A method is presented for calculating electron temperatures ( T e ) in dense plasmas, which does not assume equivalence with the excited level distribution temperatures ( T ex). The method involves the upper-level Saha ionization equation at the ionization limit, the limiting weighted population density ( N I / g I ) obtained from measured population densities and the experimentally obtained electron density. Electron temperatures calculated for 0.1-bar hydrogen and 1-atm helium and argon arcs are found to be up to twice as large as excited level distribution temperatures. For subatmospheric argon arcs, the calculated T e are equivalent to the excitation temperature of the middle levels, but are two to three times smaller than the quoted T ex for the highest levels. Reasons are discussed for the apparent invisibility of true electron temperatures and for differences between them and the excitation temperatures.
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