Optical Metrology & Interferometry and the Hot Mirror: A Working Guide

For engineers working in Optical Metrology & Interferometry, the choice of a reflective surface is rarely an afterthought. Hot Mirror components sit at the heart of…

For engineers working in Optical Metrology & Interferometry, the choice of a reflective surface is rarely an afterthought. Hot Mirror components sit at the heart of systems where comparing wavefronts to a reference with sub-wavelength accuracy, and a small improvement in coating quality can change the result of an entire measurement or process.

Think of the Hot Mirror as a precisely made float or borosilicate glass plate whose working surface is a dichroic (transmits visible, reflects IR). The result is > 90% visible transmit reflection across IR reflect / visible pass, which is exactly what most Optical Metrology & Interferometry builders are looking for.

Reflection on a first surface is straightforward physics: photons strike the coated face and are returned according to the law of reflection, angle in equals angle out. Because the coating sits on top, there is no second surface behind it to create a faint ghost image, which matters whenever contrast or measurement accuracy is at stake.

Most of the engineering in a Hot Mirror lives in its dichroic (transmits visible, reflects IR). The stack is designed for IR reflect / visible pass and delivers > 90% visible transmit, and its environmental protection layer keeps the metal from tarnishing so the mirror keeps working year after year.

A Hot Mirror starts as a float or borosilicate glass blank. We hold it to 4–6λ flatness and 60-40 surface quality, then apply the dichroic (transmits visible, reflects IR). The substrate never sees the beam directly, but its figure sets the limit on how straight the reflected wavefront stays.

When you specify a Hot Mirror, the numbers that matter are flatness 4–6λ, finish 60-40, and the reflectance > 90% visible transmit across IR reflect / visible pass. Thickness 1–3 mm is mostly about handling and mount compatibility, but it still belongs on the print. The specification table covers the common configurations.

In Optical Metrology & Interferometry, the Hot Mirror usually appears wherever comparing wavefronts to a reference with sub-wavelength accuracy. Designers value it because it keeps the beam path predictable and the loss budget small, which translates directly into a more stable instrument. The applications overview maps where each industry places it.

Where comparing wavefronts to a reference with sub-wavelength accuracy, a Hot Mirror earns its place by doing one job reliably: turning the beam without adding noise. In Optical Metrology & Interferometry that reliability is the difference between a prototype and a shippable product. More application examples are worth a look if the use case is close to yours.

Selecting a Hot Mirror for Optical Metrology & Interferometry starts with the wavelength and angle of incidence, then the acceptable loss. Match the dichroic (transmits visible, reflects IR) to IR reflect / visible pass, confirm > 90% visible transmit, and make sure the float or borosilicate glass and 1–3 mm fit the mount you already have. The spec and size tables make that comparison quick.

A Hot Mirror is tougher than it looks but softer than you think. Fingerprints on the dichroic (transmits visible, reflects IR) are the usual cause of field failures, so edge-handling and capped storage pay off. A little discipline keeps > 90% visible transmit where it belongs.

At JYOPTO we make Hot Mirror parts by cutting float or borosilicate glass with laser accuracy of ±0.01 mm, then applying the dichroic (transmits visible, reflects IR) under vacuum. Standard blanks run 1–3 mm thick, edges are smoothed for safe handling, and every shipped mirror meets 4–6λ flatness with a 60-40 surface — the same disciplines we apply across our optical glass, vacuum-coating and precision cold-processing lines since 2020.

A Hot Mirror is an optical component built so that reflection happens at the coated front face rather than through a substrate. With a dichroic (transmits visible, reflects IR) on a float or borosilicate glass base, the part delivers > 90% visible transmit reflectivity across IR reflect / visible pass while keeping the useful aperture clean and ghost-free.

For Optical Metrology & Interferometry, do not over-specify. Choose the dichroic (transmits visible, reflects IR) that covers IR reflect / visible pass at the angle you use, keep flatness at 4–6λ unless the wavefront demands more, and you will have a Hot Mirror that is both capable and economical.

Most of the engineering in a Hot Mirror lives in its dichroic (transmits visible, reflects IR). The stack is designed for IR reflect / visible pass and delivers > 90% visible transmit, and its environmental protection layer keeps the metal from tarnishing so the mirror keeps working year after year.

Beyond Optical Metrology & Interferometry, the same Hot Mirror shows up in laboratories, teaching setups and OEM builds where comparing wavefronts to a reference with sub-wavelength accuracy. Its value is generality: one well-made part serves many breadboards, which is why stocking a few standard sizes pays off.

Where comparing wavefronts to a reference with sub-wavelength accuracy, a Hot Mirror earns its place by doing one job reliably: turning the beam without adding noise. In Optical Metrology & Interferometry that reliability is the difference between a prototype and a shippable product. More application examples are worth a look if the use case is close to yours.

Selecting a Hot Mirror for Optical Metrology & Interferometry starts with the wavelength and angle of incidence, then the acceptable loss. Match the dichroic (transmits visible, reflects IR) to IR reflect / visible pass, confirm > 90% visible transmit, and make sure the float or borosilicate glass and 1–3 mm fit the mount you already have. The spec and size tables make that comparison quick.

Our production of a Hot Mirror follows a simple, repeatable route: laser-cut the float or borosilicate glass to ±0.01 mm, smooth the edges, deposit the dichroic (transmits visible, reflects IR), and inspect to 4–6λ / 60-40. Thickness options span 1–3 mm, and the same Hangzhou line that builds first-surface mirrors also runs windows, substrates and custom coatings.

Environment matters. A Hot Mirror headed for Optical Metrology & Interferometry may see condensation, vibration and frequent handling. Specifying a sealed-edge, protected coating and a stable float or borosilicate glass substrate means the mirror keeps its figure (4–6λ) and its reflectance through warranty periods and beyond.

In short

For Optical Metrology & Interferometry, the Hot Mirror is less a commodity than a tuned component. Specify the band (IR reflect / visible pass), the reflectivity (> 90% visible transmit) and the figure (4–6λ), and you will spend less time debugging light you cannot see. That is the whole game. Where your application sits among the sectors we serve changes the details, not the method.