Cosmic ray pioneer: Bibha Chowdhuri joins the ranks of the Forces of Nature. (Courtesy: Perimeter Institute for Theoretical Physics)
This edition of the Red Folder is going out of this world to celebrate the three missions arriving at Mars this month: United Arab Emirates’ Hope probe, China’s Tianwen-1 Mars probe and the US’s Perseverance rover.
One thing that space missions have to contend with is damage to equipment from cosmic rays. Canada’s Perimeter Institute for Theoretical Physics has just issued a downloadable poster of the cosmic-ray pioneer Bibha Chowdhuri in its Forces of Nature series that celebrates women who have changed science.
Born in Kolkata, India in 1913, Chowdhuri began her pioneering work on cosmic rays while doing a MSc at the University of Calcutta. She then moved to the UK where she did a PhD at the University of Manchester with the future Nobel laureate Patrick Blackett. There Chowdhuri did research on air showers of radiation, which are created when a high energy cosmic ray collides with a molecule in the upper atmosphere.
Chowdhuri returned to India after completing her PhD and worked at the Tata Institute of Fundamental Research as well as the Physical Research Laboratory and the Saha Institute of Nuclear Physics. She died in 1991.
Staying on the topic of cosmic rays, an article in TheGamerclaims that a player called DOTA_Teabag gained a boost from a wayward ionizing particle from space while playing the video game Super Mario 64. In 2013, the player was launched high into the air for no apparent reason, gaining significant advantage.
Flipping a bit
After the event, gamers around the world tried to work out how DOTA_Teabag did it, but to no avail – until now. A gamer called pannenkoek12 has shown that boost could have occurred if one specific bit in the byte that defines the player’s height was flipped at a precise moment in the game. And how could that happen? Well, the speculation is that a particle from space just happened to zap the game hardware, flipping the bit.
“Farfarout” is the name of what astronomers at the University of Hawaii believe is the most distant object observed in the Solar System. The planetoid is four times the distance from the Sun as Pluto and was first spotted in 2018. Now, after careful observations the team is confident about the object’s orbit, which puts Farfarout beyond the previous record holder “Farout” – which was also discovered in 2018 by the same team.
Farfarout takes about 1000 years to orbit the Sun , which is why it took several years to pin down its orbit.
Scientists in Russia have observed trace amounts of hydrogen chloride in Mars’ atmosphere for the first time. The detection, which was based on data from the ExoMars Trace Gas Orbiter (TGO), raises questions about the dynamics and chemistry of the Martian atmosphere and surface as well as the processes that could have formed the compound.
At local sunrise and sunset, two of the instruments aboard the TGO – the Nadir and Occultation for Mars Discovery (NOMAD) and the Atmospheric Chemistry Suite (ACS) – use spectrometers to analyse the sunlight that passes through the Martian atmosphere. These sensitive instruments make it possible to detect trace species at the parts-per-billion (ppb) level.
Dusty discovery
The TGO picked up the first signs of hydrogen chloride (HCl) shortly after a global dust storm (GDS) that occurred in Martian year 34 (MY34), equivalent to 2018 on Earth. These storms occur every 3–4 Martian years on average, when the planet’s complex orbital pattern ensures that summer in its southern hemisphere coincides with the point at which it is closest to the Sun (perihelion).
The researchers, who report their work in Science Advances, suggest that the appearance of the HCl could be due to water vapour interacting with chlorine from the dust grains. “Both dust and water vapour in the atmosphere are amplified during GDS or ‘dusty season’,” explains Oleg Korablev, who led the research at the Space Research Institute of the Russian Academy of Sciences.
Even without a GDS, however, Korablev notes that Mars’ atmosphere tends to become dustier at perihelion due to an increase in the planet’s atmospheric circulation intensity. Indeed, a separate study led by K S Olsen recently found that HCl reappeared in Mars’ atmosphere in the dusty season of the following year, MY35, when there was no GDS.
Volcanic alternative
Korablev and colleagues also put forward an alternative hypothesis for the formation of HCl in Mars’ atmosphere: the compound could be released directly from volcanoes. This possibility would be analogous to volcanic activity exhibited on Earth, where chlorine compounds and their reactions with aerosols are known to impact the ozone layer in the stratosphere.
However, the scientists say that this hypothesis is less likely because it would be hard to explain how a localized surface source could produce such widespread atmospheric traces of HCl. In addition, seismic data from a separate Mars mission, NASA’s InSight Lander, indicates that Mars does not experience much volcanic activity, and the TGO did not detect the abundance of sulphur gas that a volcanic eruption would produce.
