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The green flash

My interest in the “green flash” began at a young age. I can’t remember precisely when or where I’d read about it, but I do recall being fascinated by the thought of an effect that was supposed to produce an emerald-green flash at around sunset.

My interest was piqued at the age of 10 on a fishing trip off the south coast of England. It was a trip organized by my father and coincided with a sky that was clear and blue. We were at sea as the Sun was setting and I recall my hopes rising, despite knowing that the green flash had been described as rare, and normally best seen over a sea horizon from the tropics. On this occasion, I saw a beautiful sunset, but my hopes of seeing the green flash took a hit as nothing green appeared.

Many years later, having become an established astrophotographer, I found myself again on England’s south coast, this time trying to photograph a really thin crescent Moon in the post-sunset twilight on Selsey beach in West Sussex. I had a digital single-lens-reflex (DSLR) camera attached at the prime focus of my 100 mm refracting telescope – an arrangement where the telescope acts like a super-telephoto lens. As the Sun got lower in the sky, it was visibly contorting due to the thick, unstable atmosphere close to the horizon.

As the bottom edge of the Sun touched the horizon, I swung the telescope into position (see safety note at the end of this article), fine-tuned the focus via the review screen and started photographing. The stuttering animation of the sunset that appeared on my camera’s rear-view screen revealed large ripples running up the Sun’s disc. As they hit the top, some caused the upper edge to briefly magnify and detach. Later, as I viewed the shots on my computer, I was reminded of my childhood obsession – the upper edge of the Sun was significantly green. But what exactly is the green flash?

Emerald emanation

As light passes through the atmosphere, it gets refracted. The thicker the layer it has to pass through, the more refraction occurs, so maximum refraction occurs close to the horizon. (When the Sun appears to be touching the horizon, in reality its disc has already set.) The atmosphere acts like a prism, refracting different wavelengths by varying amounts.

At sunset the Sun’s light smears into a spectrum of colour, most of which overlaps and can’t be seen individually. However, at the vertical extremes, you can sometimes notice a bluer top edge and a redder bottom edge. The effect is small, appearing like colour fringes when seen under magnification. Unless the air is very clean, the atmosphere scatters the blue fringe away leaving a green one. This is known as the “green rim”, with the bottom red counterpart known as the “red rim”. The same effect occurs around the rising Sun and the rising or setting Moon.

For a green rim to become a green flash, the atmosphere through which you’re viewing the Sun needs to have the right temperature structure. The atmosphere’s temperature normally reduces with height, but what is needed for a green flash is an inversion layer – a layer of warmer air sandwiched between cooler air on either side – below the observer’s line of sight. This essentially creates a cylindrical lens, which both magnifies and visually detaches the upper green rim from the Sun’s disc. If the conditions and timings are right, then as the last bit of Sun slips below the horizon, a thin, bright-green blob of detached sunlight can be seen hanging above the horizon – a purist’s green flash.

Photograph of the circular Sun just as most of it has risen from the sea horizon. Mostly obscured by two long clouds, the lower part of the Sun is orangey-red, while the top visible quarter is a bright whitish colour with a small green appendage of light at the very top

A more common version occurs when the Sun remains just above the horizon or has partially set. Here, the green rim may simply elongate away from the Sun’s edge, appearing more like a “green appendage”. A less common appearance occurs as the Sun dips behind clouds close to the horizon – here a small inversion layer may be present at the top of the clouds, which can result in a “proper” detached green flash.

Surprise views

After photographing the green rim and green appendages described above, I finally got to see my first proper green flash while visiting the European Southern Observatory’s Very Large Telescope platform in Paranal, Chile, during 2013. I’d taken a small, 66 mm refracting telescope along with me for the trip and decided to see whether I could capture the green flash as the Sun set over the Pacific.

