terça-feira, 6 de outubro de 2015

Single Photonics and Quantum Information

 

Summary:

The smallest unit of light is a “photon”. Generation, manipulation and measurement of light at or near the fundamental limit of a photon can enhance the performance of many optical systems. Remote sensing, long-distance communications, biological imaging, and quantum information science are some near-term applications that would benefit immensely from better optical components and techniques that work efficiently at few or single photon levels. However, the technologies to generate, manipulate, and detect these states of light are inadequate for the emerging applications. We are developing new light sources, detectors, and measurement techniques to address these needs.

Description:

One of the activities in this group is the development of single photon technologies for quantum information science and technology. We work closely with the Nanostructure Fabrication and Metrology Project on the generation of novel non-classical states of light and the detection of single photons. Currently, we are investigating the use of nonlinear fibers and nonlinear crystals as a source of correlated photon pairs or squeezed light. We are also manipulating the squeezed light to make Schroedinger "Cat" states of light. In addition to making non-classical states of light, we build detector systems that are the best in the world at operating at the single photon level. Presently, our project is primarily focused on using two different superconducting detector technologies -- transistion-edge sensors (TES) and superconducting nanowire single photon detectors (SNSPD).

Using our sources and detectors, we also are actively involved in characterizing optical compoments at the few photon level, demonstrating new optical devices that function at the single photon level, demonstrating of new measurements at faint light levels, and demonstrating new applications that require single photons.

 

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http://www.nist.gov/pml/div686/grp06/sspd.cfm

Heart attack Risk factors

 

 

By Mayo Clinic Staff

Certain factors contribute to the unwanted buildup of fatty deposits (atherosclerosis) that narrows arteries throughout your body. You can improve or eliminate many of these risk factors to reduce your chances of having a first or subsequent heart attack.

Heart attack risk factors include:

  • Age. Men age 45 or older and women age 55 or older are more likely to have a heart attack than are younger men and women.
  • Tobacco. Smoking and long-term exposure to secondhand smoke increase the risk of a heart attack.
  • High blood pressure. Over time, high blood pressure can damage arteries that feed your heart by accelerating atherosclerosis. High blood pressure that occurs with obesity, smoking, high cholesterol or diabetes increases your risk even more.
  • High blood cholesterol or triglyceride levels. A high level of low-density lipoprotein (LDL) cholesterol (the "bad" cholesterol) is most likely to narrow arteries. A high level of triglycerides, a type of blood fat related to your diet, also ups your risk of heart attack. However, a high level of high-density lipoprotein (HDL) cholesterol (the "good" cholesterol) lowers your risk of heart attack.
  • Diabetes. Insulin, a hormone secreted by your pancreas, allows your body to use glucose, a form of sugar. Having diabetes — not producing enough insulin or not responding to insulin properly — causes your body's blood sugar levels to rise. Diabetes, especially uncontrolled, increases your risk of a heart attack.
  • Family history of heart attack. If your siblings, parents or grandparents have had early heart attacks (by age 55 for male relatives and by age 65 for female relatives), you may be at increased risk.
  • Lack of physical activity. An inactive lifestyle contributes to high blood cholesterol levels and obesity. People who get regular aerobic exercise have better cardiovascular fitness, which decreases their overall risk of heart attack. Exercise is also beneficial in lowering high blood pressure.
  • Obesity. Obesity is associated with high blood cholesterol levels, high triglyceride levels, high blood pressure and diabetes. Losing just 10 percent of your body weight can lower this risk, however.
  • Stress. You may respond to stress in ways that can increase your risk of a heart attack.
  • Illegal drug use. Using stimulant drugs, such as cocaine or amphetamines, can trigger a spasm of your coronary arteries that can cause a heart attack.
  • A history of preeclampsia. This condition causes high blood pressure during pregnancy and increases the lifetime risk of heart disease.
  • A history of an autoimmune condition, such as rheumatoid arthritis or lupus. Conditions such as rheumatoid arthritis, lupus and other autoimmune conditions can increase your risk of having a heart attack.

