Mmm, if you define "show" as "display in the form of glitchy, apparently-high-frequency corruption that is completely confusing to a beginner, completely irrelevant to a discussion prompted by a self-styled beginner, and when discovered, would necessitate that the user in question either figure out an advanced triggering mode* to isolate the glitch or switch to an oscilloscope with non-awful realtime performance like a ds1054", then yeah, I guess you are pedantically, technically correct.
* Yes, pulse width triggering mode is advanced for a beginner.
One only needs to think in terms of what digital sampling means, in order to figure this out. None of the detractors in this thread seem to appreciate DSOs as DSOs; if one wills that a cat should act like a dog, one will forever have the problem that it is a fundamentally different creature...
Not for a beginner? Probable. But a beginner will have trouble getting a stable display on an analog or RTS DSO all the same, so it's a pointless argument.
Wrong! *Some* glitches (i.e. those that have a high occurrence rate) are somewhat visible on ETS, and if they're large enough you might even recognize that there's a problem. That doesn't change the fact that most common glitches and problems simply very likely won't show up in ETS.
Just what kind of signals are you watching that have such infrequent glitches? And at a bandwidth much greater than typical?
To use your very own example of SMPS startup conditions, consider that SMPS rarely peak above 1MHz, and those are the small ones. That's 1000ns per cycle. 500ns per on-period. At 100MS/s, you have a whopping 50 samples to observe the pulse width variation in real time.
If you're looking at glitchy high speed data, you simply have the wrong instrument, period. You need a logic analyzer with that type of capability. Preferably with a glitch trigger setting, or something like that.
So again, your arguments are invalid.
Fact is that you can't use ETS to probe unknown signals (or signals with unknown components)
Have you an example of such an
alien signal?
So far in all of my work, I have not seen a single situation that was obfuscated by ETS. (The prior case of runt square waves is easily solved with advanced trigger, or a single capacitor to the trigger input.)
And even if you don't want to accept the maths/physics behind ETS then just ask yourself this: if ETS was as sufficient for common debugging work as you and others in this thread claim it is, why don't we see more new sample scopes?
Duh. Marketing. ADCs are cheap enough that the analog signal path is the limitation now. It would cost quite a bit more to design and build a preamp that's capable of driving the full ADC's analog bandwidth (which is usually a few times its max. Nyquist frequency).
They can also charge more for the scopes that do offer extreme bandwidth.
It's also a cost saving feature to avoid ET hardware and software. Although with everything going through an ASIC, it's up to the functionality in there. But even having that in the first place, Rigol (and Keysight) get tremendous value in performance and production cost.
and the upper high end (i.e. bandwidths in excess of 50GHz to 100GHz) and even in the latter area they are dying out in favor of real-time scopes.
When cost is no object, you might as well get the best.
I'm not concerned about the design of scopes that cost more than a small house.
Tim