= Solar UV =


----
 . [[ https://doi.org/10.1029/JA083iA11p05305 | Aeronomical reference spectrum for solar UV below 2000 Å ]] L. Heroux,  H. E. Hinteregger, 1978
  . Rocket experiment on April 1974, 14–2000 Å, R74113 spectrum revised to F74113
  . Atmospheric Exlorer E satellite extreme ultraviolet spectrometer 140–1850 Å
  . 157 cites
----
 . [[ https://doi.org/10.1029/94JA00518 | EUVAC: A solar EUV Flux Model for aeronomic calculations ]] P. G. Richards, J. A. Fennelly, D. G. Torr, 1994
  . Fluxes in the 37 wavelength bins that are in widespread use
  . cross sections to be used with the EUVAC flux model to calculate photoionization rates
  . cited by 771
----
 . [[ https://www.researchgate.net/profile/W_Kent_Tobiska/publication/261175281_JASTP_2000_SOLAR2000/links/0a85e5336f907854b5000000.pdf | The SOLAR2000 empirical solar irradiance model and forecast tool ]] WK Tobiska, T Woods, F Eparvier, R Viereck… - Journal of Atmospheric …, 2000
----
 . ASTM E490  ???
----
 . [[ http://hdl.handle.net/2060/20030001983 | TIMED Solar EUV Experiment: Phase E ]]
 .Woods, Tom; Eparvier, Frank; Woodraska, Don; Rottman, Gary; Solomon, Stan; Roble, Ray; deToma, Guliana; White, Dick; Lean, Judith; Tobiska, Kent;
-----
 .[[ https://www.swpc.noaa.gov/phenomena/solar-euv-irradiance | NOAA Space Weather Prediction Center Solar EUV Irradiance ]] 10 to 120 nm.  The solar EUV spectrum, between 1 and 120 nm, is dominated by spectral lines from hydrogen (H), helium (He), oxygen (O), sodium (Na), magnesium (Mg), silicon (Si), and iron (Fe).  Seemingly no data useful to me.

 .[[  https://www.ngdc.noaa.gov/stp/solar/solaruv.html | NOAA Solar Ultraviolet Spectral Irradiance ]]  THE GOOD TABLES
  . 
-----
http://www.spacewx.com/solar2000.html
 
-----
 . [[ https://archive.stsci.edu/euve/ | Extreme Ultraviolet Explorer ]] at the Space Telescope Science Institute, deep space sources, not relevant