Research on the Autonomous Navigation of Satellite Constellation Using Pulsars;
基于脉冲星的卫星星座自主导航技术研究
Research on the Spacecraft Autonomous Navigation Using Pulsars;
基于脉冲星的空间飞行器自主导航技术研究
Advance in X-Ray Pulsar Navigation Technology;
X射线脉冲星导航技术研究进展
Magnetars as X-ray Pulsars;
作为X射线脉冲星的磁星(英文)
A Modified Magnetic-Dipole Emission Model for Pulsars;
脉冲星磁偶极辐射模型的修正
Motivated by the particle acceleration problem in pulsars, it is numerically investigated for electrostatic instability of electron-positron pairs injected in an external electric field.
出于脉冲星中粒子加速问题,讨论外电场中注入的正负电子对静电不稳定性。
The comparisons between the frequency stabilities for atomic time and pulsar time are presented.
给出了毫秒脉冲星长期计时观测最新结果和脉冲星时与原子时频率稳定度的比较。
The pulsar time defined by single pulsar is influenced by several noise resources, to weaken these influences, ensemble analysis method can be used to obtain the e.
由单颗脉冲星定义的脉冲星时受多种噪声源的影响,为了削弱这些噪声源的影响,对多个单脉冲星时采取合适的综合算法得到综合脉冲星时,从而提高综合脉冲星时的长期稳定度。
Pulsar: A dense, rapidly rotating star that emits pulses of light.
脉冲星：高密度、快速旋转、发射脉冲光的星体。
Structure of a pulsar- a rotating magnetic neutron star.
脉冲星的结构。一颗旋转磁中子星。
Millisecond Pulsars Mean Pulse Dispelrsition-Limiting and De-Noising Methods Research;
毫秒脉冲星平均脉冲消色散和去噪方法研究
But certain stars, called pulsars, give off regular pulses of radio waves.
但有些恒星，所谓的脉冲星，会有规律地发出射电波脉冲。
With the implementing of the millisecond pulsar timing array( PTA), the application of pulsar time will become possible in the near future.
随着脉冲星计时阵的实施,脉冲星时的应用已为期不远。
The most famous example is the Hulse-Taylor pulsar.
最其名的例子就是哈尔斯-泰勒脉冲星。
An Inverse Compton Scattering Model for Radio Pulsars 1)
射电脉冲星的逆康普顿散射模型(英文)
Accurating and Delay Correction Analysis of Pulsar Timing Model
脉冲星时间模型精化及延迟修正分析
Analysis of Pulsar Time-of-Arrival Measurement Error and Dilution of Precision
脉冲星TOA测量误差及几何精度分析
Analysis in X-ray Pulsar Navigation Phase Ambiguity Resolution
X射线脉冲星导航中相位模糊度解算
Use of X-ray pulsar-based navigation method on interplanetary trajectory
X射线脉冲星导航在行星际轨道上的应用
Algorithm of Onboard Clock Error Correction Based on Observation of Pulsar
基于脉冲星的星载钟时间修正算法研究
The limited sensitivity of present pulsar surveys and the greater frequency drift make the more distant pulsars difficult to observe.
目前脉冲星普查的有限探测灵敏度和大的频率漂移，使我们难以观测到更遥远的脉冲星。
It is possible that an average pulsar time scale PTens may be deduced through along-term stability algorithm using precision timing data from more millisecond pulsars.
采用合适的长期稳定度算法,由多颗毫秒脉冲星计时观测可以建立综合脉冲星时间尺度。
Interest was renewed in the astronomical community with the discovery of pulsars.
天文学团体随着脉冲星的发现重新激发了兴趣。
The purple dots on the celestial sphere mark the locations of pulsars* that have already been detected.
屏保中紫色的点表示已探测到的脉冲星*位置。
The Research of the Navigation of Spacecraft Based on the X-Ray Pulsars;
基于X射线脉冲星的航天器自主导航方法研究
The Possible Contribution of Mature γ-ray Pulsars to Cosmic-ray Positrons;
成熟γ-射线脉冲星对宇宙线正电子的贡献