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المملكة: Jeddah Astronomy: A huge coronal emission from the sun… without a direct impact on the Earth

The association announced The Astronomical Societyin Jeddah announced the observation of a huge coronal mass ejection in the latest images of the coronagraph of the GOES-19 satellite, where the data showed a bright and asymmetric halo indicating the release of huge amounts of plasma from the outer atmosphere of the sun.

The president of the association, Engineer Majid Abu Zahra, said that Preliminary observations showed that this event coincided with a Type II radio emission observed at 03:10 a.m. Mecca time on October 29, 2025, adding that the estimated speed of the outburst reached about 1,279 kilometers per second, a speed described as high energy and usually associated with strong coronal ejections.

Emission source

Abu Zahra explained that analyzes indicate that the likely source of this emission is the active sunspot region AR 4246, which is currently located about four days away from reaching the eastern edge of the sun.
He added that this region is considered one of the most magnetically active regions at the present time, as repeated flares of the moderate category have been recorded in it during the past days, which reflects a state of rising turmoil in the surface of the sun.

Possible effects

Active solar cycle

The association confirmed that this event represents new evidence of the increase in solar activity in the current cycle, which is characterized by increasing coronal mass emission and strong flares, pointing out that following such phenomena is necessary to understand the evolution of solar magnetic fields and evaluate their repercussions on the space environment near the Earth.

Continuous monitoring and follow-up

Abu Zahra concluded by noting that global solar observatories such as GOES-19, the SOHO telescope, and the Solar Dynamics Observatory will continue to closely monitor this event during the coming days, in order to determine its precise speed and final direction and evaluate any potential effects on the Earth’s magnetosphere.

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