With mixers operating at increasingly higher RF and IF frequencies, instrument stability
becomes increasingly more important. In order to understand, and quantify,
the different noise mechanism's involved, we employ a technique first
described by D.W. Allan (1) and ellaborated upon by R. Schieder(2).
1.D. W. Allan, "Statistics of Atomic Frequency Standards",
2. R. Schieder, "Characterization and Measurment of System Stability",
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Example of a Quasi-optical Mixer
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HEB Stability vs Bias
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Measurement Setup
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R. Schieder and C. Kramer
J.W. Kooi, G. Chattopadhyay, M. Thielman, T.G. Phillips, and R. Schieder
T. Berg, S. Cherednichenko, V. Drakinskiy, P. Khosropanah, H. Merkel, E. Kollberg, and J. Kooi
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| Receiver Index | CSO | SMA | NRAO | Submm Physics Homepage | ALMA Band 9 Cartridge | Caltech Astronomy | Web Page created and last updated on Dec. 28, 2005, by: Jacob W. Kooi |