The detectors have different sensitivity depending on the direction of the waves, so if a wave comes from a "bad" direction (perpendicular to both arms, e.g. directly from above), a particular detector might not detect anything, even if the wave is strong.
This is why (amongst many other reasons) it's important to have multiple detectors around the world (e.g LIGO has two locations in the US, you also have Virgo in Italy, and they do collaborate), this way you can assure in theory that you can "see" every wave, no matter which direction it's coming from.
(AFAIK).
Unless there's such a thing as polarized gravitational waves, https://www.ligo.org/science/Publication-O1StochNonGR/ which might exist but are hard to discern with current detectors from what I understand. It'd be really cool to learn that there's such a thing as vector and scalar polarized gravitional waves.
Or realllly tall detectors.
> A mirror at the vertex of the arms splits a single light beam into two, directing each beam down an arm of the instrument Mirrors at the ends of the arms reflect the beams back to their origin point where they are recombined to create an interference pattern called 'fringe
Everybody knows of LIGO, but it's actually three detectors that work together, LIGO, Virgo, and KAGRA.
Even a single detector has two arms at 90 degrees to each other, which can give you a rough idea of where in the sky it came from. But now that we have multiple detectors online we get better and better about spotting the origin.