Joint exploration
Korablev says that further research on the chemical cycles of elements such as nitrogen and sulphur will be needed to characterize the processes taking place on Mars. In particular, scientists have not yet confirmed and quantified the gas-solid heterogeneous reaction that might allow chlorine salts in the Martian dust to join up with atmospheric water vapour to form HCl gas. An explanation for why the HCl gas disappears after the end of the dusty season is also lacking.
While the TGO is a collaborative project between the European Space Agency (ESA) and the Russian Roscosmos State Space Cooperation, Korablev points out that the upcoming ExoMars 2022 mission is more complex, with the success of the “mostly ESA” Rosalind Franklin rover depending on “intertwined” subsystems of the landing module. Like NASA’s just-landedPerseverance rover, ExoMars 2022 aims to understand Mars’ astrobiological and geological processes, as well as the history of Martian water. A key component will be the Franklin rover’s onboard spectrometer, the NASA-provided Mars Organic Molecule Analyzer, which will perform the first analyses of the amount and type of chemicals in the Martian subsurface – potentially confirming theories of the planet’s formation. Getting all these parts to work together will be a challenge, Korablev says; nonetheless, he thinks “the agencies will learn the lesson” and that “joint is good”.
Two’s company, but three’s a crowd – unless you’re trying to make graphene superconduct at higher temperatures. That is the finding of researchers at Harvard University in the US, who discovered that the superconducting state in three stacked and twisted layers of graphene is more robust to temperature increase than the equivalent state in two-layer graphene. The researchers also found evidence that superconductivity in the trilayer system comes from strong interactions between electrons, rather than weak ones as in most conventional superconductors – corroborating a result reported a few days earlier by a separate team at the Massachusetts Institute of Technology (MIT).
A sheet of graphene consists of a simple repetition of carbon atoms arranged in a two-dimensional hexagonal lattice. When two sheets of graphene are placed atop each other and slightly misaligned, they form a moiré pattern, or “stretched” superlattice that dramatically changes the electronic interactions in the material compared to its pristine counterpart. The misalignment angle is critical: in 2018, the MIT group, led by Pablo Jarillo-Herrero, discovered a so-called “magic” angle of 1.1° where the material switches from an insulator to a superconductor. This means the twisted graphene can carry electrical current with no resistance below a superconducting transition temperature, Tc, of 1.7 K.
More robust superconductivity
In the Harvard study, a team led by Philip Kim made twisted trilayer graphene by stacking three sheets of graphene on top of each other at small twist angles of opposite signs. The twist angle between the top and middle layer is 1.5° while that between the middle and bottom layer is -1.5°.
Kim and colleagues studied the conductivity of these sheets by applying a voltage to them and then measuring the current that circulated through them. They measured a Tc for a twisted trilayer of around 2.3 K, or about 40% higher than similarly prepared twisted bilayer graphene.
The researchers report that the new structure is also extremely sensitive to the applied voltage. By varying the electric field, they found that the superconductivity in the material stems from strong interactions between electrons – a factor that could help explain the increase in Tc.
“While weakly interacting superconductors are fragile and lose superconductivity when heated to a few Kelvin, strong coupling superconductors are much more resilient but much less understood,” explains team member Eslam Khalaf. “Realizing strong coupling superconductivity in a simple and tuneable system such as trilayer graphene could pave the way to finally develop a theoretical understanding of strongly-coupled superconductors to help realize the goal of a high temperature, maybe even room temperature, superconductor.”
Close-to-room-temperature superconductors are, he adds, the “holy grail” of condensed- matter physics, with important real-world applications in areas such as electricity transmission, transport and even quantum computing. Unfortunately, today’s superconductors, including graphene, only work at ultracold temperatures or ultra-high pressures.
The Harvard researchers, who report their work in Science, say they will continue to investigate the origin of the peculiar superconductivity they have unearthed. “We also aim to find a way to obtain even more robust superconductivity in twisted 2D materials,” Kim tells Physics World.
A monochromatic X-ray source under development for breast cancer screening can produce high-quality phantom images at significantly lower radiation dose and with greater sensitivity than conventional mammography systems. This low-dose technology could represent a paradigm change for mammography, making these exams safer for women by exposing them to less radiation dose and better identifying suspicious abnormalities, especially in dense breasts.
Developers at Imagine Scientific report that their prototype system reduces radiation dose by a factor of five to 10 times for the same signal-to-noise ratio (SNR) as a conventional mammography system. They tested the system on breast phantoms of varying thickness containing a variety of test objects. The system is being designed for both conventional 2D digital mammography and 3D digital breast tomosynthesis (DBT).
