NASA · Arazzo Workflow
NASA DONKI Space Weather Event Chain
Version 1.0.0
Walk one space weather window end to end — solar flare, coronal mass ejection, CME analysis, interplanetary shock, geomagnetic storm.
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Workflows
donki-space-weather-event-chain
Reconstruct the flare to geomagnetic storm chain across a single date window.
Pulls solar flares, coronal mass ejections, CME analysis, interplanetary shocks at Earth, and geomagnetic storms for one date window, following the physical sequence from solar event to terrestrial impact.
1
listSolarFlares
getSolarFlares
Start at the origin of the chain. Solar flares report the active region number, the class type that grades the flare's X-ray intensity, and the begin, peak, and end times that anchor everything downstream.
2
listCoronalMassEjections
getCoronalMassEjections
Pull the coronal mass ejections recorded over the same window. Each CME carries the activity ID, its start time, the source location on the solar disc, and the instruments that observed it.
3
analyzeCoronalMassEjections
getCmeAnalysis
Retrieve the CME analysis records, restricted to the most accurate measurement per event across all catalogs. Speed, half angle, latitude, and longitude are what turn an observed ejection into an arrival forecast.
4
checkInterplanetaryShocks
getInterplanetaryShocks
Check whether anything from this window actually arrived, by pulling interplanetary shocks detected at Earth across all catalogs. A shock at Earth is the observational confirmation that a CME reached us.
5
checkGeomagneticStorms
getGeomagneticStorms
Close the chain with the terrestrial impact. Geomagnetic storms report a storm ID, start time, and the observed Kp index series that quantifies how hard Earth's magnetic field was disturbed.