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Thursday, 8 October 2026
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2048-pixel line scan camera, model RA⁠-⁠LSC⁠-⁠1205

The RA⁠-⁠LSC⁠-⁠1205 line scan camera has been designed and built in four versions. The RA⁠-⁠LSC⁠-⁠1205 is a 2048-pixel line scan camera with a line rate of 951 Hz. You can use it to scan objects and to measure the width of objects on a conveyor belt. This section shows the camera's spectral response, parametric specifications, demo software features, and the specifications of each version.

Selection guide

What this camera is good for

Visible and near-IR spectrometers and low-light measurement

Tall 14 μm × 200 μm pixels are the defining feature of the RA⁠-⁠LSC⁠-⁠1205, and they are why it performs well in weak light. The sensor has 2,048 pixels on a 28.672 mm active length, responds from 350 to 1100 nm, and accepts exposures from 3 μs to 35.5 minutes. The line rate is 951.5 lines/s and the dynamic range 400:1. We offer four versions, with a 16-bit or 12-bit ADC and an FPGA or microcontroller.

Sensor
Linear CCD Array
Effective pixels
1 × 2048
Pixel size
14 μm × 200 μm
Active length
28.672 mm
Line rate
951.5 Hz
Spectral range
350 nm to 1100 nm
Dynamic range
400
ADC resolution
16 bit
Minimum exposure
3 μs
Maximum exposure
35.5 min
  • Visible and near-infrared spectrometers

    Spread the 350 to 1100 nm band over 2,048 pixels and each pixel sees about 0.37 nm of the spectrum. The 200 μm pixel height captures the whole slit image and makes spectrometer alignment much easier.

  • Laser-line position sensing

    The laser line stays on the 200 μm pixels even if it moves up or down by several tens of micrometers. By computing the intensity center over neighboring pixels, we find the line position more precisely than the 14 μm pitch. The camera gives a new reading every 1.05 ms.

  • Shadow-based width gauging on conveyors

    With a backlight, the object's shadow falls on the 2,048 pixels and the edges are found from it. In a 205 mm field of view each pixel sees 0.1 mm of the object. The tall pixels mean a slightly tilted camera mount does not cause trouble.

  • Very low-light measurement

    Each pixel has an area of about 2,800 μm², and the FPGA versions allow exposures up to 35.5 minutes. In the -P and -I versions, the 16-bit ADC records very weak signals in fine steps.

  • Near-infrared source measurement

    The sensor is sensitive up to 1100 nm, so near-IR laser lines and sources are recorded on the same array that sees the visible band. Gain adjustment up to 6 V/V in 64 steps evens out the sensitivity difference between the two ends of the spectrum.

  • Teaching and laboratory instruments

    For static and slow experiments, the microcontroller-based -S version with a 12-bit ADC, 67.9 μs to 27 ms exposure and 66.5 lines/s is fully adequate. Windows and Linux drivers and sample code for Matlab, LabVIEW, C++, C#, VB.Net and Python make setup simple.

What the specs mean in practice

Each 14 μm × 200 μm pixel has an area of 2,800 μm². At the same exposure, a larger pixel collects more light and gives a cleaner signal in weak light. At 951.5 lines/s you get a line every 1.05 ms, enough for continuous spectroscopy and process monitoring. The 400:1 dynamic range is captured by a 16-bit ADC, so the converter is never the limiting factor. The 350 to 1100 nm response lets you work with halogen lamps or near-IR lasers without changing the sensor. Exposures from 3 μs to 35.5 minutes in 1 μs steps cover light levels that differ by a factor of about 7 × 10^8.

Before you order

The lens focal length is roughly working distance × 28.672 mm ÷ field-of-view width. In a spectrometer, choose a grating that spreads the spectrum over the full 28.672 mm; for width gauging, use a backlight. A 3 μs minimum exposure against a 1.05 ms line period handles bright sources without saturation, and up to 35.5 minutes is available for weak signals. The -P version is the most complete: FPGA, 16-bit ADC, 480 Mbit/s USB, analog output, on-board RAM, a lens, a casing of your choice and customizable firmware, with 7-day delivery. The -I version has the same electronics but no lens, casing or firmware customization. The -A version has a 12-bit ADC and 12 Mbit/s USB, without analog output or RAM. The -S version uses a microcontroller, is limited to 66.5 lines/s and has timing jitter below 200 ns.

Talk to us about choosing a model

 Spectral response of the RA-LSC-1205 line scan camera
RA-LSC-2566I line scan camera made by RasaAndishan

RA⁠-⁠LSC⁠-⁠1205 USB Line Scan Camera ParametersSpecification
SensorLinear CCD Array
Pixel Size14 μm x 200 μm
Pixel Distance14 μm
Line Width200 μm
Effective Pixels1X2048
Active Length28.672 mm
Spectral Range350 nm to 1100 nm
Max Pixel Frequency2 MHz
Dynamic Range400
PGA Gain Resolution6 V/V - 64Steps
Programmable Offset Resolution300 mV - 512Steps±
Power consumption1.5 W
External PowerNot Required
Operational Temperature Range⁦−25⁩ to ⁦+65⁩ °C
Operation SystemsWindows 64-bit And Linux
Communication PortUSB2.0 Port
Multiple CamerasSupported
Device DriverYes
Sample CodesMatlab,LabView,C++,C#,VB.Net,Python
Camera Selection GuideRA⁠-⁠LSC⁠-⁠1205⁠-⁠PRA⁠-⁠LSC⁠-⁠1205⁠-⁠IRA⁠-⁠LSC⁠-⁠1205⁠-⁠ARA⁠-⁠LSC⁠-⁠1205⁠-⁠S
ProcessorFPGAFPGAFPGAMicrocontroller
Gain Adjust✓✓✓✓
Offset Adjust✓✓✓✓
ADC Resolution16 bit16 bit12 bit12 bit
USB Speed480Mbit/S480Mbit/S12Mbit/S12Mbit/S
Analog OutPut✓✓✗✗
On Board RAM✓✓✗✗
Jitter Order< 6.3 ns< 6.3 ns< 6.3 ns< 200 ns
Exposure Min3 μs3 μs3 μs67.9 μs
Exposure Max35.5 min35.5 min35.5 min27 ms
Exposure Resolution1 μs1 μs1 μs12 μs
Line Rate951.5 Hz951.5 Hz951.5 Hz66.5HZ
Lens✓✗✗✗
Casing ModelSelectable By Customer✗✗✗
Operational Temperature Range⁦−25⁩ to ⁦+65⁩ °C⁦−25⁩ to ⁦+65⁩ °C⁦−25⁩ to ⁦+65⁩ °C⁦−25⁩ to ⁦+65⁩ °C
Availability7Days After Order3Days After Order3Days After Order3Days After Order
Firmware Customizable✓✗✗✗

Where our equipment is used

Organizations, universities, industries and companies that have used our products

  • Hedayat Hooshmand Nozhan Sepehr