DocumentCode
1645650
Title
Realization of multiplying type interferometer with 2-elements 0.3K bolometer detectores
Author
Luo, Yuan ; Hattori, Makoto ; Ohta, Izumi S. ; Chinone, Y. ; Takahashi, Junichi ; Hamaji, Yoshihiro ; Matsuo, Hiroshi ; Kuno, Nario
Author_Institution
Astron. Institude, Tohoku Univ., Sendai
fYear
2008
Firstpage
213
Lastpage
215
Abstract
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.
Keywords
Fourier transforms; bolometers; interferometers; 2-elements 0.3K bolometer detectors; interferometer; millimeter wave bands; multiFourier transform interferometer; multiplying type bolometric astronomical interferometer; mutual coherence function; submillimeter wave bands; wiregrid polarizer; Bolometers; Coherence; Detectors; Fluctuations; Fourier transforms; Moon; Observatories; Polarization; Submillimeter wave devices; Submillimeter wave propagation;
fLanguage
English
Publisher
ieee
Conference_Titel
Millimeter Waves, 2008. GSMM 2008. Global Symposium on
Conference_Location
Nanjing
Print_ISBN
978-1-4244-1885-5
Electronic_ISBN
978-1-4244-1886-2
Type
conf
DOI
10.1109/GSMM.2008.4534601
Filename
4534601
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