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In search for red aurorae in ancient Japan

Ryuho Kataoka, a Japanese auroral scientist, played a seminal role in searching for evidence of super-geomagnetic storms in the past using historical methods

Karthik Vinod

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Professor Ryuho Kataoka in his office at NIPR, with the fan-shaped painting behind him, Picture courtesy: RK Works

Auroras seen on Earth are the end of a complex process that begins with a violent, dynamic process deep within the sun’s interior.

However, studying the depths of the sun is no easy task, even for scientists. The best they can do is to observe the surface using space-based telescopes. One problem that scientists are attempting to solve is how a super-geomagnetic storm on Earth comes to being. These geomagnetic storms find their roots in sunspots, that are acne-like depressions on the sun’s surface. As the sun approaches the peak of its 11-year solar cycle, these sunspots, numbering in the hundreds, occasionally release all that stored magnetic energy into deep space, in the form of coronal mass ejections (CMEs) (which are hot wisps of gas superheated to thousands of degrees).

If the earth lies in the path of an oncoming CME, the energy release from their resultant magnetic field alignment can cause intense geomagnetic storms and aurorae on Earth.

This phenomenon, which is astrophysical and also electromagnetic in nature, can have serious repercussions for our modern technological society.

Super-geomagnetic storms, a particularly worse form of geomagnetic storm, can induce power surges in our infrastructure, causing power outages that can plunge the world into darkness, and can cause irreversible damages to our infrastructure. The last recorded super-geomagnetic storm event occurred more than 150 years ago. Known as the Carrington event, the storm destroyed telegraph lines across North America and Europe in 1859. The risk for a Carrington-class event to happen again was estimated to be 1 in 500-years, which is quite low, but based on limited data. Ramifications are extremely dangerous if it were to ever happen.

However, in the past decade, it was learnt that such super-geomagnetic storms are much more common than scientists had figured. To top it all, it wasn’t just science, but it was a valuable contribution by art – specifically ancient Japanese and Chinese historical records that shaped our modern understanding of super-geomagnetic storms.

Ryuho Kataoka, a Japanese space physicist, played a seminal role in searching for evidence of super-geomagnetic storms in the past using historical methods. He is presently an associate professor in physics, holding positions at Japan’s National Institute of Polar Research, and The Graduate University for Advanced Studies.

“There is no modern digital dataset to identify extreme space weather events, particularly super-geomagnetic storms,” said Professor Kataoka. “If you have good enough data, we can input them into supercomputers to do physics-based simulation.”

However, sunspot records go until the late 18th century when sunspots were actively being cataloged. In an effort to fill the data gap, Professor Kataoka decided to be at the helm of a very new but promising interdisciplinary field combining the arts with space physics. “The data is limited by at least 50 years,” said Professor Kataoka. “So we decided to search for these red vapor events in Japanese history, and see the occurrence patterns … and if we are lucky enough, we can see detailed features in these lights, pictures or drawings.” Until the summer of 2015, Ryuho Kataoka wasn’t aware of how vast ancient Japanese and Chinese history records really were.

In the past 7 years, he’s researched a very specific red aurora, in documents extending to more than 1400 years. “Usually, auroras are known for their green colors – but during the geomagnetic storm, the situation is very different,” he said. “Red is of course unusual, but we can only see red during a powerful geomagnetic storm, especially in lower latitudes. From a scientific perspective, it’s a very reasonable way to search for red signs in historical documents.”

A vast part of these historical red aurora studies that Professor Kataoka researched came from literature explored in the last decade by the AURORA-4D collaboration. “The project title included “4D”, because we wanted to access records dating back 400 years back during the Edo period,” said Professor Kataoka.

“From the paintings, we can identify the latitude of the aurora, and calculate the magnitude or amplitude of the geomagnetic storm.” Clearly, paintings in the Edo period influenced Professor Kataoka’s line of research, for a copy of the fan-shaped red aurora painting from the manuscript Seikai (which translates to ‘stars’) hangs on the window behind his office desk at the National Institute of Polar Research.

