The sun emitted a powerful solar flare on Oct. 3, according to NASA, prompting the Space Weather Prediction Center to issue a Geomagnetic Storm Watch due to the forecasted arrival of coronal mass ejections.
They occur when the powerful magnetic fields in and around the sun reconnect and are usually associated with active regions, often visible as sunspots, where the magnetic fields are strongest, according to NASA.
Their strengths are classified on a scale ranging from the lowest B-class to C-class, followed by M-class, and then the largest, X-class, with each letter representing a tenfold increase in energy output.
“This flare is classified as an X9.0 flare. X-class denotes the most intense flares, while the number provides more information about its strength,” NASA said in the Oct 3. blog post.
Solar flares can affect radio communications, electrical power grids, and navigation signals. NASA stated that flares also pose risks to spacecraft and astronauts.
Radiation from the recent flare could lead to “strong degradation or signal loss in high-frequency (HF) communication bands over much of the sunlit side of Earth,” according to the NOAA.
Solar flares are also often accompanied by coronal mass ejection (CME), during which a large mass of plasma and highly magnetized particles is violently ejected from the sun.
“A CME is anticipated to reach and impact Earth with elevated geomagnetic response and dependent upon the orientation of the embedded magnetic field, potential exists for Strong Storm levels,” it said.
The SWPC stated that there may be “limited, minor effects to some technological infrastructure” resulting from the anticipated geomagnetic storm but that they are “mainly mitigatable.”
NOAA said that aurora lights may be visible “over many of the northern states and some of the lower Midwest to Oregon.”