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…

Some more work - the back end is mostly done; I removed most of the leaded components that were bugging me and kept only those that were needed to skywire across the board. The advantage of this is that SMD parts can still be placed underneath the skywired part, and that occurs in several instances here.
While the front end is mostly 0805, the back end around the TDA1072 is mostly 0603 for no particular reason other than that I could. The 0603 helps get more parts under a skywired component, but otherwise really doesn't save any space on this type of board.
It has been tested and is functional. Not necessarily optimized yet, but all circuit blocks appear to be working nominally.
I am not yet decided on what type of VFO / Display I will use, and where to place the audio amplifier that still needs to be built.
At some point, I will make a complete schematic for the RF board, but the TDA1072 is basically the data sheet.
Win W5JAG