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THS3061 Datasheet, PDF (15/25 Pages) Texas Instruments – LOW DISTORTION HIGH SLEW RATE CURRENT FREEBACK AMPLIFIERS
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THS3061
THS3062
SLOS394A – JULY 2002 – OCTOBER 2002
NOISE CALCULATIONS
Noise can cause errors on very small signals. This is especially true for amplifying small signals coming over a
transmission line or an antenna. The noise model for current-feedback amplifiers (CFB) is the same as for voltage
feedback amplifiers (VFB). The only difference between the two is that CFB amplifiers generally specify different
current-noise parameters for each input, while VFB amplifiers usually only specify one noise-current parameter. The
noise model is shown in Figure 49. This model includes all of the noise sources as follows:
• en = Amplifier internal voltage noise (nV/√Hz)
• IN+ = Noninverting current noise (pA/√Hz)
• IN– = Inverting current noise (pA/√Hz)
• eRx = Thermal voltage noise associated with each resistor (eRx = 4 kTRx)
RS
eRs
en
Noiseless
eni
+
_
eno
IN+
eRf
Rf
IN–
eRg
Rg
Figure 49. Noise Model
The total equivalent input noise density (eni) is calculated by using the following equation:
Ǹ ǒ Ǔ ǒ Ǔ ǒ Ǔ ǒ Ǔ eni +
ǒenǓ2 ) IN )
2
RS ) IN *
2
Rf ø Rg ) 4 kTRs ) 4 kT Rf ø Rg
where
k = Boltzmann’s constant = 1.380658 × 10–23
T = Temperature in degrees Kelvin (273 +°C)
Rf || Rg = Parallel resistance of Rf and Rg
To get the equivalent output noise of the amplifier, just multiply the equivalent input noise density (eni) by the overall
amplifier gain (AV).
ǒ Ǔ eno + eni AV
+ eni
1
)
Rf
Rg
(Noninverting Case)
As the previous equations show, to keep noise at a minimum, small value resistors should be used. As the closed-loop
gain is increased (by reducing RF and RG), the input noise is reduced considerably because of the parallel resistance
term. This leads to the general conclusion that the most dominant noise sources are the source resistor (RS) and the
internal amplifier noise voltage (en). Because noise is summed in a root-mean-squares method, noise sources
smaller than 25% of the largest noise source can be effectively ignored. This can greatly simplify the formula and
make noise calculations much easier.
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