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AI and physics unite for meta-antennas design

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AI and physics unite for meta-antennas design


AI and physics unite for meta-antennas design
Schematics of the PA-PSO algorithm. (a) and (b) Working principle of the metalens antenna. (c) and (d) Comparison between the traditional PSO and PA-PSO algorithm. The red and blue stars represent optimal and sub-optimal designs, respectively. The red dots and dashed arrows represent the positions and velocities of the particles, respectively. Credit: Opto-Electronic Science (2024). DOI: 10.29026/oes.2024.240014

Ka-band metasurface antennas, with their low-cost, low-profile design and superior beam-steering capabilities, show significant potential in the field of satellite communications. However, the constraints of limited satellite resources and significant atmospheric losses at Ka-band frequencies require these antennas to achieve wide-angle beam scanning capabilities and high antenna gain, adding considerable complexity to their design.

In order to achieve the design of a multifunctional and highly efficient meta-antenna, the design optimization will involve numerous parameters, greatly increasing the use of computational resources and optimization time. Addressing the critical issue of balancing multiple optimization objectives, such as gain and scanning angle, while improving optimization speed, remains a key challenge in the design process.

To address these challenges of meta-antenna design, researchers from the University of Electronic Science and Technology of China, Tongji University, and City University of Hong Kong have joined forces in an extensive collaboration.

Leveraging their long-term expertise in the field of meta-optics, they proposed a Ka-band meta-antenna design method based on a Physics-Assisted Particle Swarm Optimization (PA-PSO) algorithm. Using this method, they designed and fabricated a Ka-band meta-antenna. The study is published in the journal Opto-Electronic Science.

The antenna proposed in the paper is designed using the PA-PSO algorithm. Compared to the traditional PSO algorithm, the optimization direction of particles in the PA-PSO algorithm is guided by extremum conditions derived from the variational method. This not only reduces computation time but also decreases the likelihood of finding suboptimal designs.

The final optimized results indicate that the relative strength achieved by the PA-PSO algorithm is 94.62806, which is comparable to the relative strength of 94.62786 achieved by the traditional PSO algorithm. However, the computational cost of the PA-PSO algorithm is significantly lower; it reaches the optimal state after only 650 iterations, whereas the traditional PSO algorithm requires 4100 iterations.

This means the computation time of the PA-PSO algorithm is less than one-sixth of that for the PSO algorithm. Therefore, the PA-PSO method can guide particle swarms more efficiently, reducing computation time, making it an important tool for addressing complex multivariate and multi-objective optimization challenges.

  • AI and physics unite for meta-antennas design
    Performance of the PA-PSO algorithm. (a) Variation of the relative electric field intensity with respect to the times of iteration for PA-PSO and PSO algorithms. The purple line shows the calculation errors. The four hexagons from bottom to top represent phase distributions at different stages: initial phase distribution, PSO algorithm iteration 650 times, PSO algorithm iteration 1500 times, and PSO algorithm iteration 4,100 times (PA-PSO algorithm iteration 650 times). (b) Comparison of FOVs and F/D for planar lens antennas. The colors of the points indicate the fluctuation of gains when scanning within the field of view range. Credit: Opto-Electronic Science (2024). DOI: 10.29026/oes.2024.240014
  • AI and physics unite for meta-antennas design
    Gain profiles of the metalens antenna when the feed is placed on the focal plane with different displacements x. Comparison between the experimental results (blue lines) and simulation results (red lines) when the feed source position is (a) at x = 0, showing a maximum gain of 21.7 dBi, which corresponds to an angle of 0°; (b) at x = 15 mm, showing a maximum gain is 21.2 dBi, which corresponds to an angle of 25°; (c) at x = 30 mm, showing a maximum gain is 18.3 dBi, which corresponds to an angle of 55°. (d) The relationship between the maximum gain angles and the corresponding gains obtained from testing the feed source at different positions. Inset shows the sample photo and unit cell structure diagram. Credit: Opto-Electronic Science (2024). DOI: 10.29026/oes.2024.240014

Based on the phase distribution optimized by the PA-PSO algorithm, the team designed and fabricated a hexagonal meta-antenna sample with a focal length of 22 mm, diagonal length of 110 mm, and a thickness of only 1.524 mm.

The antenna has an f-number of only 0.2, a beam scanning angle of ±55°, a maximum gain of 21.7 dBi, and a gain flatness of within 4 dB. This innovative hexagonal meta-antenna, with its wide scanning angle, compact design, and high transmission gain, exhibits enormous potential for applications in satellite communication, radar systems, 5G networks, and the Internet of Things, among many other fields.

