Colossal X-class solar flare erupts from ‘rule-breaking’ sunspot and Earth is in the firing line (video) (Image Credit: Space.com)
The active sun is kicking into overdrive.
In the early morning hours today (Aug. 14), the sun unleashed the most powerful class of solar flare, in a potent X-class eruption. The solar flare peaked at 2:40 a.m. EDT (0640 GMT) and caused shortwave radio blackouts over the sunlit portion of Earth at the time of the eruption, Asia and the Indian Ocean.
What makes this X-class solar flare particularly interesting is that it erupted from ‘rule-breaking’ sunspot AR3784 which had already garnered the attention of solar scientists and aurora chasers due to its strange polarity.
The sunspot’s polarity breaks a hundred-year-old rule, Hale’s Law, whereby sunspots in the Northern Hemisphere should be polarized -+. Instead, sunspot AR3784 is polarized ±, a whole 90-degree twist, according to Spaceweather.com.
Related: Rare pair of northern lights & Perseid meteor shower delights skywatchers
It’s not the first sunspot to break the rule, according to spaceweather.com, it happens approximately 3% of the time. However, a majority of “rule-breakers” show a “reversed polarity” of +- instead of -+, but AR3784 lies somewhere between the two.
Experts at Spaceweather.com suggested that the “magnetic underpinnings of this sunspot are corkscrewing in an unusual way. If opposite magnetic polarities get twisted together too tightly, there could be an X-class solar flare.” Lo and behold the sunspot did just that.
Solar flares are eruptions on the sun‘s surface that release intense bursts of electromagnetic radiation. These flares occur when built-up magnetic energy in the solar atmosphere is suddenly released. They are classified by size into different categories, with X-class flares being the most powerful. M-class flares are 10 times less intense than X-class, followed by C-class flares, which are 10 times weaker than M-class. B-class flares are 10 times weaker than C-class, and A-class flares, which are 10 times weaker than B-class, have no significant effects on Earth. Within each class, numbers from 1 to 10 (and beyond for X-class) indicate the relative strength of the flare.
Powerful solar flares like the one released this morning can often be accompanied by a coronal mass ejection — a large plume of plasma and magnetic field from the sun — it has yet to be confirmed whether a CME joined this eruption.
Aurora hunters cross your fingers and charge those cameras! (If you hope to snap a photo of the northern lights, check out our guide on where and how to photograph auroras.)
CMEs carry electrically charged particles known as ions, and when these collide with Earth’s magnetosphere, they can trigger geomagnetic storms. During these storms, the ions interact with gases in Earth’s atmosphere, releasing energy in the form of light. This phenomenon is recognized as the northern lights, or aurora borealis, in the Northern Hemisphere, and as the southern lights, or aurora australis, in the Southern Hemisphere.
If a CME is confirmed, we could be in for yet more geomagnetic storms and heightened aurora activity, so get those cameras charged just in case. We await further confirmation.
One thing we do know that accompanied the X-flare was a strong radio blackout on Earth. The shortwave radio blackouts detected over Asia and the Indian Ocean resulted from the intense burst of X-rays and extreme ultraviolet radiation emitted during the X-flare.
Radiation from solar flares reaches Earth at the speed of light and ionizes the upper atmosphere upon arrival. This ionization creates a denser environment for high-frequency shortwave radio signals that facilitate long-distance communication to travel through.
As these radio waves pass through ionized (electrically charged) layers, they lose energy due to increased collisions with electrons, which can weaken or entirely absorb the radio signals.
Editor’s note: If you capture a stunning photo or video of the northern lights (or southern lights!) and want to share them with Space.com for a possible story, send images, comments on the view and your location, as well as use permissions to spacephotos@space.com.
