Optional program FilmStar MEASURE controls and acquires data from
popular spectrophotometers. It provides optics users with an  alternative
to the chemist's software supplied by instrument manufacturers.

MEASURE is highly integrated with FilmStar DESIGN and includes FilmStar development modules. The instruments listed below are currently supported.  Please contact us for information about other models. Please note that Hitachi and Shimadzu do not currently support third-party software. Our Hitachi support is only for older models.

Why buy MEASURE when you already have PerkinElmer or Cary software?

  • Automation...Object-level integration with other Windows software.
  • Easy-to-use software designed specifically for the optics industry.
  • Far more responsive support. Just try reaching a software engineer at
  • Integration with industry-standard database technology that connects to your company's enterprise software.
  • Same software for different instruments. Surely this is a 'no-brainer'!
PerkinElmer

Lambda 2/20/40 (etc.), 9, 19, 650-1050 (URA), 580B through 983G (IR models), Spectrum GX (2000) FTIR (Optica), Spectrum One

Agilent (HP) 8453 Diode-Array
Varian Associates Cary 1-5 (100-500, 4000- 6000i)
Hitachi U-3210, U-3410 (3200/3400)
Ocean Optics All models supported by OOIBase32
Carl Zeiss MCS 500 Series

 

Agilent 8453 Spectrometer
Agilent 8453


Varian Cary 4000

Perkin-Elmer Spectrometers
PerkinElmer Lambda 900


PerkinElmer Spectrum One


Ocean Optics


Perkin-Elmer 983


The FilmStar MEASURE fee covers all supported instruments. Program modes include
  • Transmittance (optical density)
  • V (relative) reflectance
  • VW (absolute) reflectance

Data file types include

  • Sample...scan of coated part
  • Baseline...scan of black sample, usually 0%
  • Reference...transmittance of empty sample holder, reflectance of uncoated optic, etc.
  • Standard...known values corresponding to reference scan

Data files may be loaded from disk, scanned or replaced by constants where appropriate. During data acquisition results are plotted on-screen in spectrophotometer units (usually 0-100%); final reduced values are displayed in physical units. Spectra can be utilized in DESIGN and INDEX for inverse synthesis.

Scan range is defined by wavelength/ wavenumber minimum, maximum and interval. In addition a Wave List can be specified; this is useful for filters with varying characteristics in different bands, i.e. broad-band blocking in two regions and narrow band transmission in another. The Wave List is also useful for devices whose specifications are defined at particular laser wavelengths.

Supported  formats for measured data files include

  • .csv, comma-separated values ( Excel-compatible)
  • .dx, J-CAMP spectroscopy format
  • .spc, Galactic Industries GRAMS format


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PE Lambda 900 Settings

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PE 983G Settings

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PE Spectrum GX (2000) Settings

Instrument Settings

Scan methods are edited in MEASURE and uploaded as required. While the application software supplied by spectrophotometer manufacturers is not run during MEASURE operation, there are cases where manufacturer's system software is utilized:

  • PE's Spectrum software is required for BX (1000) and GX (2000) initialization and setup. Configurations are stored as Setup Files (.set ). The name of the setup file is subsequently specified in MEASURE. Since MEASURE can change scan range, only a few Setup Files are required in practice.
  • Varian's WinUV is required for Cary 1-5 (100-500) operation. Only a minimum installation (Cary System + Scan application) is needed.
  • PE's UV Winlab 5.1 is required for Lambda 650-950 operation with URA (Universal Reflectance Accessory).

PerkinElmer Lambda 18/19 is supported on Windows 2000/XP via a new PCI board and custom cable (contact us for details). The older Lambda 19 ISA board requires Windows 95/98 and an older computer (~400MHz). The Agilent 8453 version supports NI and HP IEEE-488 cards.

Information

Need someone to service older PerkinElmer instruments? We suggest you contact Mono Instruments.


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8453 Lamp Intensity Test

8453 Diagnostic Capabilities

The Agilent (HP) 8453 version of MEASURE includes numerous diagnostic capabilities. This reduces or eliminates the need to use ChemStation software for diagnostic purposes. 

Film Thickness Module
    

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Fringe counting for
moderately thick films

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FFT method for
very thick films

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FFT verification
window

The Film Thickness Module enables users to quickly and automatically obtain film thickness in cases where films are thick enough to display fringes. Fringe counting and FFT algorithms are available. Applications include lacquers and similar coatings. While film index must be known with reasonable accuracy, the substrate index is not required. A calibration routine compensates for any resulting errors.

The program is intended as an industrial tool and runs standalone or as ActiveX client or server. It includes FilmStar BASIC and can run MEASURE or be run from MEASURE. It can be used directly with our Ocean Optics or Zeiss ActiveX servers. It provides smoothing algorithms for dealing with noisy spectra. Test spectra (with noise added) can be generated in FilmStar DESIGN.

A free 16-bit version of the program is available. This lacks any automation features.

Get Acrobat Reader A paper Film Thickness of 'Thick Thin Films' by Spectroscopy (129K) presented at the SVC 1998 meeting in Boston can be downloaded and printed.

Copyright © 2008 FTG Software Associates
Last updated on February 23, 2008