343 research outputs found
Eddy current effects in plain and hollow cylinders spinning inside homogeneous magnetic fields: Application to magnetic resonance
International audienceWe present a thorough analysis of eddy currents that develop in a rectangular cross section toroid rotating in a uniform magnetic field. The slow rotation regime is assumed. Compact expressions for the current density, the total dissipated power, and the braking torque are given. Examination of the topology of current lines reveals that depending upon the relative dimensions of the side and length of the toroid two different regimes exist. The conditions of existence of the two regimes are analytically established. In view of nuclear magnetic resonance (NMR) applications, we derive the angular variation of the magnetic field created by eddy currents and lay down the formalism necessary for calculating the effect of this field on the NMR spectra of the conductor itself or of a sample co-rotating with the conductor, a situation encountered when dealing with rotating detectors. Examples of calculations for cases of practical interest are presented. The theory is confronted with available data, and we give guidelines for the design of optimized rotating micro-coils
Optimal transport of ultracold atoms in the non-adiabatic regime
We report the transport of ultracold atoms with optical tweezers in the
non-adiabatic regime, i.e. on a time scale on the order of the oscillation
period. We have found a set of discrete transport durations for which the
transport is not accompanied by any excitation of the centre of mass of the
cloud. We show that the residual amplitude of oscillation of the dipole mode is
given by the Fourier transform of the velocity profile imposed to the trap for
the transport. This formalism leads to a simple interpretation of our data and
simple methods for optimizing trapped particles displacement in the
non-adiabatic regime
First High Contrast Imaging Using a Gaussian Aperture Pupil Mask
Placing a pupil mask with a gaussian aperture into the optical train of
current telescopes represents a way to attain high contrast imaging that
potentially improves contrast by orders of magnitude compared to current
techniques. We present here the first observations ever using a gaussian
aperture pupil mask (GAPM) on the Penn State near-IR Imager and Spectrograph
(PIRIS) at the Mt. Wilson 100 telescope. Two nearby stars were
observed, Eridani and Her A. A faint companion was detected
around Her A, confirming it as a proper motion companion. Furthermore,
the observed H and K magnitudes of the companion were used to constrain its
nature. No companions or faint structure were observed for Eridani.
We found that our observations with the GAPM achieved contrast levels similar
to our coronographic images, without blocking light from the central star. The
mask's performance also nearly reached sensitivities reported for other ground
based adaptive optics coronographs and deep HST images, but did not reach
theoretically predicted contrast levels. We outline ways that could improve the
performance of the GAPM by an order of magnitude or more.Comment: 8 pages, 4 figures, accepted by ApJ letter
Circularly Symmetric Apodization via Starshaped Masks
Recently, we introduced a class of shaped pupil masks, called spiderweb
masks, that produce point spread functions having annular dark zones. With such
masks, a single image can be used to probe a star for extrasolar planets. In
this paper, we introduce a new class of shaped pupil masks that also provide
annular dark zones. We call these masks starshaped masks. Given any circularly
symmetric apodization function, we show how to construct a corresponding
starshaped mask that has the same point-spread function (out to any given outer
working distance) as obtained by the apodization.Comment: Paper also at:
http://www.orfe.princeton.edu/~rvdb/tex/starshape/ms.pdf Updated to clarify
misleading statements regarding total throughput for apodizations and their
corresponding starshaped mask
Estimation d’une fonction de demande de monnaie pour la zone euro : une synthèse des résultats.
A Tunable Lyot Filter at Prime Focus: a Method for Tracing Supercluster Scales at z ~ 1
Tunable narrow-band, emission-line surveys have begun to show the ease with
which star forming galaxies can be identified in restricted redshift intervals
to z ~ 5 with a 4m class telescope. These surveys have been carried out with
imaging systems at the Cassegrain or Nasmyth focus and are therefore restricted
to fields smaller than 10 arcmin. We now show that tunable narrowband imaging
is possible over a 30 arcmin field with a high-performance Lyot filter placed
directly in front of a CCD mosaic at the prime focus. Our design is intended
for the f/3.3 prime focus of the AAT 3.9m, although similar devices can be
envisaged for the Subaru 8m (f/2), Palomar 5m (f/3.4), VISTA 4m (f/6), Mayall
4m (f/2.6) or CFHT 3.6m (f/4). A modified Wynne doublet ensures sub-arcsecond
performance over the field. In combination with the new Wide-Field Imaging 8K x
8K mosaic (WFI) at the AAT, the overall throughput (35%) of the system to
unpolarised light is expected to be comparable to the TAURUS Tunable Filter
(TTF). Unlike the TTF, the field is fully monochromatic and the instrumental
profile has much better wing suppression. For targetted surveys of
emission-line sources at z ~ 1, a low-resolution (R ~ 150 at 550nm) Lyot filter
on a 4m telescope is expected to be comparable or superior to current
instruments on 8-10m class telescopes. We demonstrate that the 30 arcmin field
is well matched to superclusters at these redshifts such that large-scale
structure should be directly observable.Comment: Astrophysical Journal, accepted. 53 pages, 16 figures, aaste
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