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中国物理学会期刊

一种脉冲星信号模拟新方法

CSTR: 32037.14.aps.63.219701

A new method for the pulsar signals simulation

CSTR: 32037.14.aps.63.219701
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  • 在脉冲星导航地面实验中,为解决地面无法接收脉冲星辐射的X射线信号的问题,必须在实验系统中模拟脉冲星辐射信号. 本文提出两种全新脉冲星信号模拟方法. 第一种方法基于统计物理模型,该方法克服了常用泊松模型模拟方法中仿真适应性窄、仿真速度慢和时间分辨率低等不足,实现了对任意随机过程的脉冲信号进行快速高时间分辨率的仿真;第二种方法基于优化统计模型,该方法针对非齐次泊松过程信号的特性进行优化,仿真速度比常用泊松模型模拟方法提高至少30 倍,对于低流量脉冲星,甚至提高4个数量级,可实现纳秒级时间分辨率仿真.

     

    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 the time of arrival are put forward. The first method is based on a statistical physics model, which should overcome the shortcomings of narrow adaptation, low speed, and low time resolution in normal simulation method. This method has a high time-resolution and rapid simulation for any random pulse signals. 23 Another one is for the optimization of statistical models that satisfy signals in non-homogeneous Poisson process. The is second method has an improved simulation speed at least 30 times higher than the common Poisson model, even achieves four orders of magnitude greater than that for low flow pulsars, and this method also achieves a nanosecond time resolution simulation.

     

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