AN106 - Instrumentation Circuitry Using RMS-to-DC Converters

Application Note 106 AN106-2 an106f VDD 5V –5V LTC1966 ±5V Supplies, Differential, DC-Coupled RMS-to-DC Converter 5V Single Supply, Differential, AC-C...

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Application Note 106 February 2007 Instrumentation Circuitry Using RMS-to-DC Converters RMS Converters Rectify Average Results Jim Williams INTRODUCTION

Isolated Power Line Monitor

It is widely acknowledged that RMS (Root of the Mean of the Square) measurement of waveforms furnishes the most accurate amplitude information.1 Rectify-andaverage schemes, usually calibrated to a sine wave, are only accurate for one waveshape. Departures from this waveshape result in pronounced errors. Although accurate, RMS conversion often entails limited bandwidth, restricted range, complexity and difficult to characterize dynamic and static errors. Recent developments address these issues while simultaneously improving accuracy. Figure 1 shows the LTC®1966/LTC1967/LTC1968 device family. Low frequency accuracy, including linearity and gain error, is inside 0.5% with 1% error at bandwidths extending to 500kHz. These converters employ a sigma-delta based computational scheme to achieve their performance.2

BEFORE PROCEEDING ANY FURTHER, THE READER IS WARNED THAT CAUTION MUST BE USED IN THE CONSTRUCTION, TESTING AND USE OF THIS CIRCUIT. HIGH VOLTAGE, LETHAL POTENTIALS ARE PRESENT IN THIS CIRCUIT. EXTREME CAUTION MUST BE USED IN WORKING WITH, AND MAKING CONNECTIONS TO, THIS CIRCUIT. REPEAT: THIS CIRCUIT CONTAINS DANGEROUS, HIGH VOLTAGE POTENTIALS. USE CAUTION.

Figure 2’s pinout descriptions and basic circuits reveal an easily applied device. An output filter capacitor is all that is required to form a functional RMS-to-DC converter. Split and single supply powered variants are shown. Such ease of implementation invites a broad range of application; examples begin with Figure 3.

Figure 3’s AC power line monitor has 0.5% accuracy over a sensed 90VAC to 130VAC input and provides a safe, fully isolated output. RMS conversion provides accurate reporting of AC line voltage regardless of waveform distortion, which is common. , LT, LTC and LTM are registered trademarks of Linear Technology Corporation. All other trademarks are the property of their respective owners.

1See Appendix A, “RMS-to-DC Conversion” for complete discussion of

RMS measurement. 2Appendix A details sigma-delta based RMS-to-DC converter operation.

PART NUMBER

LINEARITY ERROR TYP/MAX (%)

CONVERSION GAIN ERROR TYP/MAX (%)

1% ERROR BANDWIDTH (kHz)

3dB ERROR BANDWIDTH (kHz)

LTC1966

0.02/0.15

0.1/0.3

6

800

2.7

±5

170

LTC1967

0.02/0.15

0.1/0.3

200

4MHz

4.5

5.5

390

LTC1968

0.02/0.15

0.1/0.3

500

15MHz

4.5

5.5

2.3mA

SUPPLY VOLTAGE MIN(V) MAX(V)

ISUPPLY MAX (µA)

Figure 1. Primary Differences in RMS to DC Converter Family are Bandwidth and Supply Requirements. All Devices Have Rail-to-Rail Differential Inputs and Output

an106f

AN106-1

Application Note 106 POSITIVE SUPPLY 2.7V TO 5.5V DEPENDING ON DEVICE CHOICE

+V

DIFFERENTIAL INPUTS. MAX COMMON MODE RANGE = ±V SUPPLY. MAX DIFFERENTIAL = 1V. MINIMUM INPUT = 5mV

INPUT 1

OUTPUT TO FILTER CAPACITOR

LTC1966 LTC1967 LTC1968

INPUT 2 ENABLE

–V*

OUTPUT

OUTPUT OUTPUT REFERRED TO THIS PIN. NORMALLY GROUNDED

OUTPUT RETURN GND

SET HIGH TO LTC1966 ONLY. SHUT DOWN 0V TO –5V SUPPLY

POWER GROUND

*NO –V PIN ON THE LTC1967/LTC1968

±5V Supplies, Differential, DC-Coupled RMS-to-DC Converter

5V Single Supply, Differential, AC-Coupled RMS-to-DC Converter

5V

5V

DC + AC INPUTS (1VPEAK DIFFERENTIAL)

VDD

VDD

LTC1966

LTC1966

IN1

DC OUTPUT CAVE ZO = 85kΩ 1µF

VOUT

IN2 OUT RTN

AC INPUTS (1VPEAK DIFFERENTIAL)

VSS GND EN

VOUT

IN1

IN2 OUT RTN CC 0.1µF

DC OUTPUT CAVE ZO = 85kΩ 1µF

VSS GND EN AN106 F02

–5V

Figure 2. RMS Converter Pin Functions (Top) and Basic Circuits (Bottom). Pin Descriptions are Common to All Devices, with Minor Differences

BIAS SUPPLY 1k –5V 100µF

+ 1k

1 T1 5 LINE INPUT 90VAC TO 140VAC

A 4

5V

+ 100Ω 1W

100µF

6 7

ISOLATED LINE SENSE

B

100Ω 1W 0.25%

1k

DANGER! Lethal Potentials Present—See Text

100Ω

8 120VAC TRIM

10Ω 0.25%

RMS CONVERTER 5V

–5V

+V

–V C1 OUT LTC1966 IN2 OUT RTN EN GND

+

IN1

1µF

RMS OUT 0.9V TO 1.4V = 90VAC TO 140VAC

A1 LT®1006

– 100k*

T1 = TAMURA-PAN MAG 3FS-212 = 1N4148 = 1N4689 5.1V

100k* AN106 F03

*1% METAL FILM RESISTOR 1µF = WIMA MKS-2

Figure 3. Isolated Power Line Monitor Senses Via Transformer with 0.5% Accuracy Over 90VAC to 130VAC Input. Secondary Loading Optimizes Transformer Voltage Conversion Linearity

an106f

AN106-2

Application Note 106 The AC line voltage is divided down by T1’s ratio. An isolated and reduced potential appears across T1’s secondary B, where it is resistively scaled and presented to C1’s input. Power for C1 comes from T1’s secondary A, which is rectified, filtered and zener regulated to DC. A1 takes gain and provides a numerically convenient output. Accuracy is increased by biasing T1 to an optimal loading point, facilitated by the relatively low resistance divider values. Similarly, although C1 and A1 are capable of single supply operation, split supplies maintain symmetrical T1 loading. The circuit is calibrated by adjusting the 1k trim for 1.20V output with the AC line set at 120VAC. This adjustment is made using a variable AC line transformer and a well floated (use a line isolation transformer) RMS voltmeter.3 Figure 4’s error plot shows 0.5% accuracy from 90VAC to 130VAC, degrading to 1.4% at 140VAC. The beneficial effect of trimming at 120VAC is clearly evident; trimming at full scale would result in larger overall error, primarily due to non-ideal transformer behavior. Note that the data is specific to the transformer specified. Substitution for T1 necessitates circuit value changes and recharacterization.

