Tag Archives: system

Groundbreaking New Laser System Cuts Through Earth’s Atmosphere Like It’s Nothing

To artists and romantics, the twinkling of stars is visual poetry; a dance of distant light as it twists and bends through a turbulent ocean of air above our heads.

Not everybody is so enamoured with our atmosphere’s distortions. To many scientists and engineers, a great deal of research and ground-to-satellite communication would be a whole lot easier if the air simply wasn’t there.

 

Losing our planet’s protective bubble of gases isn’t exactly a popular option. But Australian and French researchers have teamed up to design the next best thing – a system that guides light through the tempestuous currents of rippling air with the flick of a mirror.

The result is a laser link capable of holding its own through the atmosphere with unprecedented stability.

While astronomers have a few tricks up their sleeve to correct for the atmosphere’s distortions on incoming light, it’s been a challenge to emit a coherent beam of photons from the ground to a distant receiver so they keep together and on point.

Keeping transmissions on target and coherent – with their phases remaining neatly in line – through hundreds of kilometres of shifting air would allow us to link highly precise measurement tools and communications systems.

Satellites could probe for ores or evaluate water tables with improved precision. High-speed data transfer could require less power, and contain more information.

Lead author Ben Dix-Matthews, an electrical engineer with the International Centre for Radio Astronomy Research in Australia, explained the technology to ScienceAlert.

 

“The active terminal essentially uses a small four-pixel camera, which measures the sideways movement of the received beam,” says Dix-Matthews.

“This position measurement is then used to actively control a steerable mirror that keeps the received beam centred and removes the sideways movement caused by the atmosphere.”

In effect, the system can be used to compensate for the warping effects of the moving air in three dimensions – not just up and down, or left and right, but along the beam’s trajectory, keeping the link centred and its phases in order.

So far it’s only been tested across a relatively short distance of 265 metres (about 870 feet). About 715 metres (just under half a mile) of optical fibre cable was run underground between the transmitter and receiver to carry a beam for comparison.

The results were so stable they could be used to connect the kinds of optical atomic clocks used to test fundamental physics, such as Einstein’s theories of relativity.

With the proof of concept demonstrated, there’s no reason to think a similar technique won’t one day be aiming for the sky, and beyond. Though there are a few hurdles that need to be overcome first.

 

“During this experiment we had to do the initial alignment by hand, using a visible guide laser that was in line with the stabilised infrared beam,” Dix-Matthews told ScienceAlert.

“When making links between optical atomic clocks, it would be good to have a way of doing this coarse alignment more easily.”

Fortunately Dix-Matthews’ French collaborators are working on a device that will speed up the initial coarse alignment process, promising a second generation of laser link technology that won’t require such an involved set-up.

The team also found temperature variations in the equipment affected the phase’s stability, limiting the duration of the signal to around 100 seconds. This hurdle will also be the focus of future improvements.

We might not need to wait long. The researchers are already making headway on upgrades for their system.

“We have started using a high-power laser amplifier that should help us deal with the larger power losses expected over longer distances, such as to space,” says Dix-Matthews.

“We have also completely rebuilt our active terminal to make it more sensitive to low received powers and make it more effective at cancelling out the movement of the received beam.”

With orbiting technology rapidly becoming a major focus for many data providers, potentially filling our skies with satellites, innovations that make linking communications systems across our atmosphere will only become more sought after.

As useful as our atmosphere is for, well, keeping us all alive, there are certainly some downsides to being buried under a restless blanket of warm gas.

This research was published in Nature Communications.

 

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Orange County readies second mass vaccination site at Soka University, tweaks appointment system – Orange County Register

Orange County staff and volunteers are gearing up for the opening of a mass vaccination center at Soka University in Aliso Viejo on Saturday.

It joins the first center the county opened last week at Disneyland that has been handling about 3,000 appointments a day.

“Bring your umbrellas, plan for rain, if you’re in a walker, you have to take those things into account,” county spokeswoman Molly Nichelson said. Staff and volunteers will be on hand to help visitors from the campus parking structure off Wood Canyon Drive to a gym nearby, where vaccines will take place.

The county has enough vaccines and staff on hand for a confident launch of the new Soka Super POD (point-of-distribution) this weekend, said spokeswoman Molly Nichelson. Officials have said they would not open new locations until volunteers and doses were available to make it worth it; five sites are ultimately expected.

But public health officials are tempering expectations and asking for patience after the Othena appointment system got off to a rocky start among its target users: seniors age 65 and older.

The Health Care Agency said this week the appointment process had been “simplified” to stop users from needing to constantly refresh Othena on their computers and phones in hopes of landing a slot.

For users who have completed registration, Othena will email eligible groups around 10 a.m. each day, alerting them an appointment is available to them.

Dr. Clayton Chau, Health Care Agency director and county health officer, said staff members are considering a person’s coronavirus risk while assigning appointments. Staff also will send patients to whichever super site is closest, he said.

But if users don’t respond through Othena within a few hours, they’ll be placed back in the virtual queue, Nichelson said.

“They really have to pay attention to those emails that come through,” she said.

The Health Care Agency has set up a hotline at 714-834-2000 to field questions about Othena, vaccine appointments and other related issues during weekday business hours.

At this point, people who qualify for a vaccine and want an appointment can’t call to set one up, but can call for help in registering on Othena.

