EMI Testing Using Spectrum Analyzers vs. Test Receivers Vic Hudson Rohde&Schwarz IEEE-LI Presentation Topic of the Meeting Description ⇒ Spectrum Analyzers (SA) ⇒ Test Receivers (TR) Uses and descriptions of each Reasons for using either or both units Advantages and disadvantages Making accurate measurements Q&A Who uses what ? ⇒ Spectrum Analyzers (SA) ⇒ Test Receivers (TR) Commercial, MIL-STD or Automotive? Software or front panel ? Novice, Capable, Fluent or Expert ? Overview EMI Equipment in general ⇒ Spectrum Analyzers (SA) ⇒ Test Receivers (TR) Two Most common tools are SA / TR Spectrum Analyzers for EMI Spectrum Analyzers for EMI Level [dBµV] 120 100 80 60 40 20 0 -20 30M 50M 70M 100M 200M 300M 500M 700M 1G SA Settings for EMI measurements - Span, Reference Level, RBW, VBW and detector - Span is the Stop – Start Frequency - Ref Level is typically the Highest point SA can measure - Coupling with VBW usually some multiple of the RBW - RBW usually selected per required standard Spectrum Analyzers for EMI Reasons for Using SA for EMI Measurements ⇒ Versatility: Wide range of uses ⇒ Familiarity ⇒ Speed … real or imagined ⇒ Price … real or imagined Spectrum Analyzers for EMI Level [dBµV] 120 100 80 60 40 20 0 -20 30M 50M 70M 100M 200M 300M 500M 700M SA setup for EMI Example - Set Span, RBW and detector - Span of 970 MHz / 500 points = 2 MHz resolution ! - x samples within RBW are stored - samples are weighted by some detector - Common EMI detectors are QP, Ave, Pk, RMS 1G Spectrum Analyzers for EMI Question - What was wrong with the previous setup? Answer - Frequency and amplitude accuracy depend on many samples falling within each RBW filter width. - set this parameter with frequency span Spectrum Analyzers for EMI Level [dBµV] 120 100 80 60 40 20 0 -20 30M 50M 70M 100M 200M 300M 500M Issue # 1 Subranging Required - Span of 970 MHz / 500 = 2 MHz resolution - If using 120 KHz RBW, CISPR recommends 60 KHz sample points (17 x finer than 1 MHz) - Solution: subrange in the span 700M 1G Spectrum Analyzers for EMI Level [dBµV] 120 100 80 60 40 20 0 -20 30M 50M 70M 100M 200M 300M 500M Subrange Issue Revisited - Per CISPR ½ RBW recommendation - For unit with 500 point unit = 30 MHz Spans - Solution: 970 MHz Span = 32 Spans required! 700M 1G Spectrum Analyzers for EMI Frequency Accuracy of SA - SA resolution is far too course for EMI without subranging the CISPR span - SA frequency accuracy when exploring peaks influenced by Span, RBW, VBW, marker accuracy Amplitude Accuracy of SA - 6 dB (EMI) filters vs. 3 dB QP and AVE detector times are observed Data correction for system transducers EUT specific timing issues are considered Subranges set properly for sample # RF and IF stages are not overloaded Spectrum Analyzers for EMI Issue # 2 Proper QP and Average Detectors ⇒ Is QP / AVE Detector CISPR-16-1 Compliant? Issue # 3 Correct CISPR RBW Filters - Typical Typical SA SA have have 1-3-5 1-3-5 Steps Steps RBW RBW -- EMI EMI Filters Filters ..200 ..200 Hz, Hz, 99 kHz, kHz, 120 120 kHz kHz Spectrum Analyzers for EMI Issue # 4 Dwell Time - Sweep Time vs. Span - Max Hold Issue # 5 Lack of Preselection/ Overload Protection -EMI Can be very high – wide -Real Signal or not? -How to protect your measurement/ SA -Verify RF and IF stages are not overloaded Spectrum Analyzers for EMI Has to be a better way! Test Receivers for EMI Test Receivers for EMI What exactly is a EMI Test Receiver? - Fixed Tuned receiver versus Swept Tuned - Built-in Firmware for doing only EMI Test Receivers for EMI Controls for Recievers - Frequency Span (start / stop) - RBW Filter and detector - DWELL TIME at each measurement point - FREQUENCY INCRIMENT (step size) - TR adjusts sample x depending on span - x is often 16,000 – 100,000+ - Span / x = frequency resolution Test Receivers for EMI 120 100 80 60 40 20 0 30M 57.00 50M 70M 100M 200M 300M 500M 700M 1G Level [dBµV] 50.00 40.00 30.00 20.00 10.00 0.00 79.94M 85M 90M 95M Frequency [Hz] 100M 109.63M Test Receivers for EMI EMI TR Advantages - Measurement Points - Tune and Dwell Time method - DWELL TIME at each measurement point - FREQUENCY INCRIMENT (step size) - TR adjusts sample x depending on span - EMI Specificity - Automatic Control – ATT, Preselection, Filters Test Receivers for EMI Conclusion ⇒ TR incorporates EMI control parameters - STEP SIZE between measurement points - DWELL TIME at each measurement point - # of sample points as necessary for accuracy Time Penalty ? - Time dependant on detector and EUT, not measurement speed of instruments Best Instrument for EMI? Pros and Cons of Each - SA is faster for initial preview - SA can also be used for RX and TX measurements - TR has little little use use outside outside EMI, EMI, expensive