RA 40

RA 40
SSB TRANSCEIVER 40 M BAND

Tuesday, November 3, 2009

100MHz Spectrum Analyzer

100MHz Spectrum Analyzer

Iulian Rosu, VA3IUL / YO3DAC

http://www.qsl.net/va3iul/

This Spectrum Analyzer supposes to be a cheap and a useful device for any ham radio. To build this device you need minimum test equipment, like a digital counter, an oscilloscope, Grid-meter and a multi-meter. The main design is based on SA605D, FM receiver from Philips. This circuit is very common in some old analog cell phones.
If we take a look to the main schematic, we can see that the input signal pass through a low-pass filter (L1, C2, C3), an
d it is amplified by a MMIC, MAR6, in order to boost the weak signal performance of the instrument.
It is important to remember nev
er to exceed the maximum input level specification of the Spectrum Analyzer. Do not confuse the maximum input level specification with the 1dB-compression point or third-order intercept point specification. The maximum input level specification is the maximum input level that will not damage the amplifier or mixer. The 1dB compression point or third-order intercept point refers to distortion caused by excessive input levels. The third-order intercept point usually occurs about 10dB-15dB above the 1dB-compression point. If an analyzer specifies the 1dB-compression point as 0dBm, then input levels higher than 0dBm should not be present at the output of the RF attenuator. If the RF attenuation is set for 20dB, then the input level (at the input connector) may be as high as +20dBm without exceeding the 1dB-compression point. It is always best to allow an extra few decibels of safety margin. For example, if the 1dB-compression point is 0dBm, then the input level should be kept several decibels below this point for best performance.
If we check Minicircuits catalogue we can find that the 1 dB compression point for MAR6 is 2dBm with a gain of 20dB at 100MHz. But in the same time the SBL-1 mixer support on its RF input signals only up to 9dBm. So in our case, the limit of input signals will be around –10dBm, to keep a good linearity of our measurements.
The range of the VCO, used to down convert the s
ignal to first IF, is from 150MHz to 250MHz. The VCO can use any NPN RF transistor, like BFY90, BFR90 etc. The varicap diode should be MV209 or an equivalent diode, which can give a good, voltage versus capacity linearity. L9 from the tank circuit has 3 turns, on 3mm diameter and 5mm length. With a frequency counter connected to pin 8 of SBL-1 you can measure and adjust the frequency range of the VCO.
On the output of the SBL-1 mixer, we have the firs
t IF filter on 150MHz. The bandwidth of this filter is 1MHz. Each inductor of the filter has 5 turns, 1mm silver plated wire, on 8mm diameter and 10mm length. The trimmer capacitors (2-12pF) are used to tune the filter. Another MAR6 is used to amplify the first IF signal.
The circuit SA605D is a high performance monolithic FM system incorporating a
mixer/oscillator, two limiting amplifiers, quadrature detector, logarithmic received signal strength indicator (RSSI).
The input match of SA605D is C9, C10 and L7. The tank circuit of the 139.3MHz LO (
used to down convert the signal to second IF) is C12, C13, C15, L8. L8 has 6 turns, on 4mm diameter. Check for the right LO frequency on pin nr 4. For a better frequency stability you can use a 139.3MHz crystal oscillator. The second IF is 10.7MHz. I chose this frequency because here we can find plenty of IF filters. The main schematic use only one X-tal filter, which will give to the analyzer a 15kHz RBW (resolution bandwidth). Its possible to use here switched filters, for different RBW. For 3kHz RBW, is possible to use a SSB filter and for 150kHz RBW, ceramic filters used in broadcast FM radios.
One of the most important part of SA605D is the RSSI indicator, that will be our logarithmic dete
ctor. You can see the RSSI vs Input level graph in SA605D Datasheet and SA605D Application Note.
TL084(d), in a log amplifier configuration dr
ive the Y input of the oscilloscope. The other 3 amps of TL084 (a, b, c) are used to generate the sweep signal. The output of (b) it will drive the X input of the oscilloscope.
This design expect to be a cheap Spectrum Analyzer, but in the same time with nice performances. For more improvements you can add a step attenuator, more poles to the front end low pass filter, switchable filters on 10.7MHz IF, a variable BW video amplifier for vertical output etc.

Iulian Rosu, VA3IUL / YO3DAC

Home http://www.qsl.net/va3iul/














Block Diagram







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