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Abisko

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Abisko has a reputation as the "Aurora Capital of the World" it sits directly under the "Aurora Oval", the region where the northern lights are most active. The village is blessed with a unique microclimate that creates exceptionally clear skies, minimizing cloud cover and maximizing your chances of seeing the lights. Abisko also has strict light pollution regulations, helping to ensure that the night sky is truly dark, enhancing the brilliance of the aurora.

Abisko is also home to the Aurora Sky Station this incredible viewing platform offers panoramic views of the sky and is a prime spot to catch the show.

Aurora season is between late September and early April, with the peak viewing in February and March.

Credit: Timmy Siik
Credit: Niklas Sagrén
Credit: Mathias Celis
Credit: Mathias Celis
Credit: Niklas Sagrén
Credit: Peter van der Meulen
Credit: Lucas Santos

How are my chances of seeing the aurora today?

0%

There is a 0% chance of seeing the aurora overhead in the Abisko area (forecast for 28 April 2025 at 10:22am UTC)

Kp 0.67

The Kp-index is a scale used to measure geomagnetic activity. It ranges from 0 to 9, with higher values indicating greater geomagnetic activity.

0-2 (Very low) Far north, quite dim, and not very active.
3-5 (Moderate) Can be seen further south, with increased brightness and activity. Chance of good viewing conditions nearer the pole.
6-7 (High) Visible in many northern regions, with vibrant displays.
8-9 (Extreme) Widespread visibility, often seen in areas much further south than usual, with intense and colorful displays.

Bz 2 nT

Bz refers to the north-south orientation of the magnetic field embedded in the solar wind. It is measured in nanoteslas (nT).

When Bz is negative (southward), it allows solar wind particles to penetrate the Earth’s magnetic field more easily. A strong negative Bz is often associated with increased chances of seeing the Northern Lights.

Conversely, when Bz is positive (northward), the Earth’s magnetic field tends to block the solar wind, resulting in reduced auroral activity.

Density 1.53 p/cm³

Solar wind density refers to the number of charged particles in a given volume of the solar wind, typically measured in particles per cubic centimeter (p/cm³).

A typical solar wind density is around 2.76 p/cm³.

The density of the solar wind affects how many particles reach the Earth’s magnetosphere. A higher density means more particles are available to interact with the Earth’s magnetic field. When these charged particles collide with the gases in the Earth’s atmosphere, energy is released in the form of light that we see as the aurora.

Speed 392.3 km/s

Solar wind speed refers to the velocity at which charged particles are ejected from the Sun’s outer atmosphere, known as the corona.

A typical solar wind speed is about 375 km/s. When both speed and density are high, the energy transferred to the Earth’s magnetosphere increases, enhancing the chances of seeing vibrant auroras.

Snow

4°C Feels like 1°C

High: 4°C
Low: -6°C

Precipitation: 100%
Cloud cover: 98%
Wind: 4 km/h
Rain: 3mm
Snow: 6mm

Moon

Waxing crescent

Sun rises at: 3:51am
Sun sets at: 9:32pm
Moon rises at: 3:00am
Moon sets at: 1:00am

Book an amazing adventure in Abisko

Free cancellation

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Free cancellation

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Free cancellation

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Free cancellation

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