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LETO-720 Fast LCOS Spatial Light Modulator

LETO-720 Fast LCOS Spatial Light Modulator
LETO-720 Fast LCOS Spatial Light Modulator
LETO-720 Fast LCOS Spatial Light Modulator
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LETO-720 Fast LCOS Spatial Light Modulator
LETO-720 Fast LCOS Spatial Light Modulator
LETO-720 Fast LCOS Spatial Light Modulator
Tags: SLM
LETO-720 Fast LCOS Spatial Light Modulator
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  • Model: HOLOEYE LETO
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The LETO-720 combines the high data bandwidth and low latency of the 4K resolution GAEA-2.1 (4k – 60fps – RGB888) driver and a fast display version of the LETO-3 SLM with a resolution of 1920 × 1080 pixels (~1 ms response-time at 520 nm).

LETO-720 LCOS SLM – Microdisplay Features 

  • Display Type: Reflective LCOS (Phase Only)
  • Resolution: 1920 x 1080 Pixel
  • Pixel Pitch: 6.4 µm
  • Fill Factor: 93 %
  • Active Area: 12.29 x 6.91 mm (0.55″ Diagonal)
  • Addressing: 8 Bit
  • Signal Formats: HDMI – HDTV Resolution
  • Input Frame Rate: 240 Hz
  • Display Update Rate: 240 Hz
  • 720 Hz (RGB coded)

leto 720 speckle reduction

The LETO-720 SLM offers 2 modes:

240 Hz mode: This mode utilizes the high video data bandwidth of the driver to address real 240 Hz data on the SLM. The refresh rates for both, input frames via the HDMI graphics interface and the output, are boosted to 240 Hz.

720 Hz modulation (RGB coded): This mode makes use of the RGB color channels in addition to the 240 Hz mode. Three consecutive monochrome images are stacked in one full-color image.

Versions

We currently offer one version optimized for the VIS range between 420 to 650 nm.

LETO-720 Spatial Light Modulator Wavelength Ranges

 

Reflectivity: 62-72%

Max. Phase Shift: 2.2 Pi @ 633 nm

Wavelength Range: 420 - 650 nm

 

 


Please contact us for the latest price.


HOLOEYE Photonics website

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SLM-Brochure_2025 2.59MiB Download
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A number of papers have been published by scientists around the globe who have used a HOLOEYE LETO series SLM in their research. Here are some examples:

A database of published papers, searchable by device or application, can be also found on the HOLOEYE website here.

Elementary Optical Functions

The HOLOEYE Spatial Light Modulator Pattern Generator software was developed for use with all HOLOEYE SLM models. The software allows the simple generation of diverse dynamic optical functions like gratings, lenses, axicons and apertures as well as the calculation of diffractive optical elements (DOE) from user defined images.


Besides the generation of DOEs a wide range of basic optical functions can be created directly via the menu bar. After input of the required parameters the output image appears in a new window. There are several binary and multilevel optical functions possible:

  • Blank Grey Level Screen
    With this function you can create a homogeneous gray level screen.
     
  • Horizontally Divided Screen
    With this function you will create a horizontally divided screen, consisting of two homogeneous graylevel partial screens.
     
  • Random Bitmap
    With this function you will create a random pixel distribution using 256 grayscale values. This function can be used to realize the optical function of a random phase plate.
     
  • Aperture Functions
    - Rectangular Aperture
    - Circular Aperture
    -Single Slit and Double Slit
     
  • Fresnel Zone Lenses
    -Binary Fresnel Zone Lens
    -Multilevel Fresnel Zone Lens
    -Cylindrical Fresnel Zone Lens
     
  • Binary Axicon
    With this function you will create a Binary Axicon graylevel image representation.
     
  • Axicon
    With this function you will create a 256-level Axicon graylevel image representation.
     
  • Vortex Phase
    Use this function to create a 256-graylevel image representation of a vortex phase.
     
  • Concentric ring segments
    Use this function to create binary images consisting of concentric ring segments.
     
  • Binary beam-splitter gratings
    -Linear Gratings and Crossed Linear gratings
    -Exemplary binary beam-splitter designs
     
  • Sinusoidal Grating
    With this function you will create a sinusoidal grating.
     
  • Blazed Grating
    With this function you will create a blazed grating.
     
  • Calculating a beam-shaping phase function for Gaussian Input beams
    -Transformation of a Gaussian beam to a circular ‘flat-top’ beam
    -Transformation of a Gaussian beam to a rectangular ‘flat-top’ beam
     
  • Superposition with an additional phase map
    - e.g. for compensation of aberrations of the optical system or of the SLM