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M43.0 x 0.75, 1.5mm Thick, Uncoated, Machine Vision Mounted Sapphire Window

Machine Vision Mounted Sapphire Windows

Machine Vision Mounted Sapphire Windows

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Stock #23-286 3-4 days
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£255.00
Qty 1-9
£255.00
Qty 10+
£229.50
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Abbe Number (vd):
72.24
Axis Orientation:
Random
Bevel:
Protective as needed
Birefringence (no-ne):
0.008 for Visible Light Orthogonal to Optical Axis
Clear Aperture (%):
≥90
Clear Aperture CA (mm):
36.18
Diameter (mm):
40.20 +0/-0.20
Thickness (mm):
1.50 ±0.10
Coating:
Uncoated
Coefficient of Thermal Expansion CTE (10-6/°C):
8.8
Density (g/cm3):
3.97
Edges:
Fine Ground
Index of Refraction nd:
1.77
Knoop Hardness (kg/mm2):
1900
Parallelism (arcmin):
≤3.5
Poisson's Ratio:
0.27
Substrate: Many glass manufacturers offer the same material characteristics under different trade names. Learn More
Sapphire (Al2O3)
Surface Flatness (P-V):
2λ (typical)
Surface Quality:
80-50
Type:
Protective Window
Wavelength Range (nm):
330 - 5500
Young's Modulus (GPa):
435
Filter Thread:
M43.0 x 0.75
Mount Diameter (mm):
45.00
Mount Thickness (mm):
7.0

Regulatory Compliance

RoHS:
Certificate of Conformance:

Product Family Description

  • Protective Windows for Machine Vision Applications
  • Windows Feature Extreme Surface Hardness and Chemical Resistance
  • M25.5 to M62.0 Filter Threads Available

Machine Vision Mounted Sapphire Windows are mounted in durable anodized aluminum housings with common filter threads for easy integration with most imaging lenses. The windows within the mount are manufactured from durable sapphire making them ideal for rugged environments because of their extreme surface hardness, high thermal conductivity, high dielectric constant and resistance to common chemical acids and alkalis. Machine Vision Mounted Sapphire Windows feature both male and female threads, allowing them to be combined with other mounted filters or polarizers. The uncoated windows are useful within a transmission range from 330 – 5500nm making them ideal for machine vision applications in the UV, Visible, and Infrared spectra.