The Northern Lights

Myths and legend

The northern lights have aroused the curiosity of humanity throughout history. Obviously, those cultures settled at higher latitudes were the ones that most developed myths about these strange lights that are usually seen in the dark skies in the polar regions.

Even so, there are records by other cultures established in middle latitudes. It is believed that some drawings found in caves in the South of France, around 30 000 years ago, in the Cro-Magnon era, refer to the northern lights. Eastern Asian cultures, like the Chinese, also picked up these strange lights with myths and allusive legends. Greek and Roman civilizations have also echoed them, and it is even believed that some Old Testament passages describe auroral phenomena. The northern lights continue to inspire artists of all kinds.

It was in the 18th century when important attempts to give a scientific explanation to this phenomenon started, despite some previous ones based on erroneous premises.

Aurora over Bleik, a small town not far from Andøya Space, Andøya, Norway.

What are the northern lights?

In places located at high latitudes, like Norway, we often see the northern lights (aurora borealis) on clear evenings. The northern lights are far more common in northern Norway than in southern Norway. The phenomenon extends like a luminous band around the magnetic north pole. Therefore, this oval is not concentric with the Earth rotation axis, but have a certain inclination. Areas at 69 degrees latitude are below the center of the auroral oval during the night-time, while this is happening for areas around 80 degrees for the daytime aurora oval. A similar phenomenon is found in the southern hemisphere. It is called the southern light (aurora australis). The common word for northern and southern lights is auroras.

The northern lights oval. The arrow points in the direction of the Sun, while the colors indicate intensity. Note that the oval is wider towards the night side.

Northern lights and the geomagnetic field

The English scientist Sir Edmund Halley, saw the most beautiful northern light of the 18th century in 1716. Halley explained the aurora as follows: ‘The auroral rays are due to the particles, which are affected by the magnetic field; the rays are parallel to the Earth’s magnetic field, and the shape of the vault is due to perspective phenomena.’ This is the first scientific finding that was accepted at that time and is still true. Halley, of course, is not known for the northern lights but for Halley’s comet, whose movement he could predict.

A multitude of theories was presented to explain the northern lights. A common proposal was to include a burning gas as a key part of the theory. Some of the theories of this kind had already been introduced by the ancient Greeks, more than 2 000 years before. In 1741, the Swedish scientific, Celsius, observed a connection between the northern lights and magnetic activity. In fact, he stole the result and the resulting honor from his student Hjorter. However, we should consider this result as the second correct scientific finding in the northern lights, which has been accepted since it was proposed.

The next illustration shows the geomagnetic field. This is a simple magnet created because of the movement of charged particles in the interior of the Earth. It would be symmetric in absence of external interaction.

We see it asymmetric because of the solar wind. This pushes the dayside lines of the geomagnetic field and elongates the night side by forming recombinations of the dayside filed lines that move towards the night side. The next slide shows the magnetic field lines and how they are deformed due to the interaction with the solar wind. This is the typical appearance of the Earth’s geomagnetic field lines. The major amount of lines elongates and concentrates on the night side.

Northern lights and the Sun

In 1859 the English amateur astronomer Richard Carrington also connected a very strong aurora to an event he observed on the Sun 17 hours earlier. However, no physical explanation was presented. This is called the Carrington Event.  The next figure shows Richard Carrington’s drawing in 1859 of the solar flares he identified while observing sunspots, and the magnetograms recorded at the Greenwich Observatory in London during the Carrington Event of 1859. The bottom line (D) represents the direction of the compass; the upper line (H) represents the horizontal force.

The northern lights are often associated with major eruptions in the sun, solar storms, or corona holes. In the solar magnetic storms, the magnetic field energy is converted into kinetic energy that can release plasma out of the sun. Therefore, the aurora phenomenon starts in the sun, due to the solar activity, and is produced because of the interaction of these particles with the earth’s magnetic field. On some occasions, the magnetic field of the Earth and the magnetic field associated with the bubble of plasma that is coming from the Sun coupled, and the particles from the Sun drive through the Earth magnetic lines to the polar areas, where they encounter the higher layers of the atmosphere.

The eruptions occurred near large spots on the sun. In these spots, the magnetic fields are powerful and evolve in a complicated way. The magnetic fields can suddenly produce a ‘short circuit’ and cause powerful explosions that drive an important amount of energy released into space. The next picture shows some of these eruptions and how a giant cloud of gas is thrown out, on some occasions in the direction of the Earth.

When the solar particles enter the Earth’s atmosphere they collide with atoms. The energy is transferred from the particles to the atoms. The electrons of these atoms are kicked up to higher energy states or can be completely loose. Later, these electrons release the energy coming back to the original stage by emitting a photon with certain energy (wavelength) related to the jump between states. Other atoms trap lost electrons. Note that the electrons are the same so it may well be electrons coming from other atoms. This is the light we experience as northern lights!

