ASTM E490-2000a(2014) 9815 Standard Solar Constant and Zero Air Mass Solar Spectral Irradiance Tables《标准太阳能常数和气团起始阳光能光谱辐照表》.pdf
《ASTM E490-2000a(2014) 9815 Standard Solar Constant and Zero Air Mass Solar Spectral Irradiance Tables《标准太阳能常数和气团起始阳光能光谱辐照表》.pdf》由会员分享,可在线阅读,更多相关《ASTM E490-2000a(2014) 9815 Standard Solar Constant and Zero Air Mass Solar Spectral Irradiance Tables《标准太阳能常数和气团起始阳光能光谱辐照表》.pdf(16页珍藏版)》请在麦多课文档分享上搜索。
1、Designation: E490 00a (Reapproved 2014)StandardSolar Constant and Zero Air Mass Solar Spectral IrradianceTables1This standard is issued under the fixed designation E490; the number immediately following the designation indicates the year oforiginal adoption or, in the case of revision, the year of l
2、ast 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 tables define the solar con
3、stant and zero air masssolar spectral irradiance for use in thermal analysis, thermalbalance testing, and other tests of spacecraft and spacecraftcomponents and materials. Typical applications include thecalculation of solar absorptance from spectral reflectance dataand the specification of solar UV
4、 exposure of materials duringsimulated space radiation testing.1.2 These tables are based upon data from experimentalmeasurements made from high-altitude aircraft, spacecraft, andthe earths surface and from solar spectral irradiance models.1.3 The values stated in SI units are to be regarded asstand
5、ard. Other units of measurement are included for infor-mation purposes 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 appro-priate safety and health practices and determi
6、ne the applica-bility of regulatory limitations prior to use.2. Referenced Documents2.1 ASTM Standards:2E349 Terminology Relating to Space Simulation3. Terminology3.1 air mass (optical air mass) (AM),nthe ratio of thepath length or radiation through the atmosphere (lm)atanygiven angle, Z degrees, to
7、 the sea level path length toward thezenith (lz).AM 5 lm/lzsecZ , for Z #62 (1)Symbol: AM1 (air mass one), AM2 (air mass two)3.2 astronomical unit (AU),na unit of length defined asthe mean distance between the earth and the sun, that is,149 597 890 6 500 km.3.3 integrated irradiance, nspectral irrad
8、iance integratedover a specific wavelength interval from 1to 2, measured inWm2, Symbol:E1225 *12Ed (2)3.4 irradiance at a point on a surface (E) , nquotient ofthe radiant flux incident on an element of the surface contain-ing the point, by the area of that element, measured in Wm2.3.5 irradiance, sp
9、ectral (E), nthe irradiance per unitwavelength interval at a specific wavelength, or as a functionof wavelength measured in Wm2m1.3.6 solar constant, nthe total solar irradiance at normalincidence on a surface in free space at the earths meandistance from the sun (1 AU).3.7 zero air mass (AMO),nthe
10、absence of atmosphericattenuation of the solar irradiance at one astronomical unitfrom the sun.3.8 Additional definitions will be found in TerminologyE349.4. Solar Constant4.1 The solar constant is 1366.1 Wm2. This value is themean of daily averages from six different satellites over the1978 to 1998
11、 time period, all measured with absolute cavityradiometers, as reported by Frhlich and Lean (1)3. Thestandard deviation of this mean value is 425 ppm, with a0.37 % minimum-to-maximum range (1363 to 1368 Wm2).4.2 Table 1 summarizes the results in different units, andTable 2 presents the total solar i
12、rradiance at various planetarydistances from the sun.1These tables are under the jurisdiction of ASTM Committee E21 on SpaceSimulation and Applications of Space Technology and are the direct responsibilityof Subcommittee E21.04 on Space Simulation Test Methods.Current edition approved April 1, 2014.
13、 Published April 2014. Originallyapproved in 1973. Last previous edition approved in 2006 as E49 00a(2006). DOI:10.1520/E0490-00AR14.2For referenced ASTM standards, visit the ASTM website, www.astm.org, orcontact ASTM Customer Service at serviceastm.org. For Annual Book of ASTMStandards volume infor
14、mation, refer to the standards Document Summary page onthe ASTM website.3The boldface numbers in parentheses refer to the list of references at the end ofthese tables.Copyright ASTM International, 100 Barr Harbor Drive, PO Box C700, West Conshohocken, PA 19428-2959. United States15. Solar Spectral I
15、rradiance (Zero Air Mass)5.1 The zero air mass solar spectral irradiance is based ondata from satellites, space shuttle missions, high-altitudeaircraft, rocket soundings, ground-based solar telescopes, andmodeled spectral irradiance.5.2 Table 3 presents the solar spectral irradiance in tabularform f
16、or the range from 0.1195 to 1000 m. The first columngives the wavelength () in m; the second gives the spectralirradiance (E)at in Wm2m1; the third gives the totalirradiance for the range from 0 to (E0-)inWm2; and thefourth gives the percentage of the solar constant associatedwith wavelengths shorte
17、r than (D0-).5.3 Table 4 presents an abridged version of Table 3. Fig. 1plots the Standard Solar Spectral Irradiance.5.4 The Upper Atmosphere Research Satellite (UARS)/ATLAS-2 spectrum is used between 0.1195 and 0.3795 m.The values are averages of two different instruments, the SolarUltraviolet Spec
18、tral Irradiance Monitor (SUSIM) and the SolarStellar Irradiance Comparison Experiment (SOLSTICE), re-ported by Woods et al (2). These data were obtained in April1993 during a period of moderate solar activity and were scaledby a factor of 0.968 43 to match the Neckel and Labs (3) dataover the 0.33-
19、to 0.41-m range.5.5 In the 0.41- to 0.825-m range, the values are from theMcMath Solar Telescope at Kitt Peak, Arizona, as reported byNeckel and Labs (3).5.6 In the 0.825- to 4.0-m range, the values are from thehigh-resolution solar atlas computed by Kurucz (4). These datawere smoothed to the 2- and
20、 20-nm wavelength resolution ofTable 3 and scaled by a factor of 1.000 85 to match the Neckeland Labs (3) data at 0.825 m.5.7 In the 4.0- to 1000-m range, the values are from thelogarithmic irradiance versus wavelength fits reported bySmith and Gottlieb (5). These data were scaled by a factor of0.99
21、4 37 to match the Kurucz (4) data at 4.0 m.5.8 The composite spectral irradiance data were then scaledby a factor of 0.997 45 to force the integrated total irradianceto equal the solar constant.6. Keywords6.1 extraterrestrial; solar constant; solar spectral irradiance;space; zero air massTABLE 1 The
22、 Solar Constant in Alternative UnitsSolar constant = 1366.1 Wm2SI unit= 0.136 61 Wcm2= 136.61 m Wcm2=1.3661106ergcm2s-1= 126.9 Wft2= 1.959 calcm2min1(0.03calcm2min1)= 0.0326 calcm2s1= 433.4 Btuft2h1= 0.1202 Btuft2s1= 1.956 Langleysmin1The calorie is the thermochemical calorie-gram and is defined as
23、4.1840absolute joules.The Btu is the thermochemical British thermal unit and is defined by therelationship: 1 Btu (thermochemical)/(Flb) = 1 calg (thermochemical)/(Cg).The Langley, however, is defined in terms of the older thermal unit the calorieg(mean), that is, 1 Langley = 1 calg (mean)cm2; 1 cal
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