A polar aurora stands out against the starry background of the Scandinavian sky [Source : © P. Volcke, IPAG / OSUG]
In 1741, Hiorter and Celsius noted that the polar aurora is accompanied by a disturbance of the magnetic needle.
A polar aurora is “the perturbation of the magnetosphere surrounding the Earth by the solar winds” (Science Avenir).
1741--Hiorter and Celsius note that the polar aurora is accompanied by a disturbance of the magnetic needle.
1741 - Hiorter and Anders Celsius note that the polar aurora is accompanied by a disturbance of the magnetic needle.
Many of us dream of seeing the Aurora Borealis, or Northern Lights.
Aurora around the southern pole of Saturn, photographed with the Hubble Space Telescope.
Strong magnetic disturbances are detected when a bright aurora is seen.
Strong electromagnetic disturbances are observed when a bright aurora is seen.
Strong magnetic disturbances are detected when bright aurorae are seen.
Polar lights generally have the shape of trails of draperies or veils.
1974 - David Evans presents evidence that auroral electrons are accelerated within 8000 km or so of Earth.
Birkeland also observes magnetic disturbances associated with the aurora, suggesting to him that localized "polar magnetic storms" exist in the auroral zone.
The Northern lights may appear for 5 minutes, or 10 minutes, or even for a half an hour – you never know!
Residents of northerly lattitudes were treated to the spectacle of brilliant aurora as curtains of green and white light danced across the sky.
While leading his annual aurora tour last month near Fairbanks in central Alaska, astrophotographer John Chumack and his company saw a most unusual aurora.
Where the currents intersect the ionosphere of Jupiter, an intense polar aurora is created--a process somewhat similar to the one responsible for aurora near Earth.
The more particles in the solar wind, the more chances we get for an auroral display as more particles collide with Earth’s magnetosphere.
The more particles in the solar wind, the more chances we get for an auroral display as more particles collide with Earth's magnetosphere.
The more particles in the solar wind, the more chances we get for an auroral display as more particles collide with Earth's magnetosphere.
The more particles in the solar wind, the more chances we get for an auroral display as more particles collide with Earth’s magnetosphere.
The truth started with a dream -- a dream that the spectacular Seljarlandsfoss waterfall in southern Iceland could be photographed with a backdrop of an aurora-filled sky.
In a broad sense, "meteor" meant virtually any atmospheric phenomenon, such as thunder, lightning, aurora, earthquake lights, rainfall, clouds, mist, dust devils, meteors, rainbows, halo, mirages...
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