RMS OUTPUT READING ERROR (%)

2.0 1.5 1.0

Fully Isolated 2500V Breakdown, Wideband RMS-to-DC Converter NOTE: BEFORE PROCEEDING ANY FURTHER, THE READER IS WARNED THAT CAUTION MUST BE USED IN THE CONSTRUCTION, TESTING AND USE OF THIS CIRCUIT. HIGH VOLTAGE, LETHAL POTENTIALS ARE PRESENT IN THIS CIRCUIT. EXTREME CAUTION MUST BE USED IN WORKING WITH, AND MAKING CONNECTIONS TO, THIS CIRCUIT. REPEAT: THIS CIRCUIT CONTAINS DANGEROUS, HIGH VOLTAGE POTENTIALS. USE CAUTION. Accurate RMS amplitude measurement of SCR chopped AC line related waveforms is a common requirement. This measurement is complicated by the SCR’s fast switching of a sine wave, introducing odd waveshapes with high frequency harmonic content. Figure 5’s conceptual SCRbased AC/DC converter is typical. The SCRs alternately chop the 220VAC line, responding to a loop enforced, phase modulated trigger to maintain a DC output. Figure 6’s waveforms are representative of operation. Trace A is one AC line phase, trace B the SCR cathodes. The SCR’s irregularly shaped waveform contains DC and high frequency harmonic, requiring wideband RMS conversion for measurement. Additionally, for safety and system interface considerations, the measurement must be fully isolated. 3See Appendix B, “AC Measurement and Signal Handling Practice,” for

0.5

recommendations on RMS voltmeters and other AC measurement related gossip.

120VAC TRIM POINT 0 –0.5

DANGER! Lethal Potentials Present—See Text

–1.0 220VAC –1.5

DC OUTPUT

INPUT –2.0 90

100 110 120 130 140 RMS INPUT VOLTAGE (V)

NEUTRAL

AN106 F04

Figure 4. Error Plot for Isolated Line Monitor Shows 0.5% Accuracy from 90VAC to 130VAC, Degrading to 1.4% at 140VAC. Transformer Parasitics Account for Almost All Error

220VAC

AC LINE SYNC AND PHASE MODULATION

TRIGGER AN106 F05

REF

Figure 5. Conceptual AC/DC Converter is Typical of SCR-Based Configurations. Feedback Directed, AC Line Synchronized Trigger Phase Modulates SCR Turn-On, Controlling DC Output an106f

AN106-3

Application Note 106 Figure 7 provides isolated power and data output paths to an RMS-to-DC converter, permitting safe, wideband, digital output RMS measurement. A pulse generator configured comparator combines with Q1 and Q2 to drive T1, resulting in isolated 5V power at T1’s rectified, filtered and zener regulated output. The RMS-to-DC converter senses either 135VAC or 270VAC full-scale inputs via a resistive divider. The converter’s DC output feeds a self-clocked, serially interfaced A/D converter; optocouplers convey output data across the isolation barrier. The LTC6650 provides a 1V reference to the A/D and biases the RMS-to-DC converter’s inputs to accommodate the voltage divider’s AC swing. Calibration is accomplished by adjusting the 20k trim while noting output data agreement with the input AC voltage. Circuit accuracy is within 1% in a 200kHz bandwidth.

A = 100V/DIV

B = 50V/DIV ON 170 VDC LEVEL

AN106 F06

1ms/DIV

Figure 6. Typical SCR-Based Converter Waveforms Taken at AC Line (Trace A) and SCR Cathodes (Trace B). SCR’s Irregularly Shaped Waveform Contains DC and High Frequency Harmonic, Requiring Wideband RMS Converter for Measurement

PULSE GENERATOR 1N4148

POWER DRIVER

1k 1k

220k

Q2 ZTX-749 100Ω

– 1k

0.001µF

+

5V

2Ω

Q1 2N2369 3

LT1671

ISOLATED POWER SUPPLY 1N5817

1

750k

6

4

5V ISO

+

1N4689 5.1V

1N4148

100µF

750k 5V 750k

T1 ISOLATION/POWER TRANSFORMER DANGER! Lethal Potentials Present—See Text

2500V BREAKDOWN ISOLATION BARRIER

182k* DATA ISOLATORS

5V

4.7k 5V ISO

A/D

RMS CONVERTER 182k*

5V ISO

5V ISO

SCK



+V DATA OUTPUTS

VIN

LT1006

LTC2400

5V

OUT 1µF†

SDO FO GND CS REF

INPUT 135VAC OR 270VAC FULL SCALE

0.1µF

+V

+

SCK

CALIBRATE 20k

5V ISO

IN1 LTC1967

1k*

OUT RTN IN2 GND EN

SDO

+ 5V ISO 4.7k

ISOLATORS = AGILENT-HCPL-2300-010 T1 = BI TECHNOLOGIES HM-41-11510 * = 1% METAL FILM RESISTOR † = WIMA MKS-2

10µF 5V ISO

1µF

LT6650 400mV REFERENCE

+ –

1VDC

OUT FB

15k* 1µF

= CIRCUIT COMMON = AC LINE GROUND

AN106 F07

10k*

Figure 7. Isolated RMS Converter Permits Safe, Digital Output, Wideband RMS Measurement. T1-Based Circuitry Supplies Isolated Power. RMS-to-DC Converter Senses High Voltage Input via Resistive Divider. A/D Converter Provides Digital Output Through Optoisolators. Accuracy is 1% in 200kHz Bandwidth an106f

AN106-4

Application Note 106 Low Distortion AC Line RMS Voltage Regulator

Almost all AC line voltage regulators rely on some form of waveform chopping, clipping or interruption to function. This is efficient, but introduces waveform distortion, which is unacceptable in some applications. Figure 8 regulates the AC line’s RMS value within 0.25% over wide input swings and does not introduce distortion. It does this by continuously controlling the conductivity of a series pass MOSFET in the AC lines path. Enclosing the MOSFET in a diode bridge permits it to operate during both AC line polarities.

NOTE: BEFORE PROCEEDING ANY FURTHER, THE READER IS WARNED THAT CAUTION MUST BE USED IN THE CONSTRUCTION, TESTING AND USE OF THIS CIRCUIT. HIGH VOLTAGE, LETHAL POTENTIALS ARE PRESENT IN THIS CIRCUIT. EXTREME CAUTION MUST BE USED IN WORKING WITH, AND MAKING CONNECTIONS TO, THIS CIRCUIT. REPEAT: THIS CIRCUIT CONTAINS DANGEROUS, HIGH VOLTAGE POTENTIALS. USE CAUTION.