“We view that this’ll be able to make a us more nimble,” she said.

Chau advised seniors having trouble with Othena to ask their doctor or staff at a local senior center for help.

And super sites aren’t the only option, Chau said. The Health Care Agency also is ramping up smaller-scale “mobile” vaccination clinics, which have parachuted in for a day at a couple of seniors centers with more in the works.

Meanwhile, the county is still striking a balance of marshaling vaccines, staff and volunteers to get doses into the arms of the county’s most exposed and vulnerable to COVID-19 efficiently and fairly.

During a virtual town hall Thursday with Assemblywoman Cottie Petrie-Norris, Chau said Orange County still doesn’t have enough vaccines and repeated the need for letting older seniors get their shots first, particularly those with chronic health conditions that make the coronavirus more dangerous to them.

“We are asking the community to be patient, let us give the vaccine to those 75 and older and those 65 and older with chronic problems,” he said. “Let us protect them first, because they are the ones that if they get infected, they end up in hospitals more than others.”

On Thursday, Orange County gave vaccine administrators the go-ahead to resume using Moderna vaccine lot 41L20A, which was put on hold by the state Department of Public Health after a handful of allergic reactions in San Diego last week. About 5,000 people in Orange County received shots from that batch, but there were no known adverse effects, the Heath Care Agency said earlier this week.

After an investigation, state health officials said late Wednesday there was “no scientific basis to continue the pause.”

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Solar system formation in two steps

The inner terrestrial protoplanets accrete early, inherit a substantial amount of radioactive 26Al, and hence melt, form iron cores, and degas their primordial volatile abundances rapidly. The outer Solar System planets start to accrete later and further out with less radiogenic heating, and hence retain the majority of their initially accreted volatiles. Credit: Mark A Garlick/markgarlick.com

An international team of researchers from the University of Oxford, LMU Munich, ETH Zurich, BGI Bayreuth, and the University of Zurich discovered that a two-step formation process of the early Solar System can explain the chronology and split in volatile and isotope content of the inner and outer Solar System.

Their findings will be published in Science.

The paper presents a new theoretical framework for the formation and structure of the Solar System that can explain several key features of the terrestrial planets (like Earth, Venus, and Mars), outer Solar System (like Jupiter), and composition of asteroids and meteorite families. The team’s work draws on and connects recent advances in astronomy (namely observations of other solar systems during their formation) and meteoritics—laboratory experiments and analyses on the isotope, iron, and water content in meteorites.

The suggested combination of astrophysical and geophysical phenomena during the earliest formation phase of the Sun and the Solar System itself can explain why the inner Solar System planets are small and dry with little water by mass, while the outer Solar System planets are larger and wet with lots of water. It explains the meteorite record by forming planets in two distinct steps. The inner terrestrial protoplanets accreted early and were internally heated by strong radioactive decay; this dried them out and split the inner, dry from the outer, wet planetary population. This has several implications for the distribution and necessary formation conditions of planets like Earth in extrasolar planetary systems.







https://scx2.b-cdn.net/gfx/video/2021/600973531b3e6.mp4
Video introduction of main concepts of the research. Credit: Tim Lichtenberg

The numerical experiments performed by the interdisciplinary team showed that the relative chronologies of early onset and protracted finish of accretion in the inner Solar System, and a later onset and more rapid accretion of the outer Solar System planets can be explained by two distinct formation epochs of planetesimals, the building blocks of the planets. Recent observations of planet-forming disks showed that disk midplanes, where planets form, may have relatively low levels of turbulence. Under such conditions the interactions between the dust grains embedded in the disk gas and water around the orbital location where it transitions from gas to ice phase (the snow line) can trigger an early formation burst of planetesimals in the inner Solar System and another one later and further out.

The two distinct formation episodes of the planetesimal populations, which further accrete material from the surrounding disk and via mutual collisions, result in different geophysical modes of internal evolution for the forming protoplanets. Dr. Tim Lichtenberg from the Department of Atmospheric, Oceanic and Planetary Physics at the University of Oxford and lead-author of the study notes: “The different formation time intervals of these planetesimal populations mean that their internal heat engine from radioactive decay differed substantially. Inner Solar System planetesimals became very hot, developed internal magma oceans, quickly formed iron cores, and degassed their initial volatile content, which eventually resulted in dry planet compositions. In comparison, outer Solar System planetesimals formed later and therefore experienced substantially less internal heating and therefore limited iron core formation, and volatile release.

“The early-formed and dry inner Solar System and the later-formed and wet outer Solar System were therefore set on two different evolutionary paths very early on in their history. This opens new avenues to understand the origins of the earliest atmospheres of Earth-like planets and the place of the Solar System within the context of the exoplanetary census across the galaxy.”

This research was supported by funding from the Simons Collaboration on the Origins of Life, the Swiss National Science Foundation, and the European Research Council.

The full study, “Bifurcation of planetary building blocks during Solar System formation,” will be published on 22 January 2021 in Science, 371, 6527.


Reconstructing the solar system’s original architecture


More information:
“Bifurcation of planetary building blocks during Solar System formation” Science (2021). science.sciencemag.org/cgi/doi … 1126/science.abb3091
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Solar system formation in two steps (2021, January 21)
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