PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM FILE_RECORDS = 1949 ^TABLE = "SOLAR.TAB" PRODUCT_CREATION_TIME = 1998-06-25T12:00:00 PRODUCT_TYPE = SOLAR_FLUX_DENSITY OBJECT = TABLE NAME = SOLAR_FLUX_DENSITY INTERCHANGE_FORMAT = ASCII ROWS = 1949 COLUMNS = 2 ROW_BYTES = 19 DESCRIPTION = "This is a table of the best available Spectral Solar Irradiance data which was published in the World Climate Research Programme (WCRP) Publication Series No. 7, WMO ITD-No. 149, pp 119-126, October 1986. The data was compiled by Christoph Wehrli, World Radiation Center (NRC), Davos-Dorf, Switzerland under WRC Publication No. 615, July 1985. This compilation of AM0 solar spectrum data is based on the following publications: Wavelengths Reference (micron) 0.200 to 0.310 G. Brasseur, and P. C. Simon 1981. J. Geophys. Res. 86, 7343. 0.310 to 0.330 J. C. Arvesen, R. N. Griffin and B. D. Pearson 1969. Applied Optics 8, 2215. 0.330 to 0.869 H. Neckel, and D. Labs 1984. Solar Physics 90, 205. 0.870 to ...IR E. V. P. Smith, and D. M. Gottlieb 1974. Space Sci. Rev. 16, 771. The solar constant (integral at 1 AU) is 1367 W/m^2. The spacing of samples is non-uniform, as follows: Wavelengths Spacing Line numbers (micron) (micron) 0.1995 to 0.3095 0.0010 1 to 111 0.3100 to 0.3304 0.0004 112 to 163 0.3305 to 0.6295 0.0010 164 to 463 0.6310 to 0.9990 0.0020 464 to 648 1.0025 to 2.9975 0.0050 649 to 1048 3.0050 to 9.9950 0.0100 1049 to 1748 10.0250 to 20.0250 0.0500 1749 to 1949 " OBJECT = COLUMN NAME = WAVELENGTH DATA_TYPE = ASCII_REAL START_BYTE = 1 BYTES = 7 FORMAT = "F7.4" UNIT = "micron" DESCRIPTION = "Wavelength of light in microns." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SOLAR_FLUX_DENSITY DATA_TYPE = ASCII_REAL START_BYTE = 9 BYTES = 9 FORMAT = "E9.3" UNIT = "W/m^2/micron" DESCRIPTION = "Solar flux density (pi*F) at 1 AU in W/m^2/micron." END_OBJECT = COLUMN END_OBJECT = TABLE END