The air was very clear at the platform’s 2.6 km altitude, making estimating a safe time to point the camera at the setting Sun quite tricky. As it slipped ever lower – as in my Selsey beach experience – the Sun underwent a series of impressive contortions indicating that inversion layers were present. Then, right at the final moment of sunset, a layer of green rim detached to give a beautiful green flash. Although I had thought I might get lucky, actually seeing the green flash properly for the first time caught me by surprise and was really rather emotional. (This experience was caught on camera by filmmaker Brady Haran.) Later analysis of my shots revealed that a small amount of blue flash was also present. Under less pristine skies, this rare blue light would have been scattered away. (See top image for a composite image compiled from this green flash observation.)

After seeing my first proper green flash from Paranal in August 2013, I unexpectedly saw my second in November of the same year, and this was a real surprise. I was visiting the Roque de los Muchachos Observatory in La Palma, for filming duties with the BBC’s The Sky at Night television programme. I’d taken time off from filming to watch the sunset, and as we were based around the Isaac Newton Telescope we had been allowed on the roof to take in the view. As the Sun slowly sank towards a bank of cloud, I can remember thinking I really ought to have my camera with me. However, as the cloud’s edge had a decent altitude above the horizon, I wasn’t expecting to see the green flash. Of course, nature has an inbuilt ability to detect such oversights and as the last vestiges of the Sun’s disc slipped below the cloud bank, a dramatic, emerald-green flash appeared.

Safety note

Turning a camera or telescope towards the Sun is not normally a safe thing to do. Under no circumstances ever view the Sun through a telescope or via a camera viewfinder. To do so invites eye damage, even permanent blindness. It’s safe to watch events unfold on the camera’s rear-view screen, but point at the Sun when it’s too high above the horizon and the camera could be damaged.

US astronomers call for a new space telescope with a giant 12 m mirror

Plans for a new telescope that would be one of the biggest probes ever sent into space have been outlined by a group of astronomers. If the project goes ahead, the probe – tentatively called the High-Definition Space Telescope (HDST) – would feature a 12 m mirror and could be launched in the first half of the 2030s. The plans have been unveiled by a 17-strong committee at the US Association of Universities for Research in Astronomy (AURA), which warns, however, that many additional steps need to be taken to procure funding and develop the necessary technologies before the telescope could be built.

Following the planned launch in October 2018 of the infrared James Webb Space Telescope (JWST), there are no large-scale space observatories on NASA’s schedule. The HDST would detect a similar wavelength range as the Hubble Space Telescope, from near-infrared to far-ultraviolet light, but using a substantially larger mirror than Hubble – 12 m compared with 2.4 m. Because launch systems cannot fit that size of mirror into the rocket fairing, the plan is for the main mirror to comprise 54 segments attached to a foldable backplane.

I’m hopeful that we’ll figure out a way to do it
Marc Postman, Space Telescope Science Institute

Such technology has been developed and is being utilized by the JWST, which has a 6.5 m segmented mirror, yet it is untested on a structure that would be almost twice that size. “I’m hopeful that we’ll figure out a way to do it, in a way that is technically feasible, affordable and can be done on a timescale that is not in the too distant future,” says committee member Marc Postman of the Space Telescope Science Institute in Baltimore, Maryland.

One of the HDST’s main goals would be to study planets around other stars. To do that, the telescope would use a “coronagraph” to suppress light from some 500 to 600 stars individually and hunt for planets orbiting within those stars’ habitable zones – a region where the conditions could support liquid water on an exoplanet’s surface. According to Postman, once the HDST finds these worlds, it would be possible to get a spectrum of the planet that could tell astronomers whether or not there are “potential signs of life as reflected in the atmosphere of the planet”.

Focus on galaxy formation

In addition to its exoplanet observations, the HDST could measure how most of the stars in our galaxy move over the course of 10 years. It could also study the 3D motions of nearby galaxies compared with more distant ones, revealing characteristics about the nature of dark matter. The telescope, moreover, would be the first instrument to resolve how gas flows in and out of galaxies, a crucial observation for understanding galaxy formation.

