Determination of the Composition of Low Purity Copper by Microwave Induced Plasma Atomic Emission Spectrometry Full article
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Atomic Spectroscopy
ISSN: 0195-5373 |
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| Output data | Year: 2025, Volume: 46, Number: 3, Pages: 251-257 Pages count : 7 DOI: 10.46770/AS.2025.004 | ||||||
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Abstract:
In this work, the conditions for determining impurity elements (e.g., Ag, As, Sn, Pb, Bi, Ni, Fe, Mn, Cd, Co,
Sb, and Zn) in a metal matrix with an average Eion were optimized for the first time using low purity copper as an example. The effect
of copper on the emission signals of elements is considered. It is shown that quantitative analysis should be carried out using matrix
matching calibration. The variants of nitrogen and argon in the nebulizer gas flow were compared and their optimal values were
selected, providing maximum emission signals for most impurities. To protect the torch from copper deposition, the value of the
outer nitrogen flow was increased, minimally changing the signal intensities of the elements. It is shown that the addition of argon to
the nebulizer gas flow decreases the limits of detection by several times for some elements which were in the range of 0.0003-
0.01% in mass. The method has been shown to
have satisfactory long-term stability, which is
maintained when nitrogen in the nebulizer is
replaced by argon. The accuracy of the analysis
was confirmed by the analysis of reference copper
materials and recoveries ranged from 80-113%.
The relative standard deviation was 3-12% for
most elements for two measurements.
Cite:
Trunova V.A.
, Polyakova E.V.
, Komin O.V.
, Pelipasov O.V.
Determination of the Composition of Low Purity Copper by Microwave Induced Plasma Atomic Emission Spectrometry
Atomic Spectroscopy. 2025. V.46. N3. P.251-257. DOI: 10.46770/AS.2025.004 WOS
Determination of the Composition of Low Purity Copper by Microwave Induced Plasma Atomic Emission Spectrometry
Atomic Spectroscopy. 2025. V.46. N3. P.251-257. DOI: 10.46770/AS.2025.004 WOS
Dates:
| Submitted: | Feb 2, 2025 |
| Published print: | Jul 28, 2025 |
| Published online: | Jul 28, 2025 |
Identifiers:
| Web of science: | WOS:001529002200004 |
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