会议专题

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 hands. 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 boiometer elements receives the reflected signal while the other receives the transmitted signal. Since phases of mutual coherence functions in two signals are shifted π ,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.

Yuan Luo Makoto Hattori Izumi S.Ohta Yuji Chinone Junichi Takahashi Yoshihiro Hamaji Hiroshi Matsuo Nario Kuno

Astronomical Institude,Tohoku University,6-3 Aoba Aramaki,Aoba-ku,Sendai,Miyagi,980-8578,Japan;purpl Astronomical Institude,Tohoku University,6-3 Aoba Aramaki,Aoba-ku,Sendai,Miyagi,980-8578,Japan PROGRESS TECHNOLOGIES,Inc.,6-5-1 Nishi-Shinjyuku,Shinjyuku-ku,Tokyo,163-1304,Japan Toshiba I.S.Corp.,1-1-43 Shibaura,Minato-ku,Tokyo,105-0023,Japan Advanced Technology Center,National Astronomical Observatory of Japan,1-21-2,Ohsawa,Mitaka,Tokyo,181 Nobeyama Radio Observatory,National Astronomical Observatory of Japan,462-2,Nobeyama Minamimaki,Mina

国际会议

2008 Global Symposium on Millimeter Waves(GSMM 2008)(2008全球毫米波学术大会)

南京

英文

213-215

2008-04-21(万方平台首次上网日期,不代表论文的发表时间)