The northern lights are located in an oval around each of the magnetic poles. These grow being wider when the activity increases, for example after a strong flare happens in the sun. Thus, the northern lights can be visible from southern latitudes, like southern areas in Norway. In very rare cases, northern lights can be even observed from northern parts of Africa and Mexico. Once it was reported the observation of auroras in Singapore, which is almost at the equator.

To the naked eye, the northern lights often look like a moving curtain, usually green, like waves in wind. Historically, the people thought they were quite low, and even that it was possible to reach them by going to mountains. However, the northern lights’ lower parts are located around 100 kilometers over the sea level.

Why different colors?

The colors of the aurora are probably what makes most of its charm. When people think about the aurora, they usually imagine green curtains dancing across the sky. In reality, the aurora harbors many more colors! They are related to several factors.

The most important is the entity (atom …) present: much like a neon tube glows red when its gas atoms are excited by electricity, each atom or molecule of the upper atmosphere produces a glow with a very characteristic color (wavelength) when they’re hit by solar particles. These specific colors can be viewed in an emission band spectrum measured by a spectrometer. Our eyes interpret the wavelengths as different colors. The transitions in our atmosphere are mainly produced by oxygen and nitrogen.

The main entities responsible for the aurora are monoatomic oxygen (O), diatomic nitrogen (N2), and ionized diatomic nitrogen (N2+). Oxygen emits either a red-orange or a lemon-green glow. N2 emits a deep red glow while its ionized form emits a deep blue/purple glow.  Sometimes the color limits are quite defined but most of the time the entities mix with currents at different altitudes and create other colors like pink, yellow, emerald-blue, magenta, and purple. During periods of intense geomagnetic storms, you can potentially get a lot of different colors at once. It’s also to be noted that there are other entities than O, N2, and N2+ at these altitudes: hydrogen, NO, helium … etc. Nevertheless, their interaction with solar particles doesn’t produce an auroral glow.

Altitude: the altitude determines what sort of entities are present in the air mixture. In addition, it plays a key role in allowing the entities of the atmosphere to glow. It’s all related to its density (number of entities per unit volume of the atmosphere). As a rule, the density decreases as we get further away from the Earth’s surface. This also applies to the part of the atmosphere where the aurora is created from ~ 80 km (mesosphere) to ~ 500 km (exosphere). Even at 80 km of altitude, the air is already very thin and you wouldn’t even be able to breathe. Above 300 km the density of the air is so low that the entities are too far apart from one another and rarely even bump into each other anymore! This has an impact on the colors. Certain entities take more time to emit the photon of light once hit by an electron. If another entity collides with the former before it has time to glow, it steals its energy and no glow is created! So the denser it is, the shorter time the entities have to produce the glow.

In the figure below you can see how the main colors (pink, green, red) are created. To make it simpler we just showed the collision of one particle with an oxygen atom at a high altitude producing a red glow.

Northern lights research in Norway

Norway is perfectly located on the globe for research on northern lights. The first serious scientific attempt to explain the aurora was done by Kristian Birkeland around 1905. He was the first testing that the phenomenon could be related to particles coming from the Sun. In order to check this hypothesis, he built an experiment, the Terella, with a magnetized ball representing the Earth being bombed by particles.

Birkeland and his assistant Olaf Devik with the Terella experiment.

Active research on the northern lights is ongoing in Norway. Andøya Space is an important place for making research ‘on-site’ by sending rockets with instruments for registering measurements throughout the northern lights. In addition, several ground-instrumentation is placed in Andøya and other places in Northern Norway dedicated to the understanding of this phenomenon. In Svalbard, the northern lights are observed during day time. The physical mechanisms involved are different. A complete picture of the northern light and geomagnetic field is giving by combining both, research from the night and dayside. In Svalbard, the dark time is so long and dark that it is easy to study the daylight. In addition, the archipelago is often located just below the northern light oval this time of day.

The ALOMAR observatory, placed in Andøya. ALOMAR has several instruments, including lidars, for researching the mesosphere and ionosphere.

Example of strong northern lights

In October 2001, several powerful northern lights were visible from Southern Norway. Sunday the 21st and Monday the 22nd of October fantastic northern lights were observed. The sky crackled in red and green and stripes pointed out in all directions. For many experienced viewers, this was one of the most beautiful northern lights in many years.

The northern lights were due to two powerful eruptions of the sun on the 19th of October. A new powerful eruption occurred on the 25th of October, but this did not have effects on earth. When the northern lights activity is very high, the northern lights oval is pushed so far south that it lies over southern Norway. In this particular case, it was possible to see over the head instead of towards the north. This often develops into a so-called ‘corona’, as shown below. During the corona, the northern light points out in every direction.

<< Previous chapterContent – Next chapter >>


This article is part of a pre-course program used by NAROM in Fly a Rocket! and similar programs.