Heidi Hammel, AURA executive vice president, says that the committee incorporated lessons learned from the JWST, a project that is over budget and has suffered delays. While the report does not touch on the costs required to construct the HDST, astronomers hope the study will now influence those at NASA who oversee technology development so that it is studied further.

How do you produce laser light with bespoke colours?

In less than 100 seconds, William Wadsworth reveals how he can create bespoke colours of laser light by shining a high-power laser at glass. To explain what is taking place within the glass, Wadsworth uses the analogy of a ball stuck at the bottom of a valley that can be kicked to move it up and down the asymmetric hills on either side. In a similar way, electrons inside the atoms of glass can be given a “kick” with a high-power laser, causing them to oscillate over a range of frequency components – corresponding to different colour emissions.

If lasers are your thing, then don’t forget to also check out the Physics World Focus on Optics & Photonics. This free-to-read issue includes a special feature about the giant laser interferometers underpinning the latest searches for gravitational waves.

  • With 2015 being the International Year of Light (IYL 2015) we have also produced a special edition of Physics World devoted to light and its varied applications in our lives. If you’re a member of the Institute of Physics (IOP), you can get immediate access to the special issue about light in our lives with the digital edition of the magazine on your desktop via MyIOP.org or on any iOS or Android smartphone or tablet via the Physics World app, available from the App Store and Google Play. If you’re not yet in the IOP, you can join as an IOPimember for just £15, €20 or $25 a year to get full digital access to Physics World.

Solarquest, Pluto and the importance of New Horizons

A photo of the board game Solarquest, which contains images of all nine planets, several of their moons, and a path between them

By Margaret Harris

Last night, in honour of the New Horizons mission to Pluto, I pulled out my copy of Solarquest. This classic board game was a childhood favourite of mine, and it’s basically Monopoly in space: instead of buying properties named after streets in Atlantic City, New Jersey (or London, if you’re British), you buy planets, moons and artificial satellites. Then, when your fellow players land on an object you own, you charge them rent.

Such nostalgia is all well and good, I hear you say, but what’s it got to do with New Horizons or Pluto? Well, Solarquest’s inventors clearly took their science seriously. By board game standards, there’s quite a lot of physics in it. For example, you can’t leave a planet unless you roll a number high enough to overcome its gravitational pull, and its Monopoly-like property deed cards include facts about each planet and moon as well as their prices.

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Pluto fly-by: New Horizons sails past cold, distant world

By Tushna Commissariat

After trundling through our solar system for more than 10 years, NASA’s New Horizons mission made its closest approach to the dwarf planet Pluto earlier today, at 12:49 BST. It was a mere 12,472 km from the planet’s surface – roughly the same distance from New York to Mumbai, India – making it the first-ever space mission to explore a world so far from Earth.

If you want to find out more about the New Horizons mission, read this recent news story by physicsworld.com editor Hamish Johnston. Above is best close-up view of this cold, unexplored world that the spacecraft sent back before its closest approach (when it was still 766,000 km from the surface), revealing in clear detail many of the planet’s surface features, including the “heart” at the bottom.

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LHCb claims discovery of two pentaquarks

The best evidence yet for the existence of a new type of particle called a pentaquark has been unveiled by physicists working on the LHCb experiment on the Large Hadron Collider (LHC) at CERN. Containing five bound quarks, pentaquarks were first predicted to exist in the late 1970s, and evidence for their existence emerged from several labs in the 2000s, only to be contradicted by experiments done elsewhere. While this latest evidence from LHCb is very strong, the data do not reveal exactly how the five quarks are bound together – something that will be the subject of further studies at CERN.

Most known hadrons are either mesons, which contain a quark and an antiquark, or baryons, which comprise three quarks. A proton contains two “up” quarks and one “down” quark, while a positive kaon contains an up quark and a “strange” antiquark. But the theory of the strong force – quantum chromodynamics (QCD) – allows for other types of baryons, providing that the number of quarks minus the number of antiquarks is a multiple of three. In particular, it allows for particles containing four quarks and one antiquark.

