cont'd.
Table 8.4
Element Flame AA Hg/ Hydride GFAA ICP Emission ICP-MSRh 4 20 0.02Ru 70 4 0.05S 50 500
Sb 30 0.1 0.2 60 0.02Sc 20 0.2 0.08Se 70 0.02 0.2 60 0.5Si 60 0.4 3 10Sm 2 000 0.04Sn 100 0.2 40 0.03Sr 2 0.02 0.05 0.02Ta 1 000 20 0.02Tb 600 0.01
Te 20 0.02 0.1 50 0.04Th 0.02Ti 50 1 0.5 0.06Tl 9 0.1 40 0.02
Tm 10 0.01U 10 000 10 0.01V 40 0.2 2 0.03W 1 000 20 0.06Y 50 0.2 0.02Yb 5 0.03Zn 0.8 0.01 1 0.08Zr 300 0.8 0.03All detection limits are given in micrograms per litre and were determined using elemental standards in dilute aqueous
solution. Atomic absorption (Model 5100) and ICP emission (Plasma II) detection limits are based on a 95% confidence
level (2 standard deviations) using instrumental parameters optimized for the individual element. ICP emission detection
limits obtained during multielement analyses will typically be within a factor of 2 of the values shown. Cold vapour
mercury AA detection limits were determined using an MHS-20 mercury/hydride system with an amalgamation
accessory. Furnace AA (Zeeman/5100) detection limits were determined using STPF conditions and are based on 100 μL
sample volumes. ICP-MS (ELAN) detection limits were determined using operating parameters optimized for full mass
range coverage and a 98% confidence level (3 standard deviations). ICP-MS detection limits using operating conditions
optimized for individual elements are frequently better than the values shown. ICP-MS detection limits for fluorine and