 

http://www.mayoclinic.org/diseases-conditions/heart-attack/basics/risk-factors/con-20019520

Oct. 5, 1984, Launch of History-Making STS-41G Mission

 

 

41g-90139

A Florida dawn scene on Oct. 5, 1984 forms the backdrop for the climbing Space Shuttle Challenger, its two solid rocket boosters and external fuel tank, launched on the eight-day STS-41G mission. The scene was photographed by astronaut Paul J. Weitz, who was piloting the Shuttle training aircraft (STA).

Crewed by Robert L. Crippen, Commander; Jon A. McBride, Pilot; Mission Specialists Kathryn D. Sullivan (now NOAA administrator), Sally K. Ride, David C. Leestma and Payload Specialists Marc Garneau of the Canadian Space Agency and Paul D. Scully-Power, the mission’s objectives included the deployment of the Earth Radiation Budget Satellite and the demonstration of the Orbital Refueling System by Sullivan and Leestma during a spacewalk.

On this mission, Sullivan became the first U.S. woman to perform a spacewalk. Marc Garneau became the first Canadian astronaut to fly to space. The shuttle's crew of seven was the largest ever to fly on a single spacecraft at that time, and STS-41G was the first flight to include two female astronauts. STS-41G completed 132 orbits of the Earth in 197.5 hours, before landing at Kennedy Space Center, Florida, on Oct. 13.

Image Credit: NASA

Last Updated: Oct. 5, 2015

Editor: Sarah Loff

http://www.nasa.gov/image-feature/oct-5-1984-launch-of-history-making-sts-41g-mission

Gorgeous calabash lamps transform any room into magical otherworldly realms

 

 

Why settle for a normal light when you can have one that transforms your room into a dazzling piece of art? Polish artist Przemek Krawczyński’s stunning sculptural lamps do just that, using tricks of the light to project magical shadow patterns onto walls. The Łódź-based artist handcrafts each unique lamp from dried calabash, or bottle gourds, that he intricately carves into shapes that create dazzling otherworldly atmospheres when illuminated at night.

Calabarte, Przemek Krawczyński, Calabarte Przemek Krawczyński, gourd lamps, gourd lamps Przemek Krawczyński, calabash, calabash lamps, gourd fruit, gourds, green lighting, handcrafted lamps, hand carved lamps

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Originally an engineer, Krawczyński started making calabash lamps after he came across the gourd fruit in 2009. The calabash is a vine grown for its gourd fruits that can be harvested when mature, dried, and used to make utensils, containers, and other products. Although there are many varieties of gourds that grow around the world, Krawczyński chooses to carve his lamps from the round African varieties.

Related: Andrew Mowbray Grows Square Building Blocks from Living Gourds

The beautiful calabash lamps are intricately handcrafted, from the initial sketches to the gourd processing and construction of the wood lamp base. “By day my lamp is a unique sculpture, while at night the light breathes new life into that sculpture, seeping through intricately carved wood and passing through thousands of holes,” says Krawczyński. “Flowing shadows fill the space and cast the patterns on the surrounding surfaces, which turns each interior into scene for breathtaking spectacle.” The unique lamps can take two to four months to complete, depending on the pattern and size.

+ Calabarte

Via My Modern Met

Images via Calabarte

http://inhabitat.com/gorgeous-calabash-lamps-transform-any-room-into-magical-otherworldly-realms/

Review: Optoma NuForce BE6 Bluetooth earphones

 

 

The Optoma NuForce BE6 Bluetooth earphones are available now at a suggested retail price of US$129

The Optoma NuForce BE6 Bluetooth earphones are available now at a suggested retail price of US$129 (Credit: Paul Ridden/Gizmag)

Optoma has today released the BE6 earphones, its fourth since acquiring the NuForce brand late last year, and its first wireless models. The stylish bullets are reported smaller than Bluetooth market leaders and are being aimed squarely at mobile music lovers with an ear for quality. Gizmag was sent a pre-release pair for review.

  •  
  • In addition to the BE6 Bluetooth earphones, the box contains a zipped carry case, four sizes ...
  • The BE6 earphones use a
  • The rear of each earpiece is magnetic, so that the earphones can be snapped together around ...
  • We found the BE6 Bluetooth earphone somewhat lacking in bottom end, most evident on bass-heavy tracks ...

