329 research outputs found
Microwave magnetoplasmon absorption by a 2DEG stripe
Microwave absorption by a high mobility 2DEG has been investigated
experimentally using sensitive Electron Paramagnetic Resonance cavity
technique. It is found that MW absorption spectra are chiefly governed by
confined magnetoplasmon excitations in a 2DEG stripe. Spectra of the 2D
magnetoplasmons are studied as a function of magnetic field, MW frequency and
carrier density. The electron concentration is tuned by illumination and
monitored using optical photoluminescence technique.Comment: to be published in International Journal of Modern Physics
On the Asymmetries of Extended X-ray Emission from Planetary Nebulae
Chandra X-ray Observatory (CXO) images have revealed that the X-ray emitting
regions of the molecule-rich young planetary nebulae (PNs) BD+30 3639 (BD+30)
and NGC 7027 are much more asymmetric than their optical nebulosities. To
evaluate the potential origins of these X-ray asymmetries, we analyze X-ray
images of BD+30, NGC 7027, and another planetary nebula resolved by CXO, NGC
6543, within specific energy bands. Image resolution has been optimized by
sub-pixel repositioning of individual X-ray events. The resulting
subarcsecond-resolution images reveal that the soft (E < 0.7 keV) X-ray
emission from BD+30 is more uniform than the harder emission, which is largely
confined to the eastern rim of the optical nebula. In contrast, soft X-rays
from NGC 7027 are highly localized and this PN is more axially symmetric in
harder emission. The broad-band X-ray morphologies of BD+30 and NGC 7027 are
highly anticorrelated with their distributions of visual extinction, as
determined from high-resolution, space- and ground-based optical and infrared
imaging. Hence, it is likely that the observed X-ray asymmetries of these
nebulae are due in large part to the effects of nonuniform intranebular
extinction. However, the energy-dependent X-ray structures in both nebulae and
in NGC 6543 -- which is by far the least dusty and molecule-rich of the three
PNs, and displays very uniform intranebular extinction -- suggests that other
mechanisms, such as the action of collimated outflows and heat conduction, are
also important in determining the detailed X-ray morphologies of young
planetary nebulae.Comment: 33 pages, 12 figures; to appear in the Astrophysical Journa
Improvements in diagnosis have changed the incidence of histological types in advanced gastric cancer.
The data on 912 patients with early cancer and 1245 with advanced cancer who were seen between 1971 and 1990 were compared. The incidence of undifferentiated-type cancer increased significantly in patients with advanced gastric cancer, but not in patients with early gastric cancer. When the histological types were compared with regard to sex, age and location in patients with early gastric cancer the undifferentiated type was found to increase only in males, while in patients with advanced gastric cancer the undifferentiated type increased in both sexes as well as in younger patients and in both the upper and middle third of the stomach. These differences in the trends between early and advanced cancers are probably due to the different degrees of diagnostic accuracy for the early detection of histological types
First record of a Nathusius' pipistrelle (Pipistrellus nathusii) overwintering at a latitude above 60ºN
Highly mobile species are considered to be the first to respond to climate change by transforming their ranges of distribution. There is evidence suggesting that Pipistrellus nathusii, a species capable of long-distance migration, is expanding both its reproduction and overwintering ranges to the North. We recorded the echolocation calls of bats at 16 sites in South-Western Finland on two consecutive winters, and detected calls of P. nathusii at one of the sites throughout the second winter. To our knowledge, this is the northernmost record of an overwintering P. nathusii, and contributes to evidence that the species is already responding to climate change.Peer reviewe
Observations of Sunspot Oscillations in G band and Ca II H line with Solar Optical Telescope on Hinode
Exploiting high-resolution observations made by the Solar Optical Telescope
onboard Hinode, we investigate the spatial distribution of power spectral
density of oscillatory signal in and around NOAA active region 10935. The
G-band data show that in the umbra the oscillatory power is suppressed in all
frequency ranges. On the other hand, in Ca II H intensity maps oscillations in
the umbra, so-called umbral flashes, are clearly seen with the power peaking
around 5.5 mHz. The Ca II H power distribution shows the enhanced elements with
the spatial scale of the umbral flashes over most of the umbra but there is a
region with suppressed power at the center of the umbra. The origin and
property of this node-like feature remain unexplained.Comment: 7 pages, 8 figures, accepted for publication in PASJ (Hinode Special
Issue
Fermi acceleration at fast shock in a solar flare and impulsive loop-top hard X-ray source
We propose that non-thermal electrons are efficiently accelerated by
first-order Fermi process at the fast shock, as a natural consequence of the
new magnetohydrodynamic picture of the flaring region revealed with Yohkoh. An
oblique fast shock is naturally formed below the reconnection site, and boosts
the acceleration to significantly decrease the injection energy. The slow
shocks attached to the reconnection X-point heat the plasma up to 10--20 MK,
exceeding the injection energy. The combination of the oblique shock
configuration and the pre-heating by the slow shock allows bulk electron
acceleration from the thermal pool. The accelerated electrons are trapped
between the two slow shocks due to the magnetic mirror downstream of the fast
shock, thus explaining the impulsive loop-top hard X-ray source discovered with
Yohkoh. Acceleration time scale is ~ 0.3--0.6 s, which is consistent with the
time scale of impulsive bursts. When these electrons stream away from the
region enclosed by the fast shock and the slow shocks, they are released toward
the footpoints and may form the simultaneous double-source hard X-ray structure
at the footpoints of the reconnected field lines.Comment: 13 pages, 3 postscript figures, used AASTeX macros; accepted in
Astrophysical Journal Letter
Zener Tunneling Between Landau Orbits in a High-Mobility Two-Dimensional Electron Gas
Magnetotransport in a laterally confined two-dimensional electron gas (2DEG)
can exhibit modified scattering channels owing to a tilted Hall potential.
Transitions of electrons between Landau levels with shifted guiding centers can
be accomplished through a Zener tunneling mechanism, and make a significant
contribution to the magnetoresistance. A remarkable oscillation effect in weak
field magnetoresistance has been observed in high-mobility 2DEGs in
GaAs-AlGaAs heterostructures, and can be well explained by the
Zener mechanism.Comment: 5 pages, 4 figures. Text slightly shortened, figures resize
Initial Helioseismic Observations by Hinode/SOT
Results from initial helioseismic observations by Solar Optical Telescope
onboard Hinode are reported. It has been demonstrated that intensity
oscillation data from Broadband Filter Imager can be used for various
helioseismic analyses. The k-omega power spectra, as well as corresponding
time-distance cross-correlation function that promises high-resolution
time-distance analysis below 6-Mm travelling distance, were obtained for G-band
and CaII-H data. Subsurface supergranular patterns have been observed from our
first time-distance analysis. The results show that the solar oscillation
spectrum is extended to much higher frequencies and wavenumbers, and the
time-distance diagram is extended to much shorter travel distances and times
than they were observed before, thus revealing great potential for
high-resolution helioseismic observations from Hinode.Comment: 6 pages, accepted for publication in PAS
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