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Wei Yang on the future of physics in China

Wei Yang of the National Natural Science Foundation of China

What are the main aims of the National Natural Science Foundation of China (NSFC)?

The NSFC was set up 30 years ago in 1986 after being proposed by a group of scientists led by the Nobel-prize-winning physicist Tsung-dao Lee. They told the then Chinese leader Deng Xiaoping that the US has its own National Science Foundation and China should have something similar. He agreed.

How big is your budget?

It’s increased 300-fold since the NSFC was founded. Back then it was about ¥80m ($12m) annually. Now it’s about ¥24.8bn per year.

What areas does the NSFC fund?

We support all the main branches of natural science including mathematics, physics, chemistry, biosciences, earth science, engineering and materials, IT and medicine. We also support some data-driven social and management science too.

How much money does physics get?

We have two main budget lines. Physics I is mainly condensed-matter physics, while Physics II is particle physics, theoretical physics and astronomy. Altogether, they get more than ¥1bn a year.

How many researchers does the NSFC support?

We hand out about 40,000 new research grants each year, which together support about 150,000 people when you take into account students, postdocs and research assistants too. The success rate for those applying for funding is about 22–25%, which is okay. I think a quarter is the golden ratio – neither too high nor too low.

You were appointed president of the NSFC in 2013 – what have been your main achievements during that time?

I have secured a total budget increase of 50% during my three-year tenure. And as well as paying for researchers’ “direct” costs, the NSFC now also funds their “indirect” costs, such as the money for lab space, infrastructure and so on to the hosting institutions. Previously that money went to institutions as a lump sum and they’d charge scientists a certain percentage as a management fee. I’ve also changed the regulations so that someone applying for a grant can support however many graduate students, postdocs and so on that an individual researcher needs. There’s no upper limit on how many they can request.

What are your main challenges as NSFC boss?

I’ve just written an article in Nature saying the importance of raising the quality, integrity and applicability of Chinese science (534 467). In the article, I describe how the NSFC’s mission is to be a “FRIEND” of scientists: fair in reviews; rewarding in fostering research; international in global participation; efficient in management; numerous in grants; and diversified in disciplinary coverage. I also want to get more “monumental” contributions to different branches of science, not researchers just doing more of the same.

How do you evaluate whether grant money has been well spent?

Every year we have an external evaluation where independent experts check a certain percentage of grants in our eight main areas. We don’t monitor every single grant though. We also don’t evaluate the performance of individual researchers funded by the NSFC as we feel that would make them conservative and suppress their creativity.

So how do you measure success?

Publication records are one factor, of course, though we think quality is more important than the sheer number of papers produced. We also survey researchers to find out if they were satisfied with the performance of the NSFC – and that includes asking scientists who failed to receive grants. What’s interesting is that 20 years ago, when you look at the top 0.1% most cited papers, Chinese researchers accounted for less than 0.5% of those publications. Now they contribute a fifth of those articles.

What about tackling fraud and misconduct?

That’s important, yes. I want to reduce cases of misconduct, which have gone up a bit recently, and raise the overall reputation of Chinese research work.

What’s your view on open access?

Chinese researchers can publish in any journals – they don’t have to be open-access journals. However, the official policy of the NSFC is to support green open access, which means that scientists have to place a copy of their final paper in our own NSFC electronic repository 12 months after it’s been published in a peer-reviewed scientific journal. Having said that, China published 45,000 papers in open-access journals last year, which is 21% of the world’s total and exceeds the amount from the US.

Do you follow developments in physics?

It’s been very exciting to see the Laser Interferometer Gravitational-Wave Observatory detect gravitational waves and we are planning several initiatives of our own in China in this area. We’re also building the China Jingping Underground Laboratory in south-western China and we’ve got our satellite programme to search for dark matter and carry out space-to-Earth quantum communication.

Take a swing

When the amateur golfer Bryson DeChambeau shot a five-over-par 72 at the US Masters in April this year, his score – good enough to tie for 21st place – wasn’t the only thing that attracted the media’s attention. DeChambeau, it transpired, is a physics graduate who took the unusual step of cutting all of his irons and wedges to the same length, so that he doesn’t have to adjust the plane of his swing when he changes clubs (see “Physics at the Masters”, May p3). Most golfing physicists are not so dedicated (and few, if any, are as talented – DeChambeau has since turned professional and currently ranks in the top 150 in the world), but those with a serious interest in the science of their sport will definitely want to get their gloved hands on The Science of the Perfect Swing.

