SBOA590 November   2024 OPA186 , OPA206 , OPA328 , OPA391 , OPA928

 

  1.   1
  2.   Abstract
  3.   Trademarks
  4. 1Input Offset Voltage (VOS) Definition
    1. 1.1 Input Offset Voltage Drift (dVOS/dT) Definition
    2. 1.2 VOS and VOS Temperature Drift Inside the Amplifier
    3. 1.3 Laser Trim to Adjust Performance
    4. 1.4 Package Trim (e-Trim™) to Adjust Performance
  5. 2Input bias current (IB) definition
    1. 2.1 Input Bias Current (IB) and IB Temperature Drift Inside the Amplifier
    2. 2.2 Derivation of IB Conversion to VOS
    3. 2.3 Internal Bias Current Cancelation
    4. 2.4 Super Beta Input Transistors
  6. 3Other Factors Influencing Offset
    1. 3.1 Finite Open Loop Gain (AOL)
    2. 3.2 Common Mode Rejection Ratio (CMRR)
    3. 3.3 Power Supply Rejection Ratio (PSRR)
    4. 3.4 AOL, CMRR, and PSRR Over Frequency
    5. 3.5 Electromagnetic Interference Ratio (EMIRR)
    6. 3.6 Mechanical Stress Induced Offset Shift
    7. 3.7 Parasitic Thermocouples
    8. 3.8 Flux Residue and Cleanliness
  7. 4Zero-drift Amplifiers to Minimize VOS and VOS Drift
  8. 5Calibration of VOS, IB, and Gain Error
  9. 6References
  10. 7Revision History

VOS and VOS Temperature Drift Inside the Amplifier

Both bipolar and CMOS op amps have an input differential pair used as the first stage of the amplifier (see Figure 1-5, and Figure 1-6). For bipolar devices, the offset voltage is mainly due to the mismatch of the base to emitter junction voltages (Vbe1 and Vbe2). This mismatch is due to photo-lithography effects, doping gradients, and stress introduced during packaging of the device. Similarly, the offset in CMOS devices is from the gate-to-source voltage mismatch, and the mismatch is due to the same types of fabrication issues as with bipolar.

The VOS in bipolar and CMOS op amps can be reduced by adjusting the value of Ros1 or Ros2. This process is called trimming and can be accomplished through laser-trim or package-level-trim (e-Trim®). In both cases the VOS is measured and resistors are adjusted to minimize the offset. In laser-trimming, sections of a thin film resistor are physically cut away to increase the resistance (see Section 1.3). Package-level-trim uses digital communications to open switches or fuses in a binary weighted resistor network (see Section 1.4). A third way that op amp VOS can be minimized is by using an internal self-calibration circuit. These types of amplifiers are called zero-drift amplifiers and are covered in Section 4.

OPA206 Bipolar differential input,
                    simplified op amp model Figure 1-5 Bipolar differential input, simplified op amp model
OPA206 CMOS differential input,
                    simplified op amp model Figure 1-6 CMOS differential input, simplified op amp model

The temperature drift of a bipolar op amp is linear and is directly proportionate to offset (see Figure 1-7). In fact, each millivolt of offset yields about 3.3µV/C of offset drift. Thus, trimming the offset to zero on a bipolar op amp also trims the drift close to zero (see Figure 1-7). Conversely, the drift of CMOS devices is nonlinear and is not proportional to offset as with the bipolar (see Figure 1-8). Trimming the temperature drift on a CMOS device requires adjustment of resistors R1, R2, and offset is trimed with ROS1, and ROS2 (see Figure 1-6). Furthermore, the CMOS op amp offset must be measured at multiple temperatures in order to trim the temperature drift, whereas the bipolar device temperature drift can be trimmed at a single temperature. The additional complexity of the CMOS VOS and the VOS-drift trim makes it challenging to achieve the same performance as the bipolar device.

OPA206 Bipolar VOS vs
                    Temperature Figure 1-7 Bipolar VOS vs Temperature
OPA206 CMOS VOS vs
                    Temperature Figure 1-8 CMOS VOS vs Temperature