During moderate activity, all regions below the auroral oval are ideal (60° - 70° north approximately):
It all depends on the purpose of your trip:
One last thing to consider: Iceland has become very, very busy in recent years (the country is increasingly subject to a touristic overload, the authorities are working on the problem). Choose distant places north of the country to be quiet.
I will only consider Scandinavia because it is the region that I know the best. There, the northern lights season begins end of September and finishes at the end of March.
Prefer nights without Moon to enjoy auroras. A slight crescent, however, can be useful for photographers: it will reveal the landscapes on your photos. My favorite nights are the one around the week of the new Moon.
Yes! The solar cycle is only related to the number of spots that appear on the surface of the Sun, which reaches its maximum every 11 years or so.
However, contrary to popular belief, the spots are not the the only solar events to be at the origin of northern lights. There are also the coronal holes (see the article “Understanding the northern lights”). The formation of these holes is independent of the solar cycle and they appear very regularly on the surface of the Sun.
It is pointless to choose a period of polar night to have a better chance to see northern lights. The explanation is that the Earth revolves around its geographic north pole while the auroral oval is centered around the north magnetic pole (the 2 poles are separated by approximately 8°). Consequently, all the favorable observation regions are not always located under the auroral oval.
The following animation helps us understand the phenomenon (source: K. Akasofu - Asahi aurora classroom):
We can see that the pink point in Alaska enters the auroral oval around 8 p.m. and get out of it around 4 a.m. The times will be the same whatever the country you are in: the auroral oval remains static, it does not revolve around the magnetic north pole. Therefore, be ready from 8 p.m. in the evening: this is the entrance time under the auroral oval.
Also, do not go to bed before midnight: you will be in the heart of the most active region of the oval. Even though the aurora can happen quite early in the evening, force yourself to eat well to hold all night in case of intense show.
Watching the aurora is a static activity: we don’t move a lot during several hours. You will not enjoy the show if you are cold too quickly.
A good ski equipment is enough. In case of intense cold, you will multiply the layers: ski underwear, various fleeces, hot ski pants…
Invest to cover the extremities of your body, this is where the greatest heat loss happens.
Always carry with you a pair of crampons (sold for ten euros in supermarkets): they will avoid you slips and bad falls if there is ice on the ground (or if it is hidden under the snow).
Take a few heaters (hands and feet above all). Avoid rechargeable heaters in water boiling. You will forget to recharge them and they are few comfortable (they are very hard). Disposable models will do just fine.
Finally, do not forget a headlamp. Choose one with red lighting to keep your night vision and not dazzle your observation mates.
Northern lights is a high altitude phenomenon, which occurs well beyond the clouds (from 70 kilometers altitude). Therefore, you have to watch for the weather forecast as much as the solar storm forecast.
But do not despair if an evening starts under the clouds while the solar storm forecast is good: the weather can change quickly on the Norwegian coast. So watch the satellites animations to see if cloudy gaps are heading towards you (see the links at the end of the article).
Before moving, watch over:
This is especially true in Iceland:
When you arrive there, plan to buy a snow shovel (about fifteen euros) in an auto center, it can to be of great service to you and to get you out of a difficult situation. Consider also to buy a tow rope.
Finally, never take a risk and avoid snowy road verges, they are very soft: you can make your car fall there. Think about it if you have to do a U-turn.
You will have to get away from cities and their light pollution.
Auroras will appear on the northern horizon, from west to east, or at the zenith. So make sure at least some of these horizons are far away from any major city.
Be more demanding during spotting if you plan to take quality photos: see article Photographing the northern lights.
Stay alert from approximately 7 p.m. until at least midnight (an important activity can occur at this time: you will be at the heart of the auroral oval, see above).
There will be several shockwaves: the aurora will lose its activity, then will get back some. Tell you that the auroras are capricious: you just have to want to go to bed because there is no more activity so that the auroras wakes up… Also, in case of strong solar storm, it may happen that the aurora is visible while the Sun has just set (it may still be daylight), until very late at night. One time I observed an aurora at dawn in Iceland around 5.30 p.m. which ended around 5 a.m.!
