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π The Earth was hit by heavy particles from the Sun, protons of very high energies.
--June 9, 2024--
βΌοΈ If this energy were converted into temperatures, it would correspond to about 1 billion degrees. Currently, the particle fluxes of these energies are approximately 10,000 times higher than normal levels and will remain elevated for at least 2-3 more days.
βοΈ The impact was caused by a double solar flare close to class X, originating from the same active region that has been troubling Earth for the past two months.
Since the flare was on the edge of the Sun, direct hits in this situation are almost excluded, and the Earth will receive peripheral, but still quite dense, regions. The expected strength of the kinetic impact on Earth approximately corresponds to G2-level storms.
π Please note that in the video, the proton solar storm begins immediately after the coronal mass ejection (CME) becomes visible on the western limb of the Sun. This indicates that particles are moving at nearly the speed of light, suggesting their acceleration to relativistic speeds due to the flare. (At relativistic speeds, objects or particles acquire special properties such as increased mass, shortened length, and altered time, making their behavior distinct from classical mechanics.)
π‘ Depending on the power of X-ray radiation, solar flares are classified into five classes - A, B, C, M, and X. The minimum class A0.0 signifies radiation power at Earth's orbit of 10 nanowatts per square meter. With each increment to the next class, the power increases tenfold.
π The designation M1 denotes minor flares, M5 denotes moderate ones, X1 denotes strong flares, and X20 denotes extreme ones.
π‘ Flares are usually accompanied by ejections of solar plasma, the clouds of which, upon reaching Earth, trigger magnetic storms.
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--June 9, 2024--
Since the flare was on the edge of the Sun, direct hits in this situation are almost excluded, and the Earth will receive peripheral, but still quite dense, regions. The expected strength of the kinetic impact on Earth approximately corresponds to G2-level storms.
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π SOLAR WEATHER, June 24-25, 2024
βΌοΈ Astronomical Observations: Two Solar Filament Eruptions
βοΈ Recent astronomical observations have recorded two solar filament eruptions. The first eruption occurred in the northwest quadrant of the Sun but did not produce a coronal mass ejection (CME). This was followed by the eruption of a larger filament located in the southwest quadrant.
π As a result of the latter eruption, an M1.1 post-flare loop was observed, continuing to grow behind the southwest limb of the Sun.
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βοΈ Next Friday, July 5, Earth will reach its farthest point from the Sun, known in astronomy as the solar aphelion.
This phenomenon occurs once a year and marks the moment when our planet is at the greatest distance from our star.
π The aphelion occurs due to the elliptical shape of Earth's orbit around the Sun. Earth's orbit is not a perfect circle but an ellipse, which means there are times when Earth is closer to the Sun (perihelion) and times when it is farther away (aphelion).
During the aphelion, Earth will be approximately 152,095,581 kilometers (94,506,364 miles) from the Sun.
π The perihelion, which is the opposite (when Earth is closest to the Sun), occurred earlier this year, on January 3, 2024. At that time, Earth was approximately 147,098,925 kilometers (91,403,034 miles) from the Sun.
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This phenomenon occurs once a year and marks the moment when our planet is at the greatest distance from our star.
During the aphelion, Earth will be approximately 152,095,581 kilometers (94,506,364 miles) from the Sun.
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βοΈ Powerful X1.27 Solar Flare Observed on the Sun's Surface
π Early this morning, on July 14, 2024, a powerful X1.27 solar flare occurred on the Sun in sunspot region AR3738 at 2:23 UTC. This event briefly ionized the upper layers of the atmosphere and caused significant radio blackout at R3 level in the western Pacific Ocean region.
βοΈ Scientists are currently studying the direction of the associated coronal mass ejection (CME).
π If the CME is directed towards Earth, a G-3 geomagnetic storm is expected on Tuesday, with the possibility of observing polar auroras at unusually southern latitudes by Tuesday evening.
