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http://www.SignalONE.com/radioastronomy/telescope/

5.2 Meter Radio Astronomy Project for 1420 MHz

 

Inside Equipment Description

The equipment located inside the radio room consists of three main systems: the RF system, the data acquisition system, and the positioning system. These are included in the diagram below

 

 

Radio frequency (RF) system. After emissions are received by the antenna and amplified at the feed by the low-noise preamplifier they are usually routed through a Telonic TTF-1500-5-3EE tunable bandpass filter (used ~$20). This provides some protection from out-of-band interference sources such as from RADAR sites, etc. Filters similar to this one can often be found at electronics flea markets or from surplus electronics dealers. Additional filtering is available by inserting a 2-stage tunable (1-2 GHz) YIG filter. I bought the YIG filter elements at an on-line auction site (new surplus, ~$60 each) and built the power supplies. I am planning on using the filters as part of a 1420 MHz total power receiver in the future. Following the filters is a GaAsFET "gain block" amplifier which increases signal levels by 25 dB. The signal is then split using a NARDA 4321-2 0.5-2.0 GHz power divider, which feeds the R-7000 receiver. Following the power divider another gain block amplifier is used to further boost the signal for the Tektronix 2710 spectrum analyzer. The gain block amplifiers have noise temperatures of ~200K and are available at electronics flea markets such as the Dayton, Ohio Hamvention each May. Both the R-7000 receiver (used, ~$700) and spectrum analyzers similar to the one I have (used, ~$2000) can be found on internet auction sites.
Data acquisition. Hydrogen line spectra are currently recorded with a Tektronix 2710 digital spectrum analyzer. This instrument can record up to several hundred individual spectra and average them together for improved noise reduction. Data can be downloaded from the spectrum analyzer via its IEEE-488 port. Currently I am using an old Hewlett-Packard HP-87 computer as an interface for the analyzer. The HP-87 has both IEEE-488 and RS-232 interfaces and is used as a low-cost (used, ~$25) translator. Data from the HP-87 is sent on to a Macintosh computer for collection and storage. Simple software was written for both the HP-87 and the Mac to perform this data transfer. While the use of the spectrum analyzer is convenient an ICOM R-7000 receiver is also available. This receiver is used for noise figure measurements and will also be used for hydrogen line spectra when a suitable detector is built. Audio from the receiver is measured with the A.C. voltmeter, and its D.C. output can be fed to an analog-to-digital converter board (~ $300) in the PC. Using the old HP-87 is an awkward method of converting the IEEE-488 data of the spectrum analyzer to the more common RS-232 format but it was inexpensive. A National Instruments GPIB-PCII card (used, ~$75) has recently been obtained and will be used to control the analyzer in the future.
The positioning system. The antenna is controlled by software currently running on an old 286 PC. A program has been written that can be used for tracking the sun, moon, satellites or any point in space. The program continuously calculates the position of an object and this information is compared with the actual antenna position. If the antenna is off target by more than a set amount, the drive motors are operated until a correction is completed. The antenna uses a digital inclinometer (~$100) to feed back elevation position data to the computer and a potentiometer connected to the drive mechanism provides a voltage ratio which is proportional to the antenna azimuth position. The voltage is read by the analog-to-digital converter board in the PC.

 


 

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