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Solar Plasma

Coronal Mass Ejections Magnetic Fields Solar Flares Solar Eruptions Magnetic Reconnection Sunspots Ejections and Flares Coronal Streamers Turbulent Motions Plasma Movements Behavior in Space Solar Magnetic Fields Ion Temperatures Ejections Interaction with Earth's Magnetosphere Coronal Rain Solar Material Magnetic Fluctuations Flares and Eruptions Magnetic Field Dynamics

Study Finds Solar Flares Superheat Ions 6.5 Times More Than Electrons

Researchers tie the effect to magnetic reconnection, proposing it could explain decades of unusually broad flare spectral lines.

NASA’s CODEX Maps Gusting Plasma Flows in Sun’s Outer Atmosphere

Inouye Solar Telescope Maps 20-Kilometer-Wide Magnetic Striations on Sun’s Surface

Cona Adaptive Optics Reveals Hidden Dynamics in Sun’s Corona