ACQUIRING SOLAR IMAGERY
FETCHING FRAME TIMESTAMPS…
Solar imagery
NASA SDO | AIA 193Å
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LOADING COMPOSITE LOOP
AIA 193
AIA 193Å — HOT CORONA
24H LOOP
AIA 304
AIA 304Å — CHROMOSPHERE
24H LOOP
AIA 171
AIA 171Å — MAGNETIC LOOPS
24H LOOP
AIA 211
AIA 211Å — ACTIVE REGIONS
24H LOOP
DAILY VIDEO
COMPOSITE
LIVE FRAME
EDS AI SOLAR ANALYSIS
CEREBRAS WSE-3 CORE
  Analyzing solar flux…
REAL-TIME METRICS
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KP INDEX
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WIND km/s
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DENSITY p/cm³
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X-RAY FLUX
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Bt nT
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Bz nT
NOAA SPACE WEATHER ALERTS
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TECHNICAL BRIEFING

The 24-hour SDO loop uses the Helioviewer API to find actual NASA Solar Dynamics Observatory archive frames captured every ~2 hours, giving a true time-lapse of solar activity.

AIA 193Å reveals hot coronal plasma. LASCO C3 detects coronal mass ejections. Kp ≥ 5 indicates geomagnetic storm conditions.

Bz < −10 nT signals elevated aurora and GPS disruption risk.

DATA SOURCES
NASA SDO / AIA — Helioviewer archive
NOAA GOES SUVI — EUV solar imaging
SOHO LASCO C3 — coronagraph
NOAA SWPC — Kp index, solar wind
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