Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group
  • Applied Spectroscopy
  • Vol. 54,
  • Issue 11,
  • pp. 1646-1650
  • (2000)

Calibration Procedure to Derive IRRAS Spectra from PM-IRRAS Spectra

Not Accessible

Your library or personal account may give you access

Abstract

A calibration procedure is presented to relate Fourier transform infrared reflection-absorption spectroscopy (IRRAS) spectra obtained by polarization modulation (PM) and conventional techniques. This procedure concerns only PM-IRRAS measurements obtained with a lock-in amplifier. At the first stage, it consists in measuring two calibrated spectra, by adding a linear polarizer after the sample. The corresponding corrected PM-IRRAS spectra display band intensities close to those observed on IRRAS spectra (at about 6%), but the value of the baseline is lower. The calibration procedure can be performed at the second stage, by normalizing the corrected PM-IRRAS spectra of the sample and the bare substrate. In this case, the band intensities and the baseline of the normalized corrected PM-IRRAS and IRRAS spectra are similar.

PDF Article
More Like This
Calibration improvement of Fourier transform infrared phase-modulated ellipsometry

A. Canillas, E. Pascual, and E. Bertran
J. Opt. Soc. Am. A 13(12) 2461-2467 (1996)

Simplified calibration procedure for Mueller polarimeter in transmission configuration

Haofeng Hu, Enric Garcia-Caurel, Guillaume Anna, and François Goudail
Opt. Lett. 39(3) 418-421 (2014)

Cited By

You do not have subscription access to this journal. Cited by links are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.

Contact your librarian or system administrator
or
Login to access Optica Member Subscription

Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.