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Perkin Elmer

950 UV-VIS

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Perkin Elmer950 UV-VIS
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What it is

The Perkin Elmer 950 is a UV/Vis/NIR spectrophotometer. The instrument is a double beam, double monochromator, all-reflecting optical system operating in the ultraviolet, visible, and near-infrared spectral range. The Perkin Elmer 950 covers a wavelength range of 175 nm to 3300 nm, with a usable range of 200 nm to 2500 nm for many measurements. The Perkin Elmer 950 uses tungsten-halogen and deuterium lamps as light sources.[2][3]

How it works

The Perkin Elmer 950 employs a double-beam, double-monochromator design with all-reflecting optics. The Perkin Elmer 950 uses deuterium and tungsten-halogen lamps, with automatic source change occurring during monochromator slewing. Programmed optical filters perform automatic filter changes. Interchangeable snap-in modules accommodate varied sample types. Detectors include a photomultiplier tube (PMT) and a lead sulfide (PbS) detector.[2][3]

Applications

The Perkin Elmer 950 is used for measuring total, diffuse, and specular transmission and reflectance. The instrument can determine concentration using the Beer-Lambert law, measure absorbance, and apply the Kubelka-Munk function. Applications include glancing reflectance of glass and other optical components, quantification of colored materials, identification of material concentration, determination of band-gap of semiconductors, and time-of-reaction studies.[2][3]

What do the numbers mean?

Optics & imaging2

Wavelength range
175 to 3300 nm[2]
Accurate?
Detectors
PMT and PbS Detectors[2]
Accurate?

Configuration & options5

OEM
Perkin Elmer[1]
Accurate?
Model
950[1]
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Equipment type
UV-VIS Spectrometer[1]
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Lamps
Tungsten-halogen and Deuterium lamps[2]
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Modules
Interchangeable snap-in modules for varied sample types[2]
Accurate?
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Where are the manuals?

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Not publicly documented

Field notes

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Frequently asked questions

What is the wavelength range of the Perkin Elmer 950?

The instrument covers 175 nm to 3300 nm, with a usable range of 200 nm to 2500 nm.[2][3]

What light sources does the Perkin Elmer 950 use?

The instrument uses deuterium and tungsten-halogen light sources, with automatic source change during monochromator slewing.[3]

What are some accessories for the Perkin Elmer 950?

Available accessories include a 150 mm integrating sphere, dual sampling compartments, an extended range InGaAs detector, SRS spectral standards, and an ARTA (Automated Reflectance/Transmittance Analyzer).[3]

Can the Perkin Elmer 950 measure reflectance and transmittance?

Yes, the instrument can measure total, diffuse, and specular transmission and reflectance.[3]

Not publicly documented

The following facts about the 950 UV-VIS are absent from this record as of this revision. First-hand knowledge or a citation closes a gap; every submission is reviewed before publication.

  • No publicly documented production dates or lifecycle milestones (introduction, end of production, EOL) for the 950 UV-VIS are on record.

    Answerable by: OEM historical records or a trade-press announcement

  • No publicly documented variants, configuration options, or revision breakpoints of the 950 UV-VIS are on record.

    Answerable by: an OEM product catalog or an engineer who ordered or specified the tool

  • The control-system platform and OS era of the 950 UV-VIS are not on record.

    Answerable by: an engineer who operated it or OEM installation records

  • No publicly documented failure modes or field errata for the 950 UV-VIS are on record.

    Answerable by: a field service engineer, process engineer, or maintenance technician

  • The process node or technology generation of the 950 UV-VIS is not on record.

    Answerable by: an OEM datasheet or a fab qualification report

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Sources & citations

Sources (3)Every fact above is drawn from these public sources
  1. [1]Equipment inventory listing
  2. [2]mcl.mse.utah.edu — mcl.mse.utah.edumcl.mse.utah.edu
  3. [3]Perkin Elmer LAMBDA 950 UV-VIS-NIR Spectrophotometer - ferusmedical.com — ferusmedical.comferusmedical.com
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Last updated Sep 24, 2026.

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