44,529 research outputs found
Common Bulkhead Joint Development and Evaluation Final Report
Optimized composite welded joint design for Saturn booster common bulkhea
High-shock FM transmitter Final report, phase I
Electronic component testing of high-shock FM TRANSMITTER
Development and fracture mechanics data for 6Al-6V-2 Sn titanium alloy
Fracture mechanics properties of 6Al-6V-2Sn titanium in the annealed, solution-treated, and aged condition are presented. Tensile, fracture toughness, cyclic flaw growth, and sustained-load threshold tests were conducted. Both surface flaw and compact tension-specimen geometries were employed. Temperatures and/or environments used were -65 F (220 K) air, ambient, 300 F (422 K) air, and room-temperature air containing 10 and 100% relative humidity
Measuring cosmic magnetic fields by rotation measure-galaxy cross-correlations in cosmological simulations
Using cosmological MHD simulations of the magnetic field in galaxy clusters
and filaments we evaluate the possibility to infer the magnetic field strength
in filaments by measuring cross-correlation functions between Faraday Rotation
Measures (RM) and the galaxy density field. We also test the reliability of
recent estimates considering the problem of data quality and Galactic
foreground (GF) removal in current datasets. Besides the two self-consistent
simulations of cosmological magnetic fields based on primordial seed fields and
galactic outflows analyzed here, we also explore a larger range of models
scaling up the resulting magnetic fields of one of the simulations. We find
that, if an unnormalized estimator for the cross-correlation functions and a GF
removal procedure is used, the detectability of the cosmological signal is only
possible for future instruments (e.g. SKA and ASKAP). However, mapping of the
observed RM signal to the underlying magnetization of the Universe (both in
space and time) is an extremely challenging task which is limited by the
ambiguities of our model parameters, as well as to the weak response of the RM
signal in low density environments. Therefore, we conclude that current data
cannot constrain the amplitude and distribution of magnetic fields within the
large scale structure and a detailed theoretical understanding of the build up
and distribution of magnetic fields within the Universe will be needed for the
interpretation of future observations.Comment: 11 pages, 11 figures, comparation between RM data and simulations in
fig. 8, submited to MNRAS
Sulphur molecules in the circumstellar envelopes of M-type AGB stars
The sulphur compounds SO and SO have not been widely studied in the
circumstellar envelopes of asymptotic giant branch (AGB) stars. By presenting
and modelling a large number of SO and SO lines in the low mass-loss rate
M-type AGB star R Dor, and modelling the available lines of those molecules in
a further four M-type AGB stars, we aim to determine their circumstellar
abundances and distributions. We use a detailed radiative transfer analysis
based on the accelerated lambda iteration method to model circumstellar SO and
SO line emission and molecular data files for both SO and SO that are
more extensive than those previously available. Using 17 SO lines and 98 SO2
lines to constrain our models for R Dor, we find an SO abundance of
6.7x10 and an SO abundance of 5x10 with both species having
high abundances close to the star. We also modelled SO and found an
abundance of 3.1x10, giving an SO/SO ratio of 21.6. We
derive similar results for the circumstellar SO and SO abundances and their
distributions for the low mass-loss rate object W Hya. For these stars, the
circumstellar SO and SO abundances are much higher than predicted by
chemical models and these two species may account for all available sulphur.
For the higher mass-loss rate stars, we find shell-like SO distributions with
peak abundances that decrease and peak abundance radii that increase with
increasing mass-loss rate. The positions of the peak SO abundance agree very
well with the photodissociation radii of HO. We find evidence that SO is
most likely through the photodissociation of HO and the subsequent reaction
between S and OH. The S-bearing parent molecule appears not to be HS. The
SO models suggest an origin close to the star for this species, also
disagreeing with current chemical models.Comment: 25 page
Experimental study of pop-in behavior of surface flaw-type cracks Final report
Growth behavior of surface-flaw type cracks in titanium alloy
Fatigue flaw growth behavior in stiffened and unstiffened panels loaded in biaxial tension
The effect was investigated of biaxial loading on the flaw growth rate of 2219-T87 aluminum alloy that would be typical of Space Shuttle cryogenic tankage design. The stress distribution and stress concentration factors for several integrally stiffened panels under various loading conditions were obtained. The flaw growth behavior of both stiffened and unstiffened panels under biaxial loading conditions was determined. The effect of a complex stress state was studied by introducing flaws in fillet areas of biaxially loaded stiffened panels
The KATRIN Experiment
The KArlsruhe TRitium Neutrino mass experiment, KATRIN, aims to search for
the mass of the electron neutrino with a sensitivity of 0.2 eV/c^2 (90% C.L.)
and a detection limit of 0.35 eV/c^2 (5 sigma). Both a positive or a negative
result will have far reaching implications for cosmology and the standard model
of particle physics and will give new input for astroparticle physics and
cosmology. The major components of KATRIN are being set up at the Karlsruhe
Institut of Technology in Karlsruhe, Germany, and test measurements of the
individual components have started. Data taking with tritium is scheduled to
start in 2012.Comment: 3 pages, 1 figure, proceedings of the TAUP 2009 International
Conference on Topics in Astroparticle and Underground Physics, to be
published in Journal of Physics, Conference Serie
Impossible shadows and lightness constancy
The intersection between an illumination and a reflectance edge is characterised by the
`ratio-invariant' property, that is the luminance ratio of the regions under different illumination
remains the same.
In a CRT experiment, we shaped two areas, one surrounding the other, and simulated
an illumination edge dividing them in two frames of illumination. The portion of the illumina-
tion edge standing on the surrounding area (labelled contextual background) was the contextual
edge, while the portion standing on the enclosed area (labelled mediating background) was the
mediating edge. On the mediating background, there were two patches, one per illumination
frame. Observers were asked to adjust the luminance of the patch in bright illumination to
equate the lightness of the other. We compared conditions in which the luminance ratio at the
contextual edge could be (i) equal (possible shadow), or (ii) larger (impossible shadow) than
that at the mediating edge. In addition, we manipulated the reflectance of the backgrounds.
It could be higher for the contextual than for the mediating background; or, vice versa, lower
for the contextual than for the mediating background. Results reveal that lightness constancy
significantly increases when: (i) the luminance ratio at the contextual edge is larger than that at
the mediating edge creating an impossible shadow, and (ii) the reflectance of the contextual
background is lower than that of the mediating one. We interpret our results according to the
albedo hypothesis, and suggest that the scission process is facilitated when the luminance ratio
at the contextual edge is larger than that at the mediating edge and/or the reflectance of the
including area is lower than that of the included one. This occurs even if the ratio-invariant
property is violated
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