Where it begins and where it ends
The sun, the moon and the stars belong to the eternal and predictable in the universe. On the other hand, the majestic Northern Lights – or Aurora Borealis – are elusive, changing and less predictable.
It is a phenomenon that occurs when the solar flares originating from the sun are more mighty than usual, and with the solar wind sending charged particles towards the Earth. When sun particles reach the Earths atmosphere and collide with Oxygen and Nitrogen, those atoms become overcharged, and the extra energy is emitted as a light that shines for a few seconds. To be able to see the Northern Lights, millions of small lights have to be released at the same time. That’s the exact reason why sometimes we see the Aurora in bright colours and some other times we barely can notice them.
The Northern Lights occur at the height of more than 100 km above the ground and may be observed in the night sky in a belt around the Magnetic North and South Pole. The lights in the northern hemisphere are called Aurora Borealis and the ones in southern Aurora Australis.