Historical training datasets used to determine the EUVS Model coefficients. The Purpose column indicates if the data are used to compute the long-term and/or short-term model coefficients, or to cross-calibrate the historical data with the GOES-16 EUVS Measurements.
|Data source||Purpose||Data level||Version||Wavelength (nm)||Sampling (nm)||Accuracy (%)|
|TIMED/EGSb||Long and Short-term||3||12||26–117||1||5–20|
|SDO/MEGSd||Long and Short-term||3||6||6–106||0.1||1–7|
|Bremen composite Mg II Indexe||Long-term, Cross-calibrate||Composite||5||275–285||N/A||0.3i|
|GOES-15/EUVS Eg||Short-term||Minute average||4||121.6||Lyman-α||2h|
Solar Radiation and Climate Experiment/SOLar-STellar Irradiance Comparison Experiment (McClintock et al., 2005).
Thermosphere Ionosphere Mesosphere Energetics and Dynamics/EUV Grating Spectrograph (Woods et al., 2005).
TIMED/XUV Photometer System (Woods et al., 2005).
Solar Dynamics Observatory/Multiple EUV Grating Spectrographs (Woods et al., 2010).
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