Characteristics of Instrumentation Amplifiers
Instrumentation amplifiers are known for their precise gain, high input resistance, differential input, and low offset voltage. They offer features like low bias currents, noise, high CMRR, and large bandwidth. Learn about their connection to the source, offset, noise characteristics, monolithic in-amps, input/output offset noise, and three-opamp configurations. Delve into specific models like AD620 and understand their key parameters affecting performance.
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Presentation Transcript
Instrumentation Amplifiers: characteristics By definition: Precise gain High input resistance Differential input Other important features Low input referred offset voltage Low bias currents Low input referred voltage and current noise High CMRR Large bandwidth
Instrumentation Amplifiers: connection to the source ( ) = = + = v V i R v V i R V V v 1 1 1 2 2 2 1 2 in S B S n i R S B S S S nt v v i R 1 1 2 2 nt n B S B S ( ) Balanced case (RS1=RS2=RS) = + v v R i i 1 2 nt n S B B
Offset: vn=vio, iB1-iB2=IB1-IB2=Iio ( B S io iot I R v v + = 1 ) = + I v R I 2 B io S io Noise: vnand in1, in2are represented by their PSD (power spectral density) cross-spectrum ( ) = + + 2 S 2 S S R S S S 1 2 1 2 vnt vn I I I I If ib1and ib2are uncorrelated and their PSD is SI: = + 2 2 S S R S vnt vn S I
Monolithic In-Amps ( ) = + V G V V V + out IN IN REF Typical pin configuration Function of the SENSE terminal
Input and output offset / noise Typical two-stage architecture of In-amps Generally, A2= 1, thus: v v = + = + 2 2 n n v v v 1 1 nRTI n n A G 1
Three-opamp instrumentation amplifier Mismatch of these resistors degrades the CMRR of the second stage. Resistor trimming is necessary for CMRRs > 60 dB The circuit that provides VREFmust have a very low output resistance (<<R) 2 R = 1+ 1 G R G
Instrumentation Amplifiers AD 620 ( ) = + V G + V V / V + out IN 4 . IN R REF = 1 49 G k G The RTI noise decreases with G At G 100 the amplifier BW is larger than 100kHz. The noise density starts to fall for f> 100kHz
AD 620 GBW does not increase much beyond the G=10 case: BW affected by second stage Nearly constant GBW product: BW determined by first stage Slew -Rate Settling times Output noise >> input noise Broad-Band Noise: SBB Low Frequency Noise Integrated over 0.1-10 Hz Broad-Band Noise: SBB Current Low Frequency Noise Integrated over 0.1-10 Hz
Such a small offset voltage and offset drift is the result of a laser-trimmed resistor-load BJT input pair AD 620 The effective input referred offset (RTI) is a combination of the input and output offset Input offset Output offset The input bias current and input offset current are similar, since such a small bias current is the result of internal bias current cancellation The AD 620 in-amp represent a good trade-off between input noise voltage, input bias currents and supply current (quiescent current)
AD 8429 The AD8429 has a much smaller input referred noise than the AD620 (BB-noise) .. ..... but its input current noise is much larger..
AD 8429 The bias current (dc value) is also much larger than AD620 one The AD8429 is faster than the AD620 . but it requires much more quiescent current
Instrumentation Amplifiers The INA333 is a very low-power instrumentation amplifier (Isupply: 50 A) As a result, its input referred voltage noise is larger and its bandwidth smaller.
INA 333 Small bandwidths Very low input bias current Large noise density AD620 was 9 nV/ Hz
INA 111: J-Fet input Note the presence of a sense (Feedback) terminal in the 16 pin case Offset is considerably worse than AD620 which has a BJT input stage
INA 111 . but the (integrated) low-frequency voltage noise is much worse (was 0.28 V) in the AD 620 The broad-band input referred noise density is similar to AD 620 .. The strong advantage of a JFET input is the negligible noise current density
The LTC 1100 uses an Autozero technique to cancel the input offset and flicker noise. The side-effect is foldover, resulting in an increased low-frequency noise density.