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Famous CMEs

The Halloween Storms

28 October – 4 November 2003 G5 · Extreme Measured wind & Kp · CME reconstructed

For a week around Halloween 2003, one of the most active sunspot regions of the space age threw everything it had at the inner solar system — including the most intense solar flare ever recorded. Fast CMEs drove back-to-back extreme G5 storms that failed satellites, rerouted airliners, and even tripped a power grid in Sweden.

Cinematic illustration: two back-to-back eruptions from a giant active region send CMEs toward Earth — the 2003 Halloween storms.
Artist's illustration. Solar wind and Kp here are measured archive data; the CME geometry is authored from event records (NASA's DONKI catalog begins later).
Replay the Halloween Storms in CME TrackerWatch the fast CMEs reach Earth and drive two extreme storms in a row. Open replay →

1What happened

In late October 2003, a colossal active region — AR 486 — dominated the Sun alongside two other large groups. On 28 October it produced an X17 flare and hurled a fast CME straight at Earth; it arrived the next day and drove an extreme G5 storm. Barely a day later another major eruption hit, and a second G5 storm followed on 30 October.

Then, on 4 November, as the region rotated toward the Sun's edge, it fired the largest flare ever recorded — saturating detectors at X17 and later estimated near X28–X45. Because it erupted near the limb, much of its blast missed Earth — a vivid lesson in how direction, not just size, decides a flare's effect.

2Timeline

3The science

The Halloween Storms are a case study in compounding hazards: intense flares (radiation arriving in minutes), strong solar radiation storms (energetic protons), and fast Earth-directed CMEs (the geomagnetic storms a day later) all from the same hyperactive regions. The CMEs were fast enough — well over 2,000 km/s near the Sun — that they crossed to Earth in roughly a day, and they carried strongly southward fields that pushed Kp to 9.

Direction matters. The record-setting 4 November flare is a perfect example of why this tracker draws every CME as a cone in its measured direction: an enormous eruption near the Sun's edge can be far less geoeffective than a smaller one aimed straight at us.

4Impacts

5By the numbers

~X28–X45
Most intense flare on record
2 × G5
Back-to-back extreme storms
Kp 9
Peak geomagnetic index
AR 486
Primary source region
~1 day
CME transit to Earth
Malmö
~1-hour grid blackout

6What if it happened today?

The Halloween Storms are a modern worst-case we actually lived through — with satellites, GPS, and grids already in play. They drove major investment in space-weather forecasting and grid resilience in the years that followed. A repeat today would test a far more satellite-dependent civilization, but also a far better-warned one.

7Watch it yourself

8Sources & further reading

Educational, not operational. For live forecasts and warnings, see NOAA SWPC.

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