The painting fascinated Professor Kataoka, since it depicted an aurora that originated during a super-geomagnetic storm over Kyoto in 1770. However, the painting did surprise him at first, since he wondered whether the radial patterns in the painting were real, or a mere artistic touch to make it look fierier. “That painting was special because this was the most detailed painting preserved in Japan,” remarked Professor Kataoka. “I took two years to study this, thinking this appearance was silly as an aurorae scientist. But when I calculated the field pattern from Kyoto towards the North, it was actually correct!”

Fan-shaped red aurora painting from the ‘Seikai’, dated 17th September, 1770; Picture Courtesy: Matsusaka City, Mie Prefecture.

The possibility to examine and verify historical accounts using science is also a useful incentive for scholars of Japanese literature and scientists partaking in the research.

“This is important because, if we scientists look at the real National Treasure with our eyes, we really know these sightings recorded were real,” said Professor Kataoka. “The internet is really bad for a survey because it can easily be very fake,” he said laughing. It’s not just the nature in which science was used to examine art – to examine Japanese “national treasures” that is undoubtedly appealing, but historical accounts themselves have contributed to scientific research directly.

“From our studies, we can say that the Carrington class events are more frequent than we previously expected,” said Professor Kataoka. There was a sense of pride in him as he said this. “This Carrington event is not a 1 in 200-year event, but as frequent as 1 in 100 years.” Given how electricity is the lifeblood of the 21st century, these heightened odds do ingrain a rather dystopian society in the future, that is ravaged by a super-geomagnetic storm.

Professor Kataoka’s work has found attention within the space physics community. Jonathon Eastwood, Professor of Physics at Imperial College London said to EdPublica, “The idea to use historical information and art like this is very inventive because these events are so rare and so don’t exist as information in the standard scientific record.”

There’s no physical harm from a geomagnetic storm, but the threat to global power supply and electronics is being increasingly recognized by world governments. The UK, for instance, identified “space weather” as a natural hazard in its 2011 National Risk Register. In the years that followed, the government set up a space weather division in the Met Office, the UK’s foremost weather forecasting authority, to monitor and track occurrences of these coronal mass ejections. However, these forecasts, which often supplement American predictions – namely the National Oceanic and Atmospheric Administration (NOAA) – have failed to specify previously where a magnetic storm could brew on Earth, or predict whether a coronal mass ejection would ever actually strike the Earth.

The former occurred during the evacuation process for Hurricane Irma in 2017, when amateur radio ham operators experienced the effects of a radio blackout when a magnetic storm affected the communications network across the Caribbean. The latter occurred on another occasion when a rocket launch for SpaceX’s Starlink communication satellites was disrupted by a mild geomagnetic storm, costing SpaceX a loss of over $40 million.

Professor Kataoka said he wishes space physicists from other countries participate in similar interdisciplinary collaborations to explore their native culture’s historical records for red aurora sightings. He said the greatest limitation of the AURORA-4D collaboration was the lack of historical records from other parts of the world. China apparently boasts a history of aurora records longer than Japan, with a history lasting before Christ himself. “Being Japanese, I’m not familiar with British, Finnish or Vietnamese cultures,” said Professor Kataoka. “But every country has literature researchers and scientists who can easily collaborate and perform interdisciplinary research.” And by doing so, it’s not just science which benefits from it, but so is ancient art whose beauty and relevance gains longevity.

Karthik is a science writer, and co-founder of Ed Publica. He writes and edits the science page. He's also a freelance journalist, with words in The Hindu, a prominent national newspaper in India.

Space & Physics

MIT Physicists uncover key Mechanism behind fractional charge in Graphene

In the decades-long history of studying these phenomena, no one has observed a system that naturally leads to such fractional electron effects, according to the researchers.

