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 .Woods, Tom; Eparvier, Frank; Woodraska, Don; Rottman, Gary; Solomon, Stan; Roble, Ray; deToma, Guliana; White, Dick; Lean, Judith; Tobiska, Kent; hide  .Woods, Tom; Eparvier, Frank; Woodraska, Don; Rottman, Gary; Solomon, Stan; Roble, Ray; deToma, Guliana; White, Dick; Lean, Judith; Tobiska, Kent;
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 .[[ 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
  .
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http://www.spacewx.com/solar2000.html
 
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 . [[ https://archive.stsci.edu/euve/ | Extreme Ultraviolet Explorer ]] at the Space Telescope Science Institute, deep space sources, not relevant

Solar UV





  • ASTM E490 ???


  • 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;



http://www.spacewx.com/solar2000.html


SolarUV (last edited 2019-08-02 02:20:36 by KeithLofstrom)