Conventional radiography systems use multi-wavelength X-ray emission, which extends over a broad energy band. This creates a less optimal image than an extremely narrow bandwidth beam does, and exposes patients to a higher level of radiation to obtain a diagnostic-quality image. The advantages of monochromatic X-ray radiation to improve clinical imaging are well known, but its generation requires crystal or multilayer monochromators coupled to either traditional broadband X-ray tubes or large synchrotron facilities. Both are impractical for routine clinical use.
First author Eric Silver, founder and CEO of Imagine Scientific.
Company founder Eric Silver and colleagues have developed a prototype X-ray generator that sequentially combines two X-ray emission processes to generate monochromatic X-ray beams suitable for medical imaging. The two-stage process includes bombarding a metallic target with high-energy electrons to emit broadband bremsstrahlung X-rays, which subsequently irradiate a second target that emits monochromatic X-rays via fluorescence. Additional proprietary geometric techniques produce a beam of monochromatic X-rays with sufficient intensity and large enough field-of-view for routine clinical imaging.
The prototype X-ray tube, which is comparable in size to a conventional X-ray tube, uses the inside surface of a conically-shaped annular ring to concentrate the broadband X-ray energies onto a compact, thin-foil, secondary metallic target placed at the centre of the ring. This secondary target subsequently emits monochromatic X-rays via fluorescence, with an energy determined by the elemental composition of the compact target. The team describe the design in detail in Medical Physics.
For their validation study, the researchers recorded images of four breast phantoms with thicknesses of 4.1, 4.5, 7.1 and 9.0 cm, using the prototype and a conventional 2D mammography system. The phantoms contained high- and low-contrast masses and microcalcifications, as well as regions of differing breast densities. The team compared image quality as a function of radiation dose using the measured SNR values.
The researchers reported that tissue fibres, microcalcifications and low-contrast lesions were observable in both sets of phantom images. However, the conventional system required 4.5 times the dose for the 1.0 and 0.75 mm thick lesions, and six to eight times the dose for 0.5 to 0.2 mm thick lesions to produce the same SNR as that of the monochromatic system.
“The high SNRs for very thick breast phantoms provide evidence that screening with less breast compression is possible while maintaining high image quality, helping to improve patient comfort,” write the authors. They also report that “contrast-enhanced digital mammography with monochromatic X-rays was shown to provide a simpler and more effective technique at substantially lower radiation dose”.
The technology may potentially reduce unnecessary negative biopsies and avoid the need for expensive follow-up imaging, such as breast MRI and molecular breast imaging.
“Our objective is to replace conventional broadband X-ray tubes used in 2D mammography and 3D DBT with our monochromatic X-ray source,” says Silver. “The same improvements in SNR, detectability, image quality and lower radiation dose that we demonstrated for our 2D measurements apply to 3D DBT as well.”
“The technology we are developing will provide unambiguous results, 85% lower radiation dose, examinations without painful breast compression, and the ability to perform chemical analysis of tissue in vivo.” he adds. “Any medical application that uses a conventional X-ray tube will benefit from using monochromatic radiation. The additional disciplines we are addressing include paediatric, bone, lung, heart, thyroid, prostate and dental imaging.”
Silver tells Physics World that a second-generation monochromatic X-ray tube with at least ten times higher power is currently in development to reduce exposure time, and that automatic replacement of the secondary fluorescence target is a priority. Image Scientific is planning to sponsor a series of clinical studies in leading medical centres. These include a pilot study comparing conventional and monochromatic mammography of women with dense breasts, to be followed by a large, multi-institution clinical study in 2022.
NASA’s Perseverance rover has landed on Mars, completing its seven-month journey to the red planet. The Mars 2020 mission will search for signs of ancient microbial life and collect rock samples that will be returned to Earth later in the decade. Perseverance’s arrival marks the end of a busy February for Mars exploration, with the United Arab Emirates and China successfully delivering Mars orbiters earlier this month.
At 20:55 GMT, mission control at the Jet Propulsion Laboratory in California confirmed that the car-sized rover had touched down in the Jezero Crater – a treacherous landscape pockmarked with boulders and steep cliffs. The craft was autonomously guided to the ground by the Terrain Relative Navigation system, which referenced live photos of the surface against a hazard map generated from Mars orbiters.
“What an amazing day,” says Steve Jurczyk NASA’s acting administrator. “What an amazing team, to work through all the adversity and all the challenges that go with landing a rover on Mars plus the changes of Covid.”
