According to NOAA’s Space Weather Prediction Center (SWPC), a G1-class geomagnetic storm is forecast to impact the planetlate on Saturday, January 15 and on Sunday, January 16. In the latest update from the SWPC, they say the area of impact will primarily be poleward of 60 degrees Geomagnetic Latitude. In this region, weak power grid fluctuations can occur on Earth. In space, minor impact on satellite operations are possible. Elsewhere, Mother Nature may light up the skies more south than usual; aurora could be visible at high latitudes across the northern tier of the United States, such as northern Michigan and Maine.
While a significant winter storm is expected to unfold in portions of the eastern U.S. on Sunday too, there is no direct relationship between this space weather event and the Earth weather event.
Chart showing NOAA Space Weather Scales for Geomagnetic Storms. Image: NOAA
The GOES-16 weather satellite is one tool space weather experts use to monitor the Sun’s activity. Image: NOAA
In the latest Space Weather Forecast Discussion, the SWPC writes, “Solar wind parameters are expected to continue at background levels on January 13-14 as ambient solar wind conditions persist. Enhanced conditions are expected late on January 15 as a recurrent, negative-polarity coronal hole high speed stream becomes geoeffective (CH HSS).” They add, “Late on January 15, G1 (Minor) geomagnetic storm conditions become likely due to the arrival of the aforementioned coronal hole.”
Coronal holes can develop at any time and location on the Sun, but are more common and persistent during the years around solar minimum. Coronal holes are most prevalent and stable at the solar north and south poles; but these polar holes can grow and expand to lower solar latitudes. It is also possible for coronal holes to develop in isolation from the polar holes; or for an extension of a polar hole to split off and become an isolated structure. Persistent coronal holes are long-lasting sources for high speed solar wind streams, also known as “CS HSS”. As the high speed stream interacts with the relatively slower ambient solar wind, a compression region forms, known as a co-rotating interaction region (CIR). According to the SWPC, from the perspective of a fixed observer in interplanetary space, the CIR will be seen to lead the CH HSS.
Strong CIRs and the faster CH HSS can impact Earth’s magnetosphere enough to cause periods of geomagnetic storming to the G1-G2 (Minor to Moderate) levels; although rarer cases of stronger storming may also occur.
NOAA forecasters analyze a variety of solar data from spacecraft to determine what impacts a geomagnetic storm could produce. If Earth is experiencing the effects of a coronal hole and a coronal mass ejection is forecasted to impact Earth, the combined effects could result in a more significant impact and more intense geomagnetic storming. Analyzing data from the DSCOVER and ACE satellite is one way forecasters can tell when the enhanced solar wind from a coronal hole is about to arrive at Earth. A few things they look for in the data to determine when the enhanced solar wind is arriving at Earth:• Solar wind speed increases• Temperature increases• Particle density decreases• Interplanetary magnetic field (IMF) strength increases While these solar events can help illuminate the sky with stunning aurora, they can also do considerable harm to electronics, electrical grids, and satellite and radio communications.
The Northern Lights could come to life in a brilliant way in places more south than usual during the Geomagnetic Storm.
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