Space weather data

Forecast

Live Hp30 measurements, the 3-day Hp30 outlook, solar wind conditions, and X-ray flux, everything you need to plan your aurora hunt.

Coming our way

The strongest flare in the last 24 hours, and every CME in the last three days with whether it is heading for Earth.

Solar flares

Strongest flare in the last 24 hours: M1.4 at Fri, 16 Oct, 16:42 BST. It came from sunspot region 4551, near the middle of the Sun, the part that faces Earth.

A flare this size can throw out a CME. If NASA finds one heading for Earth it will show below, usually within a few hours, and the app will send an alert.

CMEs in the last three days

None of the 9 is heading for Earth in NASA's model. Show them
  • Left the Sun Fri, 16 Oct, 13:38 BST, 247 km/s

    Not heading for Earth in NASA's model.

  • Left the Sun Fri, 16 Oct, 12:48 BST, 475 km/s

    Not heading for Earth in NASA's model.

  • Left the Sun Fri, 16 Oct, 09:12 BST, 334 km/s

    Not heading for Earth in NASA's model.

  • Left the Sun Fri, 16 Oct, 08:12 BST, 490 km/s

    Not heading for Earth in NASA's model.

  • Left the Sun Fri, 16 Oct, 07:09 BST, 324 km/s

    Not heading for Earth in NASA's model.

  • Left the Sun Thu, 15 Oct, 21:24 BST, 428 km/s

    Not heading for Earth in NASA's model.

  • Left the Sun Thu, 15 Oct, 00:12 BST, 360 km/s

    Not heading for Earth in NASA's model.

  • Left the Sun Wed, 14 Oct, 23:09 BST, 339 km/s

    Not heading for Earth in NASA's model.

  • Left the Sun Wed, 14 Oct, 14:36 BST, 236 km/s

    Not heading for Earth in NASA's model.

Hp30 History

Measured Hp30 geomagnetic index over the last 48 hours (GMT/BST) · 30-minute cadence

3568
Quiet (< 3)Active (3 to 4)Storm (5)Strong (6 to 7)Severe (8+)

Hp30 Forecast

GFZ Potsdam 3-day Hp30 forecast · 30-min cadence · shaded band shows ensemble spread

3568Sat 01:00Sat 13:00Sun 01:00Sun 13:00Mon 01:00Mon 13:00
Quiet (< 3)Active (3 to 4)Storm (5)Strong (6 to 7)Severe (8+)
25 to 75% bandhighmediumlow

Solar Wind

Real-time Bz component and solar wind speed from Solar1 / ACE · Bz < 0 (southward) favours aurora activity

Solar X-ray Flux

GOES satellite X-ray flux · log scale · flare classes A → X