First image of the Martian surface captured by Perseverance (Courtesy: NASA)
A Martian detective
The Jezero Crater, a 45-kilometre-wide basin, was selected because of its potential for holding signs of past life. Geologists believe that around 3.5 billion years ago a river in this region flowed into a large body of water, forming a river delta. This part of the Martian surface also shows signs of volcanic and hydrothermal activity – processes that likely played a role in how life emerged on Earth.
This watery region dried out once Mars’ geomagnetic field died away early in its history, leaving the Martian surface exposed to the solar wind. But what astronomers want to know is whether primitive organisms existed on our planetary neighbour before it turned into the harsh barren world we see today.
“We all have this curiosity about whether or not we are alone, or if there is a potential for life to have existed somewhere else. Being able to find evidence of that would be amazing,” says Kelsey Moore, a geobiologist at NASA’s Jet Propulsion Laboratory.
In an ideal world, astronomers would find an actual fossil of a bacterial cell or a microbial mat – the type of patchy green substance found covering rocks on Earth. But they are more likely to have to make do with chemical clues for life obtained by the rover’s SHERLOC instrument. Scanning the Martian surface with a laser, it will search for organic compounds and build a surface map of rock mineralogies.
The PIXL instrument, meanwhile, will map the chemical composition of rocks and sediments.
Hunting for life: Science instruments on the Perseverance rover (Credit: NASA)
Perseverance also carries a subsurface radar system and 19 cameras. Guided by this imaging array, the rover will collect over 30 rock cores using a drill attached to a robotic arm. These samples will eventually be returned to Earth as part of the NASA/ESA Mars Sample Return campaign, which could launch as soon as 2026.
“If we see something that is really fascinating, we’ll take a pencil-like core, seal it up and place it next to the rover,” says Luther Beegle, SHERLOC’s principal investigator. “The next rover will pick it up and bring it back to Earth where we’ll be able to look for evidence of life in terrestrial laboratories.”
Paving the way for humans
The initial science mission will last one Mars year (about 687 Earth days), though Beegle hopes it can continue doing valuable science for much longer, just like the Curiosity rover which is still operational 10 years since it landed.
The Mars 2020 mission also carried the Ingenuity Mars Helicopter, a 1.8 kg experimental device that might enable future Mars exploration to include an aerial dimension. Ingenuity will attempt up to five test flights within a 30-Martian-day (31-Earth-day) demonstration window.
Another aspect of the mission is to pave the way for human exploration. Perseverance carries materials that could be used in spacesuits to see how they cope in the Martian climate. Its MOXIE instrument, meanwhile, will produce oxygen from Mars’ carbon-dioxide atmosphere, demonstrating a way that future explorers might produce oxygen for rocket propellant as well as for breathing.
The nuclear shell model of the atomic nucleus, more than 70 years old, stays firmly in place now that researchers from CERN’s nuclear physics facility ISOLDE have shown that the series of magic numbers of nucleons does not need an update. However, their result joins a list of contradictory studies of nuclei with around 32 neutrons, which continue to puzzle physicists.
Atomic nuclei are called magic if their nucleon shells – similar to the orbitals of atomic electrons – are completely occupied by protons or neutrons. Magic nuclei are more stable against radioactive decay than their neighbors, even if they live in an exotic, very neutron-rich or proton-rich region of the chart of nuclides. Complete shells correspond to the magic numbers 2, 8, 20, 28, 50, 82 and 126. When both the numbers of protons and neutrons are magic, a nucleus is even more stable – and labeled doubly magic.
In the past two decades several experiments have hinted towards a new magic number, at least for neutrons, at N=32 (N and Z signify the numbers of neutrons and protons respectively in a nucleus). In 2013, while exploring neutron-rich calcium isotopes, the ISOLTRAP mass spectrometer at CERN revealed a sudden drop in the two-neutron separation energy of isotopes beyond N=32, which is an experimental signature for a magic number. Earlier studies of the excitation spectrum of calcium-52, also at ISOLDE, found a higher excitation energy than expected, which also is a signature for a double magic nucleus (Z=20, N=32). Furthermore, researchers from the Radioactive Ion Beam Factory at RIKEN in Japan found similar hints, not only for calcium-52 but more recently also for calcium-54 (N=34).
Charge radius
However, determination of the charge radius – a measure of the nucleus’ size – of potassium-51 and calcium-52 (both having 32 neutrons) did not show any decrease, as would be expected if doubly magic nuclei. An international group of physicists saw this in measurements previously done at CERN’s nuclear physics facility ISOLDE, which produces beams of exotic radioactive particles. Now, the researchers have looked at the very exotic potassium-52 (N=33). The goal was to check for a sudden relative increase in radius, which is another powerful indication for a magic neutron number of 32. Again, a negative result was found.
