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 Encyclopedia of Physical Science and Technology  en001d42  April 28, 2001  15:9






               770                                                                                 Atomic Spectrometry


               developing time, and chemicals for the development pro-  III. ATOMIC EMISSION SPECTROMETRY
               cess). Today, photomultipliers (PMT), photodiodes, and
               array detectors completely dominate the photon detection  A. Theoretical Background
               arena.Schematicrepresentationsforaphotomultiplierand
                                                                 In atomic emission spectrometry, the intensity of emis-
               a charge injection device (a two-dimensional array detec-
                                                                 sion from the analyte atoms depends on the number of
               tor) are shown in Fig. 4. Photomultipliers and photodiodes
                                                                 atoms that are in the excited state. If the temperature of
               are used as single-channel detectors with both monochro-
                                                                 the atom cell is increased, then more atoms undergo en-
               mators and polychromators. Array detectors are used for
                                                                 ergy exchange collisions with the surrounding hot gases.
               simultaneous detection over a given spectral range.
                                                                 More atoms then possess enough energy to be excited to
                 In photomultipliers, a photon strikes the photoactive
                                                                 an upper state and drop back down to the ground state by
               material on a photocathode, resulting in ejection of an
                                                                 loss of a photon. The expression that relates the tempera-
               electron from the surface. The initial electron is acceler-
                                                                 ture of the atom cell to the number of atoms in the excited
               ated toward the first dynode, which upon collision releases
                                                                 state is the Boltzmann expression. If n 0 is the number of
               several secondary electrons. This process is repeated by
                                                                 atoms in any given state with energy E 0 , then the number
               using several additional dynodes to yield an overall signal  ∗
                               6
               amplification of 10 . Solid-state detectors (photodiodes  n in an excited state with energy E q ,isgivenby
               and charge injection devices), however, do not intrinsi-      n  ∗    n 0 = g q g 0 e −(E q −E 0 )/kT  (1)

               cally amplify the signal. In these devices, the initial pho-
               ton results in a single charge-hole separation or single  where k is the Boltzmann constant, and T is the absolute
               charge storage. In all cases, the signal from the detec-  temperature. The constants g q and g 0 are the statistical
               tor is electronically conditioned (e.g., amplified, filtered,  weights (degeneracy), which account for the fact that there
               time-gated, etc.) and is converted into an analog or digital  are often several states with the same energy E q and E 0 ,
               format to be used with a display device (e.g., computer,  respectively.
               analog gauge, digital display, etc.).               The Boltzmann expression predicts the number of
                                                                 atoms in the excited state, relative to the number of atoms
                                                                 in the ground state. For example, considering the atomic
                                                                 emission from Cs (852 nm; E q − E 0 = 1.46 eV) and Zn
                                                                 (213.8 nm; E q − E 0 = 5.8 eV) at 4000 K, the n /n 0 ra-
                                                                                                        ∗
                                                                 tios for these elements are 2.98 × 10 −2  (g q /g 0 = 2) and
                                                                 1.48 × 10 −6  (g q /g 0 = 3), respectively. Another way to use
                                                                 the above equation is to generate a plot for the Boltzmann
                                                                 factor (e −(E q −E 0 )/kT ) as a function of the excitation tem-
                                                                 perature, as shown in Fig. 5. For a given transition ( E),
                                                                 the Boltzmann factor becomes dependent only on the tem-
                                                                 perature; as a result, higher temperatures within the atom
                                                                 cellwillgeneratealargerpopulationoftheexcitedspecies,
                                                                 which ultimately leads to higher emission intensities.
                                                                   Flames have temperatures in the 2000–3000 K range,
                                                                 while atmospheric pressure plasmas are in the 4000–
                                                                 10,000 K range. In the air–acetylene flame, which has
                                                                 a temperature of about 2540 K, it is possible to see rela-
                                                                 tively large amounts of light emitted by sodium, cesium,
                                                                 calcium, and other metals, but it is very difficult to see zinc
                                                                 emission in the same flame. If a nitrous oxide–acetylene
                                                                 flame is used, with its typical temperature of 3150 K,
                                                                 larger signals from zinc and many other metals can be
                                                                 seen. In general, flames are not a convenient source for
                                                                 atomic emission measurements in light of the fact that
                                                                 in plasmas, most elements can be determined with high
                                                                 sensitivity by AES.
                                                                   The primary variable that determines the temperature
               FIGURE 4 Examples of single-channel (photomultiplier) and two-
               dimensional array (charge injection device) detectors for spectro-  necessary to excite strong atomic emission signals from a
               scopic applications.                              particular element is the energy difference (E q − E 0 ). The
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