ASTM E424-1971(2015) 0656 Standard Test Methods for Solar Energy Transmittance and Reflectance (Terrestrial) of Sheet Materials《簿板材料的太阳能传播和反射的试验方法》.pdf

《ASTM E424-1971(2015) 0656 Standard Test Methods for Solar Energy Transmittance and Reflectance (Terrestrial) of Sheet Materials《簿板材料的太阳能传播和反射的试验方法》.pdf》由会员分享，可在线阅读，更多相关《ASTM E424-1971(2015) 0656 Standard Test Methods for Solar Energy Transmittance and Reflectance (Terrestrial) of Sheet Materials《簿板材料的太阳能传播和反射的试验方法》.pdf（5页珍藏版）》请在麦多课文档分享上搜索。

1、Designation: E424 71 (Reapproved 2015)Standard Test Methods forSolar Energy Transmittance and Reflectance (Terrestrial) ofSheet Materials1This standard is issued under the fixed designation E424; the number immediately following the designation indicates the year oforiginal adoption or, in the case

2、of revision, the year 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 U.S. Department of Defense.1. Scope1.1 These t

3、est methods cover the measurement of solarenergy transmittance and reflectance (terrestrial) of materials insheet form. MethodA, using a spectrophotometer, is applicablefor both transmittance and reflectance and is the refereemethod. Method B is applicable only for measurement oftransmittance using

4、a pyranometer in an enclosure and the sunas the energy source. Specimens for Method A are limited insize by the geometry of the spectrophotometer while Method Brequires a specimen 0.61 m2(2 ft2). For the materials studiedby the drafting task group, both test methods give essentiallyequivalent result

5、s.1.2 This standard does not purport to address all of thesafety problems, if any, associated with its use. It is theresponsibility of the user of this standard to establish appro-priate safety and health practices and determine the applica-bility of regulatory limitations prior to use.2. Referenced

6、 Documents2.1 ASTM Standards:2E259 Practice for Preparation of Pressed Powder WhiteReflectance Factor Transfer Standards for Hemisphericaland Bi-Directional GeometriesE275 Practice for Describing and Measuring Performance ofUltraviolet and Visible SpectrophotometersE308 Practice for Computing the Co

7、lors of Objects by Usingthe CIE System3. Definitions3.1 solar absorptancethe ratio of absorbed to incidentradiant solar energy (equal to unity minus the reflectance andtransmittance).3.2 solar admittancesolar heat transfer taking into ac-count reradiated and convected energy.3.3 solar energyfor thes

8、e methods the direct radiationfrom the sun at sea level over the solar spectrum as defined in3.2, its intensity being expressed in watts per unit area.3.4 solar reflectancethe percent of solar radiation (watts/unit area) reflected by a material.3.5 solar spectrumfor the purposes of these methods the

9、solar spectrum at sea level extending from 350 to 2500 nm.3.6 solar transmittancethe percent of solar radiation(watts/unit area) transmitted by a material.4. Summary of Methods4.1 Method AMeasurements of spectral transmittance, orreflectance versus a magnesium oxide standard, are made usingan integr

10、ating sphere spectrophotometer over the spectral rangefrom 350 to 2500 nm.The illumination and viewing mode shallbe normal-diffuse or diffuse-normal. The solar energy trans-mitted or reflected is obtained by integrating over a standardsolar energy distribution curve using weighted or selectedordinat

11、es for the appropriate solar-energy distribution. Thedistribution at sea level, air mass 2, is used.4.2 Method BUsing the sun as the source and a pyranom-eter as a detector the specimen is made the cover of anenclosure with the plane of the specimen perpendicular to theincident radiation; transmitta

12、nce is measured as the ratio of theenergy transmitted to the incident energy. (The apparatus ofMethod B has been used for the measurement of solar-energyreflectance but there is insufficient experience with this tech-nique for standardization at present.)1These test methods are under the jurisdictio

13、n of ASTM Committee E44 onSolar, Geothermal and Other Alternative Energy Sources and is the direct respon-sibility of Subcommittee E44.05 on Solar Heating and Cooling Systems andMaterials.Current edition approved Nov. 1, 2015. Published November 2015. Originallyapproved in 1971. Last previous editio

14、n approved in 2007 as E424-71(2007). DOI:10.1520/E0424-71R15.2For referenced ASTM standards, visit the ASTM website, 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.

