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AS
AS 1515.1-1994

AS 1515.1-1994

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Current

The latest, up-to-date edition.

Copper alloys Determination of lead in copper alloys (flame atomic absorption spectrometric method) (Reconfirmed 2016)

Available format(s)

Hardcopy , PDF 1 User , PDF 3 Users , PDF 5 Users , PDF 9 Users

Language(s)

English

Published date

09-19-1994

Publisher

Standards Australia

Specifies a flame atomic absorption spectrometric method for the determination of lead content between 0.01 percent and 10 percent in copper alloys containing a maximum of 10 percent aluminium, 80 percent copper, 5 percent iron, 5 percent manganese, 40 percent nickel, 3 percent silicon, 10 percent tin and 40 percent zinc.

This Standard sets out the flame atomic absorption spectrometric method for the determination of lead in copper alloys. It is applicable to the range of 0.01% to 10% lead. The method has been found satisfactory in the presence of the following elements up to the concentrations indicated:Aluminium . . . . . . . . . . . . . . . . . . . . . . . . 10%Copper . . . . . . . . . . . . . . . . . . . . . . . . . . . 80%Iron . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5%Manganese . . . . . . . . . . . . . . . . . . . . . . . . 5%Nickel . . . . . . . . . . . . . . . . . . . . . . . . . . . 40%Silicon . . . . . . . . . . . . . . . . . . . . . . . . . . . 3%Tin . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10%Zinc . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 40%

Committee
CH/10
DocumentType
Standard
ISBN
0 7262 8983 3
Pages
6
ProductNote
Reconfirmed 02/09/2016.This standard has been reconfirmed in Australia in 2016 and remains current in New Zealand. Reconfirmation Notice 02/09/2016
PublisherName
Standards Australia
Status
Current
Supersedes

First published as AS K209.1-1970.Revised and redesignated AS 1515.1-1994.Reconfirmed 2016. First published as AS K209.1-1970. Revised and redesignated AS 1515.1-1994.

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Hardcopy - English
PDF 1 User - English
PDF 3 Users - English
PDF 5 Users - English
PDF 9 Users - English
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