It really wasn't too long ago that those wanting to ditch the dangling cables to listen to music on the move had to make do with serious dips in sound quality, constant background hiss, and annoying pops and dropouts. As wireless technology improved and the default SBC codec started to get nudged out by more widespread adoption of aptX and AAC, so the annoying noise began to clear and the words quality and Bluetooth started to be uttered in the same breath. With the release of its new NuForce BE6 in-ear headphones, Optoma is promising to deliver the kind of audio quality over Bluetooth that was previously the exclusive domain of wired-for-sound audioholics.

The BE6 earphones use a "state of the art" Bluetooth 4.0+EDR receiver, with support for both aptX and AAC audio technologies. This heady combination should result in top notch streaming sound quality from most modern source devices over a wireless range of up to 30 m (100 ft).

Though touted as smaller than other leading wireless earphones, the Optoma NuForce BE6 in-ear headphones are still quite chunky monkeys. Each housing measures 27.2 mm (1.07 in) nose to tail (minus the silicone tip) and 13 mm (0.51 in) in diameter at its thickest stretch, and the whole shebang – both ear pieces, the cable, medium silicone tips and stabilizers – weighs just 17 g (0.6 oz).

Within the cool and stylish machined aluminum housings are brand new 10 mm dynamic drivers, with 95 dB sensitivity, 20 ohm impedance and a frequency range of 20 Hz to 20 kHz.

The inline remote hangs to the right, and is used to power on the BE6 earphones, put them into Bluetooth discovery mode, control playback, and take calls. It also facilitates communication with smartphone-based virtual assistants like Siri.

Pairing was surprise-free and straightforward for all source devices tested, which included iOS and Android smart devices, laptops and computers. The only slightly awkward point being that discovery mode can only be activated from a powered off state, so you have to switch them off and on again with a long press of the power button before they're ready for pairing.

The remote is also home to a microphone with -42 dB sensitivity and, though we found the audio on test calls over Skype via a laptop and on a smartphone to be received loud and clear, in both cases signal breakup, crackles and pops were reported at the other end.

The remote contains a cylindrical 3.7 V/80 mAh Li-ion battery. Optoma claims up to 5.5 hours of up time between charges, though we found that continuous playback at comfortable volume levels yielded a little over 5 hours for every 2.5 hours on charge. The earphones will power off automatically after 3 minutes of inactivity.

Two quick-fire beeps sound periodically during playback to announce that it might be a good idea to start looking for a wall outlet, but the LED can be consulted for a rough estimate of remaining battery life at any time by simultaneously pressing all three buttons. Two flashes indicate a low battery, three for 50 percent and four or five for full. If plugged in users have enabled voice prompts (by pressing the power and volume up buttons at the same time), battery life information will be delivered through the drivers in a human voice when the three buttons are pressed.

Optoma says that the supplied proprietary silicone tips have been specifically designed for a more balanced and comfortable fit, though two pairs of (sweat- and moisture-resistant) Comply foam tips are also included for a more secure fit.

On the subject of comfort and fit, I found the combination of shortened bud (custom designed with wider flare for optimum sound projection) and thick nozzle meant that I couldn't really push the earphones down into the ear canal like, say, with the T20 cabled in-ear headphones from RHA. This inevitably resulted in the BE6 earphones falling out mid-jog, but, more importantly, meant that the passive isolation from the sounds of the outside world was not particularly effective (which could arguably be a good thing for the safety of plugged in runners . And cyclists).

Slotting a squishy stabilizer onto each housing helped keep the earphones in position. Optoma recommends a 45 degree from north orientation for each stabilizer, then plugging the BE6s in with a twist to lock in place. However, I found 70-75 degrees suited me better so would advise some positioning experimentation if the suggested fit doesn't work out.

The rear of each earpiece is magnetic, so that the earphones can be snapped together around the neck when not in use. A small but useful detail, and quite a relief not to have buds bouncing around when bounding down the street toward the train station. The BE6 earphones are also reported splash-proof, meaning that they don't have to be quickly packed away if you're caught out by a quick shower while out on the morning run.

