19,944 research outputs found
High performance millimeter-wave microstrip circulators and isolators
Millimeter wave systems, phased array antennas, and high performance components all require wideband circulators (and isolators) to perform diplexing and switching, to improve isolation and Voltage Standing Wave Ratio (VSWR), and to construct IMPATT diode reflection amplifiers. Presently, most of the millimeter-wave circulators and isolators are available in the configurations of waveguide or stripline, both of which suffer from the shortcomings of bulky size/weight, narrow bandwidth, and poor compatibility with monolithic millimeter-wave integrated circuits (MMIC). MMW microstrip circulators/isolators can eliminate or improve these shortcomings. Stub-tuned microstrip circulator configuration were developed utilizing the electromagnetic fields perturbation technique, the adhesion problems of microstrip metallization on new ferrite substrate were overcome, the fabrication, assembly, packaging techniques were improved, and then successfully designed, fabricated a Ka band circulator which has isolation and return loss of greater than 16dB, insertion loss less than 0.7dB. To assess the steady and reliable performance of the circulator, a temperature cycling test was done over the range of -20 to +50 C for 3 continuous cycles and found no significant impact or variation of circulator performance
Asymptotic distributions of the signal-to-interference ratios of LMMSE detection in multiuser communications
Let ,
where are independent and identically distributed
random variables with and . Let
, and
\beta_k=p_k{\mathbf{s}}_k^T({\mathb
f{S}}_k{\mathbf{P}}_k{\mathbf{S}}_k^T+\sigma^2{\mathbf{I}})^{-1}{\math
bf{s}}_k, where and the is referred to as the
signal-to-interference ratio (SIR) of user with linear minimum mean-square
error (LMMSE) detection in wireless communications. The joint distribution of
the SIRs for a finite number of users and the empirical distribution of all
users' SIRs are both investigated in this paper when and tend to
infinity with the limit of their ratio being positive constant. Moreover, the
sum of the SIRs of all users, after subtracting a proper value, is shown to
have a Gaussian limit.Comment: Published at http://dx.doi.org/10.1214/105051606000000718 in the
Annals of Applied Probability (http://www.imstat.org/aap/) by the Institute
of Mathematical Statistics (http://www.imstat.org
Learning to Deblur Images with Exemplars
Human faces are one interesting object class with numerous applications.
While significant progress has been made in the generic deblurring problem,
existing methods are less effective for blurry face images. The success of the
state-of-the-art image deblurring algorithms stems mainly from implicit or
explicit restoration of salient edges for kernel estimation. However, existing
methods are less effective as only few edges can be restored from blurry face
images for kernel estimation. In this paper, we address the problem of
deblurring face images by exploiting facial structures. We propose a deblurring
algorithm based on an exemplar dataset without using coarse-to-fine strategies
or heuristic edge selections. In addition, we develop a convolutional neural
network to restore sharp edges from blurry images for deblurring. Extensive
experiments against the state-of-the-art methods demonstrate the effectiveness
of the proposed algorithms for deblurring face images. In addition, we show the
proposed algorithms can be applied to image deblurring for other object
classes.Comment: Accepted by IEEE Transactions on Pattern Analysis and Machine
Intelligence 201
Ks, Lambda and Xi production at intermediate to high pT from Au+Au collisions at \sqrt{s_{NN}} = 39, 11.5 and 7.7 GeV
We report on the pT dependence of nuclear modification factors () for
Ks, Lambda, Xi and the Anti-Lambda/Ks ratios at mid-rapidity from Au+Au
collisions at \sqrt{s_{NN}} = 39, 11.5 and 7.7 GeV. At \sqrt{s_{NN}} = 39 GeV,
the data shows a baryon/meson separation at intermediate pT and a
suppression for Ks for pT up to 4.5 GeV/; the Anti-Lambda/Ks shows baryon
enhancement in the most central collisions. However, at \sqrt{s_{NN}} = 11.5
and 7.7 GeV, shows much less baryon/meson separation and
Anti-Lambda/Ks shows almost no baryon enhancement. These observations indicate
that the matter created in Au+Au collisions at \sqrt{s_{NN}} = 11.5 or 7.7 GeV
might be distinct from that created at \sqrt{s_{NN}} = 39 GeV.Comment: 4 pages, 2 figures, to appear in the proceedings of 7th International
Workshop on Critical Point and Onset of Deconfinement (CPOD2011), Wuhan,
China, Nov. 7-11, 201
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