A shimmering display of the Aurora Borealis lights up the sky over the Perrine Bridge in Twin Falls, Idaho, |
Picture: AP |
An aurora is a natural light display in the sky
particularly in the high latitude (Arctic and Antarctic) regions, caused
by the collision of energetic charged particles with atoms in the high
altitude atmosphere (thermosphere). The charged particles originate in
the magnetosphere and solar wind and, on Earth, are directed by the
Earth's magnetic field into the atmosphere. Aurora is classified as
diffuse or discrete aurora. Most aurorae occur in a band known as the auroral zone,
which is typically 3° to 6° in latitudinal extent and at all local times or longitudes. The auroral zone is typically 10° to 20° from the magnetic pole defined by the axis of the Earth's magnetic dipole. During a geomagnetic storm, the auroral zone will expand to lower latitudes. The diffuse aurora is a featureless glow in the sky which may not be visible to the naked eye even on a dark night and defines the extent of the auroral zone. The discrete aurora are sharply defined features within the diffuse aurora which vary in brightness from just barely visible to the naked eye to bright enough to read a newspaper at night. Discrete aurorae are usually observed only in the night sky because they are not as bright as the sunlit sky. Aurorae occasionally occur poleward of the auroral zone as diffuse patches or arcs (polar cap arcs), which are generally invisible to the naked eye.
which is typically 3° to 6° in latitudinal extent and at all local times or longitudes. The auroral zone is typically 10° to 20° from the magnetic pole defined by the axis of the Earth's magnetic dipole. During a geomagnetic storm, the auroral zone will expand to lower latitudes. The diffuse aurora is a featureless glow in the sky which may not be visible to the naked eye even on a dark night and defines the extent of the auroral zone. The discrete aurora are sharply defined features within the diffuse aurora which vary in brightness from just barely visible to the naked eye to bright enough to read a newspaper at night. Discrete aurorae are usually observed only in the night sky because they are not as bright as the sunlit sky. Aurorae occasionally occur poleward of the auroral zone as diffuse patches or arcs (polar cap arcs), which are generally invisible to the naked eye.
A satellite view of aurora |
In northern latitudes, the effect is known as the aurora borealis (or the northern lights), named after the Roman goddess of dawn, Aurora, and the Greek name for the north wind, Boreas, by Pierre Gassendi in 1621.
Auroras seen near the magnetic pole may be high overhead, but from
farther away, they illuminate the northern horizon as a greenish glow or
sometimes a faint red, as if the Sun were rising from an unusual
direction. Discrete aurorae often display magnetic field
lines or curtain-like structures, and can change within seconds or glow
unchanging for hours, most often in fluorescent green. The aurora
borealis most often occurs near the equinoctes. The northern lights have
had a number of names throughout history. The Cree call this phenomenon
the "Dance of the Spirits". In Europe, in the Middle Ages, the auroras were commonly believed a sign from God.
Its southern counterpart, the aurora australis (or the southern lights), has almost identical features to the aurora borealis and changes simultaneously with changes in the northern auroral zone and is visible from high southern latitudes in Antarctica, South America, New Zealand, and Australia.
In this September 3, 2006 photo, a spectator watches the Aurora Borealis rise above the Alaska Range, in Denali National Park, Alaska. Picture: AP |
Aurorae occur on other planets. Similar to the Earth's aurora, they are visible close to the planet's magnetic poles.
Modern style guides recommend that the names of meteorological phenomena, such as aurora borealis, be uncapitalized.
Aurora Australis lights up the night sky over the Australian Antarctic Territory, 11 March, 2007. Picture: AFP |
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