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The Sun, during its solar maximum phase in 2024, emitted over 50 X-class solar flares—the most powerful category of solar flares. These intense bursts of energy, capable of disrupting satellites and communications on Earth, marked a highly active year for solar phenomena. According to reports, these flares varied in magnitude and impact, with the strongest measured at X9.0 on October 3. Below is a countdown of the ten most notable solar flares recorded this year.

February 9 – X3.38

A solar flare rated X3.38 was observed near the southwestern edge of the Sun. According to researchers, the full intensity might have been obscured due to its position. The flare showcased a “coronal wave,” with solar material visibly displaced across the Sun’s surface.

February 22 – X6.37

This flare, while registering an impressive X6.37, lacked Earth-directed coronal mass ejections (CMEs) and had limited effects beyond its intense X-ray emissions. Data from NASA highlighted its scientific importance despite its minimal impact.

May 6 – X4.52

An eruption from Active Region AR 13663 in the northern hemisphere occurred early in May. This flare, documented by NASA’s Solar Dynamics Observatory, did not produce Earth-directed CMEs, though it highlighted the active state of the Sun during this period.

May 10 – X3.98

From Active Region AR 13664, this solar flare produced a strong Earth-directed CME. Reports indicated it was part of a series of events that caused a G5 geomagnetic storm, leading to widespread auroras visible at unusually low latitudes.

May 11 – X5.89

Another eruption from AR 13664 occurred just a day later. This flare, part of a chain of CMEs, contributed to the extreme geomagnetic activity documented during this period. Its position on the solar limb reduced its direct impact on Earth.

May 14 – X8.79

A confined flare from AR 13664 produced strong X-ray emissions without a major eruption. Despite its physical size, its intensity ranked among the highest of the year, as confirmed by ESA and NASA observations.

May 15 – X3.48

The final X-class flare from AR 13664 during its rotation was recorded on May 15. Observations revealed that its intensity was partly obscured as the active region moved out of Earth’s view. ESA reports noted continued activity from this region even when it was no longer visible from Earth.

September 14 – X4.54

A strong CME directed over the Sun’s eastern limb accompanied this flare. Observers noted pixel saturation in images, a common occurrence in high-energy flares of this magnitude.

October 1 – X7.10

This flare originated from Active Region AR 13842. Despite its size, it did not produce significant geomagnetic storms. Experts observed that smaller flares from this active region later contributed to strong auroras seen worldwide.

October 3 – X9.0

The largest solar flare of 2024, and one of the strongest in recent years, was recorded at X9.0. As per data from the Solar and Heliospheric Observatory, it unleashed energy nine times the X-class threshold, cementing its place as a standout event of Solar Cycle 25.

The Sun’s activity continues to be closely monitored as solar maximum extends into 2025.

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Underwater Neutrino Telescopes in the Mediterranean for Cosmic Research

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Underwater Neutrino Telescopes in the Mediterranean for Cosmic Research

Efforts are underway in the Mediterranean Sea to install the underwater neutrino telescope known as KM3NeT, as reported by various sources. The telescopes are designed to detect high-energy neutrinos, subatomic particles emitted from unidentified cosmic sources. Unlike traditional telescopes, these devices rely on capturing light generated when neutrinos collide with seawater. This massive project spans a cubic kilometre of the Mediterranean and involves deploying hundreds of detector strands. The work aims to unveil new insights about the universe.

Unique Design and Deployment Challenges

According to experts, KM3NeT comprises two distinct telescopes featuring glass spheres, each packed with photomultiplier tubes. Simone Biagi, a physicist at Italy’s National Institute for Nuclear Physics, shared with Science News that the telescopes are situated several kilometres below the surface. Deployment involves suspending cables of sensors, resembling strands of pearls, each up to 700 metres in length. These are lowered to the seabed and gradually released to unfurl in the water. A remotely operated submersible is used to make precise connections and inspect the setup.

Scientific Goals of the Project

Sources indicate that one telescope, positioned off Sicily’s coast, is designed to observe high-energy neutrinos originating from space. The second, off the coast of France, is dedicated to studying atmospheric neutrinos and their oscillations. These oscillations provide vital data about how neutrinos shift between different forms, contributing to advancements in particle physics.

