ASTM B568-1998(2009) Standard Test Method for Measurement of Coating Thickness by X-Ray Spectrometry《用X射线光度法测量镀层厚度的标准试验方法》.pdf
《ASTM B568-1998(2009) Standard Test Method for Measurement of Coating Thickness by X-Ray Spectrometry《用X射线光度法测量镀层厚度的标准试验方法》.pdf》由会员分享,可在线阅读,更多相关《ASTM B568-1998(2009) Standard Test Method for Measurement of Coating Thickness by X-Ray Spectrometry《用X射线光度法测量镀层厚度的标准试验方法》.pdf(8页珍藏版)》请在麦多课文档分享上搜索。
1、Designation: B568 98 (Reapproved 2009)Standard Test Method forMeasurement of Coating Thickness by X-Ray Spectrometry1This standard is issued under the fixed designation B568; the number immediately following the designation indicates the year oforiginal adoption or, in the case of revision, the year
2、 of last revision. A number in parentheses indicates the year of last reapproval. Asuperscript epsilon () indicates an editorial change since the last revision or reapproval.This standard has been approved for use by agencies of the Department of Defense.1. Scope1.1 This test method covers the use o
3、f X-ray spectrometry todetermine thickness of metallic and some nonmetallic coatings.1.2 The maximum measurable thickness for a given coatingis that thickness beyond which the intensity of the character-istic secondary X radiation from the coating or the substrate isno longer sensitive to small chan
4、ges in thickness.1.3 This test method measures the mass of coating per unitarea, which can also be expressed in units of linear thicknessprovided that the density of the coating is known.1.4 Problems of personnel protection against radiation gen-erated in an X-ray tube or emanating from a radioisoto
5、pesource are not covered by this test method. For information onthis important aspect, reference should be made to currentdocuments of the National Committee on Radiation Protectionand Measurement, Federal Register, Nuclear Regulatory Com-mission, National Institute of Standards and Technology (for-
6、merly the National Bureau of Standards), and to state and localcodes if such exist.1.5 This standard does not purport to address all of thesafety concerns, if any, associated with its use. It is theresponsibility of the user of this standard to establish appro-priate safety and health practices and
7、determine the applica-bility of regulatory limitations prior to use.2. Referenced Documents2.1 ASTM Standards:2E135 Terminology Relating to Analytical Chemistry forMetals, Ores, and Related Materials2.2 International Standard:ISO 3497 Metallic CoatingsMeasurement of CoatingThicknessX-ray Spectrometr
8、ic Methods3. Terminology3.1 Definitions of technical terms used in this test methodmay be found in Terminology E135.4. Summary of Test Method4.1 ExcitationThe measurement of the thickness of coat-ings by X-ray spectrometric methods is based on the combinedinteraction of the coating and substrate wit
9、h incident radiationof sufficient energy to cause the emission of secondary radia-tions characteristic of the elements composing the coating andsubstrate. The exciting radiation may be generated by an X-raytube or by certain radioisotopes.4.1.1 Excitation by an X-Ray TubeSuitable exciting radia-tion
10、 will be produced by an X-ray tube if sufficient potential isapplied to the tube. This is on the order of 35 to 50 kV for mostthickness-measurement applications. The chief advantage ofX-ray tube excitation is the high intensity provided.4.1.2 Excitation by a RadioisotopeOf the many availableradioiso
11、topes, only a few emit gamma radiations in the energyrange suitable for coating-thickness measurement. Ideally, theexciting radiation is slightly more energetic (shorter in wave-length) than the desired characteristic X rays. The advantagesof radioisotope excitation include more compact instrumenta-
12、tion essentially monochromatic radiation, and very low back-ground intensity. The major disadvantage of radioisotopeexcitation is the much lower intensities available as comparedwith X-ray tube sources. X-ray tubes typically have intensitiesthat are several orders of magnitude greater than radioisot
13、opesources. Due to the low intensity of radioisotopes, they areunsuitable for measurements on small areas (less than 0.3 mmin diameter). Other disadvantages include the limited numberof suitable radioisotopes, their rather short useful lifetimes, andthe personnel protection problems associated with
14、high-intensity radioactive sources.4.2 DispersionThe secondary radiation resulting from theexposure of an electroplated surface to X radiation usuallycontains many components in addition to those characteristic1This test method is under the jurisdiction ofASTM Committee B08 on Metallicand Inorganic
15、Coatings and is the direct responsibility of Subcommittee B08.10 onTest Methods.Current edition approved Sept. 1, 2009. Published December 2009. Originallyapproved in 1972. Last previous edition approved in 2004 as B568 04. DOI:10.1520/B0568-98R09.2For referenced ASTM standards, visit the ASTM websi
16、te, 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 State
17、s.of the coating metal(s) and the substrate. It is necessary,therefore, to have a means of separating the desired compo-nents so that their intensities can be measured. This can bedone either by diffraction (wavelength dispersion) or byelectronic discrimination (energy dispersion).4.2.1 Wavelength D
18、ispersionBy means of a single-crystalspectrogoniometer, wavelengths characteristic of either thecoating or the substrate may be selected for measurement.Published data in tabular form are available that relate spec-trogoniometer settings to the characteristic emissions of ele-ments for each of the c
19、ommonly used analyzing crystals.4.2.2 Energy DispersionX-ray quanta are usually speci-fied in terms of their wavelengths, in angstroms (), or theirequivalent energies in kiloelectron volts (keV). The relation-ship between these units is as follows:keV!512.396where:keV = the quantum energy in thousan
20、ds of electron volts,and = the equivalent wavelength in angstroms (10-10m).In a suitable detector (see 4.3.2), X rays of different energieswill produce output pulses of different amplitudes. Aftersuitable amplification, these pulses can be sorted on the basisof their amplitudes and stored in certain
21、 designated channels ofa multichannel analyzer, each adjacent channel representing anincrement of energy. Typically, a channel may represent a spanof 20 eV for a lithium-drifted silicon detector or 150 to 200 eVfor a proportional counter. From six to sixty adjacent channelscan be used to store the p
22、ulses representing a selectedcharacteristic emission of one element, the number of channelsdepending on the width of the emission peak (usually displayedon the face of a cathode ray tube). The adjacent channels usedto store the pulses from the material under analysis are calledthe “region of interes
23、t” or ROI.4.3 Detection:4.3.1 Wavelength Dispersive SystemsThe intensity of awavelength is measured by means of an appropriate radiationdetector in conjunction with electronic pulse-counting cir-cuitry, that is, a scaler. With wavelength dispersive systems, thetypes of detectors commonly used as the
24、 gas-filled types andthe scintillation detector coupled to a photomultiplier tube.4.3.2 Energy-Dispersive SystemsFor the highest energyresolution with energy dispersive systems, a solid-state devicesuch as the lithium-drifted silicon detector must be used. Thistype of detector is maintained at a ver
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