The new results challenge current nuclear theories. “We don’t refute the outcomes of the earlier experiments, as these were done in the right way and with the best equipment available,” says Thomas Cocolios, a nuclear physicist at the KU Leuven in Belgium and member of the ISOLDE team. “But we do question the claims that those experiments would have showed the existence of a new magic number for neutrons.”
Now the ISOLDE researchers plan to perform similar measurements for calcium-53 and calcium-54, so that they can also check a N=34 magic number claim.
Last year other teams at ISOLDE showed that the established magic numbers are preserved in heavy exotic, extremely short-living nuclei like nickel-78 or tin-132, which are doubly magic and form islands of relative stability. However. in lighter nuclei this is not always the case, like in the hypothetically but non-existing oxygen-28. “But this is an extreme example,” says Cocolios, “with more than twice as many neutrons than protons.”
Sub-shell closing
The observation that while crossing N=32, the energies of the isotopes point towards magic behaviour, but not the charge radius, is something theorists will have to resolve. “They support a sub-shell closing at 32 neutrons,” says Gerda Neyens, a nuclear physicist at the KU Leuven and ISOLDE’s head of physics research. Nuclear sub-shells are analogous to the familiar atomic sub-shells for electrons. “We see a contradiction between the interpretation of experiments that all provide reliable results, and the consistent interpretation of all observables in theoretical models. This is a call for action for the theorists.”
Indeed, the researchers worked together with theorists to analyse the data using state-of-the-art models, finding that the data only challenge these. They report their results in a paper in Nature Physics and lead author Ági Koszorús, formerly at Leuven, comments, “The best models on the market cannot reproduce the data in a satisfactory way”.
According to Neyens, the theoretical models have difficulties because the strong interaction that keeps protons and neutrons together does not act directly on them, but at the sub-nucleon level, on the quarks. Cocolios adds: “This hinders our understanding of atomic nuclei, especially exotic ones. The more we study exotic nuclei, the more we realize that the models have difficulties to reproduce all experimental results in a coherent way”.
Supporting diversity Simone Hyater-Adams (left) and Corey Gray talk about their involvement in the National Mentoring Community. (Courtesy: APS (left) and Corey Gray)
2020 was a year of unexpected changes and challenges. Apart from the impact of the COVID-19 pandemic across the world, issues surrounding marginalized racial or ethnic groups, especially in the US, were brought to the forefront. The significant under-representation of minorities in physics is an issue for the community as a whole. The American Physical Society (APS) has a number of programmes geared towards inclusion, and to increase the recruitment and retention of Black/African American, Latinx, and Indigenous physicists.
For those minority students who have decided on physics as an undergrad – apart from the stresses of a difficult and demanding programme – they are often faced with a number of other barriers including isolation and a lack of representation and community support. With this in mind, the APS National Mentoring Community (NMC) was formed to increase the number of under-represented minority students who complete Bachelor’s degrees in physics.
“Essentially, the NMC was set up to provide mentoring relationships for students from backgrounds that are typically marginalized in physics. Right now, we specifically focus on undergraduate students of colour from the Black, Latinx and Indigenous communities,” says NMC programme manager Simone Hyater-Adams, who is also the APS education and diversity programmes manager. After receiving her BS in physics from Hampton University in the US, Hyater-Adams pursued graduate studies at the ATLAS Institute at the University of Colorado Boulder. Her graduate work included interdisciplinary research examining the connections between performance art and identity for Black physicists. While she was not a part of the NMC as an undergrad, she attended her first meeting as a graduate in 2017, when she was invited to give a talk.
“The idea is that this community can provide undergrad physics students with faculty mentors, hopefully at their local institutions, to support them through their degree,” she says. Mentors can also be from other institutions, from industry, and even other walks of life, as long as they have a background in physics. Mentees are encouraged to have more than one mentor, depending on their particular interests. “A local mentor will know the institution and will be able to provide guidance on how students can navigate in that specific context ,” says Hyater-Adams. “And then potentially other mentors might be able to support students in additional ways – either connect with them culturally, or perhaps they have a career path that these students are interested in. Ultimately, the goal of the programme is to retain and thereby increase the number of under-represented students who successfully complete physics Bachelor’s degrees.”
