1 Northern Lights. Aurora Borealis. 2 Appearance Arc, rays, patches, Mainly brilliant yellow-green (O- 60m) Red-rare (O- 200m) Blue (N) Purple-red (N2)

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Presentation transcript:

1 Northern Lights. Aurora Borealis

2 Appearance Arc, rays, patches, Mainly brilliant yellow-green (O- 60m) Red-rare (O- 200m) Blue (N) Purple-red (N2)

3 Intensity SUBSTORMS -Duration <30min -Recession 3-12hrs Sunspot Maximum Years -every 11years(2002)

4 Where Around the north and south magnetic poles Lower edge is miles above earth in the magnetosphere

5 How they occur Ejection of plasma from the sun hits the earth’s upper atmosphere (Solar Wind) This bombardment excites atoms and molecules in the upper atmosphere

6 Solar Wind Protons and electrons which travel from the sun to the earth Time of travel is about 3 days Largest during sunspot maximum years Causes the fluctuations in the magnetosphere that produces up to 10^6MW

7 Polar Cusps Polar Cusps allow the solar wind to penetrate into the Earth’s Ionosphere, where the excitation of atoms and molecules occur.

8 Adverse Effects -Disruption of radio communications -Radio Navigation -Radar systems -Power transmission lines -Corrosion of the trans-Alaska pipeline