 

The high points, and the lows

"NuForce is all about natural sound," Jon Gordem, Senior Director of Product Management, Optoma told us. "We want to be loyal to the source material and make sure we play audio in the way the artist intended it, regardless of the genre. This means that our sound signature needs to have explosive bass and crystalline highs all in full balance."

So did the BE6 earphones live up to that ambitious "cord-less experience without compromising on sound quality" promise? Well, we found the audio to be as clean as a whistle, with no background hiss or detectable distortion, even at unhealthy volume levels. The in-ears proved pretty good all-round performers, offering lively reproduction across genres such as blues, pop, folk, jazz, classical and rock.

We weren't presented with a huge soundstage, but it was by no means cramped. The sound signature treated all audible frequencies and instrumentation well, though in a similar fashion to the company's NE750M wired earphones, the mid-range was boosted slightly so that some guitar solos and vocals got a little more emphasis than expected. This can be a drawback for well-worn favorites, but can also be a bonus for quietly-spoken dialog in movies. While the NE750Ms offer a solid, though by no means booming, lower end performance, the BE6s do not.

Personally, I'm not overly fond of bass-heavy tuning, steering clear of Beats-like thunder-punchers in favor of a flatter, neutral response. But I found the BE6 earphones to be a little too lacking in the bass department. It was certainly present in all the tunes listened to during the review, but the arresting thump on tracks like Ain't nothing wrong with that from Robert Randolph just wasn't there, Roger Waters was resigned to a backing member of Pink Floyd rather than a loud and proud key player and Three 6 Mafia didn't come even close to generating the familiar chest-filling warm glow.

More bottom end could be brought in by tinkering with source hardware or software settings, of course, but in the interests of fairness and consistency, we opt for a flattened EQ in listening tests.

 

The bottom line

The BE6 bullets were feather light to wear, but not the most comfortable in-ears we've ever plugged in. The flat cable is just over half a meter from cable relief to boxy relief (around 22 inches), a nice length. There was little physical noise when it was handled or it brushed against clothing while running, but taps and scrapes on the remote did cut through the tunes.

The battery fell just short of the claimed 5.5 hours during review testing, managing over 5 hours of continuous playback – though you might get seven, eight or more hour long sessions at the gym before needing to break out the supplied USB cable and locate a power source.

The wireless range of up to 30 m or so meant that the source player could be left on the patio table while wandering around the garden or in the kit bag when jumping from machine to machine at the gym. Streamed audio came through clean, clear and lively, let down only by a somewhat lackluster bass presence.

The Optoma NuForce BE6 Bluetooth earphones are available from today at a suggested retail price of US$129. We were sent gray earphones for review, but they're also available in gold.

Product page: Optoma NuForce BE6

 

Efficiency from larger perovskite solar cells improved

 

 

 

A new fabrication method enabled researchers to make larger perovskite cells with few defects, helping to maintain efficiency at larger cell sizes.

Credit: Brown University / NREL

Using a newly developed fabrication method, a research team has attained better than a 15-percent energy conversion efficiency from perovskite solar cells larger than one square centimeter area. The researchers, from Brown University and the National Renewable Energy Lab (NREL), have reported their findings in the journal Advanced Materials.

Perovskites, materials with a particular crystalline structure, have caused quite a buzz in the solar energy world. Perovskite solar cells are relatively cheap to make, and the efficiency with which they can convert sunlight into electricity has been increasing rapidly in recent years. Researchers have reported efficiency in perovskite cells of higher than 20 percent, which rivals traditional silicon cells. Those high efficiency ratings, however, have been achieved using cells only a tenth of a square centimeter -- fine for lab testing, but too small to be used in a solar panel.

"The use of tiny cells for efficiency testing has prompted some to question comparison of perovskite solar cells with other established photovoltaic technologies," said Nitin Padture, professor of engineering at Brown, director of Brown's Institute for Molecular and Nanoscale Innovation, and one of the senior authors of the new research. "But here we have shown that it is feasible to obtain 15-percent efficiency on cells larger than a square centimeter through improved processing. This is real progress."

