With an input impedance of 1 MΩ and 0.9 pF capacitance, the TETRIS active probe is ideal for for today's digital systems designs. Compatible with any 50 ohm SMA or BNC input oscilloscope.
Rise time is the time taken for a signal to cross a specified lower voltage threshold followed by a specified upper voltage threshold. This is an important parameter in both digital and analog systems. In digital systems it describes how long a signal spends in the intermediate state between two valid logic levels. In analog systems it specifies the time taken for the output to rise from one specified level to another when the input is driven by an ideal edge with zero rise time. This indicates how well the system preserves a fast transition in the input signal.
So why do we need to know the rise time of an oscilloscope? The rise time of an amplifier is related to its bandwidth. If we know the bandwidth of the signal under test, we can choose an oscilloscope with an equal or greater system bandwidth and be confident that the oscilloscope will display the signal accurately. If, on the other hand, we know the rise time of our signal, it would be useful to know by how much the oscilloscope will slow down the signal and therefore add to its rise time.
The bandwidth BW in hertz of an amplifier with a rise time of tR seconds can be estimated as:
BW ≈ 0.35 / tR
BW and tR can be scaled to more convenient units such as MHz and µs, or GHz and ns.
The numerator of 0.35 in this formula is accurate if the oscilloscope's input amplifier has a simple frequency response like that of a single-pole RC filter. In reality, many oscilloscopes have a faster roll-off to give a flatter frequency response in the pass band, and this can increase the numerator to 0.45 or even higher. The formula also assumes that the rise time is measured between the 10% and 90% voltage levels of the signal.
A fast square wave signal appears to have a 10%–90% rise time of 1 ns when displayed on my oscillloscope. What is the approximate bandwidth of the oscilloscope?
Using the above formula, the scope appears to have a system bandwidth (including the probes) of:
0.35 / (10–9 s) = 0.35 x 109 Hz = 350 MHz