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Core
The Sun’s center where hydrogen fuses into helium, producing energy.
Radiative Zone
Layer where energy slowly moves outward as light
Convective Zone
→ Layer where hot gases rise and cool gases sink, carrying energy to the surface.
Photosphere →
The visible “surface” of the Sun that emits the light we see.
Corona
The Sun’s outermost atmosphere, very hot and only visible as a halo during eclipses.
Sunspots
Cooler, darker areas on the photosphere caused by strong magnetic fields.
Solar Flares / CMEs
Explosive bursts of energy and charged particles from active sunspot regions.
Solar Flares / CMEs
Explosive bursts of energy and charged particles from active sunspot regions
Prominences
Loops or arches of glowing gas that follow magnetic field lines and extend into the corona.