AC SERIES PASS AND CURRENT LIMIT DANGER! Lethal Potentials Present—See Text AC HIGH

Q2 IRF-840

1.5A SB 0.03µF

+V REGULATORS

470k

100k

0.47µF

10k

430k

170V

AC HIGH Q6 2N3904

0.7Ω

Q4 MPSA42 5V

BAT85 1N4690 5.6V

1N5281B 200V

2.2M* 0.1µF

UNREGULATED AC LINE INPUT

10k 2W 200k

0.22µF

OVERVOLTAGE Q3 2N5210 PROTECTION

FEEDBACK SENSE

170V ISOLATED GATE BIAS 1µF

200k

22k

RMS-TO-DC CONVERTER 5V

5V

C1



5.6k

Q1 2N3440

10k 1µF

+ REFERENCE IN

0.4V OUT LT6650 GND

1k

105VAC TO 120VAC ADJUST 7.32k*

1N4689 5.1V

330k 5V

+V IN1 LTC1966 IN2 OUT RTN EN –V GND

OUT

A1 LT1077

AC LOW

HEAT SINK IRF-840 *1% METAL FILM RESISTOR OPTODRIVER = TOSHIBA TLP190B

VAC REGULATED OUTPUT

0.1µF CONTROL AMPLIFIER

AC LOW

2.2µF MYLAR

1µF

FB

= 1N4005 1M

Q5 2N4393 0.22µF

100k

AN106 F08

SOFT-START/–VBIAS

Figure 8. Adjustable AC Line Voltage Regulator Introduces No Waveform Distortion. Line Voltage RMS Value is Sensed and Compared to a Reference by A1. A1 Biases Photovoltaic Optocoupler via Q1, Setting Q2-Diode Bridge Conductivity and Closing a Control Loop. VIN Must be ≥2V Above VOUT to Maintain Regulation

an106f

AN106-5

Application Note 106 The AC line voltage is applied to the Q2-diode bridge. The Q2-diode bridge output is sensed by a calibrated variable voltage divider which feeds C1. C1’s output, representing the regulated lines RMS value, is routed to control amplifier A1 and compared to a reference. A1’s output biases Q1, controlling drive to a photovoltaic optoisolator. The optoisolator’s output voltage provides level-shifted bias to diode bridge enclosed Q2, closing a control loop which regulates the output’s RMS voltage against AC line and load shifts. RC components in A1’s local feedback path stabilize the control loop. The loop operates Q2 in its linear region, much like a common low voltage DC linear regulator. The result is absence of introduced distortion at the expense of lost power. Available output power is constrained by heat dissipation. For example, with the output adjustment set to regulate 10V below the normal input, Q2 dissipates about 10W at 100W output. This figure can be improved upon. The circuit regulates for VIN ≥ 2V above VOUT, but operation in this region risks regulation dropout as VIN varies. Circuit details include JFET Q5 and associated components. The passive components associated with Q5’s gate form a slow turn-on negative supply for C1. They also provide gate bias for Q5. Q5, a soft-start, prevents abrupt AC power application to the output at start-up. When power is off, Q5 conducts, holding A1’s “+” input low. When power is applied, A1 initially has a zero volt reference, causing the control loop to set the output at zero. As the 1MΩ 0.22µF combination charges, Q5’s gate moves negative, causing its channel conductivity to gradually decay. Q5 ramps off, A1’s positive input moves smoothly towards the LT6650’s 400mV reference, and the AC output similarly ascends towards its regulation point. Current sensor Q6, measuring across the 0.7Ω shunt, limits output current to about 1A. At normal line inputs (90VAC to 135VAC) Q4 supplies 5V operating bias to the circuit. If line voltage rises beyond this point, Q3 comes on, turning off Q4 and shutting down the circuit. X1000 DC Stabilized Millivolt Preamplifier The preceding circuits furnish high level inputs to the RMS converter. Many applications lack this advantage and some form of preamplifier is required. High gain pre-amplification for the RMS converter requires more attention than might be supposed. The preamplifier must have low offset error because the RMS converter (desirably) processes DC as

legitimate input. More subtly, the preamplifier must have far more bandwidth than is immediately apparent. The amplifiers –3db bandwidth is of interest, but its closed loop 1% amplitude error bandwidth must be high enough to maintain accuracy over the RMS converter’s 1% error passband. This is not trivial, as very high open-loop gain at the maximum frequency of interest is required to avoid inaccurate closed-loop gain. Figure 9 shows an x1000 preamplifier which preserves the LTC1966’s DC-6kHz 1% accuracy. The amplifier may be either AC or DC coupled to the RMS converter. The 1mV full-scale input is split into high and low frequency paths. AC coupled A1 and A2 take a cascaded, high frequency gain of 1000. DC coupled, chopper stabilized A3 also has X1000 gain, but is restricted to DC and low frequency by its RC input filter. Assuming the switch is set to “DC + AC,” high and low frequency path information recombine at the RMS converter. The high frequency paths 650kHz –3db response combines with the low frequency sections microvolt level offset to preserve the RMS converters DC-6kHz 1% error. If only AC response is desired, the switch is set to the appropriate position. The minimum processable input, set by the circuits noise floor, is 15µV. Wideband Decade Ranged X1000 Preamplifier The LTC1968, with a 500kHz, 1% error bandwidth, poses a significant challenge for an accurate preamplifier, but Figure 10 meets the requirement. This design features decade ranged gain to X1000 with a 1% error bandwidth beyond 500kHz, preserving the RMS converters 1% error bandwidth. Its 20µV noise floor maintains wideband performance at microvolt level inputs. Q1A and Q1B form a low noise buffer, permitting high impedance inputs. A1 and A2, both gain switchable, take cascaded gain in accordance with the figure’s table. The gains are settable via reed relays controlled by a 2-bit code. A2’s output feeds the RMS converter and the converter’s output is smoothed by a Sallen-Keys active filter. The circuit maintains 1% error over a 10Hz to 500kHz bandwidth at all gains due to the preamplifiers –3db, 10MHz bandwidth. The 10Hz low frequency restriction could be eliminated with a DC stabilization path similar to Figure 9’s but its gain would have to be switched in concert with the A1-A2 path. an106f

AN106-6

Application Note 106 INPUT 0mV TO 1mV 1µF

HIGH FREQUENCY PATH

AC/DC SUMMATION

RMS CONVERTER

+

5V

A1 LT1122

1M

+



+V

A2 LT1222

10k*



–5V

1µF –V OUT LTC1966 OUT RTN

IN1 IN2

10k*

EN 1M

OUTPUT 0V TO 1V

+ 1µF

A4 LT1077



GND

536Ω* 100k

200Ω*

AN106 F09

LOW FREQUENCY/DC PATH

+ A3 LTC1050

100pF



*1% METAL FILM RESISTOR 1µF = WIMA MKS-2

DC + AC

AC RMS STAGE INPUT COUPLING

1M*

1k*

Figure 9. X1000 Preamplifier Allows 1mV Full-Scale Sensitivity RMS-to-DC Conversion. Input Splits Into High and Low Frequency Amplifier Paths, Recombining at RMS Converter. Amplifier’s –3dB, 650kHz Bandwidth Preserves RMS-to-DC Converter’s 6kHz, 1% Error Bandwidth. Noise Floor is 15µV

