Why are the ripple noise measurements of different oscilloscopes always different?

When measuring ripple and noise on the same power supply using different oscilloscopes, it's common to observe variations in the results. Even the use of different probes can significantly affect the readings. But why does this happen? Let’s explore the reasons behind these differences and how to achieve more accurate measurements.

Distinguishing Ripple from Noise

Ripple

Ripple is an AC component that appears on the DC output of a switching power supply. It arises due to the high-frequency switching action of the power transistor. During each switching cycle, energy is transferred from the input to the output capacitor, causing a charging and discharging process that results in voltage fluctuations. The frequency of this ripple matches the switching frequency of the power supply. The amplitude of ripple is typically measured as the peak-to-peak value between the highest and lowest points of the AC component.

Noise

Noise, on the other hand, is a high-frequency disturbance caused by the rapid switching of the power supply components. It is generated during the turn-on and turn-off transitions of the switch and has a much higher frequency than the ripple. The magnitude of the noise is influenced by various factors, including the power supply topology, transformer winding design, parasitic elements in the circuit, and external electromagnetic interference. Proper PCB layout and shielding are also crucial in minimizing noise.

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Understanding the difference between ripple and noise is essential before moving on to measurement techniques. Now, let’s look at why different oscilloscopes may yield different results.

Why Different Oscilloscopes Give Different Results

If you notice significant differences in your measurements, there could be several reasons:

  1. Not using a 20MHz bandwidth limit: Higher bandwidths allow more high-frequency noise to pass through, which can distort the measured ripple and noise values.
  2. Improper grounding: Using a long ground lead or not using a grounding spring can introduce unwanted electromagnetic interference into the measurement circuit.
  3. Uncalibrated probe compensation: If the probe isn't properly compensated, the amplitude measurements will be inaccurate.

It's important to remember that no single oscilloscope or brand is inherently "correct." Each device has its own limitations, such as 8-bit ADC resolution and slightly different frequency responses. Therefore, small variations in measurements are normal and expected.

The Role of Bandwidth Limitation

You might wonder why we often set a 20MHz bandwidth limit. This was originally introduced in early oscilloscopes to reduce high-frequency interference. While 20MHz is commonly used, it’s more of an empirical value rather than a strict theoretical requirement. In modern digital oscilloscopes, you have more flexibility to adjust filtering and improve accuracy without being constrained by this limit.

A More Accurate Way to Measure Ripple and Noise

Modern digital oscilloscopes come with advanced features that allow for more precise measurements. Instead of relying solely on the 20MHz limit, you can use functions like FFT, digital filtering, and statistical analysis to get better results.

1. FFT Function

Using Fast Fourier Transform (FFT), you can analyze the frequency components of the signal. This helps identify noise sources, harmonic distortion, and other characteristics. For example, the ZDS2000 series offers a 4Mpts FFT with a fine frequency resolution of 250Hz, making it ideal for identifying interference sources quickly and accurately.

2. Digital Filtering

Digital filters, such as IIR or FIR filters, can remove unwanted noise from the signal. The ZDS2024 oscilloscope, for instance, allows users to apply low-pass or high-pass filters with cutoff frequencies ranging from 100Hz to 100MHz. This enables more accurate signal analysis by eliminating high-frequency noise that may skew the results.

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Figure 1: Amplitude-Frequency Response Curve of a Low-Pass Filter

3. Automatic Measurement

Automatic measurement functions can calculate key parameters such as the average, maximum, minimum, and standard deviation of the signal. This helps in assessing the stability of the power supply and identifying potential issues. By analyzing statistical data, users can quickly detect anomalies and evaluate the overall quality of the signal.

Summary of Key Features

  • FFT: Analyze frequency content and identify noise sources.
  • Digital Filtering: Remove unwanted noise for cleaner signals.
  • Statistical Measurement: Provide detailed waveform statistics for accurate evaluation.

By leveraging these tools, engineers and technicians can achieve more reliable and consistent measurements of ripple and noise in power supplies. Whether you're troubleshooting or designing a power system, understanding and applying these techniques can greatly enhance your ability to assess and optimize performance.

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