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βοΈ Powerful Solar Flare and Coronal Mass Ejection: Possible Impact on Earth
π On October 26, a stunning X1.86-class solar flare erupted on the Sun, accompanied by a large coronal mass ejection (CME) from active regions 3872 and 3873 near the eastern edge. This solar storm is likely partially directed toward Earth, as the ejected solar material is close to the zone where it could potentially reach our planet.
π The video of the flare shows a massive eruption moving southeast, with a comparison to Earthβs scale emphasizing its impressive size.
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βοΈ New Solar Flare: X2.0 in the Northeastern Region
π Yesterday, October 31, 2024, a powerful X2.0 solar flare erupted in active region AR3878, located in the northeastern part of the Sun. The flare peaked at 21:20 UTC and was accompanied by a faint coronal mass ejection (CME) directed primarily to the northeast, resulting in a glancing impact on Earth with minimal effects.
π Nevertheless, the flare caused radio disruptions across large areas over the Pacific Ocean and in polar regions, affecting radio communications and related systems. An additional M9.5 flare followed immediately after the X-flare, but its position on the Sun minimized its impact on Earth, reducing the risk of severe space weather effects.
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βοΈ Solar Activity β 07.11.2024
π On Thursday, a large filament eruption was observed on the southwestern limb of the Sun, resulting in a beautiful partial halo CME (coronal mass ejection). This phenomenon involves the ejection of solar material beyond the Sun's atmosphere, which can potentially affect Earth's magnetic field.
π Astronomers and scientists continue to monitor the activity, anticipating possible geophysical impacts, such as geomagnetic storms, which may affect satellites and communication systems.
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βοΈ |βοΈ A strong solar storm hit Earth.
π Another solar flare has intensified the geomagnetic storm. According to meteorological data, it reaches a level of six and is one of the longest-lasting storms of the year.
π During this period, many people may experience headaches, weakness, fluctuations in blood pressure, and mood swings.
November 10, 2024
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November 10, 2024
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βοΈ |βΌοΈ Solar Eruptions, November 11β12
π Over the past 24 hours, a series of powerful eruptions have been observed on the Sun. In the southern hemisphere, a large solar filament lifted off, followed by a prominence eruption on the northeastern limb. Additionally, two more filament eruptions were recorded in the northwestern and northeastern quadrants.
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βοΈ Powerful Solar Eruption on the Sun's Western LimbβΌοΈ
π 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.
π‘ The likely source of this event is one of the Sun's active regionsβeither Region 3889 or Region 3897βlocated 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.
π 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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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.
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βοΈ November 27, 2024: The Sun Demonstrates Significant Activity
π 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.
π 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 Earthβs magnetosphere.
π 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.
βΌοΈ 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.
π Source: link
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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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βοΈ Intense Solar Activity: A Magnetic Storm Expected on New Year's EveβΌοΈ
π 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.
β‘οΈ 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.
π 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.
π 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.
π Source: meteoagent.com
π Source: Space Weather Live
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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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π Solar Filament Eruption on February 26, 2025
βοΈ On February 26, 2025, the Sun experienced a filament eruption that led to a coronal mass ejection (CME). This event was accompanied by dimming and the formation of a post-eruption arcade, with one of the CMEs directed towards Earth.
βΌοΈ Experts estimate that the CME is heading southeast and is expected to reach Earth around March 2, 2025.
π Such events can cause geomagnetic storms, potentially affecting satellite communications and triggering auroras in high-latitude regions.
Astronomers continue to monitor the situation to assess potential impacts on our planet.
π Source: Edward.Vijayakumar - X
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Astronomers continue to monitor the situation to assess potential impacts on our planet.
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βοΈ POWERFUL ERUPTION ON THE FAR SIDE OF THE SUN β CORONAL MASS EJECTION
π₯ On March 1 at 16:45 UTC, a powerful eruption was observed on the far side of the Sun, accompanied by a bright coronal mass ejection (CME). This event was preceded by a smaller eruption linked to a filament near the Sunβs western limb.
π Although this CME is not directed toward Earth, such events highlight the Sunβs high activity. Solar eruptions and coronal mass ejections can influence space weather, causing geomagnetic disturbances that may affect satellite systems and radio communications.
