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Chasing the Northern Lights

How Science Predicts the Aurora

Aurora in Alaska
Courtesy of Rob Redmon, NOAA NCEI

From September until April, when the days are at their shortest and often their darkest, the Northern Lights are at their brightest. There’s no doubt that the stunning light shows, known scientifically as the Aurora Borealis (Aurora Australis in the Southern Hemisphere), are not only an item on many people’s bucket lists, but also a boon to the local economies lucky enough to have a front-row seat for the show.

For those of us who aren’t lucky enough to view the Northern Lights from our living rooms—like residents of Iceland or the Canadian Yukon—how do we know when it’s a good time to book our plane tickets and bundle up for a trip to see this spectacle? Thankfully, science can help you!

Monitoring Space Weather to Predict Auroras

Auroras exist in both the Northern and Southern Hemispheres, but the northern counterpart is far more popular for tourists hoping to catch a glimpse of the display. The Northern Lights evolve from the sun’s activity that affects the conditions in space around our star and near Earth, commonly referred to as “space weather”. NOAA scientists and forecasters at the National Centers for Environmental Information (NCEI) and the Space Weather Prediction Center (SWPC) study, monitor, and track the phenomena related to space weather and have developed methods to predict the likelihood of aurora occurrence. Click here to learn more about the space science behind the beautiful Auroras. 

Being able to see the aurora depends mainly on two factors: geomagnetic activity (the degree of disturbance of the Earth’s magnetic field at the time) and your geographic location. Of course, local weather, light pollution from city lights, a full moon, and other factors can affect your viewing possibilities as well.

To know whether you have a chance of seeing an aurora, you need to know the level of geomagnetic activity occurring at the time you are viewing. The higher the geomagnetic activity, the brighter and further away from the polar regions the aurora will be able to be viewed. Space Weather forecasters at NOAA SWPC constantly monitor and forecast the geomagnetic activity, communicating its current and future levels through the G-scale. The G-scale is based on the values of the planetary K index, or Kp, that ranges from zero to nine and is derived from the maximum fluctuations of horizontal components of the Earth’s magnetic field measured by ground-based magnetometers during a three-hour interval. The current and near-future G-scale can be seen at the top of SWPC’s main webpage.

Graphic depicting geomagnetic storm aurora condition on a scale of zero to five. Under each number on the scale is the following text: G-0: No G-scale Geomagnetic Storming: Quiet-time. Aurora will be visible far north, quite dim in intensity, and not very active, Kp<5. G-1: Aurora will become brighter and more dynamic (motions and formations). It is commonly visible at high latitudes (e.g., northern Michigan and Maine), Kp=5. G-2: Aurora will become brighter, more active, and move further from the poles. It has been seen as low as New York and Idaho (typically 55° geomagnetic latitude), Kp=6. G-3: Aurora will become even brighter, more active, and move further from the poles. It has been seen as low as Illinois and Oregon (typically 50° geomagnetic latitude), Kp=7. G-4: Aurora will move even further towards the equator, and it will become very bright and very active. It has been seen as low as Alabama and northern California (typically 45° geomagnetic latitude), Kp=8 to 9. G-5: At this level, Aurora may be seen directly overhead from the northern states of the USA, but also at the northern horizon in southern states, such as Florida and southern Texas (typically 40° geomagnetic latitude), Kp=9
Source: NOAA Space Weather and NCEI

Below are maps showing the most southern extent of where aurora borealis might be observable for different levels of the geomagnetic Kp index (and G-scale). These limits are approximate, considering the averaged relationship between Kp and the auroral latitude, and indicate regions from which aurora may be visible (not necessarily overhead, but sometimes only at the northern horizon).

Two maps showing how far south an aurora can be observed in the Northern Hemisphere. G is the NOAA Geomagnetic Storm Index (0–5). Kp is the Planetary K Index (0–9). The first map shows aurora reaching into North America with a blue line indicating how far south aurora can be observed with aurora condition at G=0 Kp=3; a green line indicating how far south aurora can be observed with aurora condition at G=1 Kp=5; a yellow line indicating how far south aurora can be observed with aurora condition at G=3 Kp=7; and a red line indicating how far south aurora can be observed with aurora condition at G=5 Kp=9. The second map shows aurora reaching into Northern Europe, Russia, and Kazakhstan with a blue line indicating how far south aurora can be observed with aurora condition at G=0 Kp=3; a green line indicating how far south aurora can be observed with aurora condition at G=1 Kp=5; a yellow line indicating how far south aurora can be observed with aurora condition at G=3 Kp=7; and a red line indicating how far south aurora can be observed with aurora condition at G=5 Kp=9.
Two maps showing how far south an aurora can be observed in the Northern Hemisphere. G is the NOAA Geomagnetic Storm Index (0–5). Kp is the Planetary K Index (0–9). The first map shows aurora reaching into North America with a blue line indicating how far south aurora can be observed with aurora condition at G=0 Kp=3; a green line indicating how far south aurora can be observed with aurora condition at G=1 Kp=5; a yellow line indicating how far south aurora can be observed with aurora condition at G=3 Kp=7; and a red line indicating how far south aurora can be observed with aurora condition at G=5 Kp=9. The second map shows aurora reaching into Northern Europe, Russia, and Kazakhstan with a blue line indicating how far south aurora can be observed with aurora condition at G=0 Kp=3; a green line indicating how far south aurora can be observed with aurora condition at G=1 Kp=5; a yellow line indicating how far south aurora can be observed with aurora condition at G=3 Kp=7; and a red line indicating how far south aurora can be observed with aurora condition at G=5 Kp=9.
Maps showing the most southern extent of where aurora might be observable in the Northern Hemisphere for different levels of the geomagnetic Kp index (and the NOAA G-scale). Source: https://www.swpc.noaa.gov/content/tips-viewing-aurora 

To access the current SWPC’s prediction of the aurora’s visibility tonight and tomorrow night, you can access the SWPC Aurora Dashboard

After you confirm that your location is within the aurora visible region, you’ll also want to make sure you’re far enough away from a city to prevent light pollution. Check out the World Atlas of Artificial Sky Brightness: The brighter the area in this zoomable map, the harder it is to see stars and aurora in the night sky. Also, check the NOAA Weather Forecast for your area to make sure that it is not too cloudy outside. Finally, don’t forget to check out the moon phases before you go. A full moon makes it much more difficult to see an aurora because the background night sky will be brighter.

Since it is hard to forecast the Earth’s weather and space weather many weeks in advance, people that need to travel from afar to the auroral regions should consider the following information before planning their aurora hunt adventure: 1) The most favorable months to see stronger auroras are March and September, due to the best coupling between solar wind structures and the Earth’s magnetosphere around the equinoxes; 2) the best time to see auroras is around midnight (10 pm to 2 am local time); it is thus important that the aurora-hunter consider the number of hours of darkness per night at the location of interest in a particular month before traveling to the auroral region.