BackForwardInstrument:  SXEUV 

Instrument details
Acronym SXEUV
Full name Solar X-EUV imaging telescope
Purpose Space Weather - Solar activity monitoring
Short description

Fluxmeter to measure X-rays in the range approximately 1-10 keV and and Extreme UV radiation. Continuous spectra in range 5-35 nm, 110-145 nm with 0.5 nm resolution. Includes Fe-IX at 17.1 nm, Fe-XII at 19.5 nm, Fe-XV at 28.4 nm, He-II at 30.4 nm, and H-Lyman-alpha at 121.6 nm
Background

New development
Scanning Technique

Sun pointing from GEO >55 arcmin
Resolution N/A (full disk)
Coverage / Cycle Full solar disk at 1s intervals (X-ray) and 5s (EUV)
Mass Power Data Rate

 

Providing Agency CMA
Instrument Maturity Backed by strong heritage
Utilization Period: 2025 to 2040
Last update: 2025-04-07
Detailed characteristics
Satellites this instrument is flying on

Note: a red tag indicates satellites no longer operational, a green tag indicates operational satellites, a blue tag indicates future satellites

Instrument classification
  • Solar and space environment monitors
  • Solar activity monitor
WIGOS Subcomponents
  • Subcomponent 1
  • X-ray spectrograph on GEO orbit
  • X-ray spectrometer at GEO
  • Subcomponent 2
  • Solar magnetograph, solar EUV/X-ray imagery and EUV/X-ray irradiance, both on the Earth-Sun line and off the Earth-Sun line
  • Solar X-ray spectrometer [from L1, GEO, LEO]
  • Solar EUV spectrometer [from L1, GEO, LEO]
  • Subcomponent 3
  • UV spectral imagery (e.g. GEO, HEO, MEO, LEO)
  • X-ray spectrometer [from GEO, HEO, MEO, LEO]
  • EUV spectrometer [from GEO, HEO, MEO, LEO]
Mission objectives
Primary mission objectives
  • Solar EUV flux
  • Solar X-ray flux
Evaluation of Measurements

The following list indicates which measurements can typically be retrieved from this category of instrument. To see a full Gap Analysis by Variable, click on the respective variable.

Note: table can be sorted by clicking on the column headers
Note: * Primary mission objective.
VariableRelevance for measuring this variableOperational limitationsExplanation
Solar X-ray flux*3 - highNo specific limitation.Few channels, wide dynamic range
Solar EUV flux*1 - primaryNo specific limitation.Several channels, wide dynamic range