Handbook for Sound Engineers

(Wang) #1

910 Chapter 25


to some op-amps for glue. A simple, very low parts
count compressor with all the active elements contained
within this part is shown in Fig. 25-85. As can be seen,
it relates strongly to the block diagram of Fig. 25-84.


25.13 Mixing


25.13.1 Virtual-Earth Mixers


The circuit diagram of Fig. 25-86 in its simplicity belies
the hidden design that is in the relationship of the
circuitry to its mechanical and electrical environment.
This is where the care and feeding of op-amps
(Section 25.7) and grounding paths (Section 25.8) really
pay dividends. Mix-amp stages, with large numbers of
permanently assigned sources such as in the main mix
buses, are as crucial to the overall well-being of a
console as any front-end stage could be. In a typical
situation, as a unity-gain virtual-earth mixing stage with
33 sources (channels plus access), the amplifier is being
asked for about 30 dB of broadband gain, as much as
any other stage in the chain including both the micro-
phone preamp and/or secondary input stage.


25.13.2 Noise Sources

All the following about mix devices assumes that
system grounding is impeccable. Jolly good. That said:
That mix-amp gain is sometimes referred to as noise
gain is not accidental. Unless care is taken to balance
fader-back channel noise contributions against this
self-generated mix-amp noise, the latter could well
predominate and arbitrarily determine the noise floor
for the entire console. Similarly, channel noise contribu-
tion should equal or outstrip mix-amp noise, but not
excessively so: ideally they should equally contribute,
to the extent that channel-off noise contribution should
not necessarily impact the overall bus noise, while bus
noise should not significantly impact channel-on noise.
Self-noise generation in the mix-amp is predominantly
the amplified thermal noise of the paralleled source and
feedback resistances, device input current noise, and
surface generation and recombination noise. The last
two can be minimized by device choice. Thermal noise
is physics and is here to stay. Common sense on first
glance says to make the mix resistors as low in value as
possible but this has the downside that too low a value
would cause quite large signal (hence, ground) currents

Figure 25-85. A feed-forward VCA compressor using THAT 4301.

10 MF

10 MF

10 MF

10 MF

10 MF

+15 V

+

+

15 V

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+

(^1) IN
2
4
7
5
6
8
0



  • 012
    2 M
    15 V
    +15 V
    1Ve
    Ve
    10 k
    Precision rectifier
    rms detector averager
    Indicates 3300 ppm temperature
    compensating resistors
    Thresholder
    Threshold
    Ratio attenuator Summer
    IT RMS
    5.1 k

    28.8 K
    OUT
    CT
    15V
    IN 4148
    IN 4148
    22 pF 100 nF
    300 k
    392 k
    20 k
    1.43 k
    1.2 M
    "Fader" input


  • 18
    19
    20
    0
    1.65 M
    50 7
    15
    14
    169
    11
    10
    20 k (^17) VCA 13
    150 R
    20 k
    20 k
    5 K1*
    100 nF
    100 pF
    100 nF
    10 k
    10 k




  • Ratio
    +15 V
    15 V



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