pulsar

• Pulsar time scale
  脉冲星时标
• This is not a search for the known pulsars whose locations you see on the screensaver
  这并不是寻找你在屏幕保护上所能看得到位置的已知的脉冲星。
• They have discovered now , previously unimagined objects - pulsars , quasars , and black holes
  他们发现了以往想象不到的新客体? ?脉冲星、类星体和黑洞。
• 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。
• Pulsar is metrologic s triggerless , entry - level hand - held laser bar code scanner
  是metrologic公司生产的一种无扳机触发入门级的手持式激光条形码扫描仪。
• In this paper , a pulsar de - dispersion algorithm based on the short time fourier transform ( stft ) is presented
  摘要叙述了一种基于短时傅立叶变换的脉冲星消色散算法。
• If the core magnetic field started with sufficient strength , this compression could explain pulsar magnetism
  要是一开始的核心磁场够强，星体塌缩的确可以解释波霎的磁性。
• First of all the reason of the pulsar dispersion and several popular de - dispersion algrithms are introduced
  首先介绍了脉冲星的色散形成原因以及几种当今流行的消色散算法。
• Might the modulation of pulsars or the energy source of quasars , for example , have a technological origin
  比如，脉冲星波段的调制与类星体的能量来源应该有一个科技的源泉？
• From this , most young radio pulsars are inferred to have magnetic fields between 1012 and 1013 gauss
  从这个论点来推断，大部份年轻的无线电波霎应具有介于1012 ~ 1013高斯的磁场。