INPUT BUFFER

OUTPUT FILTER

5V INPUT 1µF

10µF Q1A 1M 100Ω

43k

SWITCHED GAIN AMP A = 1, 100

A1 LT1227

Q1B ZERO

+





IN1 750Ω* 470Ω

–5V

A=1 TRIM

10k 200k A = 100 TRIM

22Ω

5.62Ω* 90.9Ω*

100Ω

5V

IN2

10k

0.1µF 5V

1M 20k

= VN2222L

5.62k*

24.9k*

10µF

1µF

OUTPUT A3 LT1077

+

AN106 F10

GND

10k

A = 10 TRIM

Q1 = 2N6485. GROUND CASE *1% METAL FILM RESISTOR RELAYS = COTO-COIL 800-05-001 10µF, 1µF = WIMA MKS-2 20k

+V OUT LTC1968 OUT RTN EN

1k

5V

= 1N4148



5V 1µF

A2 LT1227

499Ω*

100Ω 50Ω

RMS CONVERTER

SWITCHED GAIN AMP A = 1, 10

+

1M

S1 S2 GAIN FS OUTPUT TRIM NOTES* LO LO HI HI

LO 1 HI 10 LO 100 HI 1000

1V 0.1V 0.01V 0.001V

TRIM A = 1 TRIM A = 10 TRIM A = 100 NO TRIM

*SET ZERO ADJUSTMENT FOR A2 OUTPUT = 0 VDC WITH INPUT GROUNDED AND S1, S2 HIGH BEFORE TRIMMING

S1 S2

Figure 10. Switched Gain 10MHz (–3dB) Preamplifier Preserves LTC1968’s 500kHz, 1% Error Bandwidth. Decade Ranged Gains (See Table) Allow 1mV Full Scale with 20µV Noise Floor. JFET Input Stage Presents High Input Impedance. AC Coupling, 3rd Order Sallen-Key Filter Maintains 1% Accuracy Down to 10Hz

an106f

AN106-7

Application Note 106 Figure 11 shows preamplifier response to a 1mV input step at a gain of X1000. A2’s output is singularly clean, with trace thickening in the pulse flat portions due to the 20µV noise floor. The 35ns risetime indicates a 10MHz bandwidth.

circuit output, in accordance with the table in the figure. Continue this procedure for the remaining three gains given in the table. A good way to generate the accurate low level inputs required is to set a 1.00VAC level and divide it down with a high grade 50Ω attenuator such as the Hewlett Packard 350D or the Tektronix 2701. It is prudent to verify the attenuator’s output with a precision RMS voltmeter.4

To calibrate this circuit first set S1 and S2 high, ground the input and trim the “zero” adjustment for zero VDC at A2’s output. Next, set S1 and S2 low, apply a 1V, 100kHz input, and trim “A = 1” for unity gain, measured at the

Wideband, Isolated, Quartz Crystal RMS Current Measurement Quartz crystal RMS operating current is critical to longterm stability, temperature coefficient and reliability. Accurate determination of RMS crystal current, especially in low power types, is complicated by the necessity to minimize introduced parasitics, particularly capacitance, which corrupt crystal operation. Figure 12, a form of Figure 10’s wideband amplifier, combines with a commercially available closed core current probe to permit the measurement. An RMS-to-DC converter supplies the RMS value. The quartz crystal test circuit shown in dashed lines exemplifies a typical measurement situation. The Tektronix CT-2 current probe monitors crystal

200mV/DIV

AN106 F11

50ns/DIV

Figure 11. Figure 10’s A2 Output Responds to a 1mV Input Step at X1000 Gain. 35ns Risetime Indicates 10MHz Bandwidth. Trace Thickening in Pulse Flat Portions Represents Noise Floor TEKTRONIX CT-2 CURRENT PROBE 1.5V 1mV/mA 100kHz

4.3k

330k

4See Appendix B for recommendations on RMS voltmeters.

10k

Q1 2N3904

150pF

680pF

CRYSTAL OSCILLATOR TEST CIRCUIT

1N4148s

A1 LT1227

50Ω*

RMS CONVERTER

PRE-AMPLIFIER A = 1000

+

5V

+



5V 1µF

A2 LT1227

499Ω*



IN1 IN2

750Ω*

EN

–5V

5.62Ω*

+V OUT LTC1968 OUT RTN

+ 1µF



GND

64.9Ω* 0.1µF

47µF

OUTPUT 0 – 1V = 0 – 1mA

10k

+ 47µF

A3 LT1077

1N5712

AN106 F12

20Ω 1mA 10k TRIM

0.1µF

*0.25% METAL FILM RESISTOR

+

5V

Figure 12. Figure 10’s Wideband Amplifier Adapted for Isolated RMS Current Measurement of Quartz Crystal Current. FET Input Buffer is Deleted; Current Probe’s 50Ω Impedance Allows Direct Connection to A1. Current Probe Provides Minimal Crystal Loading in Oscillator Test Circuit an106f

AN106-8

Application Note 106 current while introducing minimal parasitic loading (see Figure 14). The probe’s 50Ω termination allows direct connection to A1—Figure 10’s FET buffer is deleted. Additionally, because quartz crystals are not common below 4kHz, A1’s gain does not extend to low frequency. Figure 13 shows results. Crystal drive, taken at Q1’s collector (trace A), causes a 25µA RMS crystal current which is represented at the RMS-to-DC converter input (trace B). The trace enlargement is due to the preamplifier’s 5µA RMS equivalent noise contribution.

A = 0.5V/DIV

B = 50mA/DIV

2ms/DIV

AN106 F13

Figure 13. Crystal Voltage (Trace A) and Current (Trace B) for Figure 12’s Test Circuit. 25µA RMS Crystal Current Measurement Includes Preamplifier 5µA RMS Noise Floor Contribution PARAMETER

CT-1

CT-2

Sensitivity

5mV/mA

1mV/mA

Accuracy

3%

3%

Low Frequency Additional 1% Error BW*

98kHz

6.4kHz

–3dB Bandwidth

25kHz to 1GHz

1.2kHz to 200MHz

Noise Floor with Amplifier Shown*

1µA RMS

5µA RMS

Capacitive Loading

1.5pF

1.8pF

Insertion Impedance at 10MHz



0.1Ω

*As measured. Not vendor specified

Figure 14. Relevant Specifications of Two Tektronix Current Probes. Primary Trade-Off is Low Frequency Error and Sensitivity. Noise Floor is Due to Amplifier Limitations

Figure 14 details characteristics of two Tektronix closed core current probes. The primary trade-off is low frequency error versus sensitivity. There is essentially no probe noise contribution and capacitive loading is notably low. Circuit calibration is achieved by putting 1mA RMS current through the probe and adjusting the indicated trim for a 1V circuit output. To generate the 1mA, drive a 1k, 0.1% resistor with 1VRMS.5

AC Voltage Standard with Stable Frequency and Low Distortion Figure 15 utilizes the RMS-to-DC converter’s stability in an AC voltage standard. Initial circuit accuracy is 0.1% and long-term (6 months at 20°C to 30°C) drift remains within that figure. Additionally, the 4kHz operating frequency is within 0.01% and distortion inside 30ppm. A1 and its power buffer A3 sense across a bridge composed of a 4kHz quartz crystal and an RC impedance in one arm; resistors and an LED driven photocell comprise the other arm. A1 sees positive feedback at the crystals 4kHz resonance, promoting oscillation. Negative feedback, stabilizing oscillation amplitude, occurs via a control path which includes an RMS-to-DC converter and amplitude control amplifier, A5. A5 acts on the difference between A3’s RMS converted output and the LT1009 voltage reference. Its output controls the LED driven photocell to set A1’s negative feedback. RC components in A5’s feedback path stabilize the control loop. The 50k trim sets the optically driven resistor’s value to the point where lowest A3 output distortion occurs while maintaining adequate loop stability. Normally the bridge’s “bottom” would be grounded. While this connection will work, it subjects A1 to common mode swings, increasing distortion due to A1’s finite common mode rejection versus frequency. A2 eliminates this concern by forcing the bridges mid-points, and hence common mode voltage, to zero while not influencing desired circuit operation. It does this by driving the bridge “bottom” to force its input differential to zero. A2’s output swing is 180° out of phase with A3’s circuit output. This action eliminates common mode swing at A1, reducing circuit output distortion by more than an order of magnitude. Figure 16 shows the circuits 1.414VRMS (2.000VPEAK) output in trace A while trace B’s distortion constituents include noise, fundamental related residue and 2F components. The 4kHz crystal is a relatively large structure with very high Q factor. Normally, it would require more than 30 seconds to start and arrive at full regulated amplitude. This is avoided by inclusion of the Q1-LTC201 switch circuitry. At start-up A5’s output goes high, biasing Q1. Q1’s collector goes low, turning on the LTC201. This sets A1’s gain abnormally high, increasing bridge drive and 5This measurement technique has been extended to monitor 32.768kHz

