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All (?) Features of Spekwin32

  • Plot:
    • Fast scaling, zooming, rescaling with mouse
    • Status bar at bottom displays current mouse position => fast reading of data points
    • X-axis as wavelength, wavenumbers or electron volts, complementary second x-axis possible
    • Y-axis as transmittance, absorbance, molar absorption coefficient and log(absorption coefficient)
    • Automatic choice of axis types on reading spectral data files
    • Free axis caption, font, font size
    • Grid mode
    • Spectra display with arbitrary colour, line type, line width
    • Display of two-dimensional fluorescence spectra (EEM)
    • Drag&Drop for Spekwin32-readable files
    • Changing and saving many options in configuration dialog

  • Data import, Graphics/Data export:
    • Import of spectra from a multitude of spectrometers systems:
      Galactic GRAMS Software (*.spc)
      Perkin Elmer UV/VIS, fluorescence & Raman spectrometers (*.sp)
      Avantes AvaSoft Software (*.tat, *.tit, *.trt, *.ttt)
      Varian Cary 50
      (*.csv)
      Beckman Coulter DU 600/7000 (*.scn, *.asc)
      Hewlett Packard 8453 (*.csv)
      Scinco Neosys 2000 UV/Vis spectrometer (*.csv)
      Bio-Rad FTS 3000 MX FTIR spectrometer (*.csv)
      Thermo Electron Helios Alpha spectrometer (*.csv)
      WTW photoLab spectral software (*.csv)
      Milton Roy Spectronic 3000 (*.asc)
      IKS XDAP (*.spk)
      Roper Scientific / Princeton Instruments WinSpec/WinView Software binary files (*.spe)
      Princeton Instruments WinSpec 1.6-Software ASCII files (*.prn)
      UV/VIS/NIR/IR- and Raman-spectra in JCAMP-DX 4.24/5.00 standard (*.dx, *.jdx)
    • Graphics export as WMF, GIF, PNG, TIFF or BMP via Clipboard or printer
    • Data export as:
      ASCII file, 2 variations (*.dat and *.csv)
      Gnuplot parameter file
      THERMO Galactic/GRAMS *.spc file
      JCAMP-DX file (*.dx) or as
      space-saving Spekwin32 binary file
      Export to Clipboard

  • Processing of Spectra:
    • Baseline Correction
    • Spike Removal
    • Correction of fluorescence spectra
    • Normalization
    • Smoothing
    • Finding Peaks
    • Changing of legend captions
    • Cutting partial spectra
    • Sorting spectra / changing order
    • Delete spectra

  • Calculations from Spectra:
    • Addition, subtraction, multiplication, division of spectra with each others
    • Addition, subtraction, multiplication, division of spectra with constant values in x- and y-axis
    • Averaging
    • Differentiation (1. - 4. order)
    • Integration
    • Concentration from absorbance& absorption coefficient
    • absorption coefficient from absorbance& Concentration
    • Oscillatory strength
    • Effective absorbance
    • transmittance / reflectance spectra from two intensity spectra
    • film thickness determination
    • Center of gravity (with fluorescence spectra)
    • Fluorescence quantum yield (temperatur dependence possible)
    • Degree of polarization
    • Reduced spectrum from S and P polarized spectra
    • Calculation & displaying of two-dimensional fluorescence spectra
    • Calculation of excitation spectra from two-dimensional fluorescence spectra
    • Fit of Gauss curves to present spectra / simulation of spectra with Gauss curve
 © 2001-2010: Dr. Friedrich Menges. Last Change: October 12, 2011