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Credit: iStock

MIT physicists have made a significant breakthrough in understanding the phenomenon where electrons split into fractions of their usual charge, offering new insights into the behaviour of exotic electronic states in graphene and other two-dimensional materials.

This latest research builds on a discovery earlier this year, when a team led by Assistant Professor Long Ju at MIT reported that electrons in pentalayer graphene—a structure composed of five graphene layers stacked on top of boron nitride—exhibited fractional charge. Remarkably, this behaviour was observed without the application of a magnetic field, challenging prior assumptions.

Previously, scientists knew that under a strong magnetic field, electrons could split into fractions as part of the fractional quantum Hall effect. However, Ju’s findings marked the first time such fractional behaviour occurred in graphene without any magnetic influence, which led to the coining of the “fractional quantum anomalous Hall effect.” Since then, researchers have been eager to uncover how fractional charge could emerge in this unusual system.

MIT professor Senthil Todadri, who led the new study published in Physical Review Letters, offers a critical piece of the puzzle. Through detailed quantum mechanical calculations, Todadri and his team discovered that the electrons in pentalayer graphene form a crystal-like structure, which provides the ideal conditions for fractional electron behavior.

“This is a completely new mechanism,” said Todadri. “In the decades-long history of studying these phenomena, no one has observed a system that naturally leads to such fractional electron effects. It opens the door to all kinds of new experimental possibilities.”

The study, which includes contributions from Zhihuan Dong and former postdoc Adarsh Patri, is part of a wider body of research. Two other teams—one from Johns Hopkins University and another from Harvard University, UC Berkeley, and Lawrence Berkeley National Laboratory—have also reported similar findings in the same journal issue.

Building on “Twistronics” and the Magic-Angle Graphene Discovery

This research builds upon the work of MIT physicist Pablo Jarillo-Herrero and his team, who in 2018 were the first to demonstrate that twisting two sheets of graphene could give rise to novel electronic behaviors. This discovery of “magic-angle graphene” spurred a new field known as “twistronics,” focused on understanding how the interactions between twisted two-dimensional materials could lead to unusual quantum phenomena, such as superconductivity and insulating behavior.

“We quickly realized that these twisted systems could provide the right conditions for fractional electron phenomena to emerge,” said Todadri, who collaborated with Jarillo-Herrero on a 2018 study that theorized such systems might exhibit fractional charge without a magnetic field. “We saw these systems as ideal platforms to study these fractional effects.”

A Surprising Discovery and the New Crystal Model

In September 2023, Todadri received an unexpected call from Ju, who was eager to share data showing fractional charge behavior in pentalayer graphene. This discovery caught Todadri by surprise, as it did not align with his earlier predictions. In his 2018 paper, Todadri had theorized that fractional charge would emerge from a specific twisting of the electron wavefunction, and that this twisting would intensify as more graphene layers were added.

“Initially, we expected the wavefunction to wind five times in pentalayer graphene,” Todadri explained. “But Ju’s experiments showed that it only wound once. This raised a big question—how do we explain what we’re seeing?”

Uncovering the Electron “Crystal”

Todadri and his team revisited their hypothesis and discovered they had overlooked an important factor. The conventional approach in the field had been to treat electrons as independent entities and analyze their quantum properties. However, in the confined, two-dimensional space of pentalayer graphene, electrons are forced to interact with each other, behaving according to their quantum correlations in addition to their natural repulsion.

By incorporating these interelectron interactions into their model, the team was able to match their predictions with the experimental data Ju had obtained. This led them to a crucial realization: the moiré pattern formed by the stacked graphene layers induces a weak electrical potential that forces the electrons to interact and form a crystal-like structure. This electron “crystal” creates a complex pattern of quantum correlations, allowing for the formation of fractional charge.

