The Leo Bodnar LBE-1322 fast-edge pulser (30 ps rise time, 30 kHz to 300 MHz): its specifications and how we use it to measure the step and frequency response of Rigol scopes running NovaOS.
| Rise and fall time | 30±2 picosecondsProduct page |
| Frequency | 30kHz to 300MHz with 50% duty ratio and 1Hz resolutionProduct page |
| Output amplitude | 50mVpp to 1.2Vpp (set via USB); DC coupled, negative goingProduct page |
| Trigger output | 1.5Vpp amplitude into 50R load; AC coupledProduct page |
| Synchronisation input | external reference from 1MHz to 250MHz, 3.3V max; AC coupledProduct page |
| Pulse output connector | high speed SMA (BNC adaptor is included)Product page |
| Power | USB powered - requires 200mA at 5VProduct page |
| Sample unit, as tested | Risetime 29.8ps, Falltime 28.7ps, Amplitude 1.10V, Overshoot 2.1%, Undershoot 3.1%Test report, p. 1 |
Leo Bodnar's own figures, as its documents state them; each links to the page it is on.
Makes a voltage step that rises extremely fast, so how the scope draws it shows how fast a signal the scope can follow.
One capture of a very fast edge gives a channel's step response, and from it the whole frequency response: a cross-check of every band-limit filter and of the rise time.
A 30 ps edge is far faster than any of these scopes, so what a channel draws is its own step response: its rise time, its overshoot and, through the step's derivative, its whole frequency response. NovaOS's band limits were measured relative to each channel's widest setting; the pulser gives the absolute check of every band limit and of each channel's bandwidth, on the DHO924S and the MHO934.
The tests we will run with it next; the results will appear here.
Forum threads worth reading before you buy one.
Back to the bench: everything NovaOS is developed and measured with.