2元0.3K辐射热计探测器倍增型干涉仪的实现

Yuan Luo, M. Hattori, I. Ohta, Y. Chinone, J. Takahashi, Y. Hamaji, H. Matsuo, N. Kuno
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引用次数: 2

摘要

为了在毫米波和亚毫米波波段实现乘数型天文辐射热干涉仪,研制了一套优化的多傅立叶变换干涉仪(MuFT)双元0.3K高灵敏度辐射热计探测器系统。在探测器系统中设置了一个线栅偏振器。然后将引导到辐射热计探测器系统的信号分为两部分。两个测热计元件中的一个接收反射信号,而另一个接收发射信号。由于两个信号中互相干函数的相位发生了移位,反射信号和发射信号的差再现了完整的互相干函数,可以很容易地消除基线波动。该方法于2007年在日本野山射电天文台首次成功观测月球。
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Realization of multiplying type interferometer with 2-elements 0.3K bolometer detectores
We have developed two-elements 0.3K high sensitive bolometer detectors system optimized to Multi- Fourier Transform interferometer (MuFT) to realize the multiplying type bolometric astronomical interferometer in millimeter and submillimeter wave bands. A wiregrid polarizer is set in the detector system. The signal led to the bolometer detectors system is then divided into two parts. One of the two bolometer elements receives the reflected signal while the other receives the transmitted signal. Since phases of mutual coherence functions in two signals are shifted 71 ,the difference of reflected and transmitted signals reproduces full mutual coherence function and can easily remove the baseline fluctuations. This method is for the first time succeeded in moon observation at Nobeyama Radio Observatory, Japan, 2007.
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