Even classically, there is no time interval. The curvature is continuous.
Then again, the curvature is concentrated in a definable timescale around the closest approach.
Suppose that the electron is initially "at rest" - at apoapse of a bound orbit passing close to the nucleus. Such as 100s orbital - principal quantum number 100, orbital quantum number 0.
What are legal results of bremsstrahlung?
Orbital quantum number must change by 1 by a selection rule. Therefore, 100s electron can go to some p orbital. Not 1p (no such orbital) and not 100p (no transition - same energy as 100s) - but 2p, 3p...99p are all options and all of them will happen, in some ratio.
If there is a transition to 1s, it immediately tells you that the initial orbital was some p orbital (all others are forbidden to transition to s). If there is a transition to 3, but no transition to any orbital 2, you can immediately tell that 2p was forbidden by a selection rule, 3d allowed - therefore the initial orbital was a f one.
Does the selection rule of orbital angular momentum only changing by 1 also apply to unbound orbits? And in case of unbound-unbound transitions, does it constrain energies of radiation emitted?