ASTM E307-1972(2014) 0333 Standard Test Method for Normal Spectral Emittance at Elevated Temperatures《升高温度时标准光谱发射的标准试验方法》.pdf
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1、Designation: E307 72 (Reapproved 2014)Standard Test Method forNormal Spectral Emittance at Elevated Temperatures1This standard is issued under the fixed designation E307; the number immediately following the designation indicates the year oforiginal adoption or, in the case of revision, the year of
2、last revision. A number in parentheses indicates the year of last reapproval. Asuperscript epsilon () indicates an editorial change since the last revision or reapproval.1. Scope1.1 This test method describes a highly accurate techniquefor measuring the normal spectral emittance of electricallycondu
3、cting materials or materials with electrically conductingsubstrates, in the temperature range from 600 to 1400 K, and atwavelengths from 1 to 35 m.1.2 The test method requires expensive equipment andrather elaborate precautions, but produces data that are accu-rate to within a few percent. It is sui
4、table for researchlaboratories where the highest precision and accuracy aredesired, but is not recommended for routine production oracceptance testing. However, because of its high accuracy thistest method can be used as a referee method to be applied toproduction and acceptance testing in cases of
5、dispute.1.3 The values stated in SI units are to be regarded as thestandard. The values in parentheses are for information only.1.4 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
6、appro-priate safety and health practices and determine the applica-bility of regulatory limitations prior to use.2. Referenced Documents2.1 ASTM Standards:2E349 Terminology Relating to Space Simulation3. Terminology3.1 Definitions of Terms Specific to This Standard:3.1.1 spectral normal emittancethe
7、 term as used in thisspecification follows that advocated by Jones (1),3Worthing(2), and others, in that the word emittance is a property of aspecimen; it is the ratio of radiant flux emitted by a specimenper unit area (thermal-radiant exitance) to that emitted by ablackbody radiator at the same tem
8、perature and under the sameconditions. Emittance must be further qualified in order toconvey a more precise meaning. Thermal-radiant exitance thatoccurs in all possible directions is referred to as hemisphericalthermal-radiant exitance. When limited directions of propaga-tion or observation are invo
9、lved, the word directional thermal-radiant exitance is used. Thus, normal thermal-radiant exitanceis a special case of directional thermal-radiant exitance, andmeans in a direction perpendicular (normal) to the surface.Therefore, spectral normal emittance refers to the radiant fluxemitted by a speci
10、men within a narrow wavelength intervalcentered on a specific wavelength and emitted in a directionnormal to the plane of an incremental area of a specimenssurface. These restrictions in angle occur usually by themethod of measurement rather than by radiant flux emissionproperties.NOTE 1All the term
11、inology used in this test method has not beenstandardized. Terminology E349 contain some approved terms. Whenagreement on other standard terms is reached, the definitions used hereinwill be revised as required.4. Summary of Test Method4.1 The principle of the test method is a direct comparisonof the
12、 radiant flux from a specimen at a given temperature tothe radiant flux of a blackbody at the same temperature andunder the same environmental conditions of atmosphere andpressure. The details of this test method are given by Harrisonet al (3) and Richmond et al (4).4.2 The essential features of the
13、 test method are the use ofa double-beam ratio-recording infrared spectrophotometer withvariable slit widths, which combines and compares the signalsfrom the specimen and the reference blackbody through amonochromator system which covers the wavelength rangefrom1to35m(Note 2). According to Harrison
14、et al (3) adifferential thermocouple with suitable instrumentation is usedto maintain a heated specimen and the blackbody at the sametemperature.NOTE 2An electronic-null, ratio-recording spectrophotometer is pre-ferred to an optical-null instrument for this use. It may be difficult toobtain and main
15、tain linearity of response of an optical-null instrument ifthe optical paths are not identical to those of the instrument as manufac-tured.1This test method is under the jurisdiction of ASTM Committee E21 on SpaceSimulation and Applications of Space Technology and is the direct responsibility ofSubc
16、ommittee E21.04 on Space Simulation Test Methods.Current edition approved April 1, 2014. Published April 2014. Originallyapproved in 1968. Last previous edition approved in 2008 as E307 72(2008). DOI:10.1520/E0307-72R14.2For referenced ASTM standards, visit the ASTM website, www.astm.org, orcontact
17、ASTM Customer Service at serviceastm.org. For Annual Book of ASTMStandards volume information, refer to the standards Document Summary page onthe ASTM website.3The boldface numbers in parentheses refer to the list of references at the end ofthis test method.Copyright ASTM International, 100 Barr Har
18、bor Drive, PO Box C700, West Conshohocken, PA 19428-2959. United States15. Significance and Use5.1 The significant features are typified by a discussion ofthe limitations of the technique. With the description andarrangement given in the following portions of this testmethod, the instrument will rec
19、ord directly the normal spectralemittance of a specimen. However, the following conditionsmust be met within acceptable tolerance:5.1.1 The effective temperatures of the specimen and black-body must be within1Kofeach other. Practical limitationsarise, however, because the temperature uniformities ar
20、e oftennot better than a few degrees Kelvin.5.1.2 The optical path length in the two beams must beequal, or the instrument should operate in a nonabsorbingatmosphere or a vacuum, in order to eliminate the effects ofdifferential atmospheric absorption in the two beams. Measure-ments in air are in man
21、y cases important, and will notnecessarily give the same results as in a vacuum, thus theequality of the optical paths for dual beam instruments be-comes very critical.NOTE 3Very careful optical alignment of the spectrophotometer isrequired to minimize differences in absorptance along the two paths
22、of theinstrument, and careful adjustment of the chopper timing to reduce“cross-talk” (the overlap of the reference and sample signals) as well asprecautions to reduce stray radiation in the spectrometer are required tokeep the zero line flat. With the best adjustment, the “100 % line” will beflat to
23、 within 3 %; both of these measurements should be reproduciblewithin these limits (see 7.3, Note 6).5.1.3 Front-surface mirror optics must be used throughout,except for the prism in prism monochromators and the gratingin grating monochromators, and it should be emphasized thatequivalent optical elem
24、ents must be used in the two beams inorder to reduce and balance attenuation of the beams byabsorption in the optical elements. It is recommended thatoptical surfaces be free of SiO2and SiO coatings; MgF2maybe used to stabilize mirror surfaces for extended periods oftime. The optical characteristics
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