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Instrument details
Acronym
SXUS
Full name
Solar X-EUV Irradiance Sensor
Purpose
To monitor EUV and X-rays from the solar disk
Short description
Detailed description not yet available. Two units, to measure fluxes of EUV in the range 1-200 nm and X-ray in the range 2-20 keV (guess)
Background
Similar to the GOES EXIS
Scanning Technique
Sun pointing from GEO
Resolution
N/A
Coverage / Cycle
Full solar disk
Mass
Power
Data Rate
Providing Agency
CMA
Instrument Maturity
Flown on operational programme
Utilization Period:
≥2024 to ≥2031
Last update:
2021-12-16
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 spectrometer at GEO Subcomponent 2 Solar X-ray spectrometer [from L1, GEO, LEO] Solar EUV spectrometer [from L1, GEO, LEO] Subcomponent 3 X-ray spectrometer [from GEO, HEO, MEO, LEO] EUV spectrometer [from GEO, HEO, MEO, LEO]
Mission objectives
Tentative 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
Variable Relevance for measuring this variable Operational limitations Explanation
Solar X-ray flux 3 - high No specific limitation. Few channels, wide dynamic range
Solar EUV flux 1 - primary No specific limitation. Several channels, wide dynamic range
Instrument: SXUS