15、Copyright ASTM International, 100 Barr Harbor Drive, PO Box C700, West Conshohocken, PA 19428-2959. United States15. Significance and Use5.1 Solar-energy transmittance and reflectance are importantfactors in the heat admission through fenestration, most com-monly through glass or plastics. (See Appe

16、ndix X3.) Thesemethods provide a means of measuring these factors underfixed conditions of incidence and viewing. While the data maybe of assistance to designers in the selection and specificationof glazing materials, the solar-energy transmittance and reflec-tance are not sufficient to define the r

17、ate of heat transferwithout information on other important factors. The methodshave been found practical for both transparent and translucentmaterials as well as for those with transmittances reduced byhighly reflective coatings. Method B is particularly suitable forthe measurement of transmittance

18、of inhomogeneous,patterned, or corrugated materials since the transmittance isaveraged over a large area.6. Method ASpectrophotometric Method6.1 Apparatus:6.1.1 SpectrophotometerAn integrating spherespectrophotometer, by means of which the spectral character-istics of the test specimen or material m

19、ay be determinedthroughout the solar spectrum. For some materials the spec-trum region from 350 to 1800 nm may be sufficient. The designshall be such that the specimen may be placed in direct contactwith the sphere aperture for both transmission and reflection,so that the incident radiation is withi

20、n 6 of perpendicularity tothe plane of the specimen.36.1.2 Standards:6.1.2.1 For transmitting specimens, incident radiation shallbe used as the standard relative to which the transmitted lightis evaluated. Paired reflecting standards are used, prepared induplicate as described below.6.1.2.2 For refl

21、ecting specimens, use smoked magnesiumoxide (MgO) as a standard as the closest practicable approxi-mation of the completely reflecting, completely diffusingsurface for the region from 300 to 2100 nm. The preferredstandard is a layer (at least 2.0 mm in thickness) freshlyprepared from collected smoke

22、 of burning magnesium (Rec-ommend Practice E259). Pressed barium sulfate (BaSO4)orMgO are not recommended because of poor reflecting proper-ties beyond 1000 nm.6.1.3 Specimen Backing for Reflectance MeasurementTransparent and translucent specimens shall be backed by alight trap or a diffusing black

23、material which is known toabsorb the near infrared. The backing shall reflect no more than1 % at all wavelengths from 350 to 2500 nm as determinedusing the spectrophotometer.6.2 Test Specimens:6.2.1 Opaque specimens shall have at least one planesurface; transparent and translucent specimens shall ha

24、ve twosurfaces that are essentially plane and parallel.6.2.2 Comparison of translucent materials is highly depen-dent on the geometry of the specific instrument being used. Itis recommended that the specimen be placed in direct contactwith the sphere to minimize and control loss of scatteredradiatio

25、n.6.2.3 For specularly reflecting specimens the sphereconditions, especially where the reflected beam strikes thesphere wall, shall be known to be highly reflecting (95 % orhigher). It is recommended that a freshly coated sphere be usedespecially when measuring translucent or specularly reflectingsp

26、ecimens.6.3 Calibration:6.3.1 PhotometricThe calibration of the photometric scaleshall be done as recommended by the manufacturer. It shall becarefully executed at reasonable time intervals to ensureaccuracy over the entire range.6.3.2 WavelengthPeriodic calibrations should be made ofthe wavelength

27、scales. Procedures for wavelength calibrationmay be found in Recommended Practice E275. A didymiumfilter has also been used for this purpose. Although theabsorption peaks have been defined for specific resolution inthe visible spectrum it also has peaks in the near infrared;however, the wavelength o

28、f the peaks must be agreed upon,using a specific instrument.6.4 Procedure:6.4.1 TransmittanceObtain spectral transmittance datarelative to air. For measurement of transmittance of translucentspecimens, place freshly prepared matched smoked MgOsurfaces at the specimen and reference ports at the rear

29、of thesphere (Note 1). The interior of the sphere should be freshlycoated with MgO and in good condition.NOTE 1Magnesium oxide standards may be considered matched if oninterchanging them the percent reflectance is altered by no more than 1 %at any wavelength between 350 and 1800 nm.6.4.2 Reflectance

30、Obtain spectral directional reflectancedata relative to MgO. Include the specular component in thereflectance measurement. Back the test specimen with a blackdiffuse surface if it is not opaque. Depending on the requiredaccuracy, use the measured values directly or make correctionsfor instrumental 0

31、 and 100 % lines (see Method E308).6.5 CalculationSolar energy transmittance or reflectanceis calculated by integration. The distribution of solar energy asreported by Parry Moon4for sea level and air mass 2 shall beused.6.5.1 Weighted OrdinatesObtain the total solar energytransmittance, Tse, and re

32、flectance, Rse, in percent, by integrat-ing the spectral transmittance (reflectance) over the standardsolar energy distribution as follows:Tseor Rse5(5350nm52100 nmT or R!3 E(1)E for air mass 2, at 50-nm intervals, normalized to 100, isgiven in Appendix X1.6.5.1.1 This integration is easily programm

33、ed for automaticcomputation.3For additional apparatus specifications see Recommended Practice E308.4Journal of the Franklin Institute, Vol 230, 1940, p. 583, or SmithsonianPhysical Tables, Table 1, Vol 815, 1954, p. 273.E424 71 (2015)26.5.2 Selected OrdinatesIntegration is done by reading thetransmi