“The crystal has a whole set of unique properties that differentiate it from ordinary crystals,” said Todadri. “This opens up many exciting avenues for future research. In the short term, our work provides a theoretical foundation for understanding the fractional electron observations in pentalayer graphene and predicting similar phenomena in other systems.”

This new insight paves the way for further exploration into how graphene and other two-dimensional materials might be used to engineer new electronic states, with potential applications in quantum computing and other advanced technologies.

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How Shyam Gollakota is revolutionizing mobile systems and healthcare with technology

His research is already opening up new possibilities for battery-free networks, including underwater Wi-Fi, powerline communication, and even wireless cameras

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Shyam Gollakota. Image credit: By special arrangements

Prof. Shyam Gollakota, Washington Research Foundation and Thomas J. Cable Endowed Professor at the Paul G. Allen School of Computer Science and Engineering at the University of Washington, has been honored with the Infosys Prize 2024 in Engineering and Computer Science for his groundbreaking contributions to mobile systems and healthcare. His research, which spans multiple engineering domains, has had a profound societal impact, particularly in areas like smartphone-based healthcare tools, battery-free communication, and the augmentation of human auditory perception with artificial intelligence.

Prof. Gollakota’s innovations have not only advanced the field of mobile systems but have also provided scalable, affordable solutions to some of the world’s most pressing challenges. His work is reshaping how we think about the intersection of technology and healthcare, and his pioneering research promises to improve the lives of millions globally, especially in low- and middle-income countries.

At the heart of Prof. Gollakota’s innovations is his ability to repurpose existing technologies to address real-world challenges

“His work on mobile and wireless communications is game-changing. Particularly impressive is his work on active sonar systems for physiological sensing, battery-free communications, and the use of AI to selectively tailor acoustic landscapes. These innovations will continue to benefit humanity for years to come,” stated Jury Chair, Infosys Prize 2024.

Transforming Mobile Devices into Healthcare Tools

At the heart of Prof. Gollakota’s innovations is his ability to repurpose existing technologies to address real-world challenges. One of his most remarkable contributions is his development of contactless physiological sensing using smartphones. By transforming mobile devices into active sonar systems, Gollakota’s research leverages the microphones and speakers in smartphones—components that are ubiquitous in today’s devices—to detect subtle physiological movements such as breathing.

This novel approach has significant implications for mobile health, particularly in resource-constrained areas where access to traditional medical equipment is limited. According to him, the ability to perform contactless physiological sensing with just a smartphone has the potential to revolutionize medical diagnostics, and make healthcare more accessible to billions of people around the world.

Battery-Free Communication: A Leap Forward in Sustainability

In a world increasingly concerned with energy efficiency and sustainability, Prof. Gollakota’s work on battery-free communication stands out as a pioneering achievement. He developed a technique called ambient backscatter, where wireless devices communicate by reflecting existing radio signals, rather than generating their own. This method drastically reduces energy consumption, allowing devices to communicate without the need for batteries.

This research is already opening up new possibilities for battery-free networks, including underwater Wi-Fi, powerline communication, and even wireless cameras. Battery-free devices could transform industries ranging from environmental monitoring to the Internet of Things (IoT). As per his visions, we are creating a future where energy-efficient, sustainable communication systems will be a part of our everyday lives.

Augmenting Human Auditory Perception with AI

In a truly visionary move, Prof. Gollakota’s research also explores how artificial intelligence (AI) can be used to augment human auditory perception. His work in this field enables people to program their acoustic environments, allowing them to focus on specific sounds or filter out others based on semantic descriptions. This breakthrough could have significant applications in hearing aids, earbuds, and assistive listening devices, where users can customize their listening experiences.

Battery-free devices could transform industries ranging from environmental monitoring to the Internet of Things (IoT)

By using AI to isolate and manipulate soundscapes in real time, Prof. Gollakota’s research is poised to improve quality of life for millions, offering individuals greater control over their auditory experiences. This technology will soon be commonplace in consumer electronics, giving people a level of control over their hearing that was once thought impossible.

