SID Receiver overview |
Here are the main characteristics of the SID receiver:
Synoptic |
The basic principle of the SID receiver is to measure the amplitude of a VLF station and to convert it to digital data.
The signal from the antenna (usually a loop antenna) is filtered out to limit the signals to the frequencies of interest in the VLF and lower-LF frequency range.
The RF pre-amplifier section is built around one non-inverting amplifier with a gain of 21 and two inverting amplifier stages with gains adjustable between 0 and 25.
The signal is then filtered in the tuning section. The MAX275 is a continuous-time 4th-order active filter. The MAC275 is configured as a bandpass filter; center frequency, gain and Q are adjusted by resistors.
The following section is the RF post amplifier. It has a gain adjustable between 0 and 10. A buffer provides an optional carrier output with a 50Ω impedance.
Then, a full-wave rectifier and peak detector is used as a linear detector converting the RMS value of the VLF station to a DC voltage level. This level is averaged (default time constant around 1 minute) to produce a signal strength value.
DC offset can be applied to the signal strength value, before further amplification in the output amplifier section (selectable gains of x3.25, x4 and x10).
Finally, the analog to digital conversion is performed by the 12-bits ADC MAX187.
The interface between the MAX187 and the computer is done though an USB port.
The design has been highly inspired from the SID monitor of the Stanford Solar Center.
The schematics for the SID receiver as well as the bill of material is available here:
To view those files, you need a PDF viewer such as SumatraPDF (Windows): or Adobe® Reader® (Windows, Mac, Linux):
Printed Circuit Board |
Tuning |
Assembly |
Data Transfer Protocol |
SID monitoring station by Lionel LOUDET is licensed under a Creative Commons Attribution-NonCommercial-ShareAlike 3.0 Unported License. |
Last Update: 20 Jul 2013 |
Apache/2.4.62 (Debian) |