34、ttance or reflectance at selected wavelengths and cal-culating their average. Appendix X2 lists 20 selected ordinatesfor integration.56.6 ReportThe report shall include the following:6.6.1 Complete identification of the material tested, andwhether translucent, clear, or specularly reflecting,6.6.2 S

35、olar T percent or Solar R percent, or both, to thenearest 0.1 %,6.6.3 Specimen thickness,6.6.4 Identification of the instrument used, and6.6.5 Integration method.7. Method BPyranometer MethodNOTE 2The pyranometer is used to measure total global (sun and sky)radiation (previously designated a 180 pyr

36、oheliometer; presently thelatter word refers to a normal incidence measurement of direct solarradiation). See IGY Instruction Manual, Part VI, Radiation Instruments,Pergamon Press, New York, NY.7.1 Apparatus:7.1.1 EnclosureThe apparatus that has been used success-fully is a box capable of supporting

37、 a 0.61-m2(24-in.2)specimen. The box, which would normally be about 0.66-m2(26-in.2) outside, should be capable of being faced in anydirection, as on a universal mount. The inside of the box shouldbe painted flat black.3A typical unit is shown in Fig. 1.7.1.2 Sensor:7.1.2.1 The sensing element of th

38、is instrument is a pyra-nometer consisting of concentric rings, or wedges ofthermopiles, colored alternately black and white. The voltageoutput of this sensor is proportional to the intensity of the totalincident solar irradiation. The spectral sensitivity of thisinstrument extends from the ultravio

39、let to infrared wavelengths(280 to 2800 nm), thus encompassing all the solar spectrum.The pyranometer should be located inside the box so that thesensing thermopile is approximately 50 mm (2 in.) from thecenter of the bottom plane of the sample.7.1.2.2 The pyranometer has a viewing area of 180. AnEp

40、pley pyranometer with its 25-mm (1-in.) diameter sensingdisk, when placed in the center of the box, views the midpointof the edges of the test specimen as a cone of 160; thediagonal of the specimen is viewed as a cone of 166 when thethermopile is 50 mm (2 in.) below the bottom of the specimen.7.1.2.

41、3 Read-Out InstrumentationA recorder, or a nonre-cording meter capable of indicating in the 0.2 to 15-mV rangeare permissible for use. The output voltage of the pyranometerwill be affected by the input impedance of the meter to whichit is connected. Thus, the meter used to indicate solar intensitysh

42、ould have a very high input impedance, such as a precisionvacuum-tube voltmeter, or a meter which has been calibratedfor one particular sensing element, thus compensating for anyloading effects on that element.7.2 SpecimensThe test specimens should be not less than0.61 by 0.61 m (24 by 24 in.). If t

43、he cross-sectional shape ofthe specimen is not flat, care must be taken to prevent thepossibility of light leaks at the edges such as are caused by theuse of oversize specimens.7.3 Procedure:7.3.1 Conduct the tests on a clear sunny day with no cloudcover interruptions during the individual tests. Co

44、nduct testingbetween the hours of 9 a.m. and 3 p.m. local standard time; thisis when the solar radiation is at least 80 % of the value obtainedat solar noon for that day. In the Northern hemisphere takereadings between November and February only between 10a.m. and 2 p.m. Expose the test specimen app

45、roximatelynormal to the sun for 15 min prior to testing. Next, align thebox normal to the suns rays and take the average incidentsolar-energy reading over a period of time (normally severalminutes) until a steady trace, or reading is obtained. Then placethe test specimen on the box and again record

46、the average solarenergy reaching the sensor. When the test specimen has acorrugated or irregular surface move it across the sensingelement, and take readings at 10-mm (12-in.) intervals for thewidth of one corrugation or irregularity, and average thereadings. Also measure corrugated specimens with t

47、he corru-gations in the North-South direction and in the East-Westdirection.7.3.2 The solar energy transmittance of the test specimens isthe ratio of the energy measured when the test specimen isplaced between the sun and the sensor and the energy measuredby the sensor with no test specimen in place

48、.7.4 ReportThe report shall include the following:7.4.1 The source and identity of the test specimen,7.4.2 A complete description of the test specimen, that is,thickness, cross-sectional shape, color, size, translucent ortransparent, type of material,7.4.3 The percent solar energy transmittance to t

49、he nearest1%,7.4.4 The place, date, and time of the test,7.4.5 The intensity of the solar radiation,5Olson, O. H., “Selected Ordinates for SolarAbsorptivity Calculations,” AppliedOptics, Vol 2, No. 1, January 1963.FIG. 1 Typical Unit with Pyranometer Mounted in Black BoxE424 71 (2015)37.4.6 Type of sensing unit used, and7.4.7 Ambient air temperature.8. Keywords8.1 pyranometer; reflectance; solar energy; spectrophotom-eter; terrestrial reflectance; transmittanceAPPENDIXES(Nonmandatory Information)X1. SOLAR ENERGY TRANSMITTANCE OR REFLECTANCE US