RocketSTEM Issue #5 - January 2014 | Page 23

this distortion produces a magnetic field and includes loops that erupt from the Sun’s surface and trigger the formation of the Sun’s dramatic sunspots and solar prominences. This twisting action creates the solar dynamo and an 11-year solar cycle of magnetic activity. When these loops and sunspot magnetism break free from the suns magnetic field they send what we term the “solar wind” out into space. From time to time it heads directly towards planet Earth. The Solar wind is a stream of charged particles released from the upper atmosphere of our star and mostly consists of electrons and protons. If ejected in the right direction the solar wind will race Earthward at great speed 300 – 1000kms per second and faster in some cases. Imagine a car travelling at over a million miles an hour and you begin to get the idea. Once it reaches the Earth in 2-4 days it hits our atmosphere and interacts with our own magnetic field. Our planet is protected by what we term its magnetosphere, and this is what initially protects us from the blast of particles. As the wind is first channelled past the Earth, our magnetic field then acts as a mighty bow to deflect these particles. Then these particles pass the Earth and re-connect, channelling back towards us and attracting them to the weakest portion of the Earth magnetic field around the poles. At the North Polar regions we see the “Aurora Borealis”, and the South Polar region we see the “Aurora Australis”. Our Earth has quite a complex atmosphere but is primarily made of Nitrogen and Oxygen with smaller amounts of other gases. Critical in Aurora formation though is that Nitrogen and Oxygen. In our atmosphere we actually have 2 types of Oxygen; we have atomic Oxygen and molecular Oxygen as well as the Nitrogen. What happens to create the colours we see in the Aurora, is the interaction between these gaseous atoms and the particles from the Solar wind the electrons. Aurora Borealis as seen in the skies above a hotel near Reykjavik, Iceland. Photo: Andrew Green 21 www.RocketSTEM.org 21