Alternative aid
While the main goal of the NMC is to set up mentoring relationships, there are also some other key components. An essential one is the Bringing Emergency Aid to Mentees (BEAM) fund, which provides small monetary grants to mentees, to help them with unforeseen expenses that impede their ability to stay in school. BEAM serves as emergency financial assistance that mentees can apply for. “While there is a cap of around $1500 that they can apply for from the fund, a real benefit is how rapidly they can get some extra help,” explains Hyater-Adams.
“Applications undergo a very quick review, where we typically just ask ‘Are you a mentee? Do you have a mentor, and are they aware of this issue? Does this seem reasonable?’ Once approved, there is a very quick turnaround because it’s an emergency fund. Sometimes we have paid for tuition while in some other cases, mentees are in a situation where they do not have the resources to live off at that time,” she adds. Expenses cover many areas including food, medical costs, transportation, childcare and more.
Yearly meetings
Another key component of the NMC is its annual conference, which is organized in collaboration with the National Society for Black Physicists and the National Society for Hispanic Physicists. According to Hyater-Adams, the conference benefits the largest number of members, but she adds that “there’s many students who come to the conference who aren’t members of NMC, but then sign up after”. Each year, for three to four days, mentors and mentees gather for talks, panel discussions, workshops, careers fairs and visits to local institutions. The main purpose of the conference is to build and foster the community as a whole; allowing not only mentors and mentees to meet in an informal setting; but also, for students to meet peers from institutions across the US.
The 2020 conference, which took place in February at the University of Central Florida in Orlando, involved some 140 attendees. “Undergraduate-focused conferences are much needed – there’s opportunities for students to present as well as participate in sessions,” says Hyater-Adams. “For example, we offer training for mentors, including best practices on how to best support students. But the conferences also include graduate-focused offerings such as career workshops, industry talks or networking fairs, which we had at the last two conferences.”
The first plenary session of the 2020 conference was given by Laser Interferometer Gravitational-Wave Observatory (LIGO) physicist Corey Gray, who is a member of the Blackfoot tribe and the Siksika nation from southern Alberta, Canada. His talk, “A wrinkle in space–time: connecting gravitational waves and Albert Einstein with Blackfoot culture”, was a conference highlight for many.
“I’ve been involved with the NMC for a while now, so when they approached me to be a keynote speaker, I was delighted,” says Gray. “This was back in February 2020, before any of the lockdowns – I was there for two nights, and even got to visit the Kennedy Space Center as part of the conference.” The best part though, for Gray, was meeting all the other attendees. “I got to meet so many undergrads and had the chance to speak to many of them after my talk. Now, we’re friends on Instagram and Facebook. I also met other professionals and scientists like me… It’s cool when you get to network and meet people. I was really so honoured and appreciative to have that opportunity,” he adds.
“I think the students especially love the conference, because they are looking to build their community. There’s a lot of isolation with students of colour in physics, and the conference really shows them that they aren’t alone,” says Hyater-Adams. This sentiment is echoed by NMC mentee Alexander Vasquez, a physics student at Texas State University. He told APS News that the meeting “is the most valuable asset in the NMC in my opinion – I get to see other minority physics majors and know that I’m not alone”. His mentor, Texas State University physicist Alice Olmstead, agreed, adding that the conference is “so rich and has so many resources for my students to make connections that I can’t provide myself”.
Unsurprisingly, the 2021 NMC Conference will be held virtually this year, from February 18 to 21. Apart from all the usual offerings, the conference committee is encouraging more student-organized community-building sessions, as reported by APS News. According to Hyater-Adams, “these could be things like a virtual game night, a hobby chat, a murder mystery, or any other topic that you think will be beneficial for conference goers”.
Digital connections
As much of the world moved to a more virtual existence last year, plans were already under way for the NMC to create a Slack channel to facilitate more peer-mentoring among the undergrads. “The thing that I don’t think many people have considered as much when it comes to the structuring of this programme is the power dynamic. As an undergrad, reaching out and talking to faculty can be intimidating. In some cases, it may be easier for students to reach out to peers for advice – and perhaps that student might be able to foster a faculty connection,” says Hyater-Adams. The new NMC Slack workspace was set up at the end of last year, and is designed as a member resource hub, as well as a platform to host online events including the conference.
Today, the NMC is ramping up its recruitment for the programme, to get more mentors and mentees. “Part of that will be getting more pairs successfully matched, but also creating more structure for the programme, especially with our Slack workspace in place,” says Hyater-Adams. According to her, the NMC’s best success stories are those where mentees have felt truly championed by their mentors. “The most impactful mentoring relationships are those where a mentor will truly advocate for the mentee – they become that person who will look out for them, who believe in them, all the while providing them with the resources to succeed.”
