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Evaluation of the Rayleigh-Gans approximation for microwave scattering by rimed snowflakes
We have evaluated of the applicability of the Rayleigh–Gans (RGA) and Self-Similar Rayleigh–Gans (SSRGA) approximations for microwave scattering by rimed snowflakes. This study extends previous findings that showed that, for unrimed snowflakes, the RGA is in good agreement with the discrete dipole approximation (DDA), which we used as a reference method. When riming is introduced, the RGA-derived scattering properties of individual snowflakes deviate significantly — up to 20–25 dB for the backscattering cross section at the W-band — from the corresponding DDA results. In contrast, the average scattering properties given by RGA are in good agreement with DDA for all but the most heavily rimed snowflakes: the mean bias in the backscattering cross section rarely exceeds 1 dB for light and moderate riming. We also found that an adjustment that accounts for the nonspherical shapes of the ice crystals can help eliminate a small constant bias found in RGA in earlier studies. The SSRGA approximates the RGA results with good accuracy at all degrees of riming, indicating that it, too, can be used with up to moderately rimed snowflakes
Spectropolarimetry of Supernovae
Overwhelming evidence has accumulated in recent years that supernova
explosions are intrinsically 3-dimensional phenomena with significant
departures from spherical symmetry. We review the evidence derived from
spectropolarimetry that has established several key results: virtually all
supernovae are significantly aspherical near maximum light; core-collapse
supernovae behave differently than thermonuclear (Type Ia) supernovae; the
asphericity of core-collapse supernovae is stronger in the inner layers showing
that the explosion process itself is strongly aspherical; core-collapse
supernovae tend to establish a preferred direction of asymmetry; the
asphericity is stronger in the outer layers of thermonuclear supernovae
providing constraints on the burning process. We emphasize the utility of the
Q/U plane as a diagnostic tool and revisit SN 1987A and SN 1993J in a
contemporary context. An axially-symmetric geometry can explain many basic
features of core-collapse supernovae, but significant departures from axial
symmetry are needed to explain most events. We introduce a spectropolarimetry
type to classify the range of behavior observed in polarized supernovae.
Understanding asymmetries in supernovae is important for phenomena as diverse
as the origins of gamma-ray bursts and the cosmological applications of Type Ia
supernovae in studies of the dark energy content of the universe.Comment: Draft of Annual Review article prior to final copy editing; 85 pages,
13 figures, 1 tabl
Future Possibilities for Observing HI at High Redshift
We briefly review the beginnings of HI astronomy, proceed to an assessment of
our current capabilities in this area, and continue by considering what will be
necessary to push back the frontier to cosmological distances. We then consider
how such a leap in performance might be realized.Comment: 8 page LaTeX requires crckapb.sty and psfig.sty, 9 compressed and
tarred postscript figures (750kB) available at
ftp://ftp.nfra.nl/pub/outgoing/rbraun/futposhi/figs.tar.Z Complete compressed
postscript paper (790kB) available at
ftp://ftp.nfra.nl/pub/outgoing/rbraun/futposhi/paper.ps.Z To appear in "Cold
Gas at High Redshift", Eds. M.Bremer et al. (Kluwer, Dordrecht
Rotation Curves of Spiral Galaxies
Rotation curves of spiral galaxies are the major tool for determining the
distribution of mass in spiral galaxies. They provide fundamental information
for understanding the dynamics, evolution and formation of spiral galaxies. We
describe various methods to derive rotation curves, and review the results
obtained. We discuss the basic characteristics of observed rotation curves in
relation to various galaxy properties, such as Hubble type, structure,
activity, and environment.Comment: 40 pages, 6 gif figures; Ann. Rev. Astron. Astrophys. Vol. 39, p.137,
200
Multifunctional biophotonic nanostructures inspired by the longtail glasswing butterfly for medical devices
Numerous living organisms possess biophotonic nanostructures that provide colouration and other diverse functions for survival. While such structures have been actively studied and replicated in the laboratory, it remains unclear whether they can be used for biomedical applications. Here, we show a transparent photonic nanostructure inspired by the longtail glasswing butterfly (Chorinea faunus) and demonstrate its use in intraocular pressure (IOP) sensors in vivo. We exploit the phase separation between two immiscible polymers (poly(methyl methacrylate) and polystyrene) to form nanostructured features on top of a Si3_N_4 substrate. The membrane thus formed shows good angle-independent white-light transmission, strong hydrophilicity and anti-biofouling properties, which prevent adhesion of proteins, bacteria and eukaryotic cells. We then developed a microscale implantable IOP sensor using our photonic membrane as an optomechanical sensing element. Finally, we performed in vivo testing on New Zealand white rabbits, which showed that our device reduces the mean IOP measurement variation compared with conventional rebound tonometry without signs of inflammation
Optical Cloaking with Non-Magnetic Metamaterials
Artificially structured metamaterials have enabled unprecedented flexibility
in manipulating electromagnetic waves and producing new functionalities,
including the cloak of invisibility based on coordinate transformation. Here we
present the design of a non-magnetic cloak operating at optical frequencies.
The principle and structure of the proposed cylindrical cloak are analyzed, and
the general recipe for the implementation of such a device is provided. The
cloaking performance is verified using full-wave finite-element simulations.Comment: 10 pages, 4 figure
Instantaneous whole field measurement of velocity and size of air microbubbles in two-phase flows using DDPIV
Clinical practice: Swallowing problems in cerebral palsy
Cerebral palsy (CP) is the most common physical disability in early childhood. The worldwide prevalence of CP is approximately 2–2.5 per 1,000 live births. It has been clinically defined as a group of motor, cognitive, and perceptive impairments secondary to a non-progressive defect or lesion of the developing brain. Children with CP can have swallowing problems with severe drooling as one of the consequences. Malnutrition and recurrent aspiration pneumonia can increase the risk of morbidity and mortality. Early attention should be given to dysphagia and excessive drooling and their substantial contribution to the burden of a child with CP and his/her family. This review displays the important functional and anatomical issues related to swallowing problems in children with CP based on relevant literature and expert opinion. Furthermore, based on our experience, we describe a plan for approach of investigation and treatment of swallowing problems in cerebral palsy
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