In the book’s introduction, author Peter Dewhurst notes that “the general theory of impact, the science of flight, and the mechanics of motion…are among the most fascinating of the physical sciences” and they are also, of course, integral to the game of golf. Dewhurst is an emeritus professor of theoretical and applied mechanics at the University of Rhode Island, US, and his book goes into an impressive amount of detail on nearly every aspect of golf, from the ridiculousness of “low friction” tees (which, he notes, “magically add 80 pounds” to a maximum impact force of nearly 3000 pounds) to the benefits of the high-performance drivers introduced in the mid-2000s.

Most of the book is written at the level of a beginning undergraduate mechanics course, but each chapter also contains a lengthy section on the “supporting physics”, which reads more like a scientific review article. Whether it actually moves you closer to a “perfect swing” is an exercise best left to the reader, but there is, at least, some support in the book for DeChambeau’s single-length clubs. For a player “on Tour”, Dewhurst writes, “the major requirement is not ultra-long hitting, so it can only be consistency of ball striking”.

  • 2016 Oxford University Press £22.99/$35.00hb 288pp

In harm’s way

Photo of the 1980 eruption of Mount St Helens volcano, showing a towering cloud of ash emerging from the top of the peak

Seconds before a cloud of dust and ash swept his observation post off the map, the American volcanologist David Johnston managed to send one last radio message: “Vancouver! Vancouver! This is it!” “It” was the devastating eruption of Mount St Helens on 18 May 1980, which laid waste to hundreds of square kilometres around the once-picturesque peak, scattered ash across 11 US states, and killed almost 60 people, Johnston included. The many factors – scientific, political and personal – that combined to put them in danger are the subject of Steve Olson’s book Eruption.

The book gets off to a slow start, with a long section devoted to the Weyerhaeuser timber company. The connection is that Weyerhaeuser owned much of the land around the volcano, and its grip on the local economy and politics (plus its desire not to interrupt clear-cutting operations over something so trivial as an active volcano) meant that the exclusion zone set up around the mountain was smaller than the scientists would have liked. But Olson’s intense focus on Weyerhaeuser (which includes a lengthy digression on its mid-19th century founding) and its battles with conservationists leaves correspondingly less space in the book for the science of the Mount St Helens eruption, and for the stories of the individual human beings caught up in it.

This is too bad, because Olson is a gifted science communicator, and he also makes the most of his source material later in the book when writing about the narrow escapes of several survivors. In one especially harrowing passage, Olson describes how two photographers drove at 100 mph down narrow, winding roads to outrun the blast, passing a slower car on a blind bend some two miles outside the supposed danger zone. The photographers survived. The occupants of the slower car did not.

  • 2016 W W Norton £17.99/$27.95hb 320pp

The September 2016 issue of Physics World is now out

The cover story in the September 2016 issue of Physics World magazine – now live in the Physics World app for mobile and desktop – reveals the fascinating new field of “crowd breath research”, which can even shed light on how cinema audiences react during the changing scenes in a movie. You can read the article here on physicsworld.com too.

The September issue also shows how to do crystallography without crystals, explains how first data from the Gaia spacecraft could revolutionize astronomy (see the above video for more on that), and contains one physics teacher’s fascinating story about what she did to change her school’s gender balance.

Don’t miss either reader feedback on the potential impact of Britain leaving the EU on physics or Robert P Crease’s Critical Point column on why science denial is one of the most important issues in the US presidential campaign.

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Every breath we take

Back in Christmas 2013, the CineStar cinema in Mainz, Germany, became an impromptu, oversized laboratory. Over the course of 108 screenings of 16 films, it hosted an unprecedented experiment on about 9500 moviegoers. Not that most of them noticed, or even knew they were under scrutiny. Science was likely the last thing on their brains as they flocked to the cinema to see the German hit Buddy or blockbusters such as The Hunger Games: Catching Fire and The Hobbit: the Desolation of Smaug.

But Jonathan Williams, an atmospheric chemist at the Max Planck Institute for Chemistry, whose research has taken him around the world, went to his local cinema in search of a story that wasn’t being shown on a screen. He was looking for a story told by the breath of a crowd. He chose the screening room of a cinema because it’s well contained. “It’s really just a box full of people,” he says.