“watch crystal” sub-microampere operating currents. Contact the author for details. an106f

AN106-9

Application Note 106 4kHz OUTPUT 1.414VRMS

–5V 2.5k*

BRIDGE AMPLIFIER

47k

4kHz JCUT

LT1009 2.5V

RMS-TO-DC CONVERTER

10µF

100k* 39k

+

CRYSTAL BRIDGE

+ A3 LT1010

A1

–LT1792

1k*

DISTORTION TRIM

430pF



5V V+ IN1

50k

909Ω*

560k

200Ω OUTPUT SET

470Ω

+

OUT LTC1966

1µF

1k

+

28k*

– A5

+LT1006

IN2 EN RTN GND V – –5V

– A2 LT1792

5V A4 LT1077

AMPLITUDE CONTROL AMPLIFIER

1k

AN106 F15

5V

COMMON MODE SUPPRESSION AMPLIFIER

= 1N4148 5V

1M

510k

*IRC-CAR-6 1% RESISTOR GROUND CRYSTAL CASE

–5V 1/4 LTC201 START-UP

Q1 2N3904 100k

= SILONEX NSL-32SR3

Figure 15. Quartz Stabilized Sine Wave Output AC Reference Has 0.1% Long-Term Amplitude Stability. Frequency Accuracy is 0.01% with <30ppm Distortion. Positive Feedback Around A1 Causes Oscillation at Crystal’s Resonance. A5, Acting on A3’s RMS Amplitude, Supplies Negative Feedback to A1 via Bridge Network, Stabilizing RMS Output Amplitude. Optocoupler Minimizes Feedback Induced Distortion. Q1 Closes Switch During Start-Up, Ensuring Rapid Oscillation Build-Up

A = 2V/DIV

B = 30ppm DISTORTION

100µs/DIV

AN106 F16

Figure 16. A3’s 1.414VRMS (2.000VPEAK), 4kHz Reference Output (Trace A) Shows 30ppm Distortion in Trace B. Distortion Constituents Include Noise, Fundamental Related Residue and 2F Components

accelerating crystal start-up. When the bridge arrives at its operating point A5’s output drops to a lower value, Q1 and the LTC201 switch go off, and the circuit transitions into normal operation. Start-up time is several seconds. The circuit requires trimming for amplitude accuracy and lowest distortion. The distortion trim is made first. Adjust

the trim for minimal output distortion as measured on a distortion analyzer. Note that the absolute lowest level of distortion coincides with the point where control loop gain is just adequate to maintain oscillation. As such, find this point and retreat from it into the control loop’s active region. This necessitates giving up about 5ppm distortion, but 30ppm is achievable with good control loop stability. Output amplitude is trimmed with the indicated adjustment for exactly 1.414VRMS (2.000VPEAK) at the circuit output. RMS Leveled Output Random Noise Generator Figure 17 uses the RMS-to-DC converter in a leveled output random noise generator. Noise diode D1 AC biases A1, operating at a gain of 2.6 A1’s output feeds a 1kHz to 500kHz switch selectable lowpass filter. The filter output biases the variable gain amplifier, A2-A3. A2-A3, contained 6See Appendix C “Symmetrical White Gaussian Noise,” guest written by Ben Hessen-Schmidt of Noise Com, Inc. for turorial on noise and noise diodes.

an106f

AN106-10

Application Note 106 FILTER NOISE DIODE 10µF

75k

75k

NOISE DIODE PREAMP

1µF

+

15V 1µF

NC103

10kHz

160Ω

A1 LT1220

1k

1kHz

0.1µF

–3dB

0.01µF



1k

7VDC TO 10VDC +NOISE

100kHz

0.002µF

500kHz

500pF

500kHz

1k

RMS AMPLITUDE STABILIZED NOISE OUTPUT

FLAT

1µF TO ALL +VZ POINTS

VARIABLE GAIN AMPLIFIER

1N4689 5.1V

15V

LT1228

+ –

+ 100pF 900Ω

A2 ISET

0.01µF



510Ω +VZ

GAIN CONTROL AMPLIFIER 3k

10k 10k

OUT LTC1968 IN2 OUT RTN EN GND

+ 1N5712

A4 1/2 LT1013



5Ω 10µF

150k 0.1µF

+V IN1

A3

0.1µF

1µF

RMS CONVERTER

1.5k

1µF

475k* AN106 F17

1.1M*



–15V

A5 1/2 LT1013

INTERNAL

+ 1N4148

1M

10k

909k*

Q1 TPO610L

15V

4.7k

EXTERNAL 510k

SOFT-START

AMPLITUDE ADJUST

LT1004-1.2V

*1% METAL FILM RESISTOR CONNECTIONS INSIDE DASHED LINES WITHIN A SINGLE IC NC103 = NOISE COM 10µF = WIMA MKS-2

40.2k*

0V TO 1V +VZ

1M

0.33µF

Figure 17. An RMS Levelled Output Random Noise Generator. Amplified (A1) Diode Noise Is Filtered, Variable Gain Amplified (A2-A3) and RMS Converted. Converter Output Feeds Back to A5 Gain Control Amplifier, Closing RMS Stabilized Loop. Output Amplitude, Taken at A3, is Settable

on one chip, include a current controlled transconductance amplifier (A2) and an output amplifier (A3). This stage takes AC gain, biases the LTC1968 RMS-to-DC converter and is the circuit’s output. The RMS converter output at A4, feeds back to gain control amplifier A5, which compares the RMS value to a variable portion of the 5.1V zener potential. A5’s output sets A2’s gain via the 3k resistor, completing a control loop to stabilize noise RMS output amplitude. The RC components in A5’s local feedback path

stabilize this loop. Output amplitude is variable by the 10k potentiometer; a switch permits external voltage control. Q1 and associated components, a soft-start circuit, prevent output overshoot at power turn-on. Figure 18 shows circuit output noise in the 10kHz filter position; Figure 19’s spectral plot reveals essentially flat RMS noise amplitude over a 500kHz bandwidth.

an106f

AN106-11

AMPLITUDE VARIANCE –3dB/DIV

Application Note 106

2V/DIV

0

Figure 18. Figure 17’s Output in the 10kHz Filter Position

INPUT 0.4VRMS TO 5VRMS 10k

100

150

200 250 300 350 FREQUENCY (kHz)