In this episode of the Physics World Weekly podcast, we meet Hannah Coleman, Ryan Hill and Matt Brookes of the UK’s University of Nottingham, who talk about a new way of scanning the brain using quantum devices called optically pumped magnetometers. A key feature of the technique is that it allows magneto-encephalography to be used to study the brains of children, which had not been possible using other technologies.
We also hear from Adam Soule, an undersea expert at the Woods Hole Oceanographic Institution in the US. Soule talks to Physics World’s James Dacey about doing science in the Alvin submersible vehicle, which is currently be refurbished to allow it to reach the astonishing depth of 6.5 km.
Finally, my colleague Margaret Harris joins me for a chat about some of the unexpected consequences of the recent cold snap in Texas.
Space, it seems, is no longer the final frontier that it used to be. The emergence of small satellites – broadly, instruments with a mass ranging from 1 to 500 kg – has, in large part, levelled the playing field in the space industry over the past two decades. Agile start-up companies, established manufacturers and even university research groups are all now in a position to compete with the big-budget missions of government space agencies – opening up commercial and scientific opportunities in applications as diverse as remote sensing, environmental protection, asset tracking and logistics, and machine-to-machine communication for the “Internet of Things”.
The upward trajectory is clear to see: the evolution of small-satellite technologies will continue apace, squeezing more and more functionality into ever-decreasing payloads while further lowering the barriers to entry for new-entrants to the space industry. All of which translates into relentless downward pressure on the capital/operational spend of satellite developers and their engineering teams – not least when it comes to the exacting test programmes needed to qualify satellite systems for launch and, ultimately, long-term operation in orbit.
Vacuum versatility
With this in mind, US start-up Rydberg Vacuum Sciences (RVS) is busy establishing itself as a “go-to” equipment provider in the emerging test-and-measurement ecosystem serving the small-satellite community. More precisely, RVS is targeting a specialist niche in the preflight qualification workflow for small satellites and their constituent systems: the provision of affordable, off-the-shelf thermal vacuum bake-out and thermal vacuum cycling products.
“I see RVS as a direct response to the democratization of the satellite launch industry,” explains Joshua Gurian, founder and president of the Seattle-based test-and-measurement specialist. “Right now, we’re seeing more orders from private-sector entrants to the space industry, though it’s worth noting that the long-term goal is also to make our ‘drop-in-place’ test solutions accessible to burgeoning small-satellite R&D initiatives within North American universities and further afield.”
That twin-track approach is already evident. Last year, for example, RVS supplied two thermal vacuum test systems to AST&Science, which is developing a space-based cellular broadband network (SpaceMobile) to provide 4G/5G connectivity to smartphones anywhere on the planet. “We’ve shipped to AST&Science facilities in Texas and Israel, where they’re testing fold-out solar panels for their SpaceMobile satellite constellation,” says Gurian. “Another three test systems are on their way to the Space Dynamics Laboratory at Utah State University, which is looking to increase its small-satellite testing capacity for both in-house and for-hire projects.”
Passing the test
Joshua Gurian: “I see RVS as a direct response to the democratization of the satellite launch industry”. (Courtesy: RVS)
For satellite developers big and small, there are no short-cuts into orbit. Consider the thermal vacuum test programme for any small-satellite project: it’s an exhaustive undertaking that requires granular evaluation at the component, subsystem and system level. A thermal vacuum cycling test, for example, will see the craft’s hardware and instrumentation put through its paces and subjected to a “step-and-repeat” programme of extreme hot and cold temperatures in a high-vacuum environment, while a thermal balance test aims to demonstrate the effectiveness of the craft’s thermal control systems for maintaining the temperature of key systems within predefined limits. There’s also a vacuum bake-out requirement, in which the satellite hardware is heated to high temperature under high vacuum to quantify levels of material outgassing (the products of which can adversely affect the performance of on-board imaging systems, thermal radiators, solar cells and the like).
“Although the detail of the vacuum test programme is generally dictated by the satellite launch provider,” notes Gurian, “we have a lot of technical domain knowledge here at RVS to support our research and industry customers.” Equally, the RVS emphasis on off-the-shelf vacuum systems provides thermal testing at a palatable price-point for any developer seeking to launch inexpensive small satellites. “Ease-of-use is paramount,” Gurian adds. “With a footprint of just 0.6×1.2 m, installing an RVS thermal vacuum system is as simple as unpacking the crate and connecting the utilities.”
