Gain stabilization of a submillimeter SIS heterodyne receiver
Battat, J.
Blundell, R.
Hunter, T.R.
Kimberk, R.
Leiker, P.S.
Tong, C.-Y.E.
Harvard-Smithsonian Center for Astrophys., Cambridge, MA, USA;
This paper appears in: Microwave Theory and Techniques, IEEE Transactions on
Publication Date: Jan. 2005
Volume: 53,
Issue: 1
On page(s): 389- 395
ISSN: 0018-9480
INSPEC Accession Number: 8258487
Digital Object Identifier: 10.1109/TMTT.2004.839942
Current Version Published: 2005-01-17
Abstract
We have designed a system to stabilize the gain of a submillimeter heterodyne receiver against thermal fluctuations of the mixing element. In the most sensitive heterodyne receivers, the mixer is usually cooled to 4 K using a closed-cycle cryocooler, which can introduce ∼1%; fluctuations in the physical temperature of the receiver components. We compensate for the resulting mixer conversion gain fluctuations by monitoring the physical temperature of the mixer and adjusting the gain of the IF amplifier that immediately follows the mixer. This IF power stabilization scheme, developed for use at the Submillimeter Array, a submillimeter interferometer telescope located on Mauna Kea, HI, routinely achieves a receiver gain stability of one part in 6000 (rms to mean). This is an order of magnitude improvement over the typical uncorrected stability of one part in a few hundred. Our gain stabilization scheme is a useful addition to superconductor-insulator-superconductor heterodyne receivers that are cooled using closed-cycle cryocoolers in which the 4-K temperature fluctuations tend to be the leading cause of IF power fluctuations.
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