PRODUCT SHEET

Starna Stray Light Glasses (220 – 450 nm)

Stray Light Glasses are precision glass cut-off filters designed to qualify the stray light level in ultraviolet and visible spectrometers. These filters nominally cut off at 280 nm, 360 nm, and 450 nm, with each individual filter certified to account for wavelength variations of up to ±10 nm due to glass melt differences.

Stray light, also known as stray radiant energy or power, refers to any undesired light reaching the detector outside the selected spectral bandwidth. It originates from optical imperfections, internal reflections, or leaks in the spectrometer optical system and causes measurement errors by artificially increasing detected signal, especially at high absorber concentrations. Regular checking of stray light using these filters helps monitor instrument optical condition and ensures accuracy in quantitative analysis.

Features and Purposes
  • Glass cut-off filters certified individually for cut-off wavelengths at approximately 280 nm, 360 nm, and 450 nm.
  • Each filter provides a usable wavelength range below the cut-off: 210–270 nm for 280 nm filter, 270–350 nm for 360 nm filter, 350–440 nm for 450 nm filter.
  • Sliding window covers to protect filter surfaces when not in use.
  • Filters transmit all wavelengths above the cut-off and block light below, enabling stray light qualification by measuring undesired transmission below cut-off.
  • Essential for verifying spectrometer stray light, helping ensure compliance with Beer-Lambert law linearity and maintaining instrument performance.
DOCUMENTS AND RESOURCES
Certified Reference Materials for Spectroscopy
Starna Cell Catalogue Original V002 05 2024 Proof 005
Stray Light Qualification for UV and Visible Spectrophotometers Using Starna Glasses
PRODUCT SHEET

Starna Stray Light Glasses (220 – 450 nm)

Stray Light Glasses are precision glass cut-off filters designed to qualify the stray light level in ultraviolet and visible spectrometers. These filters nominally cut off at 280 nm, 360 nm, and 450 nm, with each individual filter certified to account for wavelength variations of up to ±10 nm due to glass melt differences.

Stray light, also known as stray radiant energy or power, refers to any undesired light reaching the detector outside the selected spectral bandwidth. It originates from optical imperfections, internal reflections, or leaks in the spectrometer optical system and causes measurement errors by artificially increasing detected signal, especially at high absorber concentrations. Regular checking of stray light using these filters helps monitor instrument optical condition and ensures accuracy in quantitative analysis.

Features and Purposes
  • Glass cut-off filters certified individually for cut-off wavelengths at approximately 280 nm, 360 nm, and 450 nm.
  • Each filter provides a usable wavelength range below the cut-off: 210–270 nm for 280 nm filter, 270–350 nm for 360 nm filter, 350–440 nm for 450 nm filter.
  • Sliding window covers to protect filter surfaces when not in use.
  • Filters transmit all wavelengths above the cut-off and block light below, enabling stray light qualification by measuring undesired transmission below cut-off.
  • Essential for verifying spectrometer stray light, helping ensure compliance with Beer-Lambert law linearity and maintaining instrument performance.
DOCUMENTS AND RESOURCES
Certified Reference Materials for Spectroscopy
Starna Cell Catalogue Original V002 05 2024 Proof 005
Stray Light Qualification for UV and Visible Spectrophotometers Using Starna Glasses

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