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Regenerating evanescent waves from a silver superlens
Regenerating evanescent waves from a silver superlens

The strongest magnetic fields in the universe: how strong can they
The strongest magnetic fields in the universe: how strong can they

A search for the cause of cyclical wind variability in O stars
A search for the cause of cyclical wind variability in O stars

... variability originates close to the stellar surface. The phase−velocity relation shows a maximum at −1400 km s−1 . The general trend of these observations can be well explained by the corotating interaction region (CIR) model. In this model the wind is perturbed by one or more fixed patches on the s ...
Morphological characteristics of OB spectra and environments
Morphological characteristics of OB spectra and environments

The strongest magnetic fields in the universe: how strong
The strongest magnetic fields in the universe: how strong

Paper
Paper

... surface is equivalent to photons leaving the medium without reflection and would therefore receive a momentum of hk  per incident photon. In contrast, as shown in Ref. [5], a reflecting surface within the medium will recoil with a momentum of 2nhk  per photon. In this case, the standing wave forme ...
Interferometer design for writing Bragg gratings in optical fibers
Interferometer design for writing Bragg gratings in optical fibers

... controls the apparent optical reflection angle between the phase mask and the target, and is equivalent to adjusting either the target or the phase mask angle about the y axis to bring these two components into optical alignment. This alignment is important for maintaining proper focus over the enti ...
Chemistry Review: Strategies for the CRQ`s
Chemistry Review: Strategies for the CRQ`s

... not? Your response must include information about both graphite and diamond. ...
Composition of the Chandra ACIS contaminant
Composition of the Chandra ACIS contaminant

Conference title, upper and lower case, bolded, 18 point
Conference title, upper and lower case, bolded, 18 point

... region should be left un-etched. This saves the multi-etch steps that are typically required in realizing muti-step couplers [4]. As shown in Fig. 2(d), even for the un-etched n-layer case, the coupling length is <60µm. So, thinfilm platform not only offers compact coupler region but is also simple ...
MCDT-NearMagEquiv-(PCCP subm)
MCDT-NearMagEquiv-(PCCP subm)

... be ‘extremely-strongly-coupled’, or ‘nearly-equivalent’. The NMR spectrum of nearly-equivalent spin pairs displays a single peak since the spin-spin coupling suppresses the effect of the small chemical shift difference. This situation is found at high magnetic fields when the chemical shifts of two ...
Intense switchable fluorescence in light wave coupled electrowetting
Intense switchable fluorescence in light wave coupled electrowetting

... operated as follows. Violet light is coupled at an incidence angle ␪LED into the edge of the waveguide. This violet light then propagates within the waveguide 共nsp ⬃ 1.46兲 via internal reflection. Violet light also propagates in all layers contacting the waveguide that have refractive indices greate ...
Novel Approach to the Study of Surface Plasmon Resonance and
Novel Approach to the Study of Surface Plasmon Resonance and

1 Macleod ‐ Thin Film Optics
1 Macleod ‐ Thin Film Optics

... The effects we are interested in are linear. Linear means that if we have two separate  stimuli and two separate responses then the response to the sum of the two stimuli will be  the sum of the separate responses. The important implication is that we can then break  any arbitrary light wave into a  ...
Resonances of the helium atom in a strong magnetic field
Resonances of the helium atom in a strong magnetic field

... particular the interpretation of the absorption features in the spectrum of the MWD GD 229, one of the major remaining mysteries for more than 25 years, could be solved. It was the first high-field MWD with an identified helium atmosphere 关19兴. Nevertheless, the spectra of several MWD’s with an esti ...
metamorphosis of an aspheric Type Ib explosion
metamorphosis of an aspheric Type Ib explosion

... explosion as an energetic event with peak absolute R-band magnitude −18.5 ± 0.16, which is about 1 mag brighter than the mean value (−17.6 ± 0.6) derived for well observed Type Ibc events. The SN is highly extinguished, E(B − V) = 0.63 ± 0.15 mag, mainly due to foreground material present in the hos ...
Controlling the Phase and Amplitude of Plasmon Sources at a Subwavelength Scale
Controlling the Phase and Amplitude of Plasmon Sources at a Subwavelength Scale

Porous Biomimetic Microlens Arrays as Multifunctional Optical
Porous Biomimetic Microlens Arrays as Multifunctional Optical

4. Photometric Concepts and Magnitudes
4. Photometric Concepts and Magnitudes

... correction is positive for stars both cooler or hotter than the Sun. Sometimes the correction is defined as m bol = m v + BC in which case BC ≤ 0 always. The chance for errors is, however, very small, since we must have m bol ≤ m v . The most accurate magnitude measurements are made using photoelect ...
CUT OFF FREQUENCY FOR DIFFERENT MODES
CUT OFF FREQUENCY FOR DIFFERENT MODES

Polarimeter - ScholarWorks@UNO
Polarimeter - ScholarWorks@UNO

cut off frequency for different modes - CDEEP
cut off frequency for different modes - CDEEP

Wave Optics Module Model Library
Wave Optics Module Model Library

Dispersion Compensation using a Prism-pair
Dispersion Compensation using a Prism-pair

Light–matter interaction induces a single positive vortex with swirling
Light–matter interaction induces a single positive vortex with swirling

... prepared by interposing a d = 15 µm layer of nematic LC (MLC6608 from Merck) in between two parallel planar interfaces, a glass plate and a slab of the transparent photoconductor Bi12 SiO20 (BSO), 25 × 25 mm2 , thickness 1 mm. The interior surfaces are treated to obtain the homeotropic anchoring of ...
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Magnetic circular dichroism

Magnetic circular dichroism (MCD) is the differential absorption of left and right circularly polarized (LCP and RCP) light, induced in a sample by a strong magnetic field oriented parallel to the direction of light propagation. MCD measurements can detect transitions which are too weak to be seen in conventional optical absorption spectra; they can also probe paramagnetic properties and the symmetry of the electronic levels of the studied systems, such as metal ion sites.
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