We are developing a bolometric astronomical interferometer in mm and submm wave bands by applying Martin-Puplett type Fourier transform spectrometer to aperture synthesis technique. Since the spectroscopically resolved intensity distribution of four Stokes parameters are measurable by this instrument, we refer this to multi-components Fourier transform interferometer abbreviated as MuFT. Fundamentals of the MuFT with results of laboratory experiments and current status of astronomical observations with MuFT are summarized.
Development of bolometric astronomical interferometer in mm and submm bands
2005-01-01
1705835 byte
Conference paper
Electronic Resource
English
WC5-23 Development of Bolometric Astronomical Interferometer In Mm And Submm Bands
British Library Conference Proceedings | 2005
|TC5-38 The first astronomical mm and submm observations with Multi-fourier transform interferometer
British Library Conference Proceedings | 2005
|Infrared/submm astronomy from space
Elsevier | 2005
|Infrared/submm astronomy from space
British Library Conference Proceedings | 2005
|