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βοΈ Solar Activity Intensifies: Major Coronal Mass Ejection
π December 23, 2024, marked a significant increase in solar activity. Throughout the day, 4 C-class flares and 3 M-class flares were recorded, including a particularly powerful M9 flare.
β‘οΈ Observations indicate that a coronal mass ejection (CME) occurred in the northwest region of the solar disk. The eruption was unusually gradual yet spectacular, making it a rare event.
Experts note an acceleration in the frequency of large coronal mass ejections, raising attention to solar activity and its potential impact on Earth.
Source: Dr. Keith Strong via π (Twitter)
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Experts note an acceleration in the frequency of large coronal mass ejections, raising attention to solar activity and its potential impact on Earth.
Source: Dr. Keith Strong via π (Twitter)
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#Sun #SolarFlares #CoronalMassEjection #SpaceWeather #spaceweather #CME #Aurora #Geomagneticstorms #solarstorm #SolarFlare #Space #astronomy #SolarPhenomena #climate #destruction #anomaly
π X-Class Solar Flares: Increasing Activity
π 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).
βοΈ 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.
π 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.
βΌοΈ Notably, Solar Cycle 25 has already seen 78 X-class flares β 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.
π 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.
π Source: spaceweatherlive.com
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These events may also impact satellite systems, radio communications, and create opportunities for auroras at high latitudes.
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π The Sun remains active: third X-class flare in recent days
βοΈ 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.
π 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.
π 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.
βΌοΈ The Sun continues to exhibit increasing activity, consistent with the current phase of its 25th solar cycle.
π Source: spaceweatherlive.com
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βοΈ Solar Flare: Long-Duration M1.1 Emission
π 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.
π 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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π Solar Flares on January 9, 2025: Activity in AR3947
π On January 9, 2025, the Sun exhibited increased activity associated with active region AR3947.
βοΈ 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 Sunβs 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.
π 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.
βΌοΈ Such solar activity highlights the importance of monitoring space weather to predict its impact on Earth, including satellite communications and atmospheric phenomena.
π Source: spaceweatherlive.com
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βοΈ X-Class Solar Flare Returns After More Than 50 Days
π More than 50 days have passed, and we have once again witnessed an X-class solar flare. βοΈ Sunspot region 3947 produced an X1.8 flare on January 4, followed by silence... But on February 23, the departing sunspot region 4001 generated an X2.0 flare. The activity didnβt stop thereβtoday, the Sun has already produced several M-class flares. π₯
Stay tuned for more updates on solar activity! πβ¨
π Source: spaceweatherlive.com
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Stay tuned for more updates on solar activity! π
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