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Program and Abstract Book - SRON

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19 th International Symposium on Space Terahertz Technology<br />

Design of finline SIS mixers with ultra-wide IF b<strong>and</strong>s<br />

P3-3<br />

Paul Grimes, Ghassan Yassin<br />

Astrophysics,<br />

University of Oxford,<br />

Denys Wilkinson Building,<br />

Keble Road,<br />

Oxford, OX1 3RH,UK.<br />

pxg@astro.ox.ac.uk<br />

The instantaneous b<strong>and</strong>width of heterodyne receivers is defined by their IF<br />

b<strong>and</strong>width. This b<strong>and</strong>width limits the sensitivity of SIS based receivers<br />

to continuum emission <strong>and</strong> limits the instantaneous frequency range for<br />

spectroscopic observations. New telescopes <strong>and</strong> backend processing<br />

technologies have led to dem<strong>and</strong>s for ever wider IF b<strong>and</strong>width SIS mixers.<br />

We present the design of 230 GHz finline SIS mixers with a 2-20 GHz IF<br />

b<strong>and</strong>. These mixers are intended for use in a prototype high brightness<br />

sensitivity, low spatial resolution interferometer for Sunyaev-Zeldovich<br />

effect measurements that is currently under construction in Oxford. The<br />

first batches of these devices have recently been fabricated at KOSMA,<br />

University of Cologne, <strong>and</strong> will soon be undergo initial testing in Oxford.<br />

The finline coupled mixer design is particularly suitable for use with<br />

very wide IF b<strong>and</strong>widths, as the finline transition provides a clean<br />

transition from waveguide to microstrip, <strong>and</strong> allows all of the RF tuning<br />

<strong>and</strong> IF circuits to be fabricated in planar circuit. This removes many of<br />

the problems of grounding the mixer <strong>and</strong> allows relatively large IF<br />

contacts <strong>and</strong> circuits to be included on the mixer chip.<br />

The first wide IF b<strong>and</strong> finline SIS mixers use the antipodal finline<br />

transition (as featured on our previous finline mixers <strong>and</strong> detectors) on<br />

quartz substrate to couple the input waveguide to the mixer's microstrip<br />

circuits. RF b<strong>and</strong>pass filters made up of microstrip <strong>and</strong> anodised niobium<br />

capacitors are used to provide isolation between the finline <strong>and</strong> the IF<br />

circuits. Two RF tuning designs have been used. In the first design a<br />

single SIS junction is tuned by a single series stub, terminated by a<br />

stepped microstrip RF choke. In second design, two SIS junctions are used<br />

in a single-ended dual junction tuning circuit, in conjunction with the<br />

same stepped microstrip choke.<br />

The 16 Ohm output impedance of SIS mixer is matched to the 50 Ohm input<br />

impedance of the cryogenic IF amplifier using a 5-stage stepped microstrip<br />

transformer fabricated on Rogers/Duroid 6010LM. The design of this<br />

transformer is also used to tune out the inductance of the bondwires<br />

connecting the mixer chip to the transformer.<br />

We are currently designing a finline SIS mixer utilising SOI substrate<br />

technology <strong>and</strong> beam lead connections to the IF circuit, with greatly<br />

reduced parasitic inductance in the IF connection. We have also developed<br />

a transition direct from unilateral finline to microstrip or coplanar<br />

waveguide transmission line that will allow the design of 50 Ohm<br />

characteristic impedance finline mixers, removing the need for IF matching<br />

transformers, as well as being significantly shorter than the current<br />

antipodal finline transition. Designs for these mixers will be also be<br />

presented.<br />

119

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