What Is X-Ray Fluorescence (XRF)
What Is X-Ray Fluorescence (XRF)
What Is X-Ray Fluorescence (XRF)
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When this primary X-ray beam illuminates the sample, it is said to be excited. The
excited sample in turn emits X-rays along a spectrum of wavelengths
characteristic of the types of atoms present in the sample. How does this happen?
The atoms in the sample absorb X-ray energy by ionizing, ejecting electrons from
the lower (usually K and L) energy levels. The ejected electrons are replaced by
electrons from an outer, higher energy orbital. When this happens, energy is
released due to the decreased binding energy of the inner electron orbital
compared with an outer one. This energy release is in the form of emission of
characteristic X-rays indicating the type of atom present. If a sample has many
elements present, as is typical for most minerals and rocks, the use of
aWavelength Dispersive Spectrometer much like that in an EPMA allows the
separation of a complex emitted X-ray spectrum into characteristic wavelengths
for each element present. Various types of detectors (gas flow proportional and
scintillation) are used to measure the intensity of the emitted beam. The flow
counter is commonly utilized for measuring long wavelength (>0.15 nm) X-rays
that are typical of K spectra from elements lighter than Zn. The scintillation
detector is commonly used to analyze shorter wavelengths in the X-ray spectrum
(K spectra of element from Nb to I; L spectra of Th and U). X-rays of intermediate
wavelength (K spectra produced from Zn to Zr and L spectra from Ba and the rare
earth elements) are generally measured by using both detectors in tandem. The
intensity of the energy measured by these detectors is proportional to the
abundance of the element in the sample. The exact value of this proportionality for
each element is derived by comparison to mineral or rock standards whose
composition is known from prior analyses by other techniques.
Applications
X-Ray fluorescence is used in a wide range of applications, including