Aurora Borealis, or the Northern Lights, are streaks of greenish-blue light seen in a clear night sky. As they sway and twirl, they appear and go in the blink of an eye. The auroras result from solar wind and Earth’s magnetic field interacting. Particles charged with energy are emitted from the Sun and make up the solar wind. In the Earth’s magnetic field, they are dragged towards the poles tremendously. When particles clash with atoms as well as molecules in the ionosphere, kinetic energy is converted to visible light.
What Are Northern Lights?
The aurora is caused by charged particles from the Sun colliding with the Earth’s atmosphere. The northern and southern hemispheres’ magnetic poles are visible from space, as are the lights. For those in the northern hemisphere, they go by the names “Aurora Borealis” and “Aurora australis,” respectively. Light green and pink are by far the most typical hues for auroral displays. There have been reports of hues ranging from crimson to violet. As far as color is concerned, many different shapes and sizes of lights may be seen in the sky, including streaks of light, arcs of light, rippling curtains, and shooting rays that cast a gloomy shadow over the horizon.
History of the Northern Lights
A 30,000-year-old cave picture in France shows the northern lights, while Italian scientist Galileo Galilei created the word “aurora borealis” in 1619. Astonishment has engulfed civilizations around the globe since that time, with many origin tales ascribed to the dancing lights. The northern lights are the reflection of the Valkyrie’s armour in a North American Inuit tradition, while the Vikings believed they were the reflection of the spirits playing a game of ball with a walrus head.
The northern lights were also noted in the chronicles of early astronomers. According to NASA, a royal astronomer working for King Nebuchadnezzar II of Babylon recorded observations of the aurora on a tablet dating from 567 B.C. In comparison, a Chinese account from 193 B.C. also mentions the phenomena.
It wasn’t until the start of the twentieth century that theorists attempted to explain the northern lights phenomenon. Birkeland argued that electrons released by sunspots were steered toward the poles by Earth’s magnetic field, resulting in the atmospheric lights. Birkeland died in 1917. Therefore, the hypothesis wouldn’t hold up for long.
How Scientists explain northern Lights
Fortunately, we have the Swedish Institute for Space Physics in Kiruna, studying the Northern Lights for decades. The solar wind helps the ionosphere’s particles fly at breakneck speeds. Particles clash with atoms when they enter the atmosphere. Despite losing some of its energy, the particle is able to keep moving, albeit at a slower speed. A second atom is smashed into it at some point in time.
The energy that has been released from the atoms that have collided with the particles is visible in the form of a flash of light. There are more atoms in the air the closer you go to Earth. After colliding with several atoms, the particle steadily loses energy as it slows down, eventually stopping roughly 100 km above the Earth.