Javascript must be enabled to continue!
A simulation technique of X-ray pulsar signals with high timing stability
View through CrossRef
A simulation experiment system is required presently, for the space flight experiment of X-ray pulsar based navigation is very costly. To solve the crucial issues of the timing stability and the profile precision in existing simulation techniques of pulsar signal, a new simulation technique which utilizes visible light is proposed. The simulation experiment system is set up based on the proposed technique. And some experiments are carried out to test the proposed technique. The results demonstrate that the proposed technique can be used to simulate any of known pulsars. The timing stability of simulated X-ray pulsars is raised from 10-4 to 10-9. And the accuracy of pulsar profile simulation is noticeably improved. Within the X-ray band 1-10 keV, when the observation time reaches 1200 s, and the area of the X-ray detector is 1 m2, the Pearson correlation coefficient of pulsar's observation profile with the standard template profile arrives at 0.993. And the simulation experiment system can be realized with high flexibility and low cost. On the basis of the simulation experiment system, the signal characteristic of X-ray pulsar can be investigated. On the other hand, the performances of X-ray pulsar signal processing algorithms and navigation algorithms can be surveyed in detail.
Acta Physica Sinica, Chinese Physical Society and Institute of Physics, Chinese Academy of Sciences
Title: A simulation technique of X-ray pulsar signals with high timing stability
Description:
A simulation experiment system is required presently, for the space flight experiment of X-ray pulsar based navigation is very costly.
To solve the crucial issues of the timing stability and the profile precision in existing simulation techniques of pulsar signal, a new simulation technique which utilizes visible light is proposed.
The simulation experiment system is set up based on the proposed technique.
And some experiments are carried out to test the proposed technique.
The results demonstrate that the proposed technique can be used to simulate any of known pulsars.
The timing stability of simulated X-ray pulsars is raised from 10-4 to 10-9.
And the accuracy of pulsar profile simulation is noticeably improved.
Within the X-ray band 1-10 keV, when the observation time reaches 1200 s, and the area of the X-ray detector is 1 m2, the Pearson correlation coefficient of pulsar's observation profile with the standard template profile arrives at 0.
993.
And the simulation experiment system can be realized with high flexibility and low cost.
On the basis of the simulation experiment system, the signal characteristic of X-ray pulsar can be investigated.
On the other hand, the performances of X-ray pulsar signal processing algorithms and navigation algorithms can be surveyed in detail.
Related Results
A new simulation method of X-ray pulsar signals
A new simulation method of X-ray pulsar signals
Since X-ray pulsar signals cannot be directly detected on the ground, and the space flight detection is both time-consuming and costly, simulation of X-ray pulsar signals with true...
Time delay estimation method of X-ray pulsar observed profile based on the optimal frequency band
Time delay estimation method of X-ray pulsar observed profile based on the optimal frequency band
In order to improve the time delay estimation accuracy of the observed profile in the X-ray pulsar based navigation, the spectral characteristics of the observed profile of X-ray p...
GeV emission of gamma-ray binary with pulsar scenario
GeV emission of gamma-ray binary with pulsar scenario
ABSTRACT
We study GeV emission from gamma-ray binaries by assuming that the compact object is a young pulsar. We assume that the relativistic unshocked pulsar wind w...
Kinematics, structure and abundances of supernova remnant 0540-69.3
Kinematics, structure and abundances of supernova remnant 0540-69.3
Aims. Our goal is to investigate the structure, elemental abundances, physical conditions, and the immediate surroundings of supernova remnant 0540-69.3 in the Large Magellanic Clo...
Pulsar Astrometry
Pulsar Astrometry
High precision measurements of the celestial coordinates of pulsars are desirable for a number of reasons. If carried out at several epochs, the measurements can yield angular prop...
A new method for the pulsar signals simulation
A new method for the pulsar signals simulation
Since X-ray pulsar signals cannot be detected on the ground, the pulsar signals need be simulated using the ground experiments. In this paper,two new simulation methods to obtain t...
Spectral analysis of the polarisation of drifting subpulses
Spectral analysis of the polarisation of drifting subpulses
Pulsars are among the most extreme objects in the Universe. Each one is born during a supernova – a dramatic explosion that happens when a bright star is many times bigger than our...
PULSAR SIGNAL DENOISING METHOD BASED ON LAPLACE DISTRIBUTION IN NO-SUBSAMPLING WAVELET PACKET DOMAIN
PULSAR SIGNAL DENOISING METHOD BASED ON LAPLACE DISTRIBUTION IN NO-SUBSAMPLING WAVELET PACKET DOMAIN
ABSTRACT
In order to improve the denoising effect of the pulsar signal, a new denoising method is proposed in the no-subsampling wavelet packet domain based on the l...

