The Northern Lights, also known as aurora borealis, are luminous streaks of light in the night sky near the Arctic Circle. Their counterparts in the Southern Hemisphere are called aurora australis. These natural light shows have fascinated people for centuries with their shifting greens, purples, and reds.
The phenomenon begins with solar storms on the Sun’s surface, which eject electrically charged particles called the solar wind into space. When these particles reach Earth, most are deflected by the magnetosphere. At the poles, magnetic field lines guide some particles into the atmosphere.
When charged particles collide with gases in Earth’s atmosphere—primarily oxygen and nitrogen—they transfer energy. This energy is released as glowing light, similar to how a neon lamp works, with gases glowing when energized.
Auroras occur between 97–1,000 kilometers above Earth’s surface. The height influences the color:
The Northern Lights are most often seen during winter months when nights are long and dark. They are common in countries near the Arctic Circle such as Norway, Sweden, Finland, Iceland, Canada, Alaska, and Greenland. Periods of strong solar activity increase their frequency.
While auroras depend on solar activity, scientists can forecast them by tracking solar storms and magnetic storms. Increased solar wind makes auroras brighter and more frequent.
Yes, auroras remind us of the dynamic relationship between the Earth and the Sun. They are not just spectacles of beauty but also evidence of space weather, which can affect satellites, navigation systems, and power grids.
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