AIA 304 Å — Filament Launches48-hour loop • NASA SDO • Prominences, plasma eruptions, filament launches
AIA 131 Å — Hot Plasma48-hour loop • NASA SDO • Pre-flare magnetic restructuring, 10 million degree plasma
AIA 193 Å — Coronal Holes48-hour loop • NASA SDO • Updates hourly
HMI Magnetogram — Magnetic Field48-hour loop • NASA SDO • White = positive, Black = negative polarity
SOHO LASCO C2 — Inner CoronagraphVideo loop • SOHO/NRL • CME halo detection, shock fronts, comets
SOHO LASCO C3 — Outer CoronagraphVideo loop • SOHO/NRL • Wide-field CME envelope tracking, solar wind structure
Composite 211+193+171 Å48-hour loop • NASA SDO • Active regions (purple) + coronal holes (gold) + loops (orange)
Current Moon Phase — Dial-A-MoonNASA SVS / LRO • Photorealistic CGI from Lunar Reconnaissance Orbiter data • Updates hourly
Earth–Moon Distance — True ScaleNASA SVS • Sizes and distances are real • Animation shows perigee/apogee cycle
Corona
LIVE
NASA SDO • AIA 193Å
Solar X-Ray Monitor
LIVE
GOES-19 • 0.1–0.8 nm
Live X-ray flux from the GOES-19 satellite — the same feed NOAA uses to detect solar flares in real time. When the line crosses a threshold, a flare has erupted. M-class and above cause radio blackouts and can trigger geomagnetic storms 1–3 days later.
A
B
C minor
M moderate
X extreme
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Recent Flares
No flares detected