Maintaining high efficiency on larger perovskite cells has proved to be a challenge, Padture says. "The problem with perovskite has been that when you try to make larger films using traditional methods, you get defects in the film that decrease efficiency."

The fabrication process that the Brown and NREL researchers reported in this latest paper builds on a previously reported method developed by Yuanyuan Zhou, a graduate student in Padture's lab. Perovskite precursors are dissolved in a solvent and coated onto a substrate. Then the substrate is bathed in a second solvent (called anti-solvent) that selectively grabs the precursor-solvent and whisks it away. What's left is an ultra-smooth film of perovskite crystals.

In this new study Zhou and Mengjin Yang, a postdoctoral researcher at NREL, developed a trick to grow the perovskite crystals to a larger size. The trick is to add excess organic precursor that initially "glues" the small perovskite crystals and helps them merge into larger ones during a heat-treatment, which then bakes away the excess precursor.

"The full coverage and uniformity over a large area come from the solvent method," Padture said. "Once we have that coverage, then we increase the size of the crystals. That gives us a film with fewer defects and higher efficiency." The 15-percent efficiency reached in this latest work is a good start, Padture said, but there's still room to improve. Ultimately, he would like to reach 20 to 25 percent in large-area cells, and he thinks that mark could be within reach using this method or a similar one.

Padture and colleagues at the University of Nebraska-Lincoln were recently awarded a $4-million grant by the National Science Foundation to expand their perovskite research.


Story Source:

The above post is reprinted from materials provided by Brown University. Note: Materials may be edited for content and length.


Journal Reference:

  1. Mengjin Yang, Yuanyuan Zhou, Yining Zeng, Chun-Sheng Jiang, Nitin P. Padture, Kai Zhu. Square-Centimeter Solution-Processed Planar CH3NH3PbI3Perovskite Solar Cells with Efficiency Exceeding 15%.Advanced Materials, 2015; DOI: 10.1002/adma.201502586

 

http://www.sciencedaily.com/releases/2015/10/151005132851.htm

Where to look for life? Astronomers devise 'habitability index' to guide future search

 

 

The James Webb Space Telescope, a large infrared telescope with a 6.5-meter primary mirror, is scheduled to be launched on an Ariane 5 rocket from French Guiana in October of 2018 and will be the premier NASA observatory of the next decade, serving thousands of astronomers around the world. UW astronomers have created a “habitability index for transiting planets” to help guide the ongoing search for life beyond Earth.

Credit: NASA

Powerful telescopes are coming soon. Where exactly shall we point them?

Astronomers with the University of Washington's Virtual Planetary Laboratory have created a way to compare and rank exoplanets to help prioritize which of the thousands discovered warrant close inspection in the search for life beyond Earth.

The new metric, called the "habitability index for transiting planets," is introduced in a paper accepted for publication in the Astrophysical Journal by UW astronomy professors Rory Barnes and Victoria Meadows, with research assistant and co-author Nicole Evans.

"Basically, we've devised a way to take all the observational data that are available and develop a prioritization scheme," said Barnes, "so that as we move into a time when there are hundreds of targets available, we might be able to say, 'OK, that's the one we want to start with.'"

The Kepler Space Telescope has enabled astronomers to detect thousands of exoplanets, those beyond our solar system -- far more than can be investigated one by one. The James Webb Space Telescope, set for launch in 2018, will be the first able to actually measure the atmospheric composition of a rocky, possibly Earthlike planet far off in space, and so vastly enhance the search for life.

Astronomers detect some planets when the worlds "transit" or pass in front of their host star, thus blocking some of the light. The Transiting Exoplanet Survey Satellite, or TESS, is scheduled to launch in 2017 and will find many more worlds in this way. But it's the Webb telescope and its "transit transmission spectroscopy" that will really be able to study planets closely to hunt for life.

But access to such telescopes is expensive and the work is methodical and time-consuming. The Virtual Planetary Laboratory's index is a tool to help fellow astronomers decide which worlds might have the better chance of hosting life, and so are worthy of focusing limited resources on.

