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Aurora Polaris
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Fireworks
are a wonderful spectacle on their own, but in comparison to
nature's work of art, they are nothing. One of the most
amazing and beautiful phenomenon is the aurora
borealis and the aurora australis.
When they appear in the sky, they are generally accompanied by a
cracking sound.
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They are
luminous displays that are usually seen in a variety of
forms:
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the
auroral arch, a luminous arc lying across the
magnetic meridian;
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the
auroral band, broader and more irregular than the
arch; filaments and streamers that appear at right angles
to the arch or band; the corona, which is a luminous
circle near the zenith;
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the
auroral clouds, undefined nebulous masses and
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the
auroral glow - a luminous appearance seen high up
in the sky with the filaments meeting at the zenith; and
curtains, fans, flames, or differently-shaped streamers.
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The aurora is an
atmospheric phenomenon that appears most often
above 60° North or South latitude, but also in
other parts of the world like Canada, Northern Scotland,
Norway and Sweden. Depending on where it appears, it is
named either aurora borealis (northern lights) or aurora
australis (southern lights). Together they are called
aurora polaris or the polar lights.
Research studies
made during and after the 1957 and 1958 International
Geophysical Year showed that the auroral glow is
triggered off when the solar wind carries an inflow of
high-energy atomic particles. These particles are
emitted from sunspots, which are minute
electrifying particles that burst out from the sun's interior.
This release sends electrons and protons out and they penetrate
the magnetosphere of the earth and enter the lower Van Allen
radiation belt thus overloading it. This excess number of
electrons and protons are discharged into the atmosphere over an
area that centers on the north and south |
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magnetic poles,
but extends about 20° apart from them. These particles collide
against gas molecules present in the atmosphere. The
molecules get extra energy and become excited. Electromagnetic
radiation is then given off by these particles, which is within
the visible portion of the light spectrum. This is why we are
able to see the lights. |
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The aurora is
described as being made up of rapidly shifting patches and
dancing columns of light of various hues. Large, extensive
auroral displays usually interfere with radio,
telephone, and telegraph transmission. The duration of
the maximum and minimum intensity of normal aurora is
almost exactly opposite that of the sunspot cycle,
which is an 11-year cycle; therefore the intensity of the aurora
is normally low whenever the sun is very active. When the
sunspot cycle is at its peak, the sun emits more
ultraviolet radiation than normal. This ultraviolet
radiation alters the earth's magnetosphere,
making it more resistant to the influx of
particles from the sunspots. The radiation belt
then does not overload as easily and the aurora is less intense.
But
it has also been seen that huge displays seen much beyond the
earth's poles do however, happen while the sun is very active.
Although we may try to capture the beauty on canvas or try to
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words to describe
the Aurora, it is a difficult task. So look out for more
pictures of the Aurora, since it is definitely worth knowing
about it! |
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