11,587 research outputs found
Analysis of noise measured from a propeller in a wake
In this experimental study, the acoustic characteristics of a propeller operating in a wake were studied. The propeller performance and noise were measured from two 0.25 scale propellers operating in an open jet anechoic flow environment with and without a wake. One propeller had NACA 16 series sections; the other, ARA-D. Wake thicknesses of 1 and 3 propeller chords were generated by an airfoil which spanned the full diameter of the propeller. The airfoil wake profiles were measured. Noise measurements were made in and out of the flow. The propellers were operated at 40, 83, and 100 inf of thrust. The acoustic data are analyzed, and the effects on the overall sound pressure level (OASPL) and scaled A weighted sound level L sub A with propeller thrust, wake thickness, and observer location are presented. The analysis showed that, generally, the wake increased the overall noise (OASPL) produced by the propeller; increased the harmonic content of the noise, thus the scaled L sub a; and produced an azimuthal dependence. With few exceptions, both propellers generally produced the same trends in delta OASPL and delta L sub a with thrust and wake thickness
Decoupling the coupled DGLAP evolution equations: an analytic solution to pQCD
Using Laplace transform techniques, along with newly-developed accurate
numerical inverse Laplace transform algorithms, we decouple the solutions for
the singlet structure function and of the two
leading-order coupled singlet DGLAP equations, allowing us to write fully
decoupled solutions: F_s(x,Q^2)={\cal F}_s(F_{s0}(x), G_0(x)), G(x,Q^2)={\cal
G}(F_{s0}(x), G_0(x)). Here and are known
functions---found using the DGLAP splitting functions---of the functions
and , the chosen
starting functions at the virtuality . As a proof of method, we compare
our numerical results from the above equations with the published MSTW LO gluon
and singlet distributions, starting from their initial values at . Our method completely decouples the two LO distributions, at the same
time guaranteeing that both distributions satisfy the singlet coupled DGLAP
equations. It furnishes us with a new tool for readily obtaining the effects of
the starting functions (independently) on the gluon and singlet structure
functions, as functions of both and . In addition, it can also be
used for non-singlet distributions, thus allowing one to solve analytically for
individual quark and gluon distributions values at a given and , with
typical numerical accuracies of about 1 part in , rather than having to
evolve numerically coupled integral-differential equations on a two-dimensional
grid in , as is currently done.Comment: 6 pages, 2 figure
Measurements of farfield sound generation from a flow-excited cavity
Results of 1/3-octave-band spectral measurements of internal pressures and the external acoustic field of a tangentially blown rectangular cavity are compared. Proposed mechanisms for sound generation are reviewed, and spectra and directivity plots of cavity noise are presented. Directivity plots show a slightly modified monopole pattern. Frequencies of cavity response are calculated using existing predictions and are compared with those obtained experimentally. The effect of modifying the upstream boundary layer on the noise was investigated, and its effectiveness was found to be a function of cavity geometry and flow velocity
Noise response of cavities of varying dimensions at subsonic speeds
An expression for the Strouhal number of lengthwise cavity oscillations is obtained which includes the effect of length-to-depth ratio. This expression, which agrees well with the experimental data, is also used to predict the Mach number at which cavity acoustic response is maximum. Interaction between lengthwise and depthwise modes is seen to occur at Mach numbers from 0.1 to 0.5. Cavity shape is shown to affect the noise spectra in generating either a broadband or narrowband signal
Implications of a Froissart bound saturation of - deep inelastic scattering. Part II. Ultra-high energy neutrino interactions
In Part I (in this journal) we argued that the structure function
in deep inelastic scattering, regarded as a cross
section for virtual scattering, has a saturated Froissart-bounded
form behaving as at small . This form provides an excellent
fit to the low HERA data, including the very low regions, and can be
extrapolated reliably to small using the natural variable . We
used our fit to derive quark distributions for values of down to
. We use those distributions here to evaluate ultra-high energy
(UHE) cross sections for neutrino scattering on an isoscalar nucleon,
, up to laboratory neutrino energies -
GeV where there are now limits on neutrino fluxes. We estimate that these cross
sections are accurate to 2% at the highest energies considered, with the
major uncertainty coming from the errors in the parameters that were needed to
fit . We compare our results to recently published
neutrino cross sections derived from NLO parton distribution functions, which
become much larger at high energies because of the use of power-law
extrapolations of quark distributions to small . We argue that our
calculation of the UHE cross sections is the best one can make based
the existing experimental deep inelastic scattering data. Further, we show that
the strong interaction Froissart bound of on
translates to an exact bound of for leading-order-weak
scattering. The energy dependence of total cross section measurements
consequently has important implications for hadronic interactions at enormous
cms (center-of-mass) energies not otherwise accessible.Comment: 15 pages, 6 figures. The paper is now shorter with the new results
clearly emphasize
Implications of a Froissart bound saturation of - deep inelastic scattering. Part I. Quark distributions at ultra small
We argue that the deep inelastic structure function ,
regarded as a cross section for virtual scattering, is hadronic in
nature. This implies that its growth is limited by the Froissart bound at high
hadronic energies, giving a bound on as Bjorken
. The same bound holds for the individual quark distributions.
In earlier work, we obtained a very accurate global fit to the combined HERA
data on using a fit function which respects the Froissart
bound at small , and is equivalent in its dependence to the function
used successfully to describe all high energy hadronic cross sections,
including scattering. We extrapolate that fit by a factor of
3 beyond the HERA region in the natural variable to the
values of down to and use the results to derive the quark
distributions needed for the reliable calculation of neutrino cross sections at
energies up to GeV. These distributions do not satisfy the
Feynman "wee parton" assumption, that they all converge toward a common
distribution at small and large . This was used in some
past calculations to express the dominant neutrino structure function
directly in terms of . We show that the
correct distributions nevertheless give results for
which differ only slightly from those obtained assuming that the wee parton
limit holds. In two Appendices, we develop simple analytic results for the
effects of QCD evolution and operator-product corrections on the distribution
functions at small , and show that these effects amount mainly to shifting
the values of in the initial distributions.Comment: 19 pages, 6 figures. The paper is now shorter with the new results
clearly emphasize
All Adults Once Were Children
Issue Editor, Robert Block\u27s, point of view and summary of the articles in New Morbidities 2.
The Ghostly-Silent Guns of Galveston: A Chronicle of Colonel J.G. Kellersberger, the Confederate Chief Engineer of East Texas
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