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New Geomagnetic Storm Could Illuminate Sky with Green Glowing Aurora in Time for Saint Patrick’s Day

by Weatherboy Team Meteorologist - March 15, 2022

The Northern Lights could come to life in a brilliant way on Labor Day as a solar wind is forecast to impact Earth.
The Northern Lights could come to life in a brilliant way on St. Patrick’s Day on March 17 as a new coronal mass ejection (CME) interacts with the Earth’s magnetic shield.




NASA equipment can help scientists determine the impacts from coronal holes. Image: NASA
NASA equipment can help scientists determine the impacts from coronal holes. Image: NASA

Just days after the Earth was impacted by a moderate geomagnetic storm, it appears a fresh Coronal Mass Ejection (CME) is expected to hit the Earth on March 17, perhaps illuminating the night sky of northern latitudes with dancing green auroras just in time for St. Patrick’s Day. On Sunday, March 13, an unstable filament of magnetism in the sun’s far-southern hemisphere exploded; it appears the resulting CME could directly or indirectly impact Earth’s magnetic field on Friday. At this time, NOAA’s Space Weather Prediction Center believes there’s a 45% chance of an Active or Minor Geomagnetic Storm conditions.

NOAA’s Space Weather Prediction Center (SWPC) hasn’t yet issued any  Geomagnetic Storm Watch for Friday’s event, but they continue to monitor this and other threats arriving from the sun. This new CME arrives just days after an earlier CME  impacted Earth as part of a C2-rated solar flare which leapt from the Sun late on March 10 / early on March 11. While a C2-rated flare wouldn’t typically trigger a moderate geomagnetic storm on Earth, because it lasted for so long, in which over a 12 hour period a massive amount of energy left the Sun,  the Earth experienced a moderate geomagnetic storm late on Sunday and early on Monday from that solar event.

Beyond lighting up the northern sky with Aurora, also known as Northern Lights,  power grid fluctuations can occur  on Earth while in space, satellite orientation irregularities could occur.  Communications can also be hampered: high frequency (HF) radio propagation can fade at higher latitudes.

While aurora can come in different colors, such as purples, blues, and greens, green is the most common color seen. When the solar wind hits millions of oxygen atoms in the Earth’s atmosphere at the same time, it excites the oxygen atoms for a time and they decay back to their original state; this process emits a green hue that is visible from the ground.




Chart showing NOAA Space Weather Scales for Geomagnetic Storms. Image: NOAA
Chart showing NOAA Space Weather Scales for Geomagnetic Storms. Image: NOAA

 

 

This map shows how far south the Northern Lights could appear at different KP index levels. While a KP of 3 or less would keep them in northern latitudes of Alaska and Canada, a KP of 9 would make them visible in places like Salt Lake City, St. Louis, Washington, DC, Chicago, Philadelphia, New York, Boston, and Portland. Image: NOAA
This map shows how far south the Northern Lights could appear at different KP index levels. While a KP of 3 or less would keep them in northern latitudes of Alaska and Canada, a KP of 9 would make them visible in places like Salt Lake City, St. Louis, Washington, DC, Chicago, Philadelphia, New York, Boston, and Portland. Image: NOAA

The K-index, and by extension the Planetary K-index, are used to characterize the magnitude of geomagnetic storms. The SWPC  says that Kp is an excellent indicator of disturbances in the Earth’s magnetic field and is used by SWPC to decide whether geomagnetic alerts and warnings need to be issued for users who are affected by these disturbances. Beyond signifying how bad a geomagnetic storm’s impact can be felt, the Kp index can also help indicate how low the aurora will be.

Scientists at the SWPC believe that  Kp index of  3  will be achieved on the 17th; however, further forecast refinements in the coming days could impact the ultimate Kp forecast.

CMEs are large expulsions of plasma and magnetic field from the Sun’s corona. They can eject billions of tons of coronal material and carry an embedded magnetic field that is stronger than the background solar wind interplanetary magnetic field (IMF) strength. CMEs travel outward from the Sun at speeds ranging from slower than 250 kilometers per second (km/s) to as fast as near 3000 km/s. According to the SWPC, the fastest Earth-directed CMEs can reach Earth in as little as 15-18 hours while slower CMEs can take several days to arrive. They expand in size as they propagate away from the Sun and larger CMEs can reach a size comprising nearly a quarter of the space between Earth and the Sun by the time it reaches our planet. The arrival of a CME can create a fresh geomagnetic storm event upon impact.

 

 




 

 

Aurora, also known in the Northern Hemisphere as "Northern Lights", is typically associated with clear, cold winter nights at northern latitudes.
Aurora, also known in the Northern Hemisphere as “Northern Lights”, is typically associated with clear, cold winter nights at northern latitudes. Strong geomagnetic disturbances and CMEs can also set-off the light show.

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.

A solar eruption seen by the SOHO spacecraft on July 24, 1999, with Earth inserted to give a sense of scale to the blast. Image: ESA / SOHO / EIT
A solar eruption seen by the SOHO spacecraft on July 24, 1999, with Earth inserted to give a sense of scale to the blast. Image: ESA / SOHO / EIT

The 1859 incident, which occurred on September 1-2 in 1859, is also known as the “Carrington Event.” This event unfolded as  powerful geomagnetic storm struck Earth during Solar Cycle 10. A CME hit the Earth and induced the largest geomagnetic storm on record.  The storm was so intense it created extremely bright, vivid aurora throughout the planet: people in California thought the sun rose early, people in the northeastern U.S. could read a newspaper at night from the aurora’s bright light, and people as far south as Hawaii and south-central Mexico could see the aurora in the sky.




The event severely damaged the limited electrical and communication lines that existed at that time; telegraph systems around the world failed, with some telegraph operators reporting they received electric shocks.

Artist rendering of the Parker Solar Probe in space. Image: NASA
Artist rendering of the Parker Solar Probe in space, one of the assets scientists use to better understand solar activity and their impacts to Earth . Image: NASA

A June 2013 study by Lloyd’s of London and Atmospheric and Environmental Research (AER) in the U.S. showed that if the Carrington event happened in modern times, damages in the U.S. could exceed $2.6 trillion, roughly 15% of the nation’s annual GDP.

While typically known for their weather forecasts, the National Oceanic and Atmospheric Administration (NOAA) and its National Weather Service (NWS) is also responsible for “space weather.” While there are private companies and other agencies that monitor and forecast space weather, the official source for  alerts and warnings of the space environment is the Space Weather Prediction Center (SWPC). The SWPC is located in Boulder, Colorado and is a service center of the NWS, which is part of NOAA. The Space Weather Prediction Center is also one of nine National Centers for Environmental Prediction (NCEP) as they monitor current space weather activity 24/7, 365 days a year.

 

The Sun is constantly churning material and magnetic fields which create an ever-changing landscape of features that last from milliseconds to days. NASA developed this infographic to illustrate a few of the most common features that can be seen on the Sun. Image: NASA/Mary Pat Hrybyk-Keith
The Sun is constantly churning material and magnetic fields which create an ever-changing landscape of features that last from milliseconds to days. NASA developed this infographic to illustrate a few of the most common features that can be seen on the Sun.
Image: NASA/Mary Pat Hrybyk-Keith

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