If the cold hits you, take a break to warm up during low auroral activity: have a hot drink, get moving, put your hands under your armpits.
It all starts with observing the Sun. It is constantly scrutinized by satellites like SDO (Solar Dynamics Observatory) and STEREO (Solar TErrestrial RElations Observatory) :
If a coronal mass ejection (read the article “Understanding the northern lights”) is detected, we will know it 8 minutes later, the time to the light to reach the satellites. It remains to know whether the trajectory of the solar plasma cloud will cross the Earth. Its direction and size can already be estimated from the STEREO satellite measurements.
A first 3-days forecast is then made: the cloud of plasma travels between 400 and 750 km/s approximately, it will take 2 to 3 days to cross the Earth.
2 to 3 days later, the cloud “pierces” the ACE satellite (Advanced Composition Explorer). This satellite, located 1.5 million kilometers in front of the Earth, on the path of the plasma clouds, is a real sentinel. The clouds that cross it will be analyzed: density, speed, magnetic field, etc. From these measurements, a more precise forecast for the next 1 to 2 hours will be calculated.
Above, a solar flare modeled by the STEREO satellites. The first view is a “top” view of the solar system. The second view is the same view, in profile, of the Earth. The large green spirals correspond to the lines of interplanetary magnetic fields emitted by Sun (the Parker spiral).
The Kp index is a world index of the Earth’s magnetic field deformation. It can take values between 1 and 9. This index was introduced by the German geophysicist Julius Bartel in 1938:
If a northern light occurs, then most likely the Earth’s magnetic field is strongly compressed by the solar storm that it undergoes. This is why this index is used to predict the power of the northern lights.
Consequences:
In northern Norway, a Kp between 2 and 3 is enough to see a northern light at the zenith. More to the south in Europe, a Kp greater than 8 will be necessary to see a red aurora (around north).
Other measures may be given to you on apps or on specialized websites, sometimes synthesized into a single indicator called “Power of solar wind”:
The northern lights are capricious and their predictability is not an exact science:
The shape of the aurora you will observe will depend of your position:
Auroral activity is normal or low and the aurora is static in the sky. It is not very bright, its color is white. The aurora could be mistaken with a cloud. If you have any doubts, start a photographic exposure: if the cloud appears in green on the photo, then it’s an aurora. You have to wait, especially if the Kp forecast is good for the evening.
A solar particles cloud begins to agitate the ionosphere. The aurora begins to dance softly across the sky, like a curtain flapping in the wind near an open window. The streaks of the aurora correspond to the Earth’s magnetic field lines. This phase is called the trigger phase.
Activity is at its maximum. If the solar storm is intense, the aurora can occupy the whole sky and move at incredible speeds. There may be several expansion phases during a night. Again, don’t go to bed yet, even if the northern light seems to be extinguishing.
Coronal aurora is often the end of the most active phase of an intense solar storm night. It is the most spectacular phase of the aurora, the one that you will remember for a long time because its visual power is extremely intense.
The aurora is very bright. All of its streaks seem to come from one same point, it swirls around your head: it has the shape of a crown, hence its name. It occurs at the activity peak of the night, around 12 a.m.-1 a.m., when you are in the middle of the auroral oval. It requires a strong solar storm for it to occur. So it is quite rare, and above all it does not last very long (5 minutes).
If your camera is not ready, don’t try to use it: the phenomenon will be brief. So enjoy the show.
The pulsating aurora often marks the end of the night observations. This type of aurora is part of the so-called “recovery phase”. It follows a very strong solar storm, they are therefore rare. I saw them each time around 2 or 3 a.m..
Once upon a time I saw an aurora regain intensity after a pulsatile phase. The speed and intensity of the pulsations can change: sometimes very slow, sometimes extremely fast (several flashes per second).
Here is a pulsating aurora timelapse made in January 2013 in the Lofoten Islands in Norway:
Keep the following tips in mind:
Some useful applications for smartphones: