At 5:10 a.m. EDT (0910 GMT), an X-class solar flare — the most powerful sun-storm category — blasted from a large sunspot on the sun's surface. That flare was the strongest since 2015, at X2.2, but it was dwarfed just 3 hours later, at 8:02 a.m. EDT (1202 GMT), by an X9.3 flare, according to the National Oceanic and Atmospheric Administration's Space Weather Prediction Center (SWPC). The last X9 flare occurred in 2006 (coming in at X9.0).
According to SWPC, the flares resulted in radio blackouts: high-frequency radio experienced a "wide area of blackouts, loss of contact for up to an hour over [the] sunlit side of Earth," and low frequency communication, used in navigation, was degraded for an hour.
A massive, X9.3-class solar flare blasted from the sun at 8:02 a.m. EDT (1202 GMT).
Credit: SDO/AIA/Steve Spaleta
During large solar flares, the sun can also sling a cloud of energetic plasma from its body, an event called a coronal mass ejection (CME).
"It was accompanied by radio emissions that suggest there's a potential for a CME," SWPC space scientist Rob Steenburgh told Space.com. "However, we have to wait until we get some coronagraph imagery that would capture that event for a definitive answer."
The sunspot responsible for this morning's flares, active region 2673, is the smaller of two massive spots on the sun's surface, at only seven Earths wide by nine Earths tall, according to astrophysicist Karl Battams.
Yesterday, that same sunspot emitted an M-class solar flare — one-tenth the size of an X-class flare — leading to a coronal mass ejection aimed toward Earth that could cause auroras tonight as far south as Ohio and Indiana.
NASA's Solar Dynamics Observatory captured this view of a mid-level solar flare on the sun at 4:33 pm EDT on Monday (Sept. 4).
Credit: NASA/SDO
If aimed toward Earth, such an ejection could lead to even more spectacular auroras, but could also damage satellites, communications and power systems. That cloud of charged plasma would arrive within 1 to 3 or 4 days, Steenburgh said, although CMEs triggered by energetic flares generally come quickly.
The surge of activity might seem surprising, as the sun is approaching its solar minimum, with the lowest levels of activity in its 11-year cycle.
"We are heading toward solar minimum, but the interesting thing about that is you can still have events, they're just not as frequent," Steenburgh said. "We're not having X-flares every day for a week, for instance — the activity is less frequent, but no less potentially strong."
"These kind of events are just part of living with a star," Steenburgh added.
Email Sarah Lewin at slewin@space.com or follow her @SarahExplains. Follow us @Spacedotcom, Facebook and Google+. Original article on Space.com.
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