Operational Challenges at Sea

Physicists working on this project face significant challenges, including harsh sea conditions and tight schedules. According to reports, deployment campaigns occur annually, each lasting about a month. During this period, researchers work under immense pressure to ensure all equipment functions perfectly. Any errors must be corrected immediately, as adjustments after deployment are impossible.

Experts suggest that the partially completed KM3NeT telescopes are already yielding valuable scientific data, providing insights into quantum gravity effects and neutrino behaviours.

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Virginia Mathematicians Use Algebraic Geometry to Reduce Data Centre Energy Use

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Virginia Mathematicians Use Algebraic Geometry to Reduce Data Centre Energy Use

Efforts to improve data centre efficiency have led mathematicians at Virginia Tech to develop a novel method of data storage and retrieval. According to reports, the researchers have utilised algebraic geometry to tackle issues arising from high energy consumption in data centres, which is impacting global climate goals. This breakthrough was detailed in IEEE BITS, where the team presented a fresh approach to managing the growing volume of data generated by individuals and corporations.

Innovative Use of Algebraic Structures

As per a report by Phys.org, tt was explained by Gretchen Matthews, professor of mathematics at Virginia Tech and director of the Southwest Virginia node of the Commonwealth Cyber Initiative, that conventional methods of data replication often result in duplicating vast quantities of information. As reported, Matthews noted that smarter alternatives could significantly reduce such redundancy. Hiram Lopez, assistant professor of mathematics, added that the new method employs algebraic structures to fragment data and distribute it across servers positioned in close proximity. This ensures that, in the event of server failure, the missing data can be recovered through neighbouring servers without extensive energy use.

Mathematics Behind the Solution

The use of special polynomials for data storage was highlighted as a significant advancement. Although polynomials have been linked to data storage since the 1960s, recent developments have made them more practical for applications like localised data recovery. Matthews pointed out in IEEE BITS that these structures offer an efficient and reliable way to manage data, addressing issues related to storage and retrieval energy demands.

Addressing Rising Power Consumption

The method arrives at a critical time, as energy demand across the United States continues to rise, driven by the increasing number of data centres. Matthews emphasised in the publication that sustainable improvements in existing systems could play a vital role in managing energy consumption.

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Leaves’ Resilience to Raindrops Might Help in Agriculture

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Leaves' Resilience to Raindrops Might Help in Agriculture

Research published in Physical Review Fluids has revealed the intricate dynamics between raindrops and leaves, shedding light on how plants withstand the force of falling water. The study, titled “Resonance and Damping in Drop-Cantilever Interactions,” highlights the mechanics that protect leaves and suggests innovative applications for agriculture and renewable energy. Using high-speed imaging, researchers observed the interaction between water droplets and a plastic beam, which simulated the structural behavior of leaves.

According to Professor Sunghwan Jung, from Cornell University’s Department of Biological and Environmental Engineering, in a statement, the droplet and beam move in opposing directions upon impact. This counteraction reduces vibration, offering protection to the plant. The findings align with unexplained discrepancies previously noted by scientists, which the team analysed by examining the natural frequency alignment of the beam and droplet.

Insights into Plant Adaptation

Lead author Crystal Fowler, a doctoral candidate in biological engineering, stated that the study confirmed increased damping when the droplet’s natural frequency matched the beam’s. This phenomenon resulted in a faster reduction of vibrations, potentially reducing stress on plant leaves and contributing to their longevity. The findings may also enhance understanding of water flow through forest canopies and plant morphological evolution.

Potential for Renewable Energy Applications

The research team proposed that the principles observed could extend to renewable energy. Professor Jung suggested piezoelectric materials could replace the beam to harness energy from rain-induced vibrations.

This paper marks a significant milestone for Fowler, a member of the Navajo Nation. Reflecting on her experience, she expressed enthusiasm for exploring biological engineering and its broader implications. The study not only provides a glimpse into plant resilience but also opens avenues for innovative technology inspired by natural processes.

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