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Search for temporal coherence in the sky

机译:寻找天空中的时间连贯性

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A new observation mode, a survey of temporal coherence in large fields, is described. Longitudinal coherence can arise in many astrophysical scenarios and at different wave lengths, from plasma effects, scattering of electrons on periodic electromagnetic volumes, to Einstein rings and even extraterrestrial unintended signaling. There is a plurality of coherence seeking devices, developed for military purposes, which can be easily adopted for this task. Many are based on unbalanced interferometers, with a path difference that exceeds the white light envelope. They were shown to be able to discern very weak coherent sources in a heavily cluttered environment. For searches where the coherent wave length was unknown, a signal to background ratio of 1:10,000 was demonstrated. At a known wave length (e.g. molecular lines) one can even expect 1:1,000,000 detection ratio. Once such sources are found, they can be better monitored by most astronomical interferometers, whose field of view is usually rather narrow.
机译:描述了一种新的观察模式,即大视野中的时间相干性调查。纵向相干性可能出现在许多天文学的场景中,并且在不同的波长下出现,从等离子体效应,电子在周期性电磁体上的散射,到爱因斯坦环,甚至是外星意外信号。有多种用于军事目的的相干搜寻装置,可以很容易地用于此任务。许多是基于不平衡干涉仪,其光程差超过了白光包络线。事实证明,它们在杂乱无章的环境中能够分辨出非常弱的相干源。对于相干波长未知的搜索,信号与背景之比为1:10,000。在已知的波长(例如分子线)下,甚至可以期望1:1,000,000的检测率。一旦找到此类源,就可以用大多数天文干涉仪更好地监视它们,它们的视场通常很窄。

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