{"id":19581,"date":"2015-12-03T00:45:20","date_gmt":"2015-12-02T19:15:20","guid":{"rendered":"https:\/\/yaabot.com\/?p=19581"},"modified":"2024-01-19T20:03:17","modified_gmt":"2024-01-19T14:33:17","slug":"the-science-behind-auroras","status":"publish","type":"post","link":"https:\/\/entropymag.co\/the-science-behind-auroras\/","title":{"rendered":"The Science behind Auroras"},"content":{"rendered":"\n

Our planet is a witness to multiple\u00a0natural phenomena – biological, chemical or optical. Aurora is primarily some gorgeous physics at play – but we’d also classify it as an\u00a0optical phenomenon. Predominantly observed in high latitude regions, regions possessing a weak magnetic field, auroras\u00a0are a natural light spectacle in the sky. Imagine it as a colourful sunset swirling across a clear sky. <\/p>\n\n\n\n

They’re well documented, and space and nature enthusiasts are well versed with them. The colours of an aurora that can be detected by the human eye include red, green, yellow and blue. These colours are observed at different altitude levels \u2013 red observed at high altitude and blue observed at lower altitude. Apart from these observable colours, ultraviolet and infrared light can be observed using the required equipment.<\/p>\n\n\n\n

Auroras can be observed at locations above 60o<\/sup> latitude. When observed in northern latitude, the effect is called Aurora Borealis<\/em>, named after Boreas, the Greek name for the north wind. Canada and the Scandinavian countries are the best places to watch the Northern Lights. The southern counterpart of the Aurora Borealis is called Aurora Australis<\/em>. Southern lights are best viewed from South America and Australia. Since the southern pole is less populated than the northern pole, the lights are commonly referred to as Aurora Borealis<\/em>.<\/p>\n\n\n\n

But what causes auroras in the first place?<\/p>\n\n\n\n

The Physics behind Auroras<\/h2>\n\n\n\n

The physics behind the auroras is as fascinating as the aurora itself. Openings in the Sun\u2019s atmosphere allow charged particles – electrons and protons, to flow out. These charged particles travel at extremely fast velocities towards the Earth, carried by what we call solar winds. Now the Earth happens to have a magnetic field of its own – the same field that helps align our compasses. This magnetic field acts as a barrier for the planet, and deflects most of the charged particles. <\/p>\n\n\n\n

At the poles however, the magnetic field is weaker. This allows the charged particles to breach Earth’s atmosphere. When these charged particles interact with the gaseous particles in our atmosphere, an aurora shows up in our skies. The charged particles have enough energy to knock off the gas atoms in our atmosphere – this causes the atoms to give off light, and eject more charged particles. Result? Aurora.<\/p>\n\n\n

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\"Auroras,
Auroras, result from solar storms where the sun releases energy and particles, with the Earth’s magnetic field channeling them to the poles – source<\/a><\/figcaption><\/figure><\/div>\n\n\n

The variation in colours of auroras is observed based on the type of gaseous particles, usually oxygen. The color depends on the gas atom that’s knocked off in the atmosphere:<\/p>\n\n\n\n