***** File ATLSINFO.TXT This information file is located in the SOL_ATLS subdirectory of the\DOCUMENT\APPENDIX directory. Two high resolution integrated disk solar spectra compiled from a varietyof sources are presented in this directory. One was contributed by M. A'Hearnand the other by R. Kurucz. The A'Hearn solar spectrum found in one file,SOLATLS1.FIT, is given in vacuum wavelengths (Angstrom units), calibrated influx units (erg/cm**2/s/A) covering the wavelength range 2245 A to 7000 A insteps of 0.005 A. The Kurucz solar spectrum can be found in two files,SOLATLS2.FIT AND SOLATLS3.FIT, in air wavelengths (Angstrom units), calibratedin flux units (erg/cm**2/s/A). SOLATLS2.FIT covers a wavelength range 2960 Ato 8000 A in steps of 0.005 A. SOLATLS3.FIT covers the wavelength range 8000 Ato 13,000 A in steps of 0.01 A. We note a wavelength shift between the twosolar spectra presented in this archive of approximately 0.03 A in the senseA'Hearn minus Kurucz. We therfore caution users of these files requiringwavelength accuracies better than this difference to first assess and correctthe wavelengths of the solar spectra to a rest frame. [NOTE: This paragraphwas extacted from the Spectroscopy and Spectrophotometry Discipline Appendix.] Unlike most files within the set of IHW CD-ROMs these files do not haveseparate header and data files; rather there is only one combined file, a trueFITS file. The data are one dimensional spectra. The table below summarizesthe FITS header information: File Wavelength Angstroms Source range per pixel -----------------------------------------------------------------------------SOLATLS1 2245 - 7000 0.005 (vac) "A high Resolution Solar Atlas for Fluorescence Calculations", 1983, U of Maryland TR AP83-044, A'Hearn, M., Ohlmacher, J., and Schleicher, D. SOLATLS2 2960 - 8000 0.005 (air) "Solar Flux Atlas fro 296 to 1300 nm.", 1984, National Solar Observatory Atlas No. 1, SOLATLS3 8000 - 13000 0.01 (air) "Solar Flux Atlas fro 296 to 1300 nm.", 1984, National Solar Observatory Atlas No. 1, -----------------------------------------------------------------------------