Radio frequency interference at Jodrell Bank Observatory within the protected 21 cm band.
Radio frequency interference (RFI) will provide one of the most difficult challenges to systematic Searches for Extraterrestrial Intelligence (SETI) at microwave frequencies.  The SETI-specific equipment is being optimized for the detection of signals generated by a technology rather than those generated by natural processes in the universe.  If this equipment performs as expected, then it will inevitably detect many signals originating from terrestrial technology.  If these terrestrial signals are too numerous and/or strong, the equipment will effectively be blinded to the (presumably) weaker extraterrestrial signals being sought.  It is very difficult to assess how much of a problem RFI will actually represent to future observations, without  employing the equipment and beginning the search.  In 1983 a very high resolution spectrometer was placed at the Nuffield Radio Astronomy Laboratories at Jodrell Bank, England.  This equipment permitted an investigation of the interference environment at Jodrell Bank, at that epoch, and at frequencies within the 21 cm band.  This band was chosen because it has long been "protected" by international agreement; no transmitters should have been operating at those frequencies.  The data collected at Jodrell Bank were expected to serve as a "best case" interference scenario and provide the minimum design requirements for SETI equipment that must function in the real and noisy environment.  This paper describes the data collection and analysis along with some preliminary conclusions concerning the nature of the interference environment at Jodrell Bank.
Tarter
J
J
Astronomy Department, University of California, Berkeley 94720.
D001256:Astronomy / Q000295:instrumentation; D003142:Communication; D003627:Data Interpretation, Statistical; D004739:England; D018559:Exobiology / Q000295:instrumentation*; D008872:Microwaves; D011846:Radio Waves