Your best bet for determining if there is currently aurora activity is to take a peak at the current KP value. The chart on that page shows the current KP and the expected KP over the next 30-75 minutes. KP is a global scale that ranges from 0 to 9, the higher the value, the more active the aurora is and the closer to the equator it may be visible.
Once you know the current KP, you will want to know if it is possible to see aurora where you are at that KP. This map helps with that:
Find your location on this map, If you are in the Northern Hemisphere the KP level you need is the line to the south of your location. Likewise, if you are in the southern hemisphere the value you need is on the line to the north of your location.
Finally, check your weather. Aurora displays are high in the atmosphere. If it is cloudy, the aurora will be above the clouds and you will not be able to see them.
Great question! We hear it often. The answer needs to be more than 140 characters.
The short answer is yes. There are a number of reasons Norway, Sweeden and Finland are terrific travel location for aurora hunters. But surprisingly, this has nothing to do with there aurora activity in October – it comes down to it being the right balance of warm (or at least not insanely cold) and dark.
The longer answer:
Solar storms arrive at Earth in a pattern governed by activity cycles on the Sun which are completely independent of the position of Earth or the season on Earth. Solar storms and aurora are just as likely to happen in October as in any other month.
The solar cycle can be used for determining how likely it is that your visit to a higher latitude location will coincide with an aurora show. This 11-year cycle governs the number of active regions and sunspots on the sun. Generally speaking, when there are more sunspots, solar storms from flares are more likely and aurora are more likely. So, a trip to Scandinavia during the peak of the solar cycle is more likely to reward an aurora hunter. The current solar cycle, “cycle 24”, is now in it’s declining phase, but there are still plenty of nights with aurora in store over the next several years. Here’s a graph showing the progress of the current solar cycle:
Because a solar storm can arrive any time of the year, and at any time of day, the best place to be is where it is dark for a larger percent of the day. In the northern hemisphere, this means September through March, in the southern hemisphere March through September are the best aurora hunting months.
It also has to be clear to see the aurora because they are above the clouds. So, once you’ve picked a place to visit, choose a time of year where it is more likely to be clear skies.
In Vermont, where NLN is based, we frequently hear that August is the best time of year for northern lights – which goes entirely counter to the previous paragraphs. This discrepancy is due to weather. In August is it summer, its is warm and people are camping. People spend more time outside at night, and see more aurora. In the winter it’s cold and people huddle by their fireplaces at night, so they don’t even notice the aurora going on just outside their door. This leads to a perception that summer is a better time of year to see aurora.
Autumn seems to be the most comfortable and rewarding time of year to hunt aurora. The nights get longer, and the temperature hasn’t dropped too much yet.
So yes – go visit Scandinavia during October. Even if you don’t see the lights, it’s a wonderful place to visit.
When there is a solar storm on its way towards Earth, or when there is a geomagnetic storm watch posted (as in the watch currently in effect), we often post an image of the WSA-Enlil model output. WSA in the name is an acronym of the three researchers who contributed to the model, Drs. Wang, Sheeley and Arge. Enlil in the name comes from the Sumerian God of wind and storms.
The model output can be confusing or disorienting at first. The following is a walk through of some features which should help in understanding how to read the output. We’ll use a snapshot of the today’s output (click for a larger view)
The two main features on this image are higher than average proton density expected to arrive this evening and the large area of high speed solar wind expected to arrive Wednesday from the southern coronal hole. We’ve labeled the image, here is a quick guide:
Label “A”: This is Earth! The left two radial graphs show the Solar System from the north think of is as “from above”, The Sun is in the center. The red and blue circles on the other side of the Sun are the two satellites (Stereo ahead and Stereo behind. At the time on the snapshot, plasma density at Earth is elevated but decreasing.
Label “B”: The two sets of graphs on the right show the data over time, the yellow bar shows the point in time the radial graphs are displaying. The plasma density, or the amount of material moving through space, is shown in the upper graph. The bottom shows the speed that material is moving as it arrives at the measurement location. Label B shows Stereo A (ahead), was seeing increased plasma density during the first part of Jan 23. The space weather at this location has no impact on geomagnetic conditions at Earth. We sometimes see people excited that the levels are increasing at this remote satelite wondering if there will be aurora – probably not, sorry.
Label “C”: This small increase in density shown is responsible for this evening’s predicted geomagnetic storm. The plasma density is elevated, you can see looking at the date along the bottom of the graph that this is likely to peak towards the end of the 24 hour period.
Label “D”: The two meridional slices (the image between the circle and the graph) show a side view of the Earth and the Sun. Above the earth is what is happening in space above our North Pole, below is the South Pole. In this image, we’ve freeze-framed the video at 19:00 UTC on 1/28, next Wednesday. There is a large area of high speed wind (orange and red) south of Earth that is coming from the Large Southern Hemisphere Coronal hole shown below in AIA 211 as the dark area.
Finally, Label “E”: This graph shows the expected solar wind speed at the same three measurement locations. This shows an increase to 500 km/s. This increase is related to the high speed wind from the coronal hole reaching a little father north. If this increase in solar wind is accompanied by an increase in plasma density because of an Earth-directed eruption on the Sun’s surface, we may see an additional geomagnetic watch and again have the possibility of seeing Aurora.