Southern Lights from Browns River, Kingston Beach, Tasmania |
What is the Aurora Australis?
Aurora is the collective name given to the photons
(light) emitted by atoms, molecules and ions that have been excited by
energetic charged particles (principally electrons) travelling along magnetic
field lines into the Earth’s upper atmosphere. Aurora results from the
interaction of the solar wind with the Earth’s magnetic field.
Southern Lights from Goats Bluff, South Arm Peninsula, Tasmania |
The amazing colour displays and formations are produced
by the solar wind — a stream of electrons and protons coming from the sun — as
it collides with gases in the upper atmosphere. These collisions produce
electrical discharges which energise atoms of oxygen and nitrogen causing the
release of various colours of light. Earth’s magnetic field channels these
discharges toward the poles. Variations in sunspot activity or the occurrence
of so-called ‘coronal holes’ can often considerably enhance the auroral
discharge adding to the intensity and duration of the displays.
Southern Lights from Dru Point, Margate, Tasmania |
What are the Colours of the Aurora?
Auroral displays appear in many colours with pale green
and pink the most common. However, different shades of red, yellow, green,
blue, and violet have all been observed. The brightest auroral colour is
generally a green light emitted by excited oxygen atoms. A red diffuse glow
results from another oxygen atom transition. A purple colour results from a
transition in a Nitrogen molecular ion. The mixture of the major green, red and
purple emissions may combine to give aurora a general ‘whitish’ appearance. The
colour variations are a product of the altitude of the storm and the density
and composition of the ions at that altitude. The folding effect results from
the electric field induced on either side of the auroral curtain by the
electrons.
Southern Lights from Coles Bay, Tasmania |
Source: Antarctic
Connections
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