Two powerful solar storms arriving at Earth today have captured the public's attention for their potential to spark amazing auroras, but scientists say there's another reason to watch. The solar double whammy is actually somewhat rare.
The particles from the two flares could interact as they head toward Earth, and researchers at the National Oceanic and Atmospheric Administration's Space Weather Prediction Center said they are monitoring the situation.
The sun unleashed a medium-sized flare on Monday (September 8) followed by a second, larger flare, called an Earth-directed X-class flare, on Wednesday (September 10). Both are from the same active sunspot region (Active Region 2158) and are directed at Earth, said Thomas Berger, director of the Space Weather Prediction Center, during a news conference September 11.
On supporting science journalism
If you're enjoying this article, consider supporting our award-winning journalism by subscribing. By purchasing a subscription you are helping to ensure the future of impactful stories about the discoveries and ideas shaping our world today.
Solar flares are powerful eruptions of radiation. Large flares can produce coronal mass ejections (CMEs), waves of solar plasma and charged particles that can travel millions of miles an hour through space. Last night, as expected, the first of the CMEs made its appearance and is expected to cause geomagnetic storming, reaching moderate levels, this morning, according to the Space Weather Prediction Center. [Sun Storm: See Images of the Amazing Solar Flares]
The magnitude of the new CMEs, however, isn't that unusual, Berger said. Typically, the sun launches between 100 and 200 CMEs of this size during a solar cycle, a time encompassing about 11 Earth years, he said.
"The unique thing about this event is that we've had two in close succession, and the CMEs could possibly be interacting on their way to Earth, at the Earth's orbit or beyond perhaps — we don't know that yet," Berger said.
In past solar cycles, it was not unusual to have two solar eruptions aimed at Earth at the same time. William Murtagh, a program coordinator at the Space Weather Prediction Center, told Live Science in an email.
"But we have seen very few such occurrences during this cycle," Murtagh said. "It is generally recognized that a worst-case scenario geomagnetic storm would involve two or more CMEs in succession, prolonging a geomagnetic [storm] over several days."
What's more, the second CME is moving at a faster speed and catching up to the first one.
"Currently our models show that it is not going to catch up to and interact with that CME, the first CME, when it's at the Earth's orbit," Berger said. But, he added, "the models are not exact and the inputs are not exact. So we're keeping a close watch on whether this storm is stronger than might be expected because of this possibility of interaction."
The two CMEs may lead to geomagnetic storms hitting Earth and could cause problems with radio and GPS signals, Berger said.
"It's fairly rare for two CMEs of this magnitude to come in close succession like this," he said. "Because of this we cannot rule out higher storm levels," particularly in polar regions where interactions with the Earth's magnetic field are strongest.
The International Space Station will measure the CMEs as they pass by, giving scientists on Earth a 30- to 45-minute head start to prepare for the CMEs. But, on the upside, the solar event is expected to produce an array of beautiful northern lights, visible to people living in the northern United States, said William Murtagh, a program coordinator at the Space Weather Prediction Center.
Whatever the CMEs' effects, the Space Weather Prediction Center said it would be following them closely.
"We're keeping a close eye on these events," Berger said.
The geomagnetic storming from these events is expected to continue through Sunday (September 14), according to the Space Weather Prediction Center.
Original article on Live Science.
Copyright 2014 LiveScience, a TechMediaNetwork company. All rights reserved. This material may not be published, broadcast, rewritten or redistributed.