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☀️ Powerful Solar Eruption on the Sun's Western Limb‼️

😉 On November 21, 2024, around 18:00 UTC, a powerful solar eruption occurred behind the Sun's western limb, triggering an extremely energetic coronal mass ejection (CME). The eruption was accompanied by a shock wave that accelerated protons to energies exceeding 500 MeV.

Experts report that this event has caused the most energetic solar radiation storm since 2005, or possibly since the famous Halloween storms of 2003. The storm's hard radiation spectrum highlights the magnitude of the eruption.

🟡The likely source of this event is one of the Sun's active regions—either Region 3889 or Region 3897—located on the far side of the Sun. Despite its scale, the CME does not appear to have an Earth-directed component, as the coronal wave remained localized near the western limb.

😊 Unfortunately, the Parker Solar Probe and Solar Orbiter were not in favorable positions to observe the event remotely or in situ, limiting detailed analysis of the phenomenon.

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☀️ November 27, 2024: The Sun Demonstrates Significant Activity

😉 On November 27, 2024, the Sun exhibited notable activity that captured the attention of scientists. Around 18:45 UTC, a solar filament eruption occurred in the southeastern region of the solar disk. This event was accompanied by a coronal mass ejection (CME) directed predominantly southward, minimizing its potential impact on Earth, though a slight glancing blow remains possible.

😊Later, around 20:00 UTC, a farside CME event was observed on the Sun's southeast limb. Its influence is expected to remain limited, with no significant effects on Earth’s magnetosphere.

🌈 Throughout November, solar spot numbers rose sharply, surpassing 200 once again. The monthly average reached approximately 150, significantly higher than anticipated. These findings suggest that the peak of the current Solar Cycle 25 will be stronger and occur later than previously estimated. Experts confirm there is no evidence of a "Grand Solar Minimum" at this time.

‼️ This heightened solar activity highlights the dynamic nature of the ongoing solar cycle. Monitoring continues as these solar events influence space weather, satellite operations, radio communications, and navigation systems on Earth.

🔗Source: link

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🌍 ☄️🛰️ Asteroid 2024 XA: A Close Encounter with Earth

A newly discovered asteroid, designated as 2024 XA, had an extremely close approach to Earth on December 1, 2024, passing just 843 miles (approximately 1,356 km) from the planet's center, equivalent to 0.03 astronomical units. It passed over the Pacific Ocean, marking the closest recorded asteroid flyby of the year.

The asteroid was first detected by the Catalina Sky Survey in Arizona only five hours before its closest approach.

This event highlights the importance of continuous monitoring systems to detect near-Earth objects, as the warning time in this case was minimal.

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☀️ Intense Solar Activity: A Magnetic Storm Expected on New Year's Eve‼️

😉 On December 29, 2024, a powerful X-class solar flare occurred, part of a series of strong M-class flares observed in the past two days. This activity has led to predictions of a major geomagnetic storm, expected to reach Earth during the night from December 31 to January 1.

⚡️Today, December 30, another X2 flare erupted from the same sunspot region, likely triggering another coronal mass ejection towards Earth. This flare caused an R3-level radio blackout storm in Australia, signaling intense solar activity.

🌈 The storm is expected to reach a G3 level or higher, which could lead to phenomena such as auroras visible in mid-latitudes under clear skies. At the same time, such a storm may affect people who are sensitive to weather changes, causing headaches, drowsiness, and irritability.

🌍 Experts continue to monitor the situation and warn that, in addition to visual effects, the magnetic storm could impact electrical grids, satellite systems, and navigation devices.

🔗 Source: meteoagent.com
🔗 Source: Space Weather Live

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📈 X-Class Solar Flares: Increasing Activity

😉 On January 3, 2025, two powerful X-class solar flares were recorded from active region AR13947. These events highlight the growing intensity of Solar Cycle 25 (SC25), which has already significantly outpaced Solar Cycle 24 (SC24).

☀️ The first flare, an X1.2 event, peaked at 11:40 UTC. It occurred in the eastern part of the solar disk, where its impact on Earth is minimal due to its remote location. At the time of the event, information about the associated coronal mass ejection (CME) was still limited.

😊 Less than 12 hours later, at 22:41 UTC, the same active region produced another X-class flare, rated X1.1. This flare was accompanied by a CME that, according to preliminary data, is more Earth-directed than the CME associated with the earlier event. Experts are closely monitoring to assess potential impacts on geomagnetic activity.

‼️ Notably, Solar Cycle 25 has already seen 78 X-class flares — a 280% increase compared to the same stage of Solar Cycle 24. Scientists predict a high likelihood of further flares, as repeated activity in a single solar region is a key indicator of future events.

🌍 Health Advisory: Solar flares and related geomagnetic disturbances can exacerbate symptoms such as headaches, fatigue, and irritability. It is advised to minimize stress and monitor your well-being.

These events may also impact satellite systems, radio communications, and create opportunities for auroras at high latitudes.

🔗 Source: spaceweatherlive.com

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📈 The Sun remains active: third X-class flare in recent days

☀️ On January 4, 2025, another powerful X-class solar flare was recorded, marking the third such event in recent days. This time, active region AR3947 produced an X1.8 flare that peaked at 12:48 UTC. The associated coronal mass ejection (CME) was directed eastward, similar to the CMEs from the previous two X-class flares.

😊 Region AR3939 also contributed to the solar activity, generating two long-duration C-class flares. The first, rated C9.3, occurred at 15:09 UTC, followed by a C7.6 flare at 19:15 UTC. Both events produced CMEs directed westward.

😉 These solar activities have already triggered a minor radiation storm, which may intensify in the coming days. Additionally, the CMEs associated with these events are expected to cause geomagnetic storms on Earth, potentially affecting radio communications, satellite operations, and leading to auroras visible at higher latitudes.

‼️ The Sun continues to exhibit increasing activity, consistent with the current phase of its 25th solar cycle.

🔗 Source: spaceweatherlive.com

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🌌 Forecast of Magnetic Storms (Solar Flares) for Today, January 6, 2025
😉 The forecast is updated as data from satellites and laboratories from around the world becomes available.

🔗 Source: METEOAGENT (https://meteoagent.com/solar-flares-storms)

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☀️ Solar Flare: Long-Duration M1.1 Emission

😉 On January 7 at 23:05 UTC, an M1.1-class solar flare was detected in active region AR3939, located just behind the Sun's southwestern limb.

😊This flare was long-lasting, making it notable for astronomers. However, the good news is that the associated coronal mass ejection (CME) is not Earth-directed.

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😉 Solar Flares on January 9, 2025: Activity in AR3947

😊 On January 9, 2025, the Sun exhibited increased activity associated with active region AR3947.

☀️ Early in the morning, at 01:09 UTC, a minor solar flare of class M1.1 was recorded. Later, at 10:58 UTC, a long-duration C3.9-class flare occurred near the Sun’s central disk. This event was accompanied by dimming and the formation of bright loops in the Sun's corona, indicating significant energy releases into space.

🌈 Experts anticipate possible auroras at mid-latitudes. However, data from the GOES-West satellite magnetometer has not yet confirmed significant changes in geomagnetic conditions. The effects of the solar eruption may become noticeable in the coming hours.

‼️ Such solar activity highlights the importance of monitoring space weather to predict its impact on Earth, including satellite communications and atmospheric phenomena.

🔗 Source: spaceweatherlive.com

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