More information:
Shibin Jiang et al, Ka-Band metalens antenna empowered by physics-assisted particle swarm optimization (PA-PSO) algorithm, Opto-Electronic Science (2024). DOI: 10.29026/oes.2024.240014

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AI and physics unite for meta-antennas design (2024, October 11)
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Novel algorithms detect precursory scale increase to help forecast big quakes

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Novel algorithms detect precursory scale increase to help forecast big quakes


earthquake
Credit: Pixabay/CC0 Public Domain

Many people are aware that large earthquakes are often followed by a sequence of aftershocks as stresses are redistributed in the surrounding area. Many may not be aware that there are also sequences of earthquakes that occur before most large earthquakes.

The so-called precursory scale increase (PSI) describes a sudden increase in the rate and size of earthquakes in a precursory area, with a precursor time and magnitude prior to the upcoming large earthquake. Statistical relations between the different precursor variables form the basis of the earthquake forecasting model EEPAS (Every Earthquake a Precursor According to Scale).

EEPAS aims to forecast major upcoming earthquakes in the medium term, that is, within months to decades, depending on their magnitudes. EEPAS has performed well in global testing and is an important contributor to public earthquake forecasting in New Zealand and to New Zealand’s National Seismic Hazard Model.

To date, there has been limited analysis of the precursory scale increase, most likely due to the elaborate and manual method with which it was originally detected. Recent work indicated that multiple PSI identifications could be made for a given earthquake with smaller precursory areas associated with larger precursor times and vice versa.

A more systematic approach to detecting PSI was needed to study this trade-off between area and time to confirm that small precursory areas grow as time gets closer to the mainshock. GNS Science Hazard and Risk Scientist Dr. Annemarie Christophersen is the lead author of a paper published in Seismological Research Letters that describes two algorithms which automatically detect PSI in earthquake catalogs.

The algorithms have been applied both to real earthquake catalogs and to simulated data that are based on known physics of earthquake occurrences. The algorithms identify multiple realizations of PSI for most major earthquakes with different precursor times, areas and magnitudes.

On average, an even trade-off between time and space was found for both real and synthetic data. Also, the scaling relations of the PSI parameters are consistent with the original subjectively identified scaling relations from which the EEPAS forecasting models is derived.

Dr. Christophersen says, “Our work is critical to advance our understanding of how earthquake activity builds up towards a large earthquake. Our next step is to include our findings in the EEPAS model to improve medium-term earthquake forecasting, which is a direct input into public earthquake forecasting and the National Seismic Hazard Model. These resources help us to make better decisions on where to build and to prioritize strengthening of existing infrastructure to make New Zealand more resilient to large earthquakes.”

More information:
Annemarie Christophersen et al, Algorithmic Identification of the Precursory Scale Increase Phenomenon in Earthquake Catalogs, Seismological Research Letters (2024). DOI: 10.1785/0220240233

Citation:
Novel algorithms detect precursory scale increase to help forecast big quakes (2024, October 11)
retrieved 11 October 2024
from https://phys.org/news/2024-10-algorithms-precursory-scale-big-quakes.html

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Mountain chickadees songs provide real-time evidence for Darwin’s character displacement theory

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Mountain chickadees songs provide real-time evidence for Darwin’s character displacement theory


Mountain chickadees in Boulder have evolved a different tune to avoid getting mixed up with their cousins, according to a new CU Boulder-led study published Oct. 9 in the Journal of Evolutionary Biology.

The results provide real-time evidence for one of Charles Darwin’s famous theories and shed light on how pressure from human activity can impact wildlife’s evolution.

Mountain chickadees, common in the high-elevation conifer forests on North America’s west coast and in the Rocky Mountains, are vocal animals. They constantly whistle a chirpy “bee-bee-bee-bee” song to attract mates or defend their territories.

Black-capped chickadees are their close relatives. The two birds look very similar, except that mountain chickadees have a pair of white eyebrow-like stripes above their eyes. Black-capped chickadees tend to live at lower elevations, and in certain regions, such as Colorado’s Boulder County, the two birds’ habitats overlap.

Scott Taylor, one of the paper’s senior authors and associate professor in the Department of Ecology and Evolutionary Biology, wondered whether this unique living arrangement would push the chickadees to evolve different traits. His team’s hypothesis is based on Darwin’s “character displacement” theory, which suggests that closely related species with overlapping habitats tend to diverge in traits—such as appearance and call—to reduce competition or costly hybridization between different species.

Galápagos finches are a classic example. These closely related birds on the Galápagos Islands evolved different beak shapes and sizes from one another to specialize in eating different types of seeds, reducing competition.

In Boulder, where two species of chickadee coexist, researchers wondered if the birds had started humming a different tune.

“In birds, song is an important characteristic for individuals to recognize each other,” said Olivia Taylor, the paper’s first author and a recent graduate of the Department of Ecology and Evolutionary Biology.