Breath contains valuable information, if one can figure out how to decode it. When excited, we emit more carbon dioxide. After a swig of beer, we exhale ethanol in proportion to the amount in our blood. Our breath reveals if we’ve recently eaten an apple or smoked a cigarette. A human breath contains on average more than 200 easily measured volatile organic compounds (VOCs) – chemicals that exist in a gaseous state at room temperature. Most of those are inhaled initially, but many are generated by living cells and metabolic processes in the body. Not every breath is identical: researchers have identified thousands of individual chemicals that fluctuate depending on where people are, what they’re doing, and how their bodies work. A VOC may be innocuous or harmful; natural or synthesized.

“The breath is basically garbage,” says Joachim Pleil, an analytical chemist with the US Environmental Protection Agency at Research Triangle Park in North Carolina, US, and editor-in-chief of the Journal of Breath Research. “You breathe it out, you ignore it.”

A person’s breath may reveal truths they prefer to keep secret – like how many drinks they’ve consumed. In medicine, researchers are also investigating breath’s chemical signatures as potential biomarkers for diseases or ways to gauge a person’s health. Pleil points out that doctors have been using breath analysis for a long time: about 2400 years ago the Greek physician Hippocrates described foetor hepaticus or “the breath of the dead” – now understood to be a late sign of liver failure.

“Traditionally, breath research has focused on one person, and one breath,” says Pleil. “The hope has been to say something about an individual based on what they’re breathing out.”

Williams’ work is a departure from that model. At the CineStar, Williams wasn’t interested in individual-level data. He sought meaning through the large-scale analyses of the breath of large groups. In a recent Journal of Breath Research editorial he co-authored with Pleil, the scientists call their method “crowd-based breath analysis” (2016 J. Breath. Res. 10 032001). The researchers say the method could be useful in many fields, from helping advertisers gauge an audience’s emotional response to a new product, to differentiating between healthy and unhealthy VOC profiles, to identifying people who may pose a threat of some kind. “There is huge potential for discovery within crowd breath research,” they wrote.

Watching the watchers

Like other theatres, CineStar in Mainz uses a ventilation system that pumps fresh air in through the floor and out through ceiling vents. Williams and his crew installed two devices in the outgoing ceiling ducts: an infrared gas analyser, which measured the airborne concentration of carbon dioxide (figure 1), and a proton transfer reaction time-of-flight mass spectrometer, which measured the traces of more than 100 other gases (see “The science behind crowd-based breath analysis”, below). The scientists collected real-time measurements of VOC levels every 30 seconds of a film as audiences laughed, gasped and were startled. Afterwards, they aligned individual measurements with a description of the film’s plot, broken down into 30 s chunks (2016 Scientific Reports 6 25464 ).

(a) Graph CO2 (ppm) as a function of time. The CO2 axis ranges from 400-1800 and the time from around midday on 26 December 2013 till the evening of 30 December 2013. A spikey peak is centred at approximately 8 pm each day. Each peak begins with a sharp step up, followed by dramatic spikes nearly the height of the graph, ending with a gradual tail off. (b) Same axes except the time only spans from midday on 27 December 2013 to 3 am on 28 December 2013. Here four much less jagged peaks can be seen, in turn. Each is labelled with a film, and a number to indicate the number of people in the audience: The Hunger Games 2, 96; Dinosaur 3D, 44; Buddy, 124; and Buddy, 53. The height of each peak scaled approximately with the number of people. (c) Same axes except the time only spans from midday to 5 pm on 28 December. From 1 pm, the CO2 level rises from 400 ppm up to about 900 ppm when the film (The Hunger Games 2) begins, with an audience of 104. The level continues to rise to about 1050, where it remains till the end of the film at 4pm. The CO2 level then drops to about 650 ppm by 4:45 pm. The line is not smooth –it has small jagged detail on it, fluctuating by about 30 ppm

Molecules associated with popcorn and fizzy drinks didn’t change throughout the movie. Predictably, the researchers found that carbon-dioxide levels rose and fell as audiences filled and emptied the screening rooms, respectively. So did levels of acetone and isoprene, two common by-products of metabolism. (Acetone is a by-product of fat catabolism, and isoprene is exhaled as the body makes cholesterol.) The scientists also observed that the VOC levels didn’t follow smooth curves; they were punctuated with small peaks.

Williams suspected those peaks revealed something about how people reacted to the movie. Following that hunch, he and his team identified scenes connected to these VOC peaks – such as when Katniss’ dress ignites or the final battle begins in The Hunger Games: Catching Fire. The same peaks appeared at every screening, every day, as though during those times all the audiences were breathing in synchrony (figure 2). That repetition of the pattern gave Williams confidence that the connection they were seeing was both substantial and reproducible.

