PLX Hollow Roof MirrorsTM (HRMs) are ideal for redirecting light in one coordinate and any application where a roof top or Porro prism can be used. Useful in all wavelengths, they are available in different accuracies, coatings, and configurations.

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Hollow Roof Mirrors™ (HRM)

Cat. No. Clear Aperture
Width (in/mm)
Clear Aperture
Length (in/mm)
Mirror Surface
Coating Wavelength Range (nm) Reflectance Coating Curve Diagram 3D Model
RM-102-0.25 1.0/25 2.0/51 0.25 λ/10 165 - - -
RM-102-0.5 1.0/25 2.0/51 0.5 λ/10 165 - - -
RM-102-1 1.0/25 2.0/51 1.0 λ/10 165 - - -
RM-102-2 1.0/25 2.0/51 2.0 λ/10 165 - - -
RM-102-5 1.0/25 2.0/51 5.0 λ/10 165 - - -
RM-102-15 1.0/25 2.0/51 15.0 λ/4 165 - - -

Beam Deviation is the maximum deviation from parallelism, expressed in seconds of arc, of any single return beam from any of the 6 sub-apertures of the retroreflector, when the retroreflector is fully-illuminated.

Exiting Wavefront is the resultant maximum peak-to-valley wavefront deformation from a fully-illuminated retroreflector, where lambda = 633nm.

Certain high accuracy models may be heavier than indicated here. Check with us for actual weight.

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