Optical SETI Map Conferences Map Illustrations Map Photo Galleries Map Observations Map Constructing Map
Search Engines Contents Complete Site Map Tech. Support Map Order Equip. Map OSETI Network

Search WWW Search www.coseti.org Search www.oseti.net Search www.photonstar.org Search www.opticalseti.org

colorbar.gif (4491 bytes)


Carrier-To-Noise Ratio In Coherent Systems



Graph 9006-017 illustrates how it is possible to achieve the ultimate CNR in heterodyne detection optical receivers.  A CNR = 34 dB is obtained for the -118 dBm (Pr = 1.60 x 10-15 W) signal which is received from the 1 kW alien transmitter situated 10 light years away.  This is 3 dB more CNR than obtainable with the ultimate direct detection optical receiver.  It is also 3 dB smaller than obtainable with an ideal optical homodyne receiver.  For this heterodyne receiver with a load RL = 10 kohm , the receiver is heavily shot-noise (quantum-noise) limited when the local oscillator power Po is increased to 0 dBm (1mW).  For Po = -10 dBm (100 W), the CNR is just on the threshold of being shot-noise limited, and the CNR is 3 dB less than the ultimate.  Because we are dealing with a coherent optical receiver, the slope of the CNR characteristics are 10 dB/decade as long as Po >> Pr and Pb.  This is independent of whether the receiver is or is not shot- noise limited.

Because the load impedance RL is relatively low and photodetector RC time-constants (RL.CL) are small, it should not be necessary to use transimpedance amplifiers, such as illustrated in 9008-028, unless SETI signals are discovered that are wideband.  It would be prudent however, to use such amplifiers just in case the wider bandwidth is required, if only due to the practical aspects of tuning the local oscillator, and doing a wide radio frequency spectrum analysis of the beat signal to speed up the "search".

Home Glossary
SPIE's OSETI I Conference SPIE's OSETI II Conference
SPIE's OSETI III Conference
The Columbus Optical SETI Observatory
Copyright , 1990-2006 Personal Web Site:
Last modified:  10/28/06
Contact Info