Four stacked graphs, with local time along the bottom axis ranging from 1 pm to 4:30 pm. Three vertical axes show CO2 (ppm) from 400 to 1600, acetone (ppb) from 3 to 14 and isoprene (ppb) from 1 to 8. Each graph corresponds to a showing of The Hunger Games 2. Each curve is approximately the same shape, though scaled to different sizes. Curve shape and level of jagged detail is as described in figure 1 (c). Two vertical red lines, intersecting all four films, indicate the two most significant peaks within this jagged detail

Williams and his team then set out to see if the relationship between movie scenes and VOC emissions was causal. They annotated each 30 s interval of the films with descriptive labels that identified the genre or action of the scene. (“Comedy” or “chase”, for example.) Then, using the Mogon supercomputer in Mainz, they created a model based on two-thirds of the data that connected scene descriptions to VOC levels. For the remaining third of the data, they fed the VOC levels into their model to see if they would successfully predict scene descriptions and so prove a causal relationship. They found that VOC levels most successfully predicted scenes described as “suspense” or “comedy”. Scenes labelled “chase” and “romance”, on the other hand, weren’t significantly linked to VOCs.

Norman Ratcliffe, who has spent more than two decades analysing volatiles in gas, urine, faeces and blood at the University of the West of England in Bristol, UK, thinks Williams’ crowd-based methods have the potential to help interpret what breath VOCs can tell us. “It sounds like a very good approach,” he says. And it’s efficient, to boot: “You get the responses of hundreds of people in just one measurement.”

Into the real world

The vast majority of VOCs in the atmosphere are produced by vegetation, so Williams’ research typically takes him to verdant locales such as the Amazon rainforest or boreal forest in Finland. He’s studied pollution in Beijing, China, and later this year he’ll begin studying oil industry pollution and emissions in the Persian Gulf. The cinema project, he says, was borne of a natural question: how does human breathing affect the chemical composition of the atmosphere?

As it turns out, it doesn’t. “The amount [of VOCs] we emit as human beings is actually a very small amount,” he says. However, the question had led him to wonder if he could find some way to gauge human contributions. In April 2012 Williams’ team had used a mass spectrometer to measure VOCs during a football match at the Coface Arena in Mainz. Hoping to see a surge in carbon dioxide after a goal, the scientists had been disappointed when their data didn’t deliver. That project led Williams to think about running a similar experiment in a smaller space – like a cinema.

The new findings, as a proof of concept, suggest VOCs may be used to gauge human emotion, though the field is still in its early days. In addition to marketing, that idea may influence other fields. Pleil, who had been working on a series of papers about cellular respiration when he first met Williams, sees possibilities in health and threat assessment. Crowd breath analysis could help scientists describe a baseline VOC profile, in order to be able to use breath to identify individuals exposed to harmful substances. In health care, a person with a toxic VOC exposure might get treatment before symptoms begin. In security, a person queuing at an airport with jet fuel VOCs on their breath might be detained for questioning. (Do they work at an airport, or have they just built a dirty bomb?)

“This could be a valuable resource for trying to deduce what people think without giving them the opportunity to lie about it,” says Pleil.

Although Williams is soon heading to the Middle East, his work with VOCs and films already has a sequel: he’s currently sitting down with data collected during screenings of Star Wars: the Force Awakens. May the breath be with him.

The science behind crowd-based breath analysis

The wisdom of the crowds may be in our breath: recent research at Jonathan Williams’ lab at the Max Planck Institute for Chemistry in Mainz, Germany, shows a new way to study volatile organic compounds, or VOCs, generated by crowds in a cinema.

Joachim Pleil, at the US Environmental Protection Agency, says researchers can use two kinds of analysis for studying gas composition: offline and real-time. With offline analysis techniques, scientists have to collect a sample and take it to a lab. Real-time analysis happens as the sample is being created. “What Jonathan is doing probably would be difficult, if not impossible to do, with offline analysis,” he says. “The value of crowd breath is only apparent and can only be realized if you have online analysis.”

Ventilation pipes on the outside of a building

To measure carbon dioxide, the scientists used infrared spectroscopy, which beams infrared light through a sample. The carbon-dioxide molecules absorb this light at frequencies corresponding to their vibrational modes, so the difference between the initial and final infrared light translates to a measurement of the amount of carbon dioxide.

For the VOCs, Williams and his crew needed something more sophisticated to measure hundreds of VOCs every 30 seconds. That meant collecting high-resolution data in real time. There are many different tools for that purpose, but they selected proton transfer reaction time-of-flight mass spectrometry (PTR-MS), a real-time technology that was first developed in the 1990s by physicists at Innsbruck University in Austria. PTR-MS can measure even minuscule traces of a suite of airborne VOCs.