400

450

500

AN106 F19

Figure 19. Amplitude vs Frequency for the Random Noise Generator is Essentially Flat to 500kHz. NC103 Diode Contributes Even Noise Spectrum Distribution; RMS Converter and Loop Stabilize Amplitude. Sweep Time is 2.8 Minutes, Resolution Bandwidth, 100Hz

AN106 F18

5ms/DIV

50

VARIABLE GAIN AMPLIFIER

+

100Ω

+

A1 1/2 LT1228

300Ω



OUTPUT BUFFER

1µF

A2 1/2 LT1228

+



470Ω

10k

RMS LEVELLED OUTPUT 0VRMS TO 0.5VRMS

A3 LT1220



10Ω

1k

1µF

RMS CONVERTER 0.15µF



A5 1/2 LT1013

+

100k*

A4 1/2 LT1013

100k*



5V

V+ IN1 C1 LTC1968 OUT RTN IN2 GND EN OUT

1µF

+ 10k

4.7k

GAIN CONTROL AMPLIFIER

–5V 13.3k* 10k

LT1004 1.2V REFERENCE

EXT INPUT 0V TO –0.5V OUTPUT 0VRMS TO 0.5VRMS LEVEL OUTPUT 0VRMS TO 0.5VRMS

5V 10k

0.1µF AN106 F20

*0.1% METAL FILM RESISTOR CONNECTIONS INSIDE DASHED LINES ARE WITHIN A SINGLE IC

Figure 20. RMS Amplitude Level Control Uses Figure 17’s Gain Control Loop. A1-A3 Provide Variable Gain to Input. RMS Converter Feeds Back to A5 Gain Control Amplifier, Closing Amplitude Stabilization Loop. Variable Reference Permits Settable, Calibrated RMS Output Amplitude Independent of Input Waveshape

RMS Amplitude Stabilized Level Controller Figure 20 borrows the previous circuit’s gain control loop to stabilize the RMS amplitude of an arbitrary input waveform. The unregulated input is applied to variable gain amplifier A1-A2 which feeds A3. DC coupling at A1-A2 permits passage of low frequency inputs. A3’s output is

taken by RMS-to-DC converter C1-A4, which feeds the A5 gain control amplifier. A5 compares the RMS value to a variable reference and biases A1, closing a gain control loop. The 0.15µF feedback capacitor stabilizes this loop, even for waveforms below 100Hz. This feedback action stabilizes output RMS amplitude despite large variations an106f

AN106-12

Application Note 106 in input amplitude while maintaining waveshape. Desired output level is settable with the indicated potentiometer or an external control voltage may be switched in. Figure 21 shows output response (trace B) to abrupt reference level set point changes (trace A). The output settles within 60 milliseconds for ascending and descending transitions. Faster response is possible by decreasing A5’s compensation capacitor, but low frequency waveforms

would not be processable. Similar considerations apply to Figure 22’s response to an input waveform step change. Trace A is the circuit’s input and trace B its output. The output settles in 60 milliseconds due to A5’s compensation. Reducing compensation value speeds response at the expense of low frequency waveform processing capability. Specifications include 0.1% output amplitude stability for inputs varying from 0.4VRMS to 5VRMS, 1% set point accuracy, 0.1kHz to 500kHz passband and 0.1% stability for 20% power supply deviation. Note: This Application Note was derived from a manuscript originally prepared for publication In EDN magazine.

A = 0.5V/DIV A = 2V/DIV B = 1V/DIV

B = 1V/DIV 20ms/DIV

AN106 F21

10ms/DIV

Figure 21. Amplitude Level Control Response (Trace B) to Abrupt Reference Changes (Trace A). Settling Time is Set by A5’s Compensation Capacitor, Which Must be Large Enough to Stabilize Loop at Lowest Expected Input Frequency

REFERENCES 1. Hewlett-Packard Company, “1968 Instrumentation. Electronic—Analytical—Medical,” AC Voltage Measurement, Hewlett-Packard Company, 1968, pp. 197-198. 2. Sheingold, D. H. (editor), “Nonlinear Circuits Handbook,” 2nd Edition, Analog Devices, Inc., 1976. 3. Lambda Electronics, Model LK-343A-FM Manual. 4. Grafham, D. R., “Using Low Current SCRs,” General Electric AN200.19. Jan. 1967. 5. Williams, J., “Performance Enhancement Techniques for Three-Terminal Regulators,” Linear Technology Corp. AN-2. August, 1984. “SCR Preregulator,” pp. 3-6. 6. Williams, J., “High Efficiency Linear Regulators,” Linear Technology Corporation, Application Note 32, “SCR Preregulator.” March 1989, pp. 3-4.

AN106 F22

Figure 22. Amplitude Level Control Output Reacts (Trace B) to Input Step Change (Trace A). Slow Loop Compensation Allows Overshoot But Output Settles Cleanly

7. Williams, J., “High Speed Amplifier Techniques,” Linear Technology Corporation, Application Note 47, “Parallel Path Amplifiers,” August 1991, pp. 35-37. 8. Williams, J., “Practical Circuitry for Measurement and Control Problems,” Broadband Random Noise Generator,” “Symmetrical White Gaussian Noise,” Appendix B, Linear Technology Corporation, Application Note 61, August 1994, pp.24-26, pp. 38-39. 9. Williams, J., “A Fourth Generation of LCD Backlight Technology,” “RMS Voltmeters,” Linear Technology Corporation, Application Note 65, November 1995, pp. 82-83. 10. Meacham, L. A., “The Bridge Stabilized Oscillator,” Bell System Technical Journal, Vol. 17, p. 574, October 1938. 11. Williams, Jim, “Bridge Circuits—Marrying Gain and Balance,” Linear Technology Corporation, Application Note 43, June, 1990. an106f

AN106-13

Application Note 106 APPENDIX A RMS-TO-DC CONVERSION Joseph Petrofsky Definition of RMS RMS amplitude is the consistent, fair and standard way to measure and compare dynamic signals of all shapes and sizes. Simply stated, the RMS amplitude is the heating potential of a dynamic waveform. A 1VRMS AC waveform will generate the same heat in a resistive load as will 1V DC. See Figure A1. Mathematically, RMS is the “Root of the Mean of the Square”: VRMS = V 2 1V DC

+ –

R

1V ACRMS

R

1V (AC + DC) RMS

R

SAME HEAT

AN106 FA1

The last two entries of Table A1 are chopped sine waves as is commonly created with thyristors such as SCRs and Triacs. Figure A2a shows a typical circuit and Figure A2b shows the resulting load voltage, switch voltage and load currents. The power delivered to the load depends on the firing angle, as well as any parasitic losses such as switch “ON” voltage drop. Real circuit waveforms will also typically have significant ringing at the switching transition, dependent on exact circuit parasitics. Here, “SCR Waveforms” refers to the ideal chopped sine wave, though the LTC1966/LTC1967/LTC1968 will do faithful RMS-to-DC conversion with real SCR waveforms as well. The case shown is for Θ = 90°, which corresponds to 50% of available power being delivered to the load. As noted in Table A1, when Θ = 114°, only 25% of the available power is being delivered to the load and the power drops quickly as Θ approaches 180°. With an average rectification scheme and the typical calibration to compensate for errors with sine waves, the RMS level of an input sine wave is properly reported; it is only with a non-sinusoidal waveform that errors occur. Because of this calibration, and the output reading in VRMS, the term True-RMS got coined to denote the use of an actual RMS-to-DC converter as opposed to a calibrated average rectifier.

