22,404 research outputs found
Low-Voltage High-Linearity Wideband Current Differencing Transconductance Amplifier and Its Application on Current-Mode Active Filter
A low-voltage high-linearity wideband current differencing transconductance amplifier (CDTA) is presented in this paper. The CDTA consists of a current differencing circuit and a cross-coupling transconductance circuit. The PSPICE simulations of the proposed CDTA show a good performance: -3dB frequency bandwith is about 900 MHz, low power consumption is 2.48 mW, input current linear range is ±100 µA and low current-input resistance is less than 20 Ω, high current-output resistance is more than 3 MΩ. PSpice simulations for a current-mode universal filter and a proposed high-order filter are also conducted, and the results verify the validity of the proposed CDTA
GNSS troposphere tomography based on two-step reconstructions using GPS observations and COSMIC profiles
Traditionally, balloon-based radiosonde soundings are
used to study the spatial distribution of atmospheric water vapour. However,
this approach cannot be frequently employed due to its high cost. In
contrast, GPS tomography technique can obtain water vapour in a high temporal
resolution. In the tomography technique, an iterative or non-iterative
reconstruction algorithm is usually utilised to overcome rank deficiency of
observation equations for water vapour inversion. However, the single
iterative or non-iterative reconstruction algorithm has their limitations.
For instance, the iterative reconstruction algorithm requires accurate
initial values of water vapour while the non-iterative reconstruction
algorithm needs proper constraint conditions. To overcome these drawbacks,
we present a combined iterative and non-iterative reconstruction approach
for the three-dimensional (3-D) water vapour inversion using GPS observations
and COSMIC profiles. In this approach, the non-iterative reconstruction
algorithm is first used to estimate water vapour density based on a priori
water vapour information derived from COSMIC radio occultation data. The
estimates are then employed as initial values in the iterative
reconstruction algorithm. The largest advantage of this approach is that
precise initial values of water vapour density that are essential in the
iterative reconstruction algorithm can be obtained. This combined
reconstruction algorithm (CRA) is evaluated using 10-day GPS observations in
Hong Kong and COSMIC profiles. The test results indicate that the water
vapor accuracy from CRA is 16 and 14% higher than that of iterative
and non-iterative reconstruction approaches, respectively. In addition, the
tomography results obtained from the CRA are further validated using
radiosonde data. Results indicate that water vapour densities derived from
the CRA agree with radiosonde results very well at altitudes above 2.5 km.
The average RMS value of their differences above 2.5 km is 0.44 g m<sup>−3</sup>
Isoflurane And Propofol Synergy In Reducing Heart-type Fatty Acid Binding Protein In Patients Undergoing Coronary Artery Bypass Graft Surgery
Conference Theme: Emerging Therapies for an Aging Populationpublished_or_final_versio
A Closing Lemma for a Class of Symplectic Diffeomorphisms
We prove a closing lemma for a class of partially hyperbolic symplectic
diffeomorphisms. We show that for a generic symplectic diffeomorphism, , with two dimensional center and close to a product map, the set
of all periodic points is dense
The Physical Connections Among IR QSOs, PG QSOs and Narrow-Line Seyfert 1 Galaxies
We study the properties of infrared-selected QSOs (IR QSOs),
optically-selected QSOs (PG QSOs) and Narrow Line Seyfert 1 galaxies (NLS1s).
We compare their properties from the infrared to the optical and examine
various correlations among the black hole mass, accretion rate, star formation
rate and optical and infrared luminosities. We find that the infrared excess in
IR QSOs is mostly in the far infrared, and their infrared spectral indices
suggest that the excess emission is from low temperature dust heated by
starbursts rather than AGNs. The infrared excess is therefore a useful
criterion to separate the relative contributions of starbursts and AGNs. We
further find a tight correlation between the star formation rate and the
accretion rate of central AGNs for IR QSOs. The ratio of the star formation
rate and the accretion rate is about several hundred for IR QSOs, but decreases
with the central black hole mass. This shows that the tight correlation between
the stellar mass and the central black hole mass is preserved in massive
starbursts during violent mergers. We suggest that the higher Eddington ratios
of NLS1s and IR QSOs imply that they are in the early stage of evolution toward
classical Seyfert 1's and QSOs, respectively.Comment: 32 pages, 6 figures, accepted by Ap
Luminous Infrared Galaxies in the Local Universe
We study the morphology and star formation properties of 159 local luminous
infrared galaxy (LIRG) using multi-color images from Data Release 2 (DR2) of
the Sloan Digital Sky Survey (SDSS). The LIRGs are selected from a
cross-correlation analysis between the IRAS survey and SDSS. They are all
brighter than 15.9 mag in the r-band and below redshift ~ 0.1, and so can be
reliably classified morphologically. We find that the fractions of
interacting/merging and spiral galaxies are ~ 48% and ~ 40% respectively. Our
results complement and confirm the decline (increase) in the fraction of spiral
(interacting/merging) galaxies from z ~1 to z ~ 0.1, as found by Melbourne, Koo
& Le Floc'h (2005). About 75% of spiral galaxies in the local LIRGs are barred,
indicating that bars may play an important role in triggering star formation
rates > 20 M_{sun}/yr in the local universe. Compared with high redshift LIRGs,
local LIRGs have lower specific star formation rates, smaller cold gas
fractions and a narrower range of stellar masses. Local LIRGs appear to be
either merging galaxies forming intermediate mass ellipticals or spiral
galaxies undergoing high star formation activities regulated by bars.Comment: 22 pages, 5 figures, accepted for publication in ApJ, title changed,
typos corrected,major revisions following referee's comments,updated
reference
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