A Thought Leader and Innovator

Prof. Shyam Gollakota’s career trajectory has been exceptional. A graduate of IIT Madras and MIT, where he received his Ph.D., Gollakota has quickly risen to prominence as a thought leader in mobile systems, machine learning, and human-computer interaction. He has received numerous accolades, including the National Science Foundation CAREER Award, the Alfred P. Sloan Fellowship, and the ACM Grace Murray Hopper Award. His recognition on MIT Technology Review’s 35 Innovators Under 35 list and twice on Forbes’ 30 Under 30 further cements his status as one of the brightest minds in his field.

As the director of the Mobile Intelligence Lab at the University of Washington, Gollakota is at the forefront of cutting-edge research in mobile health, networking, and battery-free computing. His work has already led to the creation of novel technologies that push the boundaries of what mobile systems can achieve, all with the potential to address key societal challenges.

The Future of Computing

Looking to the future, Prof. Gollakota’s research will continue to revolutionize mobile systems and human-computer interaction. His work in programmable sound, battery-free communication, and contactless diagnostics lays the foundation for the next generation of computing technologies. These innovations promise to reshape industries, improve global health, and enhance human capabilities.

With his visionary ideas and transformative research, Prof. Shyam Gollakota’s work will undoubtedly continue to have a profound impact on both the world of technology and the lives of people worldwide.

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Chandrayaan-3: The moon may have had a fiery past

A magma ocean might’ve wrapped the ancient moon, suggests findings from India’s robotic lunar mission, Chandrayaan-3.

Karthik Vinod

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The earth's moon. Credit: Ed Publica

On 23rd August last year, India’s Chandrayaan-3 made history being the first to soft-land on the moon’s south polar region. The landing marked the end of the high-octane phase of the mission. But its next phase was a slow-burner.

Pragyan, the suitcase-sized rover, that hitched a ride to the moon aboard the lander, Vikram, rolled off a ramp onto the lunar surface. It traversed along the dusty lunar surface slowly, at a pace even a snail could beat. Handlers at the Indian Space Research Organization (ISRO) didn’t want the suitcase-sized rover to risk stumbling over a rock or near a ridge, and jeopardize the mission.

The whitish spots are material excavated from the moon’s interior.

Nevertheless, the rover had a busy schedule to stick to. It was to probe the lunar soil, and relay that scientific data back to earth. Pragyan covered 100 meters in two weeks, before it stopped to take a nap ahead of a long lunar night. At the time, the rover’s battery pack was fully charged, thanks to the on-board solar panels soaking up sunlight during the day.

But lunar weather is harsh, especially at the south pole, where Pragyan napped, temperatures can reach as low as -250 degrees centigrade during the night. Added to that, a lunar night lasts two weeks. ISRO deemed Pragyan had only a 1% chance to survive.

Later, the expected happened, when the rover went unresponsive to ISRO’s pings to wake up.

But ISRO said the rover achieved what it was tasked to do. It relayed data all along for two weeks, examining soil from some 23 locations around the mission’s landing point, Statio Shiv Shakti. As months passed by, a slew of discoveries were made. Sulphur was discovered at the south pole, early on while the mission was ongoing. And only a few months ago, Pragyan found evidence of past weathering activity at the south pole.

But since August this year, research teams from ISRO and the Physical Research Laboratory in Ahmedabad, India, reported Pragyan’s most important findings yet – one of which sheds light onto the moon’s origins.

Chandrayaan-3’s Vikram lander, seen from the Pragyan rover’s camera

Chandrayaan-3 had carried a radioactive passenger to the moon’s surface – curium-244.

The radioactive curium helps lase the surface: firing alpha particles (which are helium nuclei) at the dusty terrain. Some of these alpha particles bounce off the dust, whereas others evict electrons from the lunar soil, thereby producing x-ray emissions. Keeping watch is the Alpha Particle X-ray Spectrometer (APXS) on-board the Pragyan rover. In August, PRL scientists published findings in the journal, Nature, based on APXS data, reporting discovery of ferroan anorthosite.

