1,024 research outputs found
Very-wide-field camera. Proposal of Space Astronomy Laboratory for second Spacelab mission
A proposal is made for inclusion of a very wide field camera onboard Spacelab. Its scientific program is outlined: detection and photometry, spectrography, and star and starlike object photography. The optics, receptor, and mechanical structure are described. Scientific and technical constraints are discussed, and a development plan is detailed. The dust contamination of Spacelab using the camera was also studied
Time-reversal in dynamically-tuned zero-gap periodic systems
We show that short pulses propagating in zero-gap periodic systems can be
reversed with 100% efficiency by using weak non-adiabatic tuning of the wave
velocity at time-scales that can be much slower than the period. Unlike
previous schemes, we demonstrate reversal of {\em broadband} (few cycle) pulses
with simple structures. Our scheme may thus open the way to time-reversal in a
variety of systems for which it was not accessible before.Comment: Accepted for publication in Phys. Rev. Letter
Spatial distribution of unidentified infrared bands and extended red emission in the compact galactic HII region Sh 152
We present visible and near IR images of the compact HII region Sh 152. Some
of these images reveal the presence of Extended Red Emission (ERE) around 698
nm and emission from Unidentified Infra Red Bands (UIRBs) at 3.3 and 6.2
micron. Other images show the near infrared (7-12 micron) continuous emission
of the nebula. The ERE emission is found to coincide with the ionized region
and significantly differ from the UIRBs location. Also some evidence is found
in favor of grains as carriers for ERE.Comment: 3 pages, 4 figures, to be published in the proceedings of the
colloquium "The universe as seen by ISO" help in Paris, October 20-23, 1998 ;
available in html format at http://www.obs-hp.fr/preprints.htm
Searching for additional heating - [OII] emission in the diffuse ionized gas of NGC891, NGC4631 and NGC3079
We present spectroscopic data of ionized gas in the disk--halo regions of
three edge-on galaxies, NGC 891, NGC 4631 and NGC 3079, covering a wavelength
range from [\ion{O}{2}] 3727\AA to [\ion{S}{2}] 6716.4\AA.
The inclusion of the [\ion{O}{2}] emission provides new constraints on the
properties of the diffuse ionized gas (DIG), in particular, the origin of the
observed spatial variations in the line intensity ratios. We used three
different methods to derive electron temperatures, abundances and ionization
fractions along the slit. The increase in the [\ion{O}{2}]/H line ratio
towards the halo in all three galaxies requires an increase either in electron
temperature or in oxygen abundance. Keeping the oxygen abundance constant
yields the most reasonable results for temperature, abundances, and ionization
fractions. Since a constant oxygen abundance seems to require an increase in
temperature towards the halo, we conclude that gradients in the electron
temperature play a significant role in the observed variations in the optical
line ratios from extraplanar DIG in these three spiral galaxies.Comment: 43 pages, 29 figure
Decay of Quasi-Particle in a Quantum Dot: the role of Energy Resolution
The disintegration of quasiparticle in a quantum dot due to the electron
interaction is considered. It was predicted recently that above the energy
\eps^{*} = \Delta(g/\ln g)^{1/2} each one particle peak in the spectrum is
split into many components ( and are the one particle level spacing
and conductance). We show that the observed value of \eps^{*} should depend
on the experimental resolution \delta \eps. In the broad region of variation
of \delta \eps the should be replaced by \ln(\Delta/ g\delta \eps).
We also give the arguments against the delocalization transition in the Fock
space. Most likely the number of satellite peaks grows continuously with
energy, being at \eps \sim \eps^{*}, but remains finite at \eps >
\eps^{*}. The predicted logarithmic distribution of inter-peak spacings may be
used for experimental confirmation of the below-Golden-Rule decay.Comment: 5 pages, REVTEX, 2 eps figures, version accepted for publication in
Phys. Rev. Let
Euphausiids of the west coast of India
The euphausiids (Class Crustacea: Order Euphausiacea) one of
the major components of the marine zooplankton occurring in the
EEZ of the west coast of India (eastern Arabian Sea) and collected
during the cruises of FORV Sugar Sampada during 1985-1992
period from the epipelagic zone were subjected to specieswise
study for their distribution in space and time and for their ecology
and biology. Seventeen species were encountered of which
Pseudeuphasia latifrons (at an average density of 258/lOOOm^ of
water), Euphausiia diomedeae (1,256), E. sibogae (1,437),
Nematoscelis gracilis (309), Stylocheiron armatum (230) and S.
qffine (216) were the most abundant and cosmopolitan in occurrence.
The other 17 species namely Thysanopoda monacantha, T.
tricuspidata, T. astylata, E. tenera, E. pseudogibba, Nematobrachion
flexipes, S. suhmii, S. microphthalma, S. longicorne, S. abbreviatum
and S. maximum were rather sparsely distributed and their average
number per lOOOm^ of water ranged between 10 and 151 only. The
major species exhibited marked variations in population during
different months and seasons mainly depending on the changes in
the environment
Chaos Thresholds in finite Fermi systems
The development of Quantum Chaos in finite interacting Fermi systems is
considered. At sufficiently high excitation energy the direct two-particle
interaction may mix into an eigen-state the exponentially large number of
simple Slater-determinant states. Nevertheless, the transition from Poisson to
Wigner-Dyson statistics of energy levels is governed by the effective high
order interaction between states very distant in the Fock space. The concrete
form of the transition depends on the way one chooses to work out the problem
of factorial divergency of the number of Feynman diagrams. In the proposed
scheme the change of statistics has a form of narrow phase transition and may
happen even below the direct interaction threshold.Comment: 9 pages, REVTEX, 2 eps figures. Enlarged versio
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