Solar Flare Observations
Early Stage Flare
Captured at 08:00 UTC - Initial magnetic field disturbances
Peak Intensity
Recorded at 10:30 UTC - Maximum energy release observed
Coronal Mass Ejection
Documented at 11:45 UTC - Large-scale plasma ejection from the corona
Post-Flare Loops
Observed at 14:20 UTC - Magnetic field reconfiguration after the event
Solar Prominence
Large-scale, arc-shaped structure extending from the Sun's surface
Sunspot Formation
Development of dark, cooler regions on the solar surface
Solar Wind Acceleration
Observation of high-speed solar wind streams
Magnetic Reconnection
Process of magnetic field lines breaking and reconnecting
Solar Filament Eruption
Eruption of a dense, cool plasma filament from the Sun's surface
X-class Solar Flare
Observation of the most intense class of solar flares
Solar Spicules
Dynamic jet-like features observed in the solar chromosphere
Coronal Loops
Arching structures in the solar corona following magnetic field lines
Solar Tsunami
Large-scale wave propagating across the Sun's surface
Coronal Hole
Regions of the Sun's corona with lower density and temperature
Solar Flare Precursor
Early signs and activities leading up to a major solar flare
Magnetic Flux Emergence
New magnetic field lines breaking through the solar surface
Solar Granulation
Convection cells visible on the solar surface
Helmet Streamer
Large, arc-shaped structure in the solar corona
Solar Flare Shockwave
Propagation of a shockwave through the solar atmosphere following a flare
Polar Plumes
Long, thin structures extending from the Sun's polar regions