expensive unit for one use - SA subranging negates any speed advantage over TR for EMI - SA amplitude accuracy easily skewed by improper settings and interpretation Which one to use? Use SA or TR for hit list Use SA or TR for maximization Att 30 dB AUTO FREQUENCY LEVEL QPK 10 dBµV 20 100 MHz 60 200 MHz 30 300 MHz RBW 120 kHz MT 1 s PREAMP ON 931.9200000 MHz dBµV 40 400 MHz 50 500 MHz 60 600 MHz 70 700 MHz 800 MHz 80 90 900 MHz 50 FCC15RB 1 PK CLRWR SGL 40 30 20 10 TR is optimum for final (dwell time & auto attenuator) 0 -10 -20 30 MHz Date: 1 GHz 8.SEP.2003 14:13:12 Making accurate measurements Overload protection Detectors for EMI RBW Filters for EMI Preamps Accurate Measurement Background Dynamic Range of SA / TR is ~ 160 dB EMC engineers don’t know what signals they are looking for initially Accuracy killers - Overloads - Incorrect detector settings - PRF & directivity of EUT emissions - Transducer correction factors Samples and pixels samples Ref Level detector detector peak peak QP QP Ave Min Peak Display Pixel n amplitude amplitude 0dB Ave Min Peak Display Pixel n + 1 Sample Points Example 120 100 80 60 40 20 0 30M 57.00 50M 70M 100M 200M 300M 500M 700M 1G Level [dBµV] 50.00 40.00 30.00 20.00 10.00 0.00 79.94M 85M 90M 95M Frequency [Hz] 100M Example: TR vs. SA sample points 109.63M RF Overload Example MARKER 1 496 MHz Ref 0 dBm 1 * Att RBW 3 MHz VBW 10 MHz SWT 10 ms 10 dB 0 Marker 2 [T1 ] -48.80 996.000000000 Marker 3 [T1 ] -48.60 1.500000000 -10 1 SA AVG Marker 1 [T1 ] 3.03 dBm 496.000000000 MHz -20 dBm MHz dBm GHz -30 -40 2 3 -50 -60 -70 -80 -90 -100 Center 1 GHz Date: 23.JUN.2004 200 MHz/ 20:33:37 Example: amplified signal at 500 MHz Span 2 GHz A IF Overload Example RF ATTENUATION 10 dB Ref 0 dBm * Att 10 dB 1 RBW 3 MHz VBW 10 MHz SWT 5 ms Marker 1 [T1 ] 6.13 dBm 502.053410569 MHz 0 OVLD 1 AP CLRWR A -10 -20 -30 -40 -50 -60 -70 -80 -90 -100 Center 502.0534106 MHz Date: 23.JUN.2004 99.02160153 MHz/ 20:55:20 Example: +6 dBm Pulse Span 990.2160153 MHz Preselection Filtering Preselector is a “tracking” RF filter - ALL RF power (noise & signals) go into mixer - high amplitude signals outside span can influence amplitude and may be aliased Cure: Suppress signals before RF or IF - SA may not warn of RF or IF overdrive - IF overload won’t show on display - Signals outside display ruin amplitude reading Overdrive and Preselection MARKERFREQUENCY START 1 1.000272533 600 MHz Ref 0 dBm GHz * Att 20 dB RBW VBW SWT 3 MHz 10 MHz 10 ms Marker [T1 ] -43.41 -62.14 1.000272533 Marker [T1 ] -54.36 -54.58 -63.57 1.501204189 0 -10 1 PK * CLRWR 1 dBm GHz 2 dBm GHz A -20 -30 -40 1 PS 1 -50 2 1 -60 2 2 -70 -80 -90 -100 Start Date: 400 600 MHz 8.SEP.2003 141.6135906 121.6135906 MHz/ Stop 13:04:47 13:03:46 13:04:13 Example: +10 dBm signal at 500 MHz 1.816135906 GHz PRF and Detectors EUT / Detector dwell time requirements - Must capture “worst case” emissions of EUT - Cycle time and pulse repetition frequency may require extended dwell in each subrange - Some detectors require extended dwell settings (ave, QP) Detector Settings QuasiPeak ???? ⇒ QP is an attempt to quantify a signals Impact on a radio receiver (annoyance) - Factors: amplitude, frequency, width, PRF Quasipeak restrictions - Dwell time (per step or subrange) > 600 mS - PRF issues increase dwell time requirements Detector Settings Peak Detector - Peak gives “worst case” - Safest detector; Fast enough to see signals even with incorrect RBW or dwell settings Average Detector - Above 1 GHz for FCC - dwell for ~ 100 mS - Watch RBW (1MHz or 120 KHz) Detector Settings Example Ref -20 dBm Att 10 RBW VBW SWT dB 120 kHz 1 MHz 175 ms Marker 1 [T1 ] -56.89 -76.57 -49.64 280.000000000 dBm MHz -20 -20 A A -30 -30 1 AV 1 QP RM * * CLRWR CLRWR -40 -40 1 -50 -50 1 -60 -60 -70 -70 1 -80 -80 -90 -90 -100 -100 -110 -110 -120 -120 Start Start Date: Date: 0 0 Hz Hz 23.JUN.2004 23.JUN.2004 50 50 MHz/ MHz/ 21:45:04 21:44:41 21:44:15 Example: -40 dBm signal at 280 MHz Stop Stop 500 500 MHz MHz Transducers and PRF Transducer correction - CISPR needed a way to eliminate effects of chambers, antennas and cable losses - Standards require normalization of these effects to compare results to limit line EUT dwell time requirements - Must capture “worst case” emissions of EUT - Cycle time and pulse repetition frequency may require extended dwell in each subrange Conclusion TR vs. SA Span Subranges step size resolution dwell time overloading preselection RF & IF Overloads RF -> Harmonics Attenuator Preamps IF -> If overload flag Ref Level amplify at antenna know linear region system check (attenuator) static below 1gz Conclusion Go Yankees… Enjoy the Game! Vic Hudson Rohde&Schwarz EMC Systems Ph 847 612-0618 Vic.Hudson@rohde-schwarz.com