NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, WV MEMORANDUM November 14, 1997 TO: R. Fisher, R. Lacasse, R. Norrod, M. McKinnon, C. Niday, T. Weadon FROM: R. Lacasse SUBJ: Minutes of Interference Protection Group 11/11/97 Meeting In attendance: Fisher, Lacasse, McKinnon, and Niday, Weadon Minutes Minutes from the last meeting were approved. RFI Call-outs A signal at 4880 MHz (420 MHz in the IF) was observed by Lacasse at the 140'. Grammer did a variety of things to the receiver (shutting down amplifiers, etc.) to show that the interference was not internally generated. Lacasse and Grammer placed several aluminum plates on top of the large feed effectively covering approximately 90% of the aperture. This did not make the spike disappear, but was the only test which affected the amplitude of the signal. Information was forwarded to Sizemore who is pursuing it. Episodes such as this highlight the need for a good monitoring station, and for a database of observed interference. Budget Items Several people reported on the costs of items in the budget. The first of these was an A/D system on a PC to facilitate continuum measurements. Specification for this item were discussed. A sample rate of 1 to 10KHz was deemed adequate, as was a resolution of 12 bits, although 16 bit resolution would be preferable. The intial estimates for 16-bit systems that will sample at several hundred KHz (PC, A/D board, and software) is $6K to $7K. Weadon agreed to look into slower sampling devices that have only the basic sampling functions to see whether something is available at lower cost. The monitoring station cost was estimated at $7400. A power meter and head was estimated at $4K, and a low frequency antenna (30MHz to 1GHz) was estimated at $3500. Priorities of the items were discussed. It was decided to purchase the A/D system first, and spend any left over money on the monitoring station. GB School LAN Status Although the current state of the LAN installation at the school was unknown, the discussion quickly digressed into the best ways of dealing with the interference potential of the school. The school has a technical committee, of which John Ford is a member; this seems the most appropriate conduit for technical information flow between NRAO and the school. It was decided to invite John to the IPG meetings every couple of months to keep him abreast of the IPG's activities. The possibility of providing presentations or tours to school personnel to give them an appreciation for the interference problem was also discussed. Workstation/PC Shielded Enclosure The shop is working on it. It should be ready in about 2 weeks. Power filters for the box have been received. Since the decision to locate the GBT control building in the Jansky lab addition has been made, the need for shielding workstations is not as critical. Preliminary shielding effectiveness measurements on the second floor of the new addition show that the rooms have about 75db of shielding. Equipment Testing Further tests of the 1500MHz oscillator for the laser ranging system have been completed. Some leakage still exists. A separate memo, documenting the tests, has been written. Next Meeting TBD