β οΈ Astronomers continue to closely monitor solar activity to assess potential impacts from future eruptions.
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βοΈ Solar Activity on March 7 and Forecast for March 8β10
π On March 7, several significant coronal mass ejections (CMEs) were observed on the Sun. One particularly impressive eruption occurred in the evening, along with an M1.6 flare from Active Region AR14016, where plasma movement was detected, potentially leading to a CME.
π Additionally, an impressive filament eruption was recorded in the southeastern quadrant of the Sun. However, preliminary data suggests that it does not have an Earth-directed component.
π Space Weather Forecast for March 8β10
π March 8β9: Increased geomagnetic activity is expected as a high-speed solar wind stream (HSS) from a coronal hole reaches Earth. Active conditions and G1 (minor) geomagnetic storms are likely, with a small chance of isolated G2 (moderate) storms.
π March 10: Unstable and active conditions will persist, with the continued influence of high-speed solar wind, bringing another chance of a G1 storm.
β‘οΈ Additionally, a large coronal hole facing Earth is already impacting the planetβs magnetic field, which could lead to further disturbances. π
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π Space Weather Forecast for March 8β10
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βοΈ Solar Eruption Heading Toward Earth: Geomagnetic Disturbances Expected βοΈ π
π On March 21, 2025, significant dimmings were observed near the center of the solar disk following an M1.2 solar flare in Active Region AR 14028, located in the southwestern (lower right) quadrant of the Sun. This phenomenon may be an example of a sympathetic eruption triggered by unseen wave-like disturbances.
βΌοΈ According to preliminary forecasts, the coronal mass ejection (CME) is expected to reach Earth late on March 23 or on March 24.
π΄ Possible effects:
β‘οΈ Bright auroras visible even in mid-latitude regions.
β‘οΈ βͺοΈ Disruptions in satellite and GPS systems.
β‘οΈ Radio communication and power grid disturbances.
π Attention, weather-sensitive individuals!
The anticipated geomagnetic storms may cause headaches, blood pressure fluctuations, fatigue, and insomnia. It is recommended to avoid stress, monitor your well-being, stay hydrated, and have necessary medications on hand.
β οΈ Residents of high-latitude regions should prepare for potential communication disruptions, while satellite system operators should take precautionary measures to minimize operational issues.
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The anticipated geomagnetic storms may cause headaches, blood pressure fluctuations, fatigue, and insomnia. It is recommended to avoid stress, monitor your well-being, stay hydrated, and have necessary medications on hand.
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βοΈ Powerful Solar Storm Approaching Earth
π A powerful solar storm is heading toward Earth, triggered by multiple coronal mass ejections from the Sun earlier this week. These bursts of solar energy prompted NOAAβs Space Weather Prediction Center (SWPC) to issue a geomagnetic storm warning.
π The peak of geomagnetic disturbances is expected between April 23 and 24, with G2-level geomagnetic activity likely. The strongest geophysical effects may persist until 9:00 PM on April 24, after which Earthβs magnetic field is expected to stabilize between April 25 and 29.
π‘ In addition to auroras, intense solar storms can impact radio communications and GPS systems.
π According to NASA and NOAA experts, this active phase of the current solar cycle is expected to continue at least through the end of the year, although the exact peak remains uncertain. βThe intensity of the auroras depends on how Earthβs magnetic field interacts with the solar particles,β explained SWPC meteorologist Shawn Dahl.
π Source: alertageo
π According to NASA and NOAA experts, this active phase of the current solar cycle is expected to continue at least through the end of the year, although the exact peak remains uncertain. βThe intensity of the auroras depends on how Earthβs magnetic field interacts with the solar particles,β explained SWPC meteorologist Shawn Dahl.
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βοΈ Solar Event: Coronal Mass Ejection Not Directed Toward Earth
(May 19, 2025)
π Around 21:00 UT, a beautiful filament eruption was observed in the northeastern region of the Sun. This resulted in a coronal mass ejection (CME) that is primarily directed north of Earth.
π‘ According to experts, the eruption produced a decent-sized partial halo CME, but its trajectory indicates no impact on our planet.
π This event highlights ongoing solar activity but poses no threat to Earth.
(May 19, 2025)
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