Sunspot region 3089 is one of four sunspot regions being monitored that have a notable flare probability, though it is the only one capable of triggering a powerful geomagnetic storm in the Earth’s atmosphere.
“This sunspot region was active a few days ago but has quieted down considerably. Remarkable as it does have a magnetic delta structure,” SpaceWeatherLive, which tracks real-time auroral and solar activity, stated in its latest report on the sunspot region.
The presence of a magnetic delta structure means it has the potential to release an X-class flare - the biggest type of flare.
X-class flares are rare occurences but can produce as much energy as a billion hydrogen bombs, according to Nasa.
“If they’re directed at Earth, such flares and associated coronal mass ejections (CMEs) can create long lasting radiation storms that can harm satellites, communications systems, and even ground-based technologies and power grids,” the US space agency warned.
“X-class flares on 5 December and 6 December, 2006, for example, triggered a CME that interfered with GPS signals being sent to ground-based receivers... With advance warning many satellites and spacecraft can be protected from the worst effects.”
The current probability that Sunspot region 3089 will produce an X-class flare is 5 per cent, according to National Oceanic and Atmospheric Administration (NOAA) in the US.
The position of the sunspot means it is “absolutely something to keep an eye on” in the days ahead, SpaceWeatherLive’s report stated.
It concluded: “If the group producing a strong solar flare launches a coronal mass ejection the chances are high that it will have an earth-directed component.”
If it does reach Earth, the resulting geomagnetic storm could cause damage to satellites and telecommunication infrastructure.
Experts warn that severe solar storms could even result in widespread blackouts, with Dr Mike Hapgood, chair of the Space Environment Impacts Expert Group (SEIEG) told The Independent that such an event could wreak havoc with GPS systems.