The tool first creates ions by attaching extra protons to molecules of ordinary water. Then it sends the ionized water vapour through a sample of air. When the ions collide with ordinary atmospheric ingredients such as nitrogen or oxygen, nothing happens. But when they collide with VOC molecules, the proton attaches itself to the VOC. That’s because most VOCs have a higher proton affinity than water, and gases such as nitrogen and oxygen have a lower proton affinity than water. With the protons attached, the tagged VOCs can then be measured in real time by a mass analyser, which identifies the individual varieties of VOC. “We use this method widely, and it measures fast,” says Williams.

How to use a mountain to detect neutrinos

Aiming high: Zhen Cao explains how to use a mountain to detect tau neutrinos

By Hamish Johnston in Beijing

This evening I had dinner with Zhen Cao, who is one of China’s leading particle astrophysicists and works at the Institute of High Energy Physics of the Chinese Academy of Sciences here in Beijing.

Cao has found a great way to combine his passion for mountains and neutrinos: the Cosmic Ray Tau Neutrino Telescope (CRTNT), which, if built, will use an entire mountain in western China as a cosmic neutrino detector.

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US board gives student assistants unionization rights

The United States National Labor Relations Board (NLRB) ruled last week that graduate students in private universities and colleges, who work as teaching or research assistants, are statutory employees of their institutions who have the right to join unions. The decision, made in response to a plea by graduate students at Columbia University, overturns a 2004 decision that denied the students union rights. Groups of student assistants have already reacted to the decision by filing for certification of local unions to represent them.

Tremendous victory

“Graduate employees deserve a seat at the table and a voice in higher education. Collective bargaining can provide that,” says Howard Bunsis, who chairs the American Association of University Professors’ Collective Bargaining Congress. “This is a tremendous victory for student workers.” Not surprisingly, representatives of private universities disagree. “We are disappointed that [the decision] has overruled years of precedent finding that graduate students are not employees for unionization purposes,” says Stanford University spokesman Brad Hayward.

The issue before the board focused on the relevance of the work that student teaching assistants carry out to their overall education. Students argued that their teaching duties are independent of, and can actually detract from, their research. “I took a lot of my time preparing lectures,” Mickey McDonald, a Columbia physicist who has just defended his doctoral research on ultracold molecules, told physicsworld.com. “And grading undergraduates’ lab reports can take up to 15 hours per week.” The ability to join unions, students added, will allow them to negotiate liveable stipends and working hours. They also pointed out that teaching assistants at state universities can already unionize, because they are protected by local state laws, and that the private New York University voluntarily unionized in 2013.

Influencing issues

Columbia University authorities countered that teaching assistantships give graduate students the skills and expertise they will need in future careers as researchers and teachers. Participation in collective bargaining, they added, could destroy the traditional mentor–student relationship. Indeed, they raised the possibility that student-assistants’ unions could influence issues beyond students’ economic situations – by trying to negotiate class sizes taught by teaching assistants, for example, or the details of examinations they mark. Prominent research universities such as Harvard, MIT and Princeton supported the Columbia arguments in “friends-of-the-court” briefs.

Graduate employees deserve a seat at the table and a voice in higher education. Collective bargaining can provide that

Howard Bunsis, chair, American Association of University Professors' Collective Bargaining Congress

In its 2004 decision on a case brought by Brown University student assistants, the NLRB largely agreed with those arguments. The board rejected the idea that student assistants could be considered employees of their universities because they “are primarily students and have a primarily educational, not economic, relationship with their university”. Last week’s decision rejected that thinking by a three-to-one majority. The 2004 decision, the board commented, had “deprived an entire category of workers of the protections of the National Labor Relations Act without a convincing justification”.

Pros and cons

Krista Freeman, a graduate student in physics at Carnegie Mellon University, who chairs the American Physical Society’s Forum on Graduate Student Affairs, welcomes the decision. “Many aspects of graduate student life are unsavoury and uncertain, and collective bargaining power could go a long way to correcting these issues,” she says. “This can only lead to healthier, happier and more financially stable students.”