In the early 2000s several independent groups of physicists reported the observation of pentaquarks, most with masses in the 1520–1560 MeV/c2 range. Since then, however, other research groups have failed to find further evidence for these pentaquarks, and by the start of this decade, the consensus in the particle-physics community was that the pentaquark had yet to be discovered.

9σ significance

Now, physicists at LHCb have found compelling evidence for the existence of pentaquarks – this time at the much higher mass of about 4400 MeV/c2. The team studied the decay of the Λb baryon into three other particles: a J/ψ, proton and a charged kaon. A careful analysis of the decay products revealed that two intermediate states were sometimes involved in their production. Dubbed Pc+ (4450) and Pc+ (4380) – where the numbers are the particle masses in units of MeV/c2 – both particles have been observed with statistical significances greater than 9σ. In particle physics a significance greater than 5σ is consider to be a discovery.

The LHCb team is confident that the particles are indeed pentaquarks that comprise two up quarks, one down quark, one charm quark and one anticharm quark. “Benefitting from the large data set provided by the LHC, and the excellent precision of our detector, we have examined all possibilities for these signals, and conclude that they can only be explained by pentaquark states,” explains LHCb physicist Tomasz Skwarnicki of Syracuse University in the US.

LHCb physicist Tim Gershon of the University of Warwick in the UK explains why he is confident of the result: “The LHCb analysis is significantly different from those of previous experiments that found hints of [pentaquarks] that were later disproved.” He adds that “LHCb has analysed all of the available information in the decay distribution to prove that the peak in the mass distribution cannot be a fake caused by other processes.”

Subatomic molecules

The LHCb data do not, however, reveal how the five quarks are bound within the pentaquark. The five quarks could be tightly bound within a single structure, for example. Another possibility is that a quark and antiquark are bound together to form a meson and the remaining three quarks form a baryon. The meson and baryon could then be bound to each other to create a structure resembling a subatomic molecule.

“Studying [the pentaquark’s] properties may allow us to understand better how ordinary matter, the protons and neutrons from which we’re all made, is constituted,” says LHCb spokesperson Guy Wilkinson. This will have to wait for more data from the current run of the LHC, which started last month.

The pentaquarks are described in a paper submitted to Physical Review Letters and a preprint is available on arXiv.

Settling scientific disputes in public

Poster advertising the Science in Public 2015 event
By Margaret Harris

Here’s a Tuesday quiz for you. If you disagree with a colleague about something scientific, what should you do? Your choices are:

(a) Nothing. This is science, and the truth will win out no matter what I do;
(b) Take them aside and explain, privately, why you think they are wrong. Then, if they still disagree with you, get even by writing snarky anonymous reviews of their papers;
(c) Organize a panel “discussion” and tear them to shreds in front of all your colleagues;
(d) Take your case to the public by writing a popular-science book explaining the superiority of your own theory.

Okay, this is a trick question: I’m not sure any of those options is really a good idea (although I’m sure they’ve all been tried). I’d like to focus on the last one, though, because it was the subject of an interesting talk at the Science in Public conference, held last week in Physics World’s home city of Bristol.

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A quest for ultimate reality

When Amanda Gefter asked the cosmologist Kip Thorne to explain John Wheeler’s ideas on the universe and physical reality, Thorne was dismissive. “I think we [physicists] are less in a position to probe those issues than philosophers are…I steer clear of asking what is ultimate reality.” But Gefter was not to be dissuaded. Her quest to understand what physics has to say about that “ultimate reality” is the subject of her book Trespassing on Einstein’s Lawn and, on balance, I think she makes a good job of it. I certainly felt that I learned something, even though the book, like the quest itself, has some ups and downs along the way.

