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On the other hand, sodium atoms are excited more easily than the atoms of most other

               elements. Nevertheless, at 3000 K only 1 sodium atom is excited for every 1000 atoms in the

               ground state. In a normal atom population there are very few atoms in states E1, E2, E3, and
               higher.

                       The total amount of radiation absorbed depends, among other things, on how many
               atoms  are  available  in  the  lower-energy  state  to  absorb  radiation  and  become  excited.

               Consequently,  the  total  amount  of  radiation  absorbed  is  greatest  for  absorptions  from  the

               ground state. Excited to excited state transitions are very rare, because there are so few excited
               atoms; only the ground state resonance lines are useful analytically in AAS.

                       For practical purposes, all absorption in AAS is by atoms in the ground state. This greatly
               restricts the number of absorption lines that can be observed and used for measurement in atomic

               absorption. Quite frequently only three or four useful lines are available in the UV/VIS spectral
               region for each element, and in some cases fewer than that.

                       AAS is useful for the analysis of approximately 70 elements, almost all of them metal or

               metalloid elements. Grotrian diagrams correctly predict that the energy required to reach even
               the first excited state of nonmetals is so great that they cannot be excited by normal UV radiation

               (>190 nm). The resonance lines of nonmetals lie in the vacuum UV region.
                       Commercial AAS systems generally have air in the optical path, and the most common

               atomizer,  the  flame,  must  operate  in  air.  Consequently,  using  flame  atomizers,  atomic

               absorption cannot be used for the direct determination of nonmetals. However, nonmetals
               have been determined by indirect methods, as will be discussed in the applications section.
























               I.2.1  SPECTRAL LINE WIDTHS
                       In flames, absorptive bandwidths of atoms typically vary from about 0.001 to 0.01 nm.

               The narrow bands of absorbed or emitted radiation that are observed with atoms are referred to
               as  spectral  lines.  For  some  elements,  such  as  iron  and  uranium,  hundreds  of  such  electron

               transitions are observed. Potassium was chosen for inclusion in because of the relatively small
               number of observed transitions.




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