π‘ Solar flares are classified based on the intensity of their X-ray emissions: the most powerful belong to class X, emitting β₯10-1 erg/(cmΒ²s) in the 1-8 Γ
range. Class M flares are 10 times weaker, and class C flares are 100 times weaker compared to class X flares.
π Stay tuned for further updates on space weather.
π£ Source: link (https://www.spaceweatherlive.com/en/solar-activity/solar-flares.html)
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βοΈ βΌοΈ Radio blackouts could occur on Earth due to a dark plasma eruption on the Sun, reports the Daily Mail .
β οΈ The probability of this happening is 60%, according to NASA.
The eruption could disrupt aviation communications and satellite operations as early as this week.
π₯ In the NASA video, a dark cloud of the flare can be seen erupting from the Sun, resembling black smoke.
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The eruption could disrupt aviation communications and satellite operations as early as this week.
π₯ In the NASA video, a dark cloud of the flare can be seen erupting from the Sun, resembling black smoke.
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π SOLAR WEATHER, July 28, 2024 βοΈ Solar Flare and Its Consequences
π On July 28, a powerful M9.9-class solar flare occurred near the central disk of the Sun, accompanied by a coronal wave and dimming. This flare caused a coronal mass ejection (CME) directed towards Earth. The CME is expected to reach our planet on July 31.
π‘ When such ejections reach Earth, they can cause disturbances in our planet's magnetic field, leading to geomagnetic storms. This can affect satellites, communications, and even cause the appearance of auroras. We recommend being prepared for possible communication disruptions and keeping an eye on space weather updates.
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π¬π§ | π‘ Amazing Night: Northern Lights Over Sutherland, Scotland, UK
βΌοΈ Last night, residents and visitors of Sutherland, Scotland, were treated to a truly unforgettable spectacle β the Northern Lights. The vibrant colors of the night sky, including unusual purplish-pink hues for auroras, were captured in stunning photographs taken by Monika Focht.
The aurora, caused by a solar storm, painted the sky in bright colors, attracting the attention of many people, including astronomy enthusiasts and photographers. 28.08.2024
πΈ Monika Focht
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The aurora, caused by a solar storm, painted the sky in bright colors, attracting the attention of many people, including astronomy enthusiasts and photographers. 28.08.2024
πΈ Monika Focht
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βοΈ Solar Flare and Comet in One Observation! π
βοΈ Today, October 8, 2024, a spectacular eruption of solar material was observed on the Sun, directed southward. This event was captured by the coronagraph aboard the Solar and Heliospheric Observatory (SOHO).
π« At the same time, Comet C/2023 A3 appeared in the coronagraph's field of view, moving further into the observable area and potentially becoming one of the brightest comets ever recorded by SOHO.
Letβs keep an eye on these exciting phenomena in space!π
π£ Source: link (https://www.spaceweatherlive.com/en/solar-activity/solar-flares.html)
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Letβs keep an eye on these exciting phenomena in space!
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βοΈ Solar Weather, October 9, 2024
π X-Class Flare with Earth-Directed Plasma Ejection
βΌοΈ Today, reports emerged of a new X-class solar flare. The radiation began to increase at 01:25 UT, reaching its peak at 01:58. There are several key points to consider. First, a significant plasma ejection was recorded, and even if models suggest otherwise, its configuration rules out the possibility of missing Earth. Second, the flareβs location is noteworthy. The explosion occurred in a large sunspot in the northern part of the Sun, which has been notable for its size over the past 10 days but only just became active.
β οΈ Important Warning: This event could lead to communication disruptions, and the appearance of auroras at lower latitudes is expected. People sensitive to geomagnetic activity should take precautions, as heightened magnetic disturbances may follow.
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βοΈ |π Update on Comet Tsuchinshan-Atlas
π Recently, updated information about the movement of Comet Tsuchinshan-Atlas has appeared on social media. Its passage seems to coincide with a powerful coronal mass ejection (CME) in the plane of the sky; however, in three-dimensional space, it may look different. Scientists continue to closely monitor these phenomena.
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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 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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