Universities remain unconvinced. In a letter to the Columbia University community following last week’s decision, provost John Coatsworth speaks of the potential benefits and drawbacks of having student assistants’ interests represented by the United Auto Workers (which now focuses on employees beyond the car industry). “I am concerned about the impact of having a non-academic third party involved in the highly individualized and varied contexts in which faculty teach and train students in their departments, classrooms and laboratories,” he writes. Harvard University agrees. “We continue to believe that the relationship between students and the university is primarily about education, and that unionization will disrupt academic programmes and freedoms, mentoring and research at Harvard,” an official statement notes.

Nevertheless, the move to unionize has already started. On Monday, graduate students in 10 Yale University departments, including physics, geology and geophysics, and mathematics, filed a petition to the NLRB requesting certification of a local union to represent them.

Why use silicon qubits for quantum computing?

Computers based on quantum processes have the potential to be exponentially more powerful than today’s computers. At present, research groups across the world are exploring various different approaches to creating quantum computers – a difficult technological challenge given the delicate nature of quantum systems. In this video, Andrea Morello explains the approach taken by his group at the University of New South Wales in Australia, which is inspired by classical computing. It involves encoding data into the spins of phosphorous atoms embedded within silicon microchips.

This video is part of our 100 Second Science series, in which researchers give concise presentations covering the spectrum of physics.

Seismic ‘weather bomb’ lights up Earth’s interior

A powerful extratropical cyclone east of Japan in January 2013

A new type of rare deep-Earth tremor, created by fast-developing ocean storms, has been detected by researchers from Japan. The signals from this kind of faint Earth tremor – known as an “S-wave microseism” – may provide geophysicists with a new tool to study not only oceanic storms but also the Earth’s interior.

First observed in the 1940s, microseisms are faint Earth tremors generated by the sloshing of ocean waves on the sea floor during storm events. The strongest microseisms are generated by the interaction of directly opposing wave systems. These create pressure excitations that travel almost unattenuated to the sea floor because of the nonlinear effects of the fluid – unlike with normal ocean surface waves, which decay with depth.

Seismic signals

Microseisms – which are observed globally – may either travel across the surface of the Earth, or through its interior as body waves. Like the seismic waves generated by earthquakes, these body waves may either be compressional (P-waves) or transverse (S-waves) – although until now, because of their larger amplitude, only the former had been observed – and, unlike surface-wave microseisms, can be tracked back to their point of origin.

In their study, Kiwamu Nishida of the University of Tokyo and Ryota Takagi of Tohoku University looked at a special kind of small, fast-developing extra-tropical cyclone colloquial dubbed a “weather bomb”. Seismic signals from one of these storm events – which developed in the North Atlantic between Iceland and Greenland in the December of 2014 – were recorded on the Japanese High Sensitivity Seismograph Network. The researchers found signals not only of P-wave but also S-wave microseisms, both in vertically (SV) and horizontally (SH) polarized forms. While modelling had only predicted the creation of SV waves, the researchers believe that the SH waves may be generated by the repeated reverberation of shear waves in poorly layered shallow sediments on the ocean floor.

The discovery of S-wave microseisms may offer a new way of understanding the nature of these couplings between the atmosphere and deep Earth. “The energy ratio between P- and S-wave microseisms is crucial for inferring the excitation mechanism,” says Nishida. For example, he explains, “excitation sources on the sea surface excite P-waves dominantly, whereas excitation sources on the seaf loor excite larger S-waves.”

Crustal analyses

At the same time, the shorter wavelengths of S-wave in comparison to P-wave microseisms make them more sensitive to temperature, pressure and resultant composition changes within the Earth – potentially allowing for more detailed analyses of crust and upper-mantle structures.

“The excitation of transverse surface waves – Love waves – had been established before, but because of the small amplitude of body waves compared to surface waves, the observations of Nishida and Takagi are a surprise,” says Roel Snieder, a geophysicist at the Colorado School of Mines, who was not involved in this study. “Since array techniques are in general quite robust, their detection of SH waves is convincing.”

With their initial study complete, the researchers are now looking to develop new methods to use body-wave microseisms to explore the nature of the Earth’s interior beneath oceanic storms. To this end, they are presently compiling a catalogue of storm events, similar to the weather bomb already examined, for use in such studies.

The research is described in the journal Science.

A physics tour of Beijing

Dusk falls on Beijing

By Hamish Johnston in Beijing 

It’s a lovely warm evening here in Beijing. I have just arrived for an action-packed visit in which I will have a chance to meet some of China’s top physicists and science policy makers.

Over the next few days I’m looking forward to meeting people at the Chinese Physical Society (CPS),  the China Association for Science and Technology (CAST), the Ministry of Science and Technology of China (MOST), the National Natural Science Foundation of China (NSFC) and more.

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