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Red Line (630.0 nm)

Definition

The deep-red oxygen emission from high altitudes, prominent in strong storms and distant displays.

In plain language

Above about 150 miles, oxygen glows red instead of green — but only where the air is thin enough to leave excited atoms undisturbed for minutes. Sky-filling red is the classic mark of an extreme storm.

The science

The 630.0 nm O(¹D → ³P) transition has a ~110 s radiative lifetime, restricting emission to altitudes above ~150–200 km where collisional quenching is negligible. Type-d red auroras characterize severe storms.

Why it matters for aurora viewing

Mid-latitude observers often see red first or only — the tall red tops clear the horizon while the green base stays hidden below it.

See this in action on tonight's data.