X-Class Solar Flare Causes Radio Blackouts on U.S. West Coast and Pacific Ocean

ICARO Media Group
News
22/02/2024 18h19

Yesterday, Earth experienced the impact of a powerful X1.9-class solar flare emitted by sunspot AR3590. This volatile sunspot with a "beta-gamma-delta" magnetic field configuration is known for producing X-class solar flares. Space weather physicist Tamitha Skov reported on Twitter, now known as X, that the solar flare resulted in an R3-level #RadioBlackout over regions in the Western Pacific, including the Western USA, Canada, New Zealand, Eastern Australia, and Indonesia. Additionally, Skov mentioned that a few hours later, the same sunspot released another X1.7-class solar flare, adding to the heightened solar activity.

Solar flares are intense bursts of radiation originating from the sun's surface, often linked to strong magnetic activity in sunspots. They are categorized based on their strength with X-class flares being the most potent, and are known for their ability to cause radio blackouts on Earth. X-class flares like the recent one that occurred are less frequent but carry substantial impacts, including radiation storms that can affect satellite operations and expose airlines to heightened levels of solar radiation.

The occurrence of X-class solar flares is expected to increase as the sun approaches its solar maximum phase, marked by heightened sunspot activity. The next solar maximum is anticipated to take place by the start of 2026, indicating a period of more frequent and intense solar weather events. Despite the risk posed by solar flares, the likelihood of an event as severe as the historical Carrington Event of 1859, which caused widespread disruptions to telegraph systems globally, is currently low.

As the world relies more heavily on technology and space-based systems, monitoring and understanding solar weather phenomena become crucial to mitigating potential impacts. While the chances of a Carrington Event-level solar flare directly affecting Earth are slim, the significance of preparedness and precautionary measures cannot be overstated in safeguarding against potential disruptions from solar activity.

The views expressed in this article do not reflect the opinion of ICARO, or any of its affiliates.

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