Unpredictable Forces: Solar Storms, Sun Cycles, and Cosmic Chaos

The Point by Modern Sciences - July 31, 2024

By The Modern Sciences Team

July 31, 2024

Dear Cultivators of Curiosity,


Welcome to the 9th edition of The Point by Modern Sciences! This volume casts light on the powerful forces shaping our planet and beyond—from the impact of solar storms on Earth's infrastructure to the dramatic possibilities of celestial mechanics as portrayed in popular science fiction.


In this issue, we explore how a recent geomagnetic storm disrupted modern farming technologies, what the peak of the Sun’s activity cycle means for our planet, and the intriguing chaos of the three-body problem in both theoretical physics and narrative fiction. These articles not only offer a glimpse into the dynamic interactions between technology and natural phenomena but also challenge us to think critically about the delicate balance of our increasingly interconnected world.


TECH

Solar storm knocks out farmers’ high-tech tractors – an electrical engineer explains how a larger storm could take down the power grid and the internet

Geomagnetic storms, like the May 2024 event, result from coronal mass ejections from the Sun. These ejections disrupt Earth's magnetic field and cause phenomena such as the aurora borealis, which is visible even in Mexico. Read more.



Notable points:

  • Impact of geomagnetic storms: The geomagnetic storm that began on May 10, 2024, caused spectacular auroras visible as far south as Mexico but also disrupted GPS-guided farming equipment. Coronal mass ejections from the Sun, composed of superheated plasma, cause such storms by distorting Earth's magnetic field upon impact.

  • Historical context and potential damage: Stronger geomagnetic storms have occurred in the past, such as the Carrington Event of 1859, which disrupted telegraph systems globally. Modern technology, which relies heavily on electrical and communication systems, is even more vulnerable. A storm of similar magnitude today could lead to catastrophic damage, affecting power grids, internet infrastructure, and satellite operations.

  • Need for protective measures: Given the inevitability of future geomagnetic storms, it is crucial to develop protective strategies. This includes installing shielding devices for electrical components, creating protocols for adjusting grid loads during solar storms, and enhancing space weather prediction capabilities to minimize potential disruptions and economic losses.



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SPACE

The Sun is reaching the peak of its activity – here’s how that could cause more auroras and solar storms

The Sun is at the peak of an 11-year activity cycle, leading to more particle outbursts that cause auroras and geomagnetic storms, which can damage infrastructure. These storms can induce electrical currents in power lines, pipelines, and satellites, potentially damaging infrastructure and disrupting communication. Read more.



Critical notes:

  • Widespread visibility of auroras: A fairly recent solar storm allowed more people worldwide to see the northern and southern lights. This event occurred as the Sun reached the peak of its 11-year activity cycle, causing high-energy particles to interact with Earth's magnetic field, generating auroras and geomagnetic storms.

  • Impact on infrastructure: The solar storm's effects on Earth's magnetic field can induce electrical currents in power lines, pipelines, and satellites, posing risks such as power outages and satellite failures. The May 10-11 geomagnetic storm was particularly strong, highlighting the potential for significant damage to modern infrastructure.

  • Scientific insights and simulations: Auroras reveal important information about planetary magnetic fields. Scientists use devices like the "planeterella" to simulate auroras in controlled environments, studying how they change with varying magnetic field strengths. These observations help improve our understanding of and protection against geomagnetic storms.



MATH AND THE SCIENCES

The planetary orbit in Netflix’s ‘3 Body Problem’ is random and chaotic, but could it exist?

The three-body problem, a fundamental challenge in theoretical physics, lacks a general solution, making long-term predictions for such systems unpredictable. However, computational analysis has been instrumental in understanding complex models of the universe’s evolution. Read more.



Essential observations:

  • Exploration of the three-body problem in fiction: Both Frederic Brown's short story "Placet is a Crazy Place" and Liu Cixin's science fiction trilogy "Remembrance of Earth's Past," the first book of which Netflix has adapted into a series, centrally explore the three-body problem, which describes the unpredictable motion of three celestial bodies in orbit around each other. These works imagine complex and often chaotic orbits that highlight the challenges of predicting celestial movements.

  • Three-body systems' chaotic nature: Unlike the two-body problem, which Isaac Newton famously solved, the three-body problem lacks a general solution. This implies that while we can predict the motion of two bodies, such as the Earth and the Moon, with high precision, the addition of a third body renders the system chaotic, leading to unpredictable long-term behavior. Special cases and computational models, such as those used in cosmology, help study these complex interactions, but they can only predict short-term behaviors with certainty.

  • Fiction vs. reality in astrophysics: In "3 Body Problem," the fictional planet Trisolaris suffers from unpredictable climate changes due to the chaotic orbits of its three suns. This concept, while thrilling in fiction, simplifies the complex nature of such systems. Real three-body systems, such as the actual Alpha Centauri star system, are difficult to predict, but they follow chaotic rather than stochastic patterns. The series and novel highlight the fascination and difficulty of understanding chaotic systems, emphasizing the distinction between the compelling narratives of science fiction and the intricate realities of astrophysics.