Such an ensemble average can reduce the level of the instabilities originating from individual pulsar and other sources of noise.

 
  • 采用合適的長(cháng)期穩定度算法,由多顆毫秒脈沖星計時(shí)觀(guān)測可以建立綜合脈沖星時(shí)間尺度。
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