Recently I have been asked to look at a few designs of seismic amplifiers and filters used by PSN members. Two points that I have not previously noticed are worth considering. re: not amplifying all the noise: The first point is that even when an amplifier is not specifically being used as a low pass filter, but only for signal gain, the frequency response should still be limited to the low frequencies generally used in seismic work. There is no point amplifying all the noise, especially 60 hz noise. This may be strong enough that after a gain of 1000 it might even saturate a later amplifier stage. The solution is to always use a capacitor in parallel with the high value feedback resistor that sets the amplifier gain. For example, for a gain of 40 db or x 100, the feedback R would be 990k ohm to the inverting input, with 10k ohm to ground. If the 990k is paralleled with a 0.005 uf capacitor, the frequency response would begin to decrease by 6 db per octave at f=/2*pi*R*C or 32 hz. Otherwise it would only be limited by the gain-bandwidth figure of the amplifier. This frequency is usually selected to be well away from the response shaping multi-pole filters that are used, so it could be ignored in the circuit analysis. In the seismic amplifier I have posted, the first stage has a 0.001uf, which when in parallel with the highest gain resistor of 1.4 megohms (where less noise amplification is needed most), has a frequency of 114 hz. Only three gains are selectable for the second stage, so a capacitor is used for each, with a corner at about 25 hz. The following four-pole unity-gain filter has an effective corner at 19.5 hz. This consideration of "by passing" high value resistors should be used in variable gain stages as well as any offset adjustment arrangements (although I prefer to use the relatively low power LM308 amplifiers because they have little appreciable offset problems and produce little heat). Every effort is needed to eliminate any gain at 60 hz and above, especially where such noise will be amplified by later gain stages. If radio telemetry is used, further care in by-passing any vestige of it from the power supply rails, the input circuitry, etc, is needed. For RF suppression, low inductance ceramic capacitors should be used. Often low value (100 ohm) wire-wound (= inductive) resistors are used in series with the DC supplies at the inputs to a circuit card, which are then by-passed to common with both ceramic AND large electrolytic capacitors. Re: multi-pole filters The other observation is that simply cascading identical 2-pole filters is not the way to achieve multi-pole performance. The individual response curves don't stack up as one would expect because of interaction between the stages. In fact, different effective frequencies and/or damping are selected for each stage, depending on the total number of poles, to achieve the overall result of total attenuation and the shape of the rolloff (Buttworth, Chebyshev. Bessel, etc). "Stacking" identical filters with any appreciable gain often results in oscillation. Even multi-pole Butterworth filters have the same frequency but radically different damping (and gain) per stage. But Bessel filters are preferred in seismic amplifiers because of their uniform phase delay. For an example of the range of values, a 6-pole low pass Bessel filter will have three second-order sections with frequencies of 1.609f, 1.694f, 1.910f, and damping per section of 1.96, 1.64, 0.98, where "f" is the overall cutoff (-3db down) frequency. The "compromise" filter, also called a Thompson-Butterworth, has frequencies of 1.268f, 1.301f, 1.382f, and damping of 1.95, 1.52, 0.71. Even the flattest response Butterworth filter, where the frequencies are all 1.000f, has damping values of 1.93, 1.41, and 0.52 per section. Among the references I use, two give very workable designs and tables for multi-pole filters. The NASA publication, "An RC Active Filter Design Handbook", NASA SP-5104, 1977, gives standard designs for up to 8 poles, and uses a constant resistance algorithm for unity gain 1 khz filters that unfortunately results in very uncommon capacitor values. The designs are impedance and frequency scaled by multiplying/ dividing the R and C values. I have found that the odd capacitor values can usually be made up with two common values. The unity gain design is stable and simplifies inclusion in precision amplifier designs. The other reference is the Sams publication "Active-Filter Cookbook" by Don Lancster; Howard W. Sams & co, 1975, Indianapolis; ISBN 0-672-21168-8; Library of Congress 74-33839. He uses an algorithm that gives equal values for all the capacitors, with the frequency and damping changed by the filter and feedback resistors. The designs are also scaleable from 1 khz. Since the damping of each stage is controlled by the feedback resistance, this results in gain variability depending on the response selected and number of poles. There are excellent tables for filters of 7 different characteristics and up through sixth order (or poles) with all the resistance values, gains, and component tolerances calculated and graphs for frequency scaling the capacitor values. I prefer the NASA filters because they are all unity gain and often use a constant resistance for all the stages, which helps quantity buying of 1% values. The capacitor values are usually made up with a larger value, like 0.47, which can be purchased in quantity, and smaller parallel values, which cost much less and can be selected for value with a meter. So if your filter design involves several identical stages but doesn't realize the multi-pole performance you want, or even oscillates, you might want to look at these references. Regards, Sean-Thomas __________________________________________________________ Public Seismic Network Mailing List (PSN-L)
Larry Cochrane <cochrane@..............>