Figure A1 + VLOAD –

Alternatives to RMS Other ways to quantify dynamic waveforms include peak detection and average rectification. In both cases, an average (DC) value results, but the value is only accurate at the one chosen waveform type for which it is calibrated, typically sine waves. The errors with average rectification are shown in Table A1. Peak detection is worse in all cases and is rarely used. Table A1. Errors with Average Rectification vs True RMS WAVEFORM Square Wave Sine Wave Triangle Wave SCR at 1/2 Power, Θ = 90° SCR at 1/4 Power, Θ = 114°

VRMS 1.000 1.000 1.000 1.000

AVERAGE RECTIFIED (V) 1.000 0.900 0.866 0.637

1.000

0.536

AC MAINS

+

ILOAD

VLINE

CONTROL



+ –

VTHY

AN106 FA2a

Figure A2a VLINE Θ VLOAD VTHY

ERROR* 11% *Calibrate for 0% Error –3.8% –29.3%

ILOAD AN106 FA2b

Figure A2b

–40.4% an106f

AN106-14

Application Note 106 How an RMS-to-DC Converter Works Monolithic RMS-to-DC converters use an implicit computation to calculate the RMS value of an input signal. The fundamental building block is an analog multiply/divide used as shown in Figure A3. Analysis of this topology is easy and starts by identifying the inputs and the output of the lowpass filter. The input to the LPF is the calculation from the multiplier/divider; (VIN)2/VOUT. The lowpass filter will take the average of this to create the output, mathematically: VOUT

⎛ (V )2 ⎞ = ⎜ IN ⎟ , ⎜⎝ VOUT ⎟⎠

VIN VOUT

∆-Σ REF

LPF

VOUT AN106 FA4

Figure A4. Topology of the LTC1966/LTC1967/LTC1968

( ) 2

The ΔΣ modulator has a single-bit output whose average duty cycle (⎯D) will be proportional to the ratio of the input signal divided by the output. The ΔΣ is a 2nd order modulator with excellent linearity. The single-bit output is used to selectively buffer or invert the input signal. Again, this is a circuit with excellent linearity, because it operates at only two points: ±1 gain; the average effective multiplication over time will be on the straight line between these two points. The combination of these two elements again creates a lowpass filter input signal equal to (VIN)2/VOUT, which, as shown above, results in RMS-to-DC conversion.

((V ) ) , and = 2

IN

VOUT

(VOUT )2 = (VIN)2, or (VIN)2 = RMS (VIN) (VIN )2 VOUT VIN



±1

⎛ (V )2 ⎞ (VIN) , so ⎜ IN ⎟ = VOUT ⎜⎝ VOUT ⎟⎠

VOUT =

The LTC1966/LTC1967/LTC1968 use a completely new topology for RMS-to-DC conversion, in which a ΔΣ modulator acts as the divider, and a simple polarity switch is used as the multiplier as shown in Figure A4.

VIN

Because VOUT is DC,

VOUT

How the LTC1966/LTC1967/LTC1968 RMS-to-DC Converters Work

× ÷

LPF

VOUT AN106 FA3

Figure A3 RMS-to-DC Converter with Implicit Computation

Unlike the prior generation RMS-to-DC converters, the LTC1966/LTC1967/LTC1968 computation does NOT use log/antilog circuits, which have all the same problems, and more, of log/antilog multipliers/dividers, i.e., linearity is poor, the bandwidth changes with the signal amplitude and the gain drifts with temperature.

The lowpass filter performs the averaging of the RMS function and must be a lower corner frequency than the lowest frequency of interest. For line frequency measurements, this filter is simply too large to implement on-chip, but the LTC1966/LTC1967/LTC1968 need only one capacitor on the output to implement the lowpass filter. The user can select this capacitor depending on frequency range and settling time requirements. This topology is inherently more stable and linear than log/antilog implementations primarily because all of the signal processing occurs in circuits with high gain op amps operating closed loop. Note that the internal scalings are such that the ΔΣ output duty cycle is limited to 0% or 100% only when VIN exceeds ±4 • VOUT.

an106f

AN106-15

Application Note 106 Linearity of an RMS-to-DC Converter Linearity may seem like an odd property for a device that implements a function that includes two very nonlinear processes: squaring and square rooting. However, an RMS-to-DC converter has a transfer function, RMS volts in to DC volts out, that should ideally have a 1:1 transfer function. To the extent that the input to output transfer function does not lie on a straight line, the part is nonlinear. A more complete look at linearity uses the simple model shown in Figure A5. Here an ideal RMS core is corrupted by both input circuitry and output circuitry that have imperfect transfer functions. As noted, input offset is introduced in the input circuitry, while output offset is introduced in the output circuitry. Any nonlinearity that occurs in the output circuity will corrupt the RMS in to DC out transfer function. A nonlinearity in the input circuitry will typically corrupt that transfer function far less simply because with an AC input, the RMS-to-DC conversion will average the nonlinearity from a whole range of input values together.

INPUT

INPUT CIRCUITRY • VIOS • INPUT NONLINEARITY

But the input nonlinearity will still cause problems in an RMS-to-DC converter because it will corrupt the accuracy as the input signal shape changes. Although an RMS-to-DC converter will convert any input waveform to a DC output, the accuracy is not necessarily as good for all waveforms as it is with sine waves. A common way to describe dynamic signal wave shapes is Crest Factor. The crest factor is the ratio of the peak value relative to the RMS value of a waveform. A signal with a crest factor of 4, for instance, has a peak that is four times its RMS value. Because this peak has energy (proportional to voltage squared) that is 16 times (42) the energy of the RMS value, the peak is necessarily present for at most 6.25% (1/16) of the time. The LTC1966/LTC1967/LTC1968 perform very well with crest factors of 4 or less and will respond with reduced accuracy to signals with higher crest factors. The high performance with crest factors less than 4 is directly attributable to the high linearity throughout the LTC1966/ LTC1967/LTC1968.

IDEAL RMS-TO-DC CONVERTER

OUTPUT CIRCUITRY • VOOS • OUTPUT NONLINEARITY

OUTPUT AN106 FA5

Figure A5. Linearity Model of an RMS-to-DC Converter

an106f

AN106-16

Application Note 106 APPENDIX B AC Measurement and Signal Handling Practice Accurate AC measurement requires trustworthy instrumentation, proper signal routing technique, parasitic minimization, attention to layout and care in component selection. The text circuits DC-500kHz, 1% error bandwidth seems benign, but unpleasant surprises await the unwary. An accurate RMS voltmeter is required for serious AC work. Figure B1 lists types used in our laboratory. These are high grade, specialized instruments specifically intended for precise RMS measurement. All are thermally based1. The first three entries, general purpose instruments with many ranges and features, are easily used and meet almost all AC measurement needs. The last entry is more of a component than an instrument. The A55 series of “thermal converters” provide millivolt level outputs for various inputs. Typical input ranges are 0.5VRMS, 1VRMS, 2VRMS and 5VRMS and each converter is supplied with individual calibration data. They are somewhat cumbersome to use and easily destroyed but are highly accurate. Their primary use is as reference standards to check other instrument’s performance. AC signal handling for high accuracy is a broad topic, involving a considerable degree of depth. This forum must suffer brevity, but some gossip is possible.

