13,737 research outputs found
Interstellar Scintillations of Polarization of Compact Sources
We demostrate that the measurement of fluctuations of polarization due to the
galactic interstellar scintillations may be used to study the structure of the
radiation field at compact radio sources. We develop a mathematical formalism
and demonstrate it on a simple analytical model in which the scale of the
polarization variation through the source is comparable to the source size. The
predicted amplitude of modulation of the polarized radiation flux is ~20% x
(pi_s) x (m_sc), where (pi_s) is the characteristic degree of polarization of
radiation at the source and (m_sc) is the typical modulation index due to
scattering, i.e., (m_sc)~1 for diffractive scintillations and (m_sc)<1 for
refractive scintillations.Comment: 5 pages, 2 figures, emilateapj.sty. Submitted to ApJ
Do Visual-Olfactory Associations Strengthen the Real-Object Preference?
Current knowledge of human object perception relies heavily on studies using images as proxies for real objects. However, real objects are fundamentally different from images. For example, real objects have multisensory properties while images do not. Given that research shows that people look longer at real objects than images of objects, known as the real object preference, and that people look longer at objects when they are presented along with an associated smell, the present pilot study aimed to assess whether visual-olfactory associations contribute to the real-object preference. The present study used a within-subjects design including four participants. Participants viewed a real object alongside an identical image of the object while presented with either a congruent odor (e.g., viewed orange and smelled orange), incongruent odor (e.g., viewed orange and smelled coffee), or neutral odor (e.g., viewed orange and smelled odorless air). Participants’ eyes were tracked using an eye tracker as they viewed the objects, and the percent looking time at the real object was analyzed. Preliminary results suggest that participants looked more at the real object than the image in the neutral odor condition, replicating the real-object preference. Further, the results demonstrated a trend in which congruent odors maintained the real-object preference while incongruent odors decreased the real-object preference. Prior to future data collection, researchers should focus on refining the current experimental design
Experimental assessment of presumed filtered density function models
Measured filtered density functions (FDFs) as well as assumed beta distribution model of mixture fraction and “subgrid” scale (SGS) scalar variance, used typically in large eddy simulations, were studied by analysing experimental data, obtained from two-dimensional planar, laser induced fluorescence measurements in isothermal swirling turbulent flows at a constant Reynolds number of 29 000 for different swirl numbers (0.3, 0.58, and 1.07)
Comparison of imaging with sub-wavelength resolution in the canalization and resonant tunnelling regimes
We compare the properties of subwavelength imaging in the visible wavelength
range for metal-dielectric multilayers operating in the canalization and the
resonant tunnelling regimes. The analysis is based on the transfer matrix
method and time domain simulations. We show that Point Spread Functions for the
first two resonances in the canalization regime are approximately Gaussian in
shape. Material losses suppress transmission for higher resonances, regularise
the PSF but do not compromise the resolution. In the resonant tunnelling
regime, the MTF may dramatically vary in their phase dependence. Resulting PSF
may have a sub-wavelength thickness as well as may be broad with multiple
maxima and a rapid phase modulation. We show that the width of PSF may be
reduced by further propagation in free space, and we provide arguments to
explain this surprising observation.Comment: 17 pages,12 figure
Growth of Perturbation in Gravitational Collapse and Accretion
When a self-gravitating spherical gas cloud collapses or accretes onto a
central mass, the inner region of the cloud develops a density profile
and the velocity approaches free-fall. We show that in
this region, nonspherical perturbations grow with decreasing radius. In the
linear regime, the tangential velocity perturbation increases as ,
while the Lagrangian density perturbation, , grows as
. Faster growth occurs if the central collapsed object maintains a
finite multiple moment, in which case increases as ,
where specifies the angular degree of the perturbation. These scaling
relations are different from those obtained for the collapse of a homogeneous
cloud. Our numerical calculations indicate that nonspherical perturbations are
damped in the subsonic region, and that they grow and approach the asymptotic
scalings in the supersonic region. The implications of our results to
asymmetric supernova collapse and to black hole accretion are briefly
discussed.Comment: 23 pages including 6 ps figures; Minor changes and update; To appear
in ApJ, 200
Hysteretic and chaotic dynamics of viscous drops in creeping flows with rotation
It has been shown in our previous publication
(Blawzdziewicz,Cristini,Loewenberg,2003) that high-viscosity drops in two
dimensional linear creeping flows with a nonzero vorticity component may have
two stable stationary states. One state corresponds to a nearly spherical,
compact drop stabilized primarily by rotation, and the other to an elongated
drop stabilized primarily by capillary forces. Here we explore consequences of
the drop bistability for the dynamics of highly viscous drops. Using both
boundary-integral simulations and small-deformation theory we show that a
quasi-static change of the flow vorticity gives rise to a hysteretic response
of the drop shape, with rapid changes between the compact and elongated
solutions at critical values of the vorticity. In flows with sinusoidal
temporal variation of the vorticity we find chaotic drop dynamics in response
to the periodic forcing. A cascade of period-doubling bifurcations is found to
be directly responsible for the transition to chaos. In random flows we obtain
a bimodal drop-length distribution. Some analogies with the dynamics of
macromolecules and vesicles are pointed out.Comment: 22 pages, 13 figures. submitted to Journal of Fluid Mechanic
An Extinction Study of the Taurus Dark Cloud Complex
We present a study of the detailed distribution of extinction in a region of
the Taurus dark cloud complex. Our study uses new BVR images of the region,
spectral classification data for 95 stars, and IRAS Sky Survey Atlas (ISSA) 60
and 100 micron images. We study the extinction of the region in four different
ways, and we present the first inter-comparison of all these methods, which
are: 1) using the color excess of background stars for which spectral types are
known; 2) using the ISSA 60 and 100 micron images; 3) using star counts; and 4)
using an optical (V and R) version of the average color excess method used by
Lada et al. (1994). We find that all four methods give generally similar
results, with important exceptions. To study the structure in the dust
distribution, we compare the ISSA extinction and the extinction measured for
individual stars. From the comparison, we conclude that in the relatively low
extinction regions studied, with 0.9 < A_V < 3.0 mag (away from filamentary
dark clouds and IRAS cores), there are no fluctuations in the dust column
density greater than 45% (at the 99.7% confidence level), on scales smaller
than 0.2 pc. We also report the discovery of a previously unknown stellar
cluster behind the Taurus dark cloud near R.A 4h19m00s, Dec. 27:30:00 (B1950)Comment: 49 pages (which include 6 pages of tables and 6 pages of figures
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