Vocab 4 Flashcards
The ability to separate adjacent absorption bands or spectral lines; equivalent to the spectral bandpass or amount of energy exiting a monochromator at any one time.
Resolution
The amount of radiation exiting a monochromator relative to the amount that enters the monochromator.
throughput
a general optical, acoustic, or radio frequency instrument that uses interference phenomena between a reference wave and an experimental wave, or between two parts of an experimental wave, to determine wavelengths and wave velocities, measure very small distances and thicknesses, or calculate indices of refraction.
interfoerometer
an optical instrument that produces interference fringes by dividing the source radiation with a beamsplitter such that one beam is directed into an arm of the interferometer and strikes a fixed mirror, while a second beam is directed into a different arm of the interferometer and strikes a movable mirror. When the reflected beams are brought back together, an interference pattern (the interferogram) results.
Michelson Interferometer
An optical material that is partially transmitting and partially reflecting
beamsplitter
The optical path difference between radiation in the two arms of a Michelson interferometer
optical retardation
Two electromagnetic waves having a phase difference of 180° or 180° plus an integer multiple of 360°
destructive interference
The encoding of a carrier wave by varying its frequency in accordance with an input signal.
modulation
A recording of the interference pattern generated by an interferometer.
interferogram
When radiation of multiple wavelengths is emitted by a source, the measure is the summation of the individual interferograms corresponding to each wavelength in the spectrum.
polychromatic interferogram
In a Michelson interferometer, the term that contains information about the intensities of all the frequencies that have been modulated by the interferometer.
spectrum
The point of zero path difference in an interferometer, i.e. OM = OF; in a polychromatic interferogram it is the one point at which all wavelengths constructively interfere.
centerburst
The reduction in measurement time that results from measuring all the source radiation wavelengths simultaneously in a Fourier transform instrument. demonstrated by the signal-to-noise improvement of an FT instrument over a dispersive instrument
Fellgett’s advantage / multiplex advantage
The number of measurement subdivisions, n, contained in a spectral range between wavenumber limits
resolution elements
increased signal-to-noise ratio that results from the increases signal strength observed by the detector; related to the optical throughput of an interferometric IR spectrometer θI relative to the optical throughput of a grating IR spectrometer
jacquinot’s advantage / throughput advantage
The inherent precision in the wavenumber scale of Fourier transform IR spectrometers compared to dispersive IR instruments; this inherent precision is due to the referencing of the mirror position of the moving mirror in the interferometer to an internal laser source, thereby allowing very precise measurement of d, the optical retardation
cone’s advantage / precision advantage
The process of finding a weighting function that minimizes the distortions produced by truncation of the interferogram in experimental Fourier transform infrared spectroscopy.
apodization
default truncation function in experimental interferograms that induces distortions in the resultant FT-IR spectra.
boxcar apodization function
One of the most common of the interferogram apodization functions used to minimize distortions in FT-IR spectra
triangular apodization function
Any waveform that is a sinusoidal function of time or distance can be digitized unambiguously using a sampling frequency equal to twice the bandwidth of the system. Required digitization frequency and time can be expressed as
nyquist sampling theorem
The point where the sinusoidal output signal of the reference He-Ne laser crosses the 0 voltage level in the detector electronics of an FT-IR instrument. For a 632.8 nm He-Ne laser, each zero- crossing occurs at 316.4 nm, which corresponds to the retardation distance of the moving mirror between zero-crossings.
zero-crossing
A spectroscopic instrument in which the background reference or blank is obtained separately and independently from the sample. The background is usually stored in a computer file for subsequent calculation of absorbance, transmittance, etc
single-beam spectrophotometer