To explore this, the team collaborated with researchers at the University of Western Ontario and Cornell University, who recorded more than 2,000 chickadee songs. They sampled black-capped and mountain chickadees in Boulder, where the two species coexist. They also followed populations of mountain chickadees in California and black-capped chickadees in New York, where each species lives by themselves.

They found that Boulder’s mountain chickadees sing differently compared to those in California. Instead of the common four-note “bee-bee-bee-bee” song, Boulder’s mountain chickadees whistle with more notes. For instance, many of their songs have five to six notes, which is significantly longer than the two-note songs of black-capped chickadees living in the same area.

Boulder’s mountain chickadees are also more likely to include one or two introductory notes—short chirps at the beginning of a song—compared with the Californian mountain chickadees and their black-capped cousins.

“Our ears couldn’t really pick up these longer introductory notes, and we only noticed that after we recorded and analyzed the songs. But the birds’ hearing is so much better than ours, so they can certainly tell them apart,” said Scott Taylor, who has led the Boulder Chickadee Study at CU Boulder’s Mountain Research Station for six years.

Previous research shows black-capped chickadees are dominant over mountain chickadees when they coexist. Black-capped chickadees often chase mountain chickadees away if they get too close, and mountain chickadees usually wait for black-capped chickadees to finish eating and leave before they approach feeders.

While the two species can breed with each other, female hybrid offspring produced from a black-capped chickadee and a mountain chickadee are likely sterile.

Singing a different song can help mountain chickadees distinguish between friends or foes and avoid interbreeding, the authors said.

“There’s a reproductive cost in hybridizing with each other. From an evolutionary perspective, sterile females are a dead-end in reproduction. And maybe the hybrid males also suffer some physiological costs we don’t yet know about. Given the two species are adapted to different elevations, some hybrids may struggle to survive cold winters in the high mountains,” Scott Taylor said.

A few hundred years ago, mountain chickadees inhabited Boulder’s conifer forests alongside likely far fewer black-capped chickadees than today. As settlers moved in and planted ash and maple trees, they also created excellent habitats for black-capped chickadees. As a result, the black-capped population is likely much larger now, and the birds are interacting more frequently with local mountain chickadees.

“It’s very interesting to see how these species are responding to what is ultimately a human-introduced pressure,” said Olivia Taylor. “For that, I think it’s important to document and understand our impacts on wildlife and how they adapt to co-exist.”

More information:
Olivia Taylor et al, Chickadees sing different songs in sympatry versus allopatry, Journal of Evolutionary Biology (2024). DOI: 10.1093/jeb/voae114

Citation:
Mountain chickadees songs provide real-time evidence for Darwin’s character displacement theory (2024, October 11)
retrieved 11 October 2024
from https://phys.org/news/2024-10-mountain-chickadees-songs-real-evidence.html

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Skygazers treated to another aurora show

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Skygazers treated to another aurora show


A couple looks out at the southern lights on the outskirts of Christchurch in New Zealand
A couple looks out at the southern lights on the outskirts of Christchurch in New Zealand.

Scientist Jim Wild has traveled to the Arctic Circle numerous times to study the northern lights, but on Thursday night he only needed to look out of his bedroom window in the English city of Lancaster.

For at least the second time this year, skygazers in many parts of the world were treated to colorful auroras at latitudes beyond the polar extremes where they normally light up the skies.

The dazzling celestial shows were caused by a gigantic ball of plasma—and an accompanying magnetic field—which erupted from the sun earlier this week.

When this eruption, called a coronal mass ejection (CME), arrived at Earth at around 1600 GMT on Thursday, it triggered a strong geomagnetic storm.

This storm in turn sparked northern and southern lights—aurora borealis and aurora australis—in swathes of Europe, the United States, Australia and elsewhere.

While Wild could see the shimmering reds and greens from his back garden, he jumped in the car with his family to get a better look away from the bright lights of Lancaster.

“All the little back roads and parking spots were full of people with flasks of coffee and deck chairs looking at the northern lights,” he told AFP.

“It was a party atmosphere,” he said, comparing the scenes to UFO spotters looking up at the sky in the movie “Close Encounters of the Third Kind”.

The aurora borealis seen from Shenandoah National Park in Rileyville, in the US state of Virginia
The aurora borealis seen from Shenandoah National Park in Rileyville, in the US state of Virginia.

While Wild was explaining the phenomenon to his 11- and 13-year-old children, another nearby skygazer approached and asked how come he knew so much about it.

“Well, actually, this is what I study for a living,” responded the professor in space physics at Lancaster University, who specializes in how solar weather disrupts power grids and transport here on Earth.

‘Perfect hit’

Auroras were also visible across northern Europe, including near London and Berlin, and as far south in the US as the state of Virginia. In the Southern Hemisphere, areas of Australia and New Zealand were also treated to a show, AFP photos showed.