Gefter’s story begins when she is in high school. Disillusioned by her science classes, she is encouraged by her father to tackle the more “philosophical” ideas within physics – ideas about cosmology, gravity and quantum mechanics, as well as classic questions such as “What is nothing?” and “Where did the universe come from?” Gradually, Gefter and her father begin delving into physics together, seeking the answers to the universe more or less as a hobby. And while she goes on to study philosophy and creative writing (rather than science) at university, she later becomes a science writer as a pretext for continuing her quest – a quest in which she slowly realizes that the universe is far less “real” than we could ever imagine.

Initially, Gefter’s narrative reads like a very ordinary coming-of-age story, and aspects of it feel rather forced and unremarkable. She does, however, flag up some interesting issues. One is the importance of showing children the relevance of science at school, beyond simply abstract facts. Children need to understand how what they are learning fits into the real world, particularly the world with which they are familiar. Without this, the facts have no meaning. Another is “impostor syndrome”, which leads talented, intelligent people to believe they are not good enough and will soon be “found out” by colleagues or superiors. Gefter saw her transition from student to writer as extraordinary because she felt that she was just pretending. In truth, I think many people – especially, but not exclusively, women – experience this. Awed by our colleagues’ intelligence or performance, we end up always feeling like we are winging it.

Once Gefter embraces her own status as a bona fide science writer, her story somehow becomes more compelling. The concept of her journey resonated with me, as I have recently undertaken a similar one myself (although in my case, I have been learning about the Northern Lights rather than cosmology). Finding things out on this scale can be a transformational experience and is as much about the people as the physics, so it was good to hear about the physicists Gefter met along the way. I enjoyed the stories about Wheeler, the Los Alamos physicists and Einstein peering through ­Hubble’s telescope; indeed, there could have been more.

The narrative ties back nicely to discussions between Gefter and her father many years previously, showing not only how the small seed he planted had grown and blossomed, but also how his early ideas related to what physicists think about reality.

One of the first things that Gefter learns during her quest is that scientific theories aren’t about “things” at all. Instead, they are about mathematical structure. Our interpretations of theories – such as “gravity is a force that masses exert on one another from a distance” (Newton), or “gravity is the local curvature of space–time” (Einstein) – are just different stories we contrive to make sense of the maths. This helps to explain why Newtonian gravity looks the same as Einstein’s gravity in the low-energy limit. Newton was not wrong; he was simply looking at a small corner of the picture. The overall structure is the same.

Reading this reminded me of an anecdote I heard from another physicist at a conference. He had been visit­ing the cathedral in Seville, Spain, when he noticed that the floor he was standing on was laid out in a beautiful star pattern. He took a picture of it. Then he lifted the focus of his camera and took a picture of the rest of the floor. At this point he realized that the floor was not made of stars at all, but was a black-and-white pattern of squares and triangles. Only when viewed in isolation did small patches look like stars. The global view changed the picture.

This global view may help us reconcile classical physics with modern physics, but when it comes to the universe, there is no “God’s-eye” view. There are just different reference frames, and this problem lies at the heart of the incompatibility between general relativity and quantum mechanics. In relativity, observers are inside the system (space–time), whereas in quantum mechanics they are outside making the measurements. But to view the universe from outside is impossible.

While studying in London, Gefter realizes that what is real is what survives the translation between reference frames – in other words, what is invariant. She draws an analogy with languages. “Love” and “amor”, she points out, are not totally different things simply because they look different. The terms refer to the same thing. The underlying structure (the concept) is what is real, not the word itself (the description). Similarly, anything real must survive the translation between observers’ reference frames. Armed with this knowledge, Gefter and her father go on a search for invariance.

The middle of the book becomes somewhat convoluted, presenting multiple views from different physicists and using extensive dialogue. This confusion is compounded by the use of jargon and acronyms, which often make it difficult to grasp the essence of an exchange. Fortunately there are helpful summaries in the last chapters. Gefter also has some nice, almost poetic, ways of ­expressing things, as in phrases such as “the gravitational lifeblood of stars and galaxies” and she gives good, simple analogies for difficult concepts. She should, however, be careful of the lazy use of cliché in descriptions, and her style was often too colloquial for my taste. One can, I think, have an authentic “voice” without resorting to expletives.

