Pretty much. The same effect that causes stars to twinkle limits the resolution of space-based spy satellites imagery of the ground.
Could you clarify what you mean by this?
And yeah, I should have been more clear in my original question; I was lumping mathematical advances under "technology".
In radioastronomy, there are arrays of dishes that use this technique. There are good pictures in the Wikipedia article. [0]
One military implementation was a connected three-satellite constellation, built by the US Navy for scanning the surface of the world's oceans. [1]
But those tools work in (relatively) long wavelengths.
I have never heard of free-flight multi-aperature interferometry that works in optical or near-optical wavelengths.
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[0] "Very-long-baseline interferometry" https://en.wikipedia.org/wiki/Very-long-baseline_interferome...
[0] "How VLBI Works" https://en.wikipedia.org/wiki/Very-long-baseline_interferome...
[1] "White Cloud | PARCAE | NOSS" https://en.wikipedia.org/wiki/Naval_Ocean_Surveillance_Syste...
Keep in mind that there are a lot of people that track satellites, even spy satellites, as a hobby. I haven't heard of anyone discovering two or more satellites orbiting in the sort of tight formation you would expect would be required for this.