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An Improved Superhet for WRMI reception
This, hopefully, will be a "new and improved" version of the simple superhet for reception of WRMI that was previously shown here.
Improvements will include wider range frequency coverage, better image rejection, and improved selectivity, achieved principally by changing from a single down conversion to an intermediate freque3ncy of 455 KHz, to a dual conversion up converting to 10.7 MHz as the first intermediate frequency.
With the use of a simple low pass filter as the front end, reception from the broadcast band to seven MHz or so should be readily accomplished. Images will be in the range above 22 Mhz so unlikely to present any issues, and a crystal filter at 10.7 Mhz will establish the initial selectivity ahead of the second IF.
Construction has begun. The Front end filter, mixer, and second conversion local oscillator are complete.
A TDA1072 again is used as the main device of the…







Over the weekend, I switched out the toroid inductors in the front end for much smaller SMD inductors, a very worthwhile change, I think.
I also installed a tentative AGC controlled PIN diode attenuator between the first mixer output and the input of the MAR-6SM IF amplifier, and am in the testing / adjustment phase of that.
I am starting to work on some additional documentation. Here is the graphic of the audio filter response at the output of the TDA1072 with the presently installed components. It matches up nicely with the 6 KHz Murata filter. I had Google AI generate the graph, so take it with a grain of salt, but it does correspond with what I hear.
73,
Win W5JAG