ASTM E1361-2002(2007) Standard Guide for Correction of Interelement Effects in X-Ray Spectrometric Analysis《X射线光谱测定分析中共存元素效应校正的标准指南》.pdf
《ASTM E1361-2002(2007) Standard Guide for Correction of Interelement Effects in X-Ray Spectrometric Analysis《X射线光谱测定分析中共存元素效应校正的标准指南》.pdf》由会员分享,可在线阅读,更多相关《ASTM E1361-2002(2007) Standard Guide for Correction of Interelement Effects in X-Ray Spectrometric Analysis《X射线光谱测定分析中共存元素效应校正的标准指南》.pdf(12页珍藏版)》请在麦多课文档分享上搜索。
1、Designation: E 1361 02 (Reapproved 2007)Standard Guide forCorrection of Interelement Effects in X-Ray SpectrometricAnalysis1This standard is issued under the fixed designation E 1361; the number immediately following the designation indicates the year oforiginal adoption or, in the case of revision,
2、 the year of last revision. A number in parentheses indicates the year of last reapproval. Asuperscript epsilon (e) indicates an editorial change since the last revision or reapproval.1. Scope1.1 This guide is an introduction to mathematical proce-dures for correction of interelement (matrix) effect
3、s in quanti-tative X-ray spectrometric analysis.1.1.1 The procedures described correct only for the inter-element effect(s) arising from a homogeneous chemical com-position of the specimen. Effects related to either particle size,or mineralogical or metallurgical phases in a specimen are nottreated.
4、1.1.2 These procedures apply to both wavelength andenergy-dispersive X-ray spectrometry where the specimen isconsidered to be infinitely thick, flat, and homogeneous withrespect to the depth of penetration of the exciting X rays (1).21.2 This document is not intended to be a comprehensivetreatment o
5、f the many different techniques employed to com-pensate for interelement effects. Consult Refs (2-5) for descrip-tions of other commonly used techniques such as standardaddition, internal standardization, etc.2. Referenced Documents2.1 ASTM Standards:3E 135 Terminology Relating to Analytical Chemist
6、ry forMetals, Ores, and Related Materials3. Terminology3.1 For definitions of terms used in this guide, refer toTerminology E 135.3.2 Definitions of Terms Specific to This Standard:3.2.1 absorption edgethe maximum wavelength (mini-mum X-ray photon energy) that can expel an electron from agiven level
7、 in an atom of a given element.3.2.2 analytean element in the specimen whose concen-tration is to be determined.3.2.3 characteristic radiationX radiation produced by anelement in the specimen as a result of electron transitionsbetween different atomic shells.3.2.4 coherent (Rayleigh) scatterthe emis
8、sion of energyfrom a loosely bound electron that has undergone collisionwith an incident X-ray photon and has been caused to vibrate.The vibration is at the same frequency as the incident photonand the photon loses no energy. (See 3.2.7.)3.2.5 dead-timetime interval during which the X-raydetection s
9、ystem, after having responded to an incident photon,cannot respond properly to a successive incident photon.3.2.6 fluorescence yielda ratio of the number of photonsof all X-ray lines in a particular series divided by the numberof shell vacancies originally produced.3.2.7 incoherent (Compton) scatter
10、the emission of energyfrom a loosely bound electron that has undergone collisionwith an incident photon and the electron has recoiled under theimpact, carrying away some of the energy of the photon.3.2.8 influence coeffcientdesignated by a (b, g, d andother Greek letters are also used in certain mat
11、hematicalmodels), a correction factor for converting apparent massfractions to actual mass fractions in a specimen. Other termscommonly used are alpha coefficient and interelement effectcoefficient.3.2.9 mass absorption coeffcientdesignated by , anatomic property of each element which expresses the
12、X-rayabsorption per unit mass per unit area, cm2/g.3.2.10 primary absorptionabsorption of incident X raysby the specimen. The extent of primary absorption depends onthe composition of the specimen and the X-ray source primaryspectral distribution.3.2.11 primary spectral distributionthe output X-rays
13、pectral distribution usually from an X-ray tube. The X-raycontinuum is usually expressed in units of absolute intensityper unit wavelength per electron per unit solid angle.3.2.12 relative intensitythe ratio of an analyte X-ray lineintensity measured from the specimen to that of the pureanalyte elem
14、ent. It is sometimes expressed relative to theanalyte element in a multi-component reference material.1This guide is under the jurisdiction of ASTM Committee E01 on AnalyticalChemistry for Metals, Ores and Related Materials and is the direct responsibility ofSubcommittee E01.20 on Fundamental Practi
15、ces.Current edition approved Jan. 15, 2007. Published January 2007. Originallyapproved in 1990. Last previous edition approved in 2002 as E 1361 02.2The boldface numbers in parentheses refer to the list of references at the end ofthis standard.3For referenced ASTM standards, visit the ASTM website,
16、www.astm.org, orcontact ASTM Customer Service at serviceastm.org. For Annual Book of ASTMStandards volume information, refer to the standards Document Summary page onthe ASTM website.1Copyright ASTM International, 100 Barr Harbor Drive, PO Box C700, West Conshohocken, PA 19428-2959, United States.3.
17、2.13 secondary absorptionthe absorption of the charac-teristic X radiation produced in the specimen by all elements inthe specimen.3.2.14 secondary fluorescence (enhancement)the genera-tion of X rays from the analyte caused by characteristic X raysfrom other elements in the sample whose energies are
18、 greaterthan the absorption edge of the analyte.3.2.15 mass fractiona concentration unit expressed as aratio of the mass of analyte to the total mass.3.2.16 X-ray sourcean excitation source which producesX rays such as an X-ray tube, radioactive isotope, or secondarytarget emitter.4. Significance an
19、d Use4.1 Accuracy in quantitative X-ray spectrometric analysisdepends upon adequate accounting for interelement effectseither through sample preparation or through mathematicalcorrection procedures, or both. This guide is intended to serveas an introduction to users of X-ray fluorescence correctionm
20、ethods. For this reason, only selected mathematical modelsfor correcting interelement effects are presented. The reader isreferred to several texts for a more comprehensive treatment ofthe subject (2-7).5. Description of Interelement Effects5.1 Matrix effects in X-ray spectrometry are caused byabsor
21、ption and enhancement of X rays in the specimen.Primary absorption occurs as the specimen absorbs the X -raysfrom the source. The extent of primary absorption depends onthe composition of the specimen, the output energy distributionof the exciting source, such as an X-ray tube, and the geometryof th
22、e spectrometer. Secondary absorption occurs as the char-acteristic X radiation produced in the specimen is absorbed bythe elements in the specimen. When matrix elements emitcharacteristic X-ray lines that lie on the short-wavelength (highenergy) side of the analyte absorption edge, the analyte can b
23、eexcited to emit characteristic radiation in addition to thatexcited directly by the X-ray source. This is called secondaryfluorescence or enhancement.5.2 These effects can be represented as shown in Fig. 1using binary alloys as examples. When matrix effects are eithernegligible or constant, Curve A
24、 in Fig. 1 would be obtained.That is, a plot of analyte relative intensity (corrected forbackground, dead-time, etc.) versus analyte mass fractionwould yield a straight line over a wide mass fraction range andwould be independent of the other elements present in thespecimen (Note 1). Linear relation
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