aurora (photo by Ian Law)
In many parts of Europe, the aurora is unfortunately a rare phenomenon, but in Scandinavia,
North America, and also at the South Pole it is frequently visible. It comprises luminescent
bands, arcs and streamers. which sometimes have a typical curtain-like structure and
periodically light up in a rhythmic fashion. The light comes from very great heights in the
atmosphere (100 to 300 km). The light of an aurora is often not very intense (like that of the
Milky Way), but sometimes it becomes very bright, and its beautiful colours are then visible.
The red higher part of the aurora is polarized, the lower green and purple parts of it are not.
The direction of polarization is perpendicular to that of the magnetic field of the Earth, hence
directed mainly west-east. The polarization is maximal when we look perpendicularly to the
magnetic zenith, which is at a height of about 70º in the northern sky for central England.
Theoretically, the degree of polarization of the red light can amount to as much as 60 %. The
best chance to see this polarization in Western Europe is low near the northern horizon where
the degree of polarization must be about 55 %. In the case of rare bright displays, which may
even extend in Western Europe to the south of the firmament, the most favourable point is in
the south at a height of roughly 20º
This polarization is related to the Zeeman effect, and manifests itself as a consequence of the
magnetic field of the Earth. However, not every atomic transition is sensitive to it, and that is
why only the red aurora has a considerable degree of polarization. The aurora is the only
phenomenon of this kind that shows polarization in Nature; other electrical effects do not show
it to any noticeable degree. The reason is that other discharges (lightning for example) take
place at a much higher atmospheric pressure so that the influence of magnetic fields is
negligible.
It seems probable that shifting of colour in the aurora can be seen with a polarizing filter: when
the filter is held in such a way that the red has been maximally extinguished, the (unpolarized)
green must become relatively brighter. The yellow part of the aurora (where red and green are
mixed) will consequently have to shift up or down, according to the position of the filter, since
the ratio between red and green light has changed. So, for a minimal transmission of the filter,
the lower part of the red will have to turn yellowish and the yellow to greenish: the effect will be
reverse in the case of a maximum transmission.
Note
- An auroral display in
the Northern Hemisphere is called the aurora borealis, or the
northern lights; in the Southern Hemisphere it is called the aurora australis (or the southern lights)