Hardware Description

The quasioptical frontend uses a Martin-Puplett interferometer to suppress noise and atmospheric signatures from the unused sideband and a second Martin-Puplett interferometer as diplexer to feed the local oscillator (LO) to the mixer. The LO operating at 276.3 GHz uses a Gunn oscillator at 92.1 GHz and a tripler. For high frequency stability a phaselock system is applied. The downconversion to the intermediate frequency of 2.1 0.5 GHz is performed by a cryogenic single-ended Schottky mixer operating at about 100K. The LN2 dewar also encloses the low noise IF amplifier and two cold loads. The systems noise temperature including quasioptics and the low-noise cryogenic amplifier is 1200 K at center frequency. Baseline ripples caused by standing waves in the quasioptical transmission path are suppressed by a rooftop like mirror reciprocating by about 0.4 mm. The high spectral resolution of 1 MHz over an instantaneous IF bandwith of 1 GHz is achieved by an acusto-optical spectrometer.


Schematic diagram of the 278 GHz radiometer (35 kB)

For comments mail to (last modification: September 19th, 2005)
MIRA-home