Science

Types of Auroral Phenomena

Types Of Auroral Phenomena is a structured science dataset with 15 entries. Its fields include Type, Hemisphere, Altitude (km). The source values are preserved as a structured reference table.

Every row is shown below and is also available as CSV, JSON, or Excel.

15rows
6columns
37views
0downloads
Source:Community curated
Updated:4/9/2026

Dataset details

Table scope
All 15 rows
Fields
6 columns
Source
Community curated
Data updated
Apr 9, 2026

Included fields: Type, Hemisphere, Altitude (km), Typical Color, Cause, and 1 more.

The table contains every record in this dataset; the same records are available in each download format.

Preview observations

Altitude (km) range
90 to 500
Across 15 preview rows
Hemisphere groups
6 distinct values
Across 15 preview rows

Useful for

  • Comparing Type, Hemisphere, and Altitude (km) across science entries
  • Building reference tables, charts, or analyses from 15 downloadable records
15/15
Type
Hemisphere
Altitude (km)
Typical Color
Cause
Notes
Aurora Borealis
Northern100Green, pink, purpleCharged solar wind particles exciting oxygen and nitrogenBest seen near magnetic poles; Norway, Iceland, Alaska, Canada
Aurora Australis
Southern100Green, red, purpleSame as borealis, around south magnetic poleVisible from Tasmania, southern New Zealand, Antarctica
STEVE
Northern and Southern450Purple and mauve ribbonSub-Auroral Ion Drift heating; hot gas flowing at 6 km/sDiscovered by amateurs in 2016; not a classic aurora
Picket Fence
Northern and Southern110Green vertical barsWavelike particle precipitation; often accompanies STEVELooks like a glowing picket fence beside STEVE ribbon
Diffuse Aurora
Both100Faint green glowLow-energy electron rain over wide areasOften unnoticed; covers much of polar sky
Discrete Aurora (Arcs)
Both110Bright green arcsFocused electron beams from magnetotailSharp bright bands stretching across sky
Rayed Aurora
Both120Green with red topsMagnetic field lines channeling particlesVertical rays or curtains that ripple like fabric
Coronal Aurora
Both120Radiating green and redRays seen in perspective straight overheadLooks like light radiating from a single zenith point
Pulsating Aurora
Both100Green patchesElectron precipitation with 5-15 second periodPatches blink on and off across the sky
Proton Aurora
Both120Faint red/ultravioletEnergetic protons instead of electronsMostly invisible to naked eye; detected in UV
Red Aurora
Both300Deep redHigh-altitude oxygen emissions during strong stormsRare; seen during major geomagnetic storms at lower latitudes
Blue/Purple Aurora
Both90Blue-purpleNitrogen molecule emissions below 100 kmUsually at the base of very active auroras
Black Aurora
Both100Dark gaps in auroraRegions where electrons are deflected upwardVoids within a glowing aurora curtain
Aurora on Jupiter
Both (Jovian)500Ultraviolet/blueParticles from Io's plasma torus in Jupiter's magnetospherePowered by planet's rotation, not solar wind; seen by Hubble
Aurora on Mars
Both (Martian)120Ultraviolet greenSolar wind hitting residual crustal magnetic fieldsDetected by MAVEN and ExoMars TGO

Free to explore · No signup needed