CME TRACKER
CME TrackerLearn › Module 4
Module 4 of 5 · about 20 minutes

Predict it yourself

Forecasters commit to numbers before reality arrives. Your turn — no peeking before you've made your call.

Exercise A — the July 2012 monster

A CME leaves the Sun at ~2,500–3,000 km/s — one of the fastest ever recorded. Earth's orbit is about 150 million km out. Your call: roughly how many hours from launch to Earth's distance? (Distance ÷ speed. Ignore deceleration for the estimate.)

Reveal what happened

At 2,500 km/s: 150,000,000 ÷ 2,500 = 60,000 seconds ≈ 17 hours. The real event crossed to 1 AU in under a day and slammed into the STEREO-A spacecraft, which measured a Carrington-class storm. Earth had been at that exact spot in its orbit about nine days earlier.

The uncomfortable lesson: the most dangerous CMEs give the least warning. A three-day forecast window is a luxury of slow storms.

▶ Replay the near miss 📖 The full story

Exercise B — the St. Patrick's Day surprise

March 2015: a thoroughly ordinary CME leaves the Sun — moderate speed, taking a leisurely ~2 days to arrive. Nothing about the launch looks special. Your call: what storm level would you forecast — minor (G1), moderate (G2), strong (G3) or worse?

Reveal what happened

It drove a G4 (severe) storm, Kp ≈ 8 — the biggest storm of the entire solar cycle to that point. The launch data couldn't have told you: what mattered was the CME's internal magnetic field, which pointed strongly southward for hours and poured energy into Earth's field. That orientation is essentially unmeasurable until the CME reaches the L1 spacecraft, an hour before arrival.

The lesson every forecaster lives with: arrival time is predictable days out; storm strength often isn't known until the last hour. Two different forecasts, two different confidence levels.

▶ Replay it 📖 The full story

Exercise C — the storm lab: dial your own CME

This isn't a toy calculator: the sliders below run the same drag-based physics model this site uses for its real forecasts. Launch a CME and watch what the solar wind does to it.

Transit time (drag model)
If speed never changed
Speed on arrival
Storm potential (est. band)
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