We have fabricated and tested both single junctions and series arrays
of YBCO step edge junctions for four photon parametric effects at X ba
nd as a first step in developing a parametric amplifier at 60 GHz. The
series array of 25 junctions at 10.3 Ghz shows a 10 dB increase in re
flected signal power as the pump power is increased, while the single
junction at 12.2 GHz indicates a 2 dB change. The reflected power at t
he characteristic idler frequency of 2omega(p)-omega(s) is evidence of
true Josephson junction parametric interaction. We are currently inve
stigating the use of thallium based films at 60 GHz which offer a broa
der range of operating temperatures than does YBCO. Our design for a p
arametric amplifier at V band is a combination of microstrip based ser
ies arrays of junctions and an antipodal finline transition.