Space Weather
Service Centers
Royal Observatory of Belgium
Royal Observatory of Belgium
Belgian Institute for Space Aeronomy Royal Meterological Institute of Belgium
Royal Observatory of Belgium
Belgian Institute for Space Aeronomy Royal Meterological Institute of Belgium
STCE
Solar-Terrestrial Center of ExcellenceSpace Weather
Observational
SUNSPOT GROUP SOLAR FLARE USET DIARAD TOTAL SOLAR IRRADIANCE FILAMENT
CORONAL HOLE SUNSPOT GROUP CORONAL MASS EJECTION FILAMENT SOLAR FLARE
USET SWAP LYRA
DIARAD TOTAL SOLAR IRRADIANCE
CORONAL HOLE SUNSPOT GROUP CORONAL MASS EJECTION RADIO SHOCK FILAMENT SOLAR FLARE
USET SWAP LYRA HUMAIN DIARAD
TOTAL SOLAR IRRADIANCE
CORONAL HOLE SUNSPOT GROUP CORONAL MASS EJECTION RADIO SHOCK FILAMENT SOLAR FLARE
USET SWAP LYRA HUMAIN DIARAD
TOTAL SOLAR IRRADIANCE
CORONAL HOLE SUNSPOT GROUP CORONAL MASS EJECTION RADIO SHOCK FILAMENT SOLAR FLARE
USET SWAP LYRA HUMAIN
GEOMAG STORM DOURBES GEOMAG DIARAD TOTAL SOLAR IRRADIANCE NEUTRAL MONITOR COSMIC RAYS
CORONAL HOLE SUNSPOT GROUP CORONAL MASS EJECTION RADIO SHOCK FILAMENT SOLAR FLARE
USET SWAP LYRA HUMAIN
GEOMAG STORM IONOSPHERE DISTURBED DOURBES GEOMAG GNSS DIARAD TOTAL SOLAR IRRADIANCE NEUTRAL MONITOR COSMIC RAYS
CATEGORIES &
EXAMPLES
sensors
on the ground
sensors
in space
in-situ
observations
Earth’s magnetic field,
ground level events
solar wind plasma,
space particle radiation
remote sensing
observations
Earth’s ionsphere
solar surface
radio astronomy
solar corona
& solar flares
ESA science satellites
Ground-based Solar
Observations
1. Ground-based solar observations need international networks to cover 24 hours
2. World Data Centers with global impact should not be depend on very constrained institutional resources