A rugged GEM board photomultiplier uses titanium, ceramic, and atmospheric-pressure operation to withstand heat and vibration.
Intersecting antenna and bias portions convert polarization components into electron emission, simplifying electromagnetic wave detection.
An alkali metal layer lowers work function and suppresses charge-up, helping metasurface electron emitters achieve higher sensitivity.
Integrating data-handling circuitry inside the active display area removes opaque borders and beam splitters, cutting night vision bulk and weight.
A trivalent metal oxide barrier blocks alkali migration and gas permeation, preserving photomultiplier sensitivity and limiting after-pulses at high temperature.
Placing display circuitry within the active area removes opaque borders, shrinking night vision overlays and avoiding bulky beam splitters.
An electron backscatter layer redirects primary electrons onto a booster layer, raising MCP first strike efficiency and low-light SNR.
A biased transparent conductive and dielectric interface pulls photoelectrons from the recombination zone to raise photocathode quantum yield.
Multiple meta-surface conversion units with different patterns broaden detectable wavelengths, enabling simultaneous gas component detection.
A Pt particle resistance layer stabilizes MCP resistance and current across -60°C to +60°C, extending electron multiplier operation.
A bimetal coupling matched to sapphire limits thermal stress, keeps vacuum tightness, and supports high-temperature GaN photocathode activation.
Elastic biasing portions hold the photocathode plate in stable electrical contact despite assembly tolerances and thermal deformation.
A reflective photocathode array generates photoelectrons directed toward nested dynode structures within a compact photomultiplier tube housing.
Bonding a prism parallel to the casing wall simplifies electron tube alignment while reflecting light back to the photocathode to increase quantum efficiency.