Traditionally, astronomers have focused the search by looking for planets in their star's "habitable zone" -- more informally called the "Goldilocks zone" -- which is the swath of space that's "just right" to allow an orbiting Earth-like planet to have liquid water on its surface, perhaps giving life a chance. But so far that has been just a sort of binary designation, indicating only whether a planet is, or is not, within that area considered right for life.

"That was a great first step, but it doesn't make any distinctions within the habitable zone," Barnes said. "Now it's as if Goldilocks has hundreds of bowls of porridge to choose from."

The new index is more nuanced, producing a continuum of values that astronomers can punch into a Virtual Planetary Laboratory Web form to arrive at the single-number habitability index, representing the probability that a planet can maintain liquid water at its surface.

In creating the index, the researchers factored in estimates of a planet's rockiness, rocky planets being the more Earth-like. They also accounted for a phenomenon called "eccentricity-albedo degeneracy," which comments on a sort of balancing act between the a planet's albedo -- the energy reflected back to space from its surface -- and the circularity of its orbit, which affects how much energy it receives from its host star.

The two counteract each other. The higher a planet's albedo, the more light and energy are reflected off to space, leaving less at the surface to warm the world and aid possible life. But the more noncircular or eccentric a planet's orbit, the more intense is the energy it gets when passing close to its star in its elliptic journey.

A life-friendly energy equilibrium for a planet near the inner edge of the habitable zone -- in danger of being too hot for life -- Barnes said, would be a higher albedo, to cool the world by reflecting some of that heat into space. Conversely, a planet near the cool outer edge of the habitable zone would perhaps need a higher level of orbital eccentricity to provide the energy needed for life.

Barnes, Meadows and Evans ranked in this way planets so far found by the Kepler Space Telescope, in its original mission as well as its "K2" follow-up mission. They found that the best candidates for habitability and life are those planets that get about 60 percent to 90 percent of the solar radiation that the Earth receives from the sun, which is in keeping with current thinking about a star's habitable zone.

The research is part of the ongoing work of the Virtual Planetary Laboratory to study faraway planets in the ongoing search for life, and was funded by the NASA Astrobiology Institute.

"This innovative step allows us to move beyond the two-dimensional habitable zone concept to generate a flexible framework for prioritization that can include multiple observable characteristics and factors that affect planetary habitability," Meadows said.

"The power of the habitability index will grow as we learn more about exoplanets from both observations and theory."


Story Source:

The above post is reprinted from materials provided by University of Washington. The original item was written by Peter Kelley. Note: Materials may be edited for content and length.


Journal Reference:

  1. Rory Barnes, Victoria S. Meadows, Nicole Evans. Comparative Habitability of Transiting Exoplanets. Astrophysical Journal, 2015 [link]

 

http://www.sciencedaily.com/releases/2015/10/151005184638.htm

segunda-feira, 5 de outubro de 2015

Suiça espetacular

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One Scientist’s Hopeful View On How to Repair the Planet

 

 

Ecological crises may be piling up in a seemingly hopeless cascade, but Swedish scientist Johan Rockström says the next few decades offer an unparalleled opportunity to undo the damage.

by diane toomey

Johan RockströmJohan Rockström

For a researcher who studies how humanity is pushing the earth close to potentially disastrous tipping points, Johan Rockström is surprisingly optimistic. Although he reckons that our species has crossed four of nine “planetary boundaries” — including those on climate change and deforestation — he believes there is still time to pull back from the brink and create a sustainable future based on renewable energy and a “circular” economy that continually reuses resources.
In an interview with Yale Environment 360, Rockström — executive director of the
Stockholm Resilience Center and author of a new book, Big World, Small Planet — offers his take on the state of the planet and explains why he thinks there has “never been so much reason for hope as today.” He outlines how humanity can step back inside planetary boundaries, which he calls “the safe operating space of the hard-wired biophysical process of the earth’s system,” and describes how an alignment of science, technological advances, and a growing public and political hunger for action will get civilization back on track.
“It’s not a journey where we are backing into the caves,” says Rockström. “It’s a journey of high technology, good health, of better democracy, and huge, multiple benefits that [go] well beyond saving the planet.”