It wasn’t the first ever detection per se of ferroan anorthosite. In fact, Apollo 11 had brought back anorthosite rocks to earth, where they were identified as such. That was in 1969, and Apollo sampled them from the equator. Successive missions by the Soviet Union and most recently China affirmed likewise from mid-latitude – equatorial regions as well. But Pragyan’s detection of the rock type was the first ever from the polar region.

The Pragyan rover’s payload.

Anorthosites are common on earth. In fact, just a year after the Apollo 11 sampled the rock, scientists had evidence of the earth and the moon’s entangled history. The authors noted the similar composition between these rocks, that are geographically widespread. Furthermore, ferroan anorthosite is an igneous rock that forms on earth when hot lava produced in volcanic eruptions cools down.

And scientists had piled up evidence in support of a similar process that underwent on the moon. The anorthosite rocks on the moon are old, in fact, more than 4 billion years ago – a figure close to the earth’s inception with rest of the solar system – around 4.5 billion years. Scientific consensus has been that the moon was formed from remnants of a collision between the early earth and a rogue Mars-sized planetary body.

But the collision energy would have yielded a moon that was molten. A lava blanketing the surface – aka a global magma ocean. As this ocean cooled, minerals amongst which is plagioclase (a class of feldspar) crystallized and formed the anorthosite rocks on the moon. It’s commonly called the lunar magma ocean hypothesis.

When Pragyan treaded over the dusty lunar terrain, it didn’t register the anorthosite as a physical rock per se. Instead, it observed remnants of the rock, as fine powder.

Meteorites beat down rocks to fine powder, as they slam into the moon from space with regular impunity. On earth, the ground is saved by the presence of an atmosphere. But the moon virtually has no atmosphere. Nor does it have water to wear down the rocks. The surface is extremely hot during the lunar day – in fact, when Chandrayaan-3 landed on the moon, the surface temperature was some 50 degrees centigrade. Just a few months ago, Pragyan revealed possible signs of rock degradation from the rims of a crater.

Moon dust opens doors to the past

The fact the moon doesn’t (and can’t) sustain an atmosphere helps it make an attractive destination to learn more about our planet and the satellite’s shared origins. There’s no chemistry to remove traces of the moon’s early evolution from the lunar dust. As such, the dust opens doors to the past.

Space explorations missions soft-landing on the surface study this dust – or sample and shuttle them to earth for scientists to study them in detail.

In fact, Pragyan revealed a crater that’s amongst the oldest ever discovered on the moon. The findings were published in the journal, Icarus, in September. Hidden in plain sight, the rover’s navigation camera, NavCam, spotted subtle stretch marks on the surface, that were confirmed later with the Chandrayaan-2 orbiter (which has been orbiting the moon since 2019). In fact, this crater was found buried under nearby craters, most notably the South Pole-Aitkin basin located 350 km away. The basin is the largest impact crater in the entire solar system (some 2,500 km wide and 8 km deep) touted to have formed millions of years ago.

And this became subject to an earlier paper that PRL scientists authored, and was published in August. Pragyan identified material thought to have emerged from the moon’s interior. The APXS instrument picked up unusually high magnesium content in the vicinity. The authors speculate the meteorite that created the basin probably dug up magnesium from deep inside the moon’s upper mantle, and spewed them into Pragyan’s vicinity. 

But some experts believe in an alternate explanation. They believe the magnesium might have come from surface rocks in the vicinity, and not from the upper mantle. In fact, the authors acknowledged this amongst other possible alternatives. Nonetheless, the Chandrayaan-3’s findings doesn’t dispute the lunar magma ocean hypothesis either, if not backing it outright. Saying that, the theory lives on to fight another day.

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