A Proton Aurora
Credit:
IMAGE Satellite,
NASA
What are auroras made out of?
Triggered by solar activity,
normal auroras are caused by
collisions between fast-moving
electrons
and the oxygen and nitrogen in Earth's upper atmosphere.
The electrons come from the
magnetosphere, the region of space controlled by
Earth's magnetic field.
As the excited oxygen and nitrogen molecules
return to their low energy state, they emit light,
seen as the auroral glow.
Sometimes, however,
auroras can be caused by collisions with heavier
protons,
causing a more energetic display with strong
ultraviolet
emission.
In addition, protons can temporarily capture an electron and emit
light for themselves.
Such a proton aurora is seen above, recorded by the
IMAGE satellite.
A special feature is the bright
spot near picture center, embedded
in a ring of auroral emission around
the north magnetic pole of planet Earth.
Most solar wind protons
never reach the Earth to cause
auroras because they are completely deflected away at a
great distance by the Earth's magnetic field.
The bright spot in the
auroral ring
indicates a particularly
deep crack
in the Earth's magnetic field where
protons
were able to flow along a temporarily connected
region between the
Sun and the Earth,
relatively undeflected, until they impacted the
Earth's ionosphere.