New Product Recommendation | ATP7810 Ultra-Wide Range Infrared Spectrometer Series

01  Spectral measurement requires a wider field of view

In fields such as materials research, infrared spectrum analysis, remote sensing, and optical device testing, traditional spectrometers are often limited by their narrow band range and struggle to balance wide coverage with high resolution.

The ATP7810 is a wide-band, high-resolution spectrometer. It uses software-controlled rotating grating for wavelength scanning, achieving high-precision spectral measurement results. It provides a more flexible testing solution for scientific research and industrial applications.

02  ATP7810 Product Principle

The signal light enters the ATP7810 optical platform through an SMA905 fiber interface. After passing through the fixed entrance slit, the light reaches a mirror. After reflection, the light arrives at the rotating grating. The rotating grating rotates at a constant speed on a turntable, establishing a one-to-one correspondence between the grating's dispersion angle and wavelength. Finally, the signal light passes through another mirror, reaches the detector, where the optical signal is converted into an electrical signal and recorded by a computer. The entire operation and spectral calculation are completed by our computer software.

03  ATP7810 Key Highlights

Ultra-Wide Band Coverage

Up to 0.9–5 μm

Multiple band models available:

– 0.9–2.5 μm

– 0.9–5 μm

Covering from near-infrared to mid-far infrared. By selecting the appropriate grating, you gain more freedom in wavelength and resolution choices.

Motorized Rotating Grating Design

A high-precision rotating grating structure achieves:

– Higher measurement accuracy

– More flexible band selection

– Better spectral resolution

One-click scan measurement, simple and efficient operation.

High-Performance Detection System

Supports multiple detector configurations:

– InGaAs detector

– MCT detector

High SNR, high dynamic range, high stability detection.

Flexible Configuration and Expansion

Rich input/output interface design:

Light input methods:

– SMA905 fiber input

– Free space input

Data output interfaces:

– USB 2.0

– UART

Expansion interfaces:

– 15-pin expansion interface

– External trigger signal support

It can accept either SMA905 fiber input or free space light, output spectral data via USB 2.0 or UART, and requires only a single +12 V DC power supply for easy use. All controls can be electronically managed via software.

04  ATP7810 Applications

For more information, please contact:

Email: optoskyphotonics@gmail.com

Web: www.optosky.net