Dispersive spectrometers measure transmission as a function of frequency (wavelength) - sequentially--same as typical CD Interferometric spectrometers.

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Presentation transcript:

Dispersive spectrometers measure transmission as a function of frequency (wavelength) - sequentially--same as typical CD Interferometric spectrometers measure intensity as a function of mirror position, all frequencies simultaneously--Multiplex advantage Sample radiation source transmitted radiation Techniques of Absorption Spectroscopy UV-vis and Infrared spectroscopy deals with absorption of radiation--detect attenuation of beam by sample at detector Frequency selector detector IoIo I T = I/I o A = -log 10 (T)

Dispersive and FT-NIR Spectrometer Wolfram-Lampe(Tungsten lamp); Gitter(Grating); Spalt(Slit); Lichtquelle(Light source); Spiegel(Mirror), Detektor(Detector); Probe(Sample), Spektrum(Spectrum)

Single, double or triple monochromator Detector: PMT or CCD for multiplex Filter Lens Sample Laser Dispersive Fluorescence or Raman -use filter or double monochromator to eliminate the intense Rayleigh scattered & reflected light --Fluorescence not big problem –Raman typically 10 8 weaker than excitation Disperse the light onto a detector to generate a spectrum Polarizer Detect intensity, I, against zero background--ideal