Development of Coherent Detector Technologies for Sub-Millimetre Wave Astronomy Observations
The thesis describes the development of receiver technologies for sub-millimetre astronomy instruments, focusing on high performance coherent cryogenic detectors operating close to the superconductor gap frequency. The mixer chip which comprises the SIS devices, fed by a unilateral finline and matching planar circuits was fabricated on 15 micron silicon substrate using the recently developed Silicon-On-Insulator (SOI) technology. This offered broadband IF and RF performance, with fully integrated on-chip planar circuits resulting in an easily reproducible mixer chip and a simple mixer block. An important consequence of this design is that it can be extended to the supra-THz region and making the fabrication of multi-pixel heterodyne arrays feasible. The extension of the operation of major telescopes such as ALMA, APEX and the GLT from single pixel to large format arrays is the subject of extensive research at present time since it will allow fast mapping combined with high resolution of the submillimetre sky. The technology described in this thesis makes a major contribution to this effort.
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2 Multiple FlareAngle SmoothWalled Horn
3 SIS Mixer Theory
4 Design of Unilateral Finline SIS Mixer
5 SingleEnded Mixer Tests
6 SingleChip Integrated Balanced SIS Mixer
7 Design of 700 GHz Single Sideband SIS Mixers
8 The Characteristics of an SIS Junction Near Its Superconducting Gap
10 CO3rightarrow2 Observations of NGC 2976 and NGC 3351
11 Concluding Remarks
Appendix A Ancillary Data of Individual Tested Device
Appendix B Ancillary Data of Individual Tested BalancedDevice
Appendix C List of All Beam Patterns Measured Up to Date
Appendix D 230GHz Scalable Design
9 Generation of Local Oscillator Signal via Photomixing
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