29,773 research outputs found
Track estimation with binary derivative observations
We focus in this paper in the estimation of a target trajectory defined by
whether a time constant parameter in a simple stochastic process or a random
walk with binary observations. The binary observation comes from binary
derivative sensors, that is, the target is getting closer or moving away. Such
a binary observation has a time property that will be used to ensure the
quality of a max-likelihood estimation, through single index model or
classification for the constant velocity movement. In the second part of this
paper we present a new algorithm for target tracking within a binary sensor
network when the target trajectory is assumed to be modelled by a random walk.
For a given target, this algorithm provides an estimation of its velocity and
its position. The greatest improvements are made through a position correction
and velocity analysis
Non-conservative Evolution of Cataclysmic Variables
We suggest a new mechanism to account for the loss of angular momentum in
binaries with non-conservative mass exchange. It is shown that in some cases
the loss of matter can result in increase of the orbital angular momentum of a
binary. If included into consideration in evolutionary calculations, this
mechanism appreciably extends the range of mass ratios of components for which
mass exchange in binaries is stable. It becomes possible to explain the
existence of some observed cataclysmic binaries with high donor/accretor mass
ratio, which was prohibited in conservative evolution models.Comment: LaTeX, 32 pages, to be published in Astron. Z
Binary system delays and timing noise in searches for gravitational waves from known pulsars
The majority of fast millisecond pulsars are in binary systems, so that any
periodic signal they emit is modulated by both Doppler and relativistic
effects. Here we show how well-established binary models can be used to account
for these effects in searches for gravitational waves from known pulsars within
binary systems. A seperate issue affecting certain pulsar signals is that of
timing noise and we show how this, with particular reference to the Crab
pulsar, can be compensated for by using regularly updated timing ephemerides.Comment: 10 pages, 11 figures, accepted by Phys. Rev.
Orbital Variability in the Eclipsing Pulsar Binary PSR B1957+20
We have conducted timing observations of the eclipsing millisecond binary
pulsar PSR~B1957+20, extending the span of data on this pulsar to more than
five years. During this time the orbital period of the system has varied by
roughly , changing quadratically with time
and displaying an orbital period second derivative s. The previous measurement of a large negative
orbital period derivative reflected only the short-term behavior of the system
during the early observations; the orbital period derivative is now positive
and increasing rapidly. If, as we suspect, the PSR~B1957+20 system is
undergoing quasi-cyclic orbital period variations similar to those found in
other close binaries such as Algol and RS CVn, then the
companion to PSR~B1957+20 is most likely non-degenerate, convective, and
magnetically active.Comment: 9 pages, 3 figures, LaTeX, submitted ApJL 13 Dec. 1993, arz-00
The Angular Resolution of Space-Based Gravitational Wave Detectors
Proposed space-based gravitational wave antennas involve satellites arrayed
either in an equilateral triangle around the earth in the ecliptic plane (the
ecliptic-plane option) or in an equilateral triangle orbiting the sun in such a
way that the plane of the triangle is tilted at 60 degrees relative to the
ecliptic (the precessing-plane option). In this paper, we explore the angular
resolution of these two classes of detectors for two kinds of sources
(essentially monochromatic compact binaries and coalescing massive-black-hole
binaries) using time-domain expressions for the gravitational waveform that are
accurate to 4/2 PN order. Our results display an interesting effect not
previously reported in the literature, and underline the importance of
including the higher-order PN terms in the waveform when predicting the angular
resolution of ecliptic-plane detector arrays.Comment: 13 pages, 6 figures, submitted to Phys Rev D. The current version
corrects an error in our original paper and adds some clarifying language.
The error also required correction of the graphs now shown in Figures 3
through
Millisecond and Binary Pulsars as Nature's Frequency Standards. II. Effects of Low-Frequency Timing Noise on Residuals and Measured Parameters
Pulsars are the most stable natural frequency standards. They can be applied
to a number of principal problems of modern astronomy and time-keeping
metrology. The full exploration of pulsar properties requires obtaining
unbiased estimates of the spin and orbital parameters. These estimates depend
essentially on the random noise component being revealed in the residuals of
time of arrivals (TOA). In the present paper, the influence of low-frequency
("red") timing noise with spectral indices from 1 to 6 on TOA residuals,
variances, and covariances of estimates of measured parameters of single and
binary pulsars are studied. In order to determine their functional dependence
on time, an analytic technique of processing of observational data in time
domain is developed which takes into account both stationary and non-stationary
components of noise. Our analysis includes a simplified timing model of a
binary pulsar in a circular orbit and procedure of estimation of pulsar
parameters and residuals under the influence of red noise. We reconfirm that
uncorrelated white noise of errors of measurements of TOA brings on gradually
decreasing residuals, variances and covariances of all parameters. On the other
hand, we show that any red noise causes the residuals, variances, and
covariances of certain parameters to increase with time. Hence, the low
frequency noise corrupts our observations and reduces experimental
possibilities for better tests of General Relativity Theory. We also treat in
detail the influence of a polynomial drift of noise on the residuals and
fitting parameters. Results of the analitic analysis are used for discussion of
a statistic describing stabilities of kinematic and dynamic pulsar time scales.Comment: 40 pages, 1 postscript figure, 1 picture, uses mn.sty, accepted to
Mon. Not. Roy. Astron. So
Decentralized Estimation over Orthogonal Multiple-access Fading Channels in Wireless Sensor Networks - Optimal and Suboptimal Estimators
Optimal and suboptimal decentralized estimators in wireless sensor networks
(WSNs) over orthogonal multiple-access fading channels are studied in this
paper. Considering multiple-bit quantization before digital transmission, we
develop maximum likelihood estimators (MLEs) with both known and unknown
channel state information (CSI). When training symbols are available, we derive
a MLE that is a special case of the MLE with unknown CSI. It implicitly uses
the training symbols to estimate the channel coefficients and exploits the
estimated CSI in an optimal way. To reduce the computational complexity, we
propose suboptimal estimators. These estimators exploit both signal and data
level redundant information to improve the estimation performance. The proposed
MLEs reduce to traditional fusion based or diversity based estimators when
communications or observations are perfect. By introducing a general message
function, the proposed estimators can be applied when various analog or digital
transmission schemes are used. The simulations show that the estimators using
digital communications with multiple-bit quantization outperform the estimator
using analog-and-forwarding transmission in fading channels. When considering
the total bandwidth and energy constraints, the MLE using multiple-bit
quantization is superior to that using binary quantization at medium and high
observation signal-to-noise ratio levels
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