Yale Environment 360: As you lay out in your book, the period of the Holocene — basically the last 12,000 years — was stable and conducive to the flourishing of human civilizations. Opinions differ on when the earth entered the Anthropocene. Where do you mark the beginning point?

Johan Rockström: What does the Anthropocene really mean? It means, strictly speaking, that we humans have become a global force of change at the planetary scale, surpassing the magnitude and frequency of natural changes to the planet.
If you look back over the past 12,000 years, over the entire Holocene period, it’s true that we started domesticating animals and plants, we started to move out from our hunter and gatherer society to cut down forests and start the transformation of land. But it’s clear that through that entire period — from 8,000 years back all up until the mid-1950s — we see no evidence of humans affecting the resilience and stability of the entire earth system. Then something happens in the mid-1950s, which is clearly the exponential rise of human pressure on the planet. And then these exponential rises are multiple, from greenhouse gases all the way to loss of biodiversity, eutrophication, deforestation, land degradation, pollution of water. So essentially the whole set of parameters putting pressure on the earth system kicks off in the 1950s. So to me, that’s the entry of the Anthropocene. If you would push me really hard, I would actually say perhaps we didn’t enter the Anthropocene truly until the end of 1989. Because from 1955 up until the late 1980s, the earth system was clearly so resilient that it could buffer even that exponential rise in pressure.
So even though we were the largest pressure point, it didn’t result in abrupt shocks and stresses. It didn’t lead the earth system to start sending big shocks and waves — or what I often call invoices — back. It’s not until 1989-90 that we start to see big collapses. The codfish fished out of Newfoundland in 1990, big freshwater systems flipping over from oxygen-rich to anoxic, the Baltic Sea flipping over, the accelerated melt of Arctic sea ice, ecosystems going from productive to degraded states.

e360: You and colleagues have determined nine planetary boundaries — safe operating zones, as you put it. We’ve already exceeded four of them, including the climate boundary of 350 parts per million of CO2. Where else are we doing badly?

Rockström: It’s our most recent assessment, which was published in Science in January 2015, which concludes that we’ve transgressed four boundaries. So apart from climate change, it’s on biodiversity loss, eutrophication — interference with the global nitrogen and phosphorous cycles — and it’s on deforestation, or global land-use change. These are the ones that are already in the danger zone.

e360: Your other planetary boundaries include ocean acidification, freshwater consumption, and a few others. You write that adhering to these boundaries won’t hinder economic growth, even with an expected global population of 9 billion. Lay out how that’s possible.

Rockström: To begin with, it’s important to understand what the planetary boundary framework is. As a thought experiment, we can take humans away from planet earth, and place every human being on another planet for a moment. And what we do is simply try to interview Mother Earth, and ask her, “Where are your biophysical boundaries beyond which we see changes in feedbacks that lead to crossing of thresholds that can take us out of the Holocene equilibrium?” And science has now advanced so far over the last 30 years, in particular, that we are able to translate the voice of earth into quantified bounds. These nine processes are the ones that regulate the stability of the earth system. Once quantified, they give us the safe operating space of the hard-wired biophysical process of the earth’s system. They have nothing to do with humans. It’s really the biophysical boundaries. Once these are defined, we can put humans back. And then something quite interesting may occur, because the question arises, “Is there anything in the planetary boundary research that hinders growth?” And the answer is no. Because we have a safe operating space, which is the safe playing ground for humans.
So I give you one example: Is it possible to think of a world economy growing, but powered by the sun instead of fossil fuels? Meaning that we would stay safe on climate, and still have a high degree of modern energy use that could power economic development in the world. And the answer is yes. Now, if you define growth in GDP terms, where you have no consideration whatsoever of the deterioration and use of natural capital, then of course you are always at risk of pushing us outside of the boundaries. But if you combine a zero-carbon economy — an energy system that is entirely renewable — with a circular economic logic, where you try to recycle all the resources and all the ecosystem functions and services that you’re tapping out of the earth system, you can actually think of a world that has good economic development within a safe operