> end of each test.<br />
Author (revised)<br />
Refractivity; Carbon Compounds; Fluorine Compounds<br />
20040121086 Polish Academy of Sciences, Warsaw, Pol<strong>and</strong><br />
High Pressure X-Ray Diffraction Studies of Nanocrystalline Materials<br />
Palosz, B.; Stel’makh, S.; Grzanka, E.; Gierlotka, S.; Palosz, W.; [2004]; 1 pp.; In English; 22nd European Cristallographic<br />
Meeting, 26-31 Aug. 2004, Budapest, Hungary<br />
Contract(s)/Grant(s): NAS8-02096; No Copyright; Avail: Other Sources; Abstract Only<br />
Experimental evidence obtained for a variety of nanocrystalline materials suggest that the crystallographic structure of a<br />
very small size particle deviates from that in the bulk crystals. In this paper we show the effect of the surface of nanocrystals<br />
on their structure by the analysis of generation <strong>and</strong> distribution of macro- <strong>and</strong> micro-strains at high pressures <strong>and</strong> their<br />
dependence on the grain size in nanocrystalline powders of Sic. We studied the structure of Sic nanocrystals by in-situ<br />
high-pressure powder diffraction technique using synchrotron <strong>and</strong> neutron sources <strong>and</strong> hydrostatic or isostatic pressure<br />
conditions. The diffraction measurements were done in HASYLAB at DESY using a Diamond Anvil Cell (DAC) in the energy<br />
dispersive geometry in the diffraction vector range up to 3.5 - 4/A <strong>and</strong> under pressures up to 50 GPa at room temperature.<br />
In-situ high pressure neutron diffraction measurements were done at LANSCE in Los Alamos National Laboratory using the<br />
HIPD <strong>and</strong> HIPPO diffractometers with the Paris-Edinburgh <strong>and</strong> TAP-98 cells, respectively, in the diffraction vector range up<br />
to 26 Examination of the response of the material to external stresses requires nonst<strong>and</strong>ard methodology of the materials<br />
characterization <strong>and</strong> description. Although every diffraction pattern contains a complete information on macro- <strong>and</strong><br />
micro-strains, a high pressure experiment can reveal only those factors which contribute to the characteristic diffraction<br />
patterns of the crystalline phases present in the sample. The elastic properties of powders with the grain size from several nm<br />
to micrometers were examined using three methodologies: (l), the analysis of positions <strong>and</strong> widths of individual Bragg<br />
reflections (used for calculating macro- <strong>and</strong> micro-strains generated during densification) [I], (2). the analysis of the<br />
dependence of the experimental apparent lattice parameter, alp, on the diffraction vector Q [2], <strong>and</strong> (3), the atomic Pair<br />
Distribution Function (PDF) technique [3]. The results of our studies show, that Sic nanocrystals have the features of two<br />
phases, each with its distinct elastic properties. <strong>and</strong> under pressures up to 8 GPa.<br />
Author<br />
Nanocrystals; X Ray Diffraction; High Pressure; Crystal Structure; Grain Size; Distribution Functions<br />
20040121105 Universidad del Turabo, Puerto Rico<br />
Hydrogen Purification Using Natural Zeolite Membranes<br />
DelValle, William; 2003 Research <strong>Reports</strong>: <strong>NASA</strong>/ASEE Fellowship Program; December 15, 2003, pp. F1 - F7; In English;<br />
See also 20040121096; No Copyright; Avail: CASI; A02, Hardcopy<br />
The School of Science at Universidad del Turabo (UT) have a long-lasting investigation plan to study the hydrogen<br />
cleaning <strong>and</strong> purification technologies. We proposed a research project for the synthesis, phase analysis <strong>and</strong> porosity<br />
characterization of zeolite based ceramic perm-selective membranes for hydrogen cleaning to support <strong>NASA</strong>’s commitment<br />
to achieving a broad-based research capability focusing on aerospace-related issues. The present study will focus on<br />
technology transfer by utilizing inorganic membranes for production of ultra-clean hydrogen for application in combustion.<br />
We tested three different natural zeolite membranes (different particle size at different temperatures <strong>and</strong> time of exposure). Our<br />
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