During her quest, Gefter learns that many concepts we regard as invariant are, in truth, observer-dependent. Acknowledging this is difficult because it requires us to drop long-held assumptions, equivalent to recognizing the speed of light as finite. Even Einstein, who made the mental leap to formulate rela­tivity, had trouble accepting quantum mechanics. The concepts are tricky and counter-intuitive, but ultimately Gefter’s book is an enlightening journey through the extremes of modern physics to the edge of the universe.

  • 2014 Bantam £18.49/$28.00hb 432pp

Computer-chip features shrink to 7 nm

Scientists at IBM Research have made the first working prototype computer chips with circuit features as small as 7 nm. The milestone was achieved in collaboration with GlobalFoundries, Samsung and researchers at the SUNY Polytechnic Institute Colleges of Nanoscale Science and Engineering. Key features of the chips were made using silicon-germanium, rather than conventional silicon. The new technology could soon make it possible to pack 20 billion transistors onto a single chip – twice as many as is possible today.

In 1965 Gordon Moore, the co-founder of Intel, predicted that the number of transistors per unit area on integrated circuits would double every year, and this concept came to be known as Moore’s Law. The silicon industry has succeeded in following this law until quite recently, and this has given us myriad low-cost consumer electronics. Today, the smallest features on commercial chips measure 14 nm across, and some progress has been made on 10 nm and 7 nm devices. However, using conventional silicon-processing techniques to create working chips with features smaller than 10 nm requires several significant technological challenges to be overcome.

Bypassing convention

Now, the IBM-led collaboration has eschewed conventional semiconductor-manufacturing processes to create the first prototype 7 nm chip. The transistors used in the device are called “FinFETs” – complex devices that incorporate two gates. The transistor channels of the device – the parts that conduct electricity – are made from silicon-germanium (SiGe), rather than pure silicon. SiGe has higher electron mobility than pure silicon, which means that it is better suited for making tiny transistors.

The researchers have also managed to make use of very short wavelengths of ultraviolet light – extreme ultraviolet light (EUV) – to improve the lithography process for etching their tiny devices. EUV lithography can create much thinner lines than conventional techniques that rely on longer-wavelength light, although the etching rate is slower for EUV.

IBM also says that it used an “innovative” process to place the transistors closer together on a chip. Indeed, the devices boast a 30 nm pitch, which is the distance between the front edge of one transistor and the front edge of it neighbour.

Extending mainstream technologies

Mukesh Khare, vice president for semiconductor research at IBM, says that his company “has committed to spending $3bn on chip research and development aimed at further extending today’s mainstream semiconductor technologies”. He adds that IBM is also looking into materials other than silicon as the primary material in semiconductors and the use of transistors for processing data.

Stephen Chou, head of the NanoStructure Laboratory at Princeton University who was not involved in this work, says the 7 nm technology is a “significant step” for the integrated-circuit industry – in terms of both scaling and manufacturing. “Although my group fabricated the world’s smallest working individual silicon [transistors] (as small as 7 nm – in both length and width) in 1996, making [transistors] with similar dimensions on the industrial scale is extremely challenging and requires many innovations and billions of dollars of investment,” he says.

ILC Science Club, science fiction versus science fact and siblings in physics

 

By Hamish Johnston

At the end of next week millions of children in England and Wales will start their summer holidays and many parents will now be scrambling to find activities to keep their little dears occupied. Physics World can recommend a virtual trip to ILC Science Kids Club courtesy of the Tokyo Cable Network and Japan’s Advanced Accelerator Association. ILC stands for International Linear Collider, which is one of several proposed to take over when the Large Hadron Collider is eventually retired. In the first video of the series, a boy called Haru learns why scientists are keen on building accelerators from his Uncle Tomo. The video is in Japanese with English subtitles, so as well as learning about particle physics, your little tykes might even pick up a little Japanese.

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