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Group for Advanced Receiver Development (GARD)Radio & Space Science DepartmentChalmers
University of Technology |
Radio camera employs 4x4 diagonal horn array followed by 16 fix-tuned SIS
mixers. The camera will operate at 85-115 GHz frequency band as SSB receiver.
Status: Ongoing / Recently the Group is working on
"light" version of the camera (2x2 mixer array while optics and
hardware is for the full version 4x4 mixers). The receiver have been installed
on Onsala 20 m antenna during the November/December 1997 for evaluation.
Cassegrain Focal Number |
f#cass = 4.7 |
Subreflector Edge Taper: |
TE = -12 dB |
Imaging Array Size |
|
Beam Separation |
angle, 54" |
Beam Switch |
Flipping mirrors*, fmax= 5 Hz |
Beam Derotator |
Software de-rotation |
Frequency Range |
85 - 115 GHz |
IF Frequency |
fIF = 3.4- 4.6 GHz |
SSB System Noise Temperature |
Tsys < 150 K** |
** The SSB noise temperature below 150K has been achieved after improving optics and image load in lab (summer 1998).
** Optical layout shows previous design with a chopper wheel for beam switch. Recent design employs flipping mirrors and is more compact. We still need to work out vibration caused by the flipping mirror drivers.
Some terms from the picture above:
Kinoform is a like hologram plate (binary phase change) that
converts a plane wave from mm-wave source into 16 partial beams (see for
reference G. Delgado's Ph.D. thesis).
Attenuator is of quasioptical type, employs a semiconductor material
sensitive to IR radiation. IR diodes used to modulate the electron density in
the material that influences on "transparency" of the material for
mm-radiation (see for reference G. Delgado's Ph.D. thesis).
RPI is Rotation Polarization Interferometer (see N. Erikson paper in
Int. J. Infrared and MM Waves).
Two pictures shows the design of the RPI and its placement into the dewar;
The mixer assembly with cryogenics;
The whole dewar however without LO injection.
The cooler is 3 stage JT machine created by Bert Hansson. The machine cooling capacity isabout 2.25 W at ~4 K. Here you can see a picture of the machine.
All pictures have been taken by Bert Hansson ©
This page was last modified November 6, 1998, by Victor Belitsky. belitsky(a)oso.chalmers.se