The CME that triggered Thursday’s auroras erupted from a spot on the sun pointed directly at Earth, said Juha-Pekka Luntama, the head of the European Space Agency’s Space Weather Office.

“It was a perfect hit,” he told AFP.

The southern lights seen from south of the Australian city of Melbourne
The southern lights seen from south of the Australian city of Melbourne.

The CME caused a “severe” geomagnetic storm given a rating of G4. This fell narrowly short of the highest level of G5, which was seen in May, when auroras delighted many skygazers across swathes of the world.

Storms on the sun have been intensifying as solar activity approaches—or may have already reached—the peak of its 11-year cycle.

While such storms offer pretty light shows for skygazers, they can pose a serious threat to satellites, GPS services, power grids and even astronauts in space.

The US Space Weather Prediction Center warned on Thursday that the geomagnetic storm could disrupt emergencies services already stretched thin by deadly hurricanes Helene and Milton.

Luntama said the European Space Agency had not received any information about disruptions caused by the latest storm, but sometimes this can take days.

The storm is “gradually dissipating”, he added, which means that any auroras on Friday night or over the weekend will likely be farther north in Europe, such as central Sweden.

  • The light show over Haraldsted Lake near Ringsted in Denmark
    The light show over Haraldsted Lake near Ringsted in Denmark.
  • Northern lights over the Baltic Sea near Kiel in northern Germany
    Northern lights over the Baltic Sea near Kiel in northern Germany.

‘Delighted’

But for those still hoping to see an aurora, there could be some more chances in the next couple of years.

Luntama explained that during past solar cycles, the biggest eruptions have come in the two years after the sun passed its peak.

Wild also did not expect a repeat of Thursday’s “magical” display.

But space weather—like Earth’s weather—is not an “exact art,” he emphasized.

And if there is an aurora lighting up the sky nearby, it is worth seeking out.

Wild said his neighbors had traveled to Norway twice to see the northern lights—but had been foiled by clouds both times.

Then on Thursday night, they saw an aurora from their garden.

“They were really delighted to finally have seen it,” Wild said.

© 2024 AFP

Citation:
‘Party atmosphere’: Skygazers treated to another aurora show (2024, October 11)
retrieved 11 October 2024
from https://phys.org/news/2024-10-party-atmosphere-skygazers-aurora.html

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Bat data study reveals conservation priorities in San Diego County

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Bat data study reveals conservation priorities in San Diego County


Researchers use bat data to prioritize areas in San Diego in need of management
Townsend’s big-eared bat captured in a mist net during field studies in California. Credit: Drew Stokes, CC-BY 4.0 (https://creativecommons.org/licenses/by/4.0/)

A team of wildlife managers at the U.S. Geological Survey in San Diego, California, working with a colleague from the San Diego Natural History Museum, have uncovered the areas in San Diego County that need the most scrutiny if bat populations in the area are to be saved.

In their study published in PLOS ONE, the group used existing data on the bat population in the San Diego County area to find out which bats need the most attention to avoid extinction.

As the research team points out, San Diego County hosts 22 of 41 known bat species in the United States. Sixteen of those species are at risk of extinction. Preserving bat populations is important in the San Diego area and around the world as bats are a major natural source of insect control. A single bat can eat up to 1,000 insects in just one hour. In this new effort, the researchers sought out which parts of San Diego County should be prioritized for bat conservation efforts.

The researchers analyzed bat population data from San Diego County. Most notably, they focused on two data points—species richness and threats. The species richness data revealed information regarding bat diversity, including population size and health and current conservation efforts surrounding each. Threats included anything in the environment that could jeopardize individual bats or their communities.

The research team mapped the places where different species of bats lived and hunted for food. They found that the bats faced three major threats: artificial lights, urbanization and non-conserved land (land not in its natural state). They noted that urbanization and artificial lighting make life particularly hard for bats because they impinge on their natural behaviors.

Researchers use long-term bat community survey data to prioritize areas in San Diego in need of management
Quantification of threats to bats at localized spatial scales for conservation and management. Credit: PLOS ONE (2024). DOI: 10.1371/journal.pone.0310812

Urbanization means fewer resources and artificial lighting can confuse the bats because they are nocturnal and use light to tell them when to feed and when to head back to their shelter. The data also helped plan conservation efforts involving the installation of bat boxes and the planting of native vegetation.

The team’s efforts helped establish a plan of action centered on helping the bats in San Diego survive as humans continue to change the landscape in which they live.

More information:
Brian M. Myers et al, Quantification of threats to bats at localized spatial scales for conservation and management, PLOS ONE (2024). DOI: 10.1371/journal.pone.0310812

© 2024 Science X Network

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Bat data study reveals conservation priorities in San Diego County (2024, October 11)
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