Layout is critical. The most prevalent parasitic in AC measurement is stray capacitance. Keep signal path connections short and small area. A few picofarrads of coupling into a high impedance node can upset a 500kHz, 1% accuracy signal path. To the extent possible, keep impedances low to minimize parasitic capacitive effects. Consider individual component parasitics and plan to accommodate them. Examine effects of component placement and orientation on the circuit board. If a ground plane is in use it may be necessary to relieve it in the vicinity of critical circuit nodes or even individual components. Passive components have parasitics that must be kept in mind. Resistors suffer shunt capacitance whose effects vary with frequency and resistor value. It is worth noting that different brands of resistors, although nominally similar, may exhibit markedly different parasitic behavior. Capacitors in the signal path should be used so that their outer foil is connected to the less sensitive node, affording some relief from pick-up and stray capacitance induced effects. Some capacitors are marked to indicate the outer foil terminal, others require consulting the data sheet or vendor contact. Avoid ceramic capacitors in the signal path. Their piezoelectric responses make them unsuitable for precision AC circuitry. In general, any component in the signal path should be examined in terms of its potential parasitic contribution. 1See references 1 and 2 for details on thermally based RMS-to-DC

conversion. MODEL

MANUFACTURER

1V RANGE

INPUT

BANDWIDTH

3400A/3400B

Hewlett-Packard

1%

AC

10MHz/20MHz

COMMENTS

3403C

Hewlett-Packard

0.2%

AC, AC + DC

100MHz

Digital Display, 1µV Sensitivity (2MHz BW), dB Ranges, Relative dB

8920/8921A

Fluke

0.7%

AC, AC + DC

20MHz

Digital Display, 10µV Sensitivity (2MHz BW), dB Ranges, Relative dB

A55

Fluke

0.05%

AC + DC

50MHz

Set of Individually Calibrated Thermal Converters. Reference Standards. Not for General Purpose Measurement

Metered Instrument. Most Common RMS Voltmeter

Figure B1. Precision Wideband RMS Voltmeters Useful for AC Measurement. All are Thermally Based, Permitting High Accuracy and Wide Bandwidth Independent of Input Waveshape. A55 Reference Standards, Although Unsuitable for General Purpose Measurement, Have Best Accuracy

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AN106-17

Application Note 106 Active components, such as amplifiers, must be treated as potential error sources. In particular, as stated in the text, ensure that there is enough open loop gain at the frequency of interest to assure needed closed loop gain accuracy. Margins of 100:1 are not unreasonable. Keep feedback values as low as possible to minimize parasitic effects. Route signals to and from the circuit board coaxially and at low impedance, preferably 50Ω, for best results. In 50Ω systems, remember that terminators and attenuators

APPENDIX C by Ben Hessen-Schmidt, NOISE COM, INC. White noise provides instantaneous coverage of all frequencies within a band of interest with a very flat output spectrum. This makes it useful both as a broadband stimulus and as a power-level reference. Symmetrical white Gaussian noise is naturally generated in resistors. The noise in resistors is due to vibrations of the conducting electrons and holes, as described by Johnson and Nyquist.1 The distribution of the noise voltage is symmetrically Gaussian, and the average noise voltage is: (1)

where: k = 1.38E–23 J/K (Boltzmann’s constant) T = temperature of the resistor in Kelvin f = frequency in Hz h = 6.62E–34 Js (Planck’s constant) R(f) = resistance in ohms as a function of frequency p(f) =

[

hf

]

kT exp(hf/kT) − 1

This all seems painful but is an essential part of achieving 1% accurate, 500kHz signal integrity. Failure to observe the precautions listed above risks degrading the RMSto-DC converters system level performance.

p(f) is close to unity for frequencies below 40GHz when T is equal to 290°K. The resistance is often assumed to be independent of frequency, and Údf is equal to the noise bandwidth (B). The available noise power is obtained when the load is a conjugate match to the resistor, and it is:

Symmetrical White Gaussian Noise

Vn = 2 kT ∫ R(f) p(f) df

have tolerances that can corrupt a 1% amplitude accuracy measurement. Verify such terminator and attenuator tolerances by measurement and account for them when interpreting measurement results. Similarly, verify the accuracy of any associated instruments 50Ω input or output impedance and account for deviations.

(2)

2

V N = n = kTB 4R

(3)

where the “4” results from the fact that only half of the noise voltage and hence only 1/4 of the noise power is delivered to a matched load. Equation 3 shows that the available noise power is proportional to the temperature of the resistor; thus it is often called thermal noise power, Equation 3 also shows that white noise power is proportional to the bandwidth. An important source of symmetrical white Gaussian noise is the noise diode. A good noise diode generates a high level of symmetrical white Gaussian noise. The level is often specified in terms of excess noise ratio (ENR).

(

)

ENR in dB = 10Log

(Te − 290) 290

(4)

Te is the physical temperature that a load (with the same impedance as the noise diode) must be at to generate the same amount of noise. 1See “Additional Reading” at the end of this section.

an106f

AN106-18

Application Note 106 The ENR expresses how many times the effective noise power delivered to a non-emitting, nonreflecting load exceeds the noise power available from a load held at the reference temperature of 290°K (16.8°C or 62.3°F). The importance of high ENR becomes obvious when the noise is amplified, because the noise contributions of the amplifier may be disregarded when the ENR is 17dB larger than the noise figure of the amplifier (the difference in total noise power is then less than 0.1dB). The ENR can easily be converted to noise spectral density in dBm/Hz or µV/√Hz by use of the white noise conversion formulas in Table 1. Table 1. Useful White Noise Conversion dBm dBm dBm dBm/Hz dBm/Hz

= = = = =

dBm/Hz + 10log (BW) 20log (Vn) – 10log(R) + 30dB 20log(Vn) + 13dB for R = 50Ω 20log(µVn√Hz) – 10log(R) – 90dB –174dBm/Hz + ENR for ENR > 17dB

When amplifying noise it is important to remember that the noise voltage has a Gaussian distribution. The peak voltages of noise are therefore much larger than the average or RMS voltage. The ratio of peak voltage to RMS voltage is called crest factor, and a good crest factor for Gaussian noise is between 5:1 and 10:1 (14 to 20dB). An amplifier’s 1dB gain-compression point should therefore be typically 20dB larger than the desired average noise-output power to avoid clipping of the noise. For more information about noise diodes, please contact NOISE COM, INC. at (973) 386-9696. Additional Reading 1. Johnson, J.B, “Thermal Agitation of Electricity in Conductors,” Physical Review, July 1928, pp. 97-109. 2. Nyquist, H. “Thermal Agitation of Electric Charge in Conductors,” Physical Review, July 1928, pp. 110-113.

an106f

Information furnished by Linear Technology Corporation is believed to be accurate and reliable. However, no responsibility is assumed for its use. Linear Technology Corporation makes no representation that the interconnection of its circuits as described herein will not infringe on existing patent rights.

AN106-19

Application Note 106

an106f

AN106-20

Linear Technology Corporation

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