The moving mirror's radiation can be understood as squeezed Rindler/Milne (Hawking/partner) modes, and the squeezing explains why the spectrum deviates from and yet approximates a thermal distribution while adding correlations.
In this case, the particles observed by an inertial observer atI + R consist of both squeezed Rindler and Milne modes
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Squeezed quantum states and partner modes in the moving mirror model of black hole evaporation
The moving mirror's radiation can be understood as squeezed Rindler/Milne (Hawking/partner) modes, and the squeezing explains why the spectrum deviates from and yet approximates a thermal distribution while adding correlations.