Modelling vs real-world measurement
As part of the prelaunch test programme, a satellite developer will typically generate a model of the temperature extremes the craft is likely to experience once it’s in orbit and traversing from day to night on the dark side of the Earth. Trouble is, many satellite subsystems – for example, battery packs and on-board cameras – are not optimized to handle the environmental extremes encountered in orbit. As such, thermal vacuum testing is essential to validate the modelling and to ensure that any localized heating/cooling units are having the desired effect.
A typical thermal vacuum cycling test might look something like this: an engineer first pumps the test chamber down to high vacuum (say 10-6 mbar) before taking the unit under test (UUT) up to Tmax – ramping at roughly 3 °C/min to 100 °C, for example. After which the UUT will undergo a “soak” for typically 4 h (but anywhere from 1–24 h) at Tmax, before cycling down for another extended soak at Tmin (at –100 °C), before a gradual ramp again to Tmax. “The whole step-and-repeat programme is often run more than 10 times over a period of several days, after which the UUT is brought back to room temperature to make sure that everything is still working to specification,” adds Gurian.
For RVS, the task is to provide the vacuum infrastructure to support this test-and-measurement workflow, helping customers to ensure that their small-satellite components/subsystems are fit-for-purpose and guaranteed for long-term survivability in orbit. “The thermal test regime generates lots of data – there are thermocouples slapped all over the UUT,” concludes Gurian. “Those data allow the user to compare the actual thermal performance of the UUT versus the modelled behaviour and to make mission-critical design adjustments ahead of launch.”
The RVS line of small-satellite test systems provides a “drop-in-place” solution for compliance with GSFC-STD-7000 or MIL-STD-1540 test standards. Key specifications include…
Operational performance: atmospheric pressure to high vacuum in <30 min; temperature range –150 °C to +150 °C; controllable ramp rate up to 5 °C/min
A 6U vacuum test volume (370×240×120 mm)
Turbomolecular pump (300 l/s) backed by a frame-integrated dry Roots pump
Temperature-controlled platen with 50×50 mm M6 grid for UUT fixturing and integrated thermal radiation shielding
Two blank ISO-100LF user ports for pass-through of electrical/instrumentation cabling and gas lines as required
Optional accessories include: residual gas analyser (100–300 amu); optical witness sample holder; and temperature-controlled quartz-crystal microbalance.
Standard vacuum test systems ship in 8–10 weeks, with rental options also available for customers requiring a short-term testing capability.
MRI-guided radiotherapy (MRIgRT) systems have the capacity to acquire functional, quantitative images in addition to the anatomical images required for online treatment guidance. This creates the potential to bring two important concepts in modern radiotherapy together: adaptive radiotherapy and biological targeting. Based on frequent anatomical and functional imaging, monitoring the changes that occur in volume, shape as well as biological characteristics, a treatment plan can be updated regularly to accommodate the observed treatment response. For this purpose, quantitative imaging biomarkers (QIB) need to be identified that show changes early during treatment and predict treatment outcome.
The first pilot studies have shown that QIB measurements are feasible on MRIgRT systems. However, the MR parts of these systems differ from regular diagnostic systems. This impacts the performance of QIB measurements and warrants technical validation. To ensure that the results of QIB studies on MRIgRT systems are also valid for diagnostic platforms outside the MRIgRT domain, QIB trials should be designed to establish reproducibility between systems. To identify if changes observed during the course of treatment are significant, the trials should include test-retest acquisition of the QIB prior to the first irradiation.
Within the Elekta MR-Linac Consortium, a working group on MRI biomarkers for response assessment is active in developing trial strategies, acquisition and analysis methods to make QIB research on Elekta Unity possible.
In this webinar, hosted by Prof. Uulke A van der Heide, an overview of the activities within the working group will be presented.
Uulke van der Heide received his training as medical physicist at the department of radiotherapy of the University Medical Center in Utrecht, the Netherlands, and worked there as a medical physicist until 2011. Since then, he has worked as a medical physicist and senior group leader at the Netherlands Cancer Institute in Amsterdam, the Netherlands. He holds a chair as professor of imaging in radiotherapy at the Leiden University Medical Center.
His research group works on the improvement of target definition in radiotherapy by application of MRI and the development and validation of quantitative imaging methods for tumour characterization for radiotherapy dose painting. He further leads the MR-guided radiotherapy programme at the Netherlands Cancer Institute.
Uulke van der Heide received his training as medical physicist at the department of radiotherapy of the University Medical Center in Utrecht, the Netherlands, and worked there as a medical physicist until 2011. Since then, he has worked as a medical physicist and senior group leader at the Netherlands Cancer Institute in Amsterdam, the Netherlands. He holds a chair as professor of imaging in radiotherapy at the Leiden University Medical Center.