Solar activity

See what is happening on the Sun: sunspots mark active regions, while dark coronal holes can release faster solar wind.

Solar X-ray flux

B1.9 1.89e-7 W/m²
Observed

Flare strength runs from A through B, C and M to X. At the same number, each letter class is ten times stronger than the previous one.

Updated at · Oct 31, 2026, 05:01 UTCNOAA SWPC

Sunspot regions

Sunspot regions
NASA SDO / HMI

Flare probability

Forecasts & alerts →
C15%
Forecast · Oct 30, 2026, 00:00
M1%
Forecast · Oct 30, 2026, 00:00
X1%
Forecast · Oct 30, 2026, 00:00

Sunspot regions

2026-10-31 · UTC
RegionLocationSunspotsArea (MH)ClassificationC / M / X
4565N12E61160A · Hsx0% / 0% / 0%
4563S19W0*110A · Axx0% / 0% / 0%
4564N04E41430B · Cro0% / 0% / 0%
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Coronal holes

Coronal holes
NASA SDO / AIA 193 Å

Synoptic Map

Synoptic Map
NOAA SWPC

What do bright and dark areas mean?

Image colours depend on the instrument and wavelength. Compare images from the same channel; a dark coronal hole is not a hole in the Sun.

Do more sunspots mean a stronger storm?

Sunspot count alone is not enough. Region size and magnetic complexity help assess flare potential, but neither predicts a storm at Earth.

Can a far-side active region predict a storm?

It can suggest a region to watch as the Sun rotates. It cannot establish the time, strength or Earthward direction of a future eruption.

Public scientific observations and forecasts may be delayed or revised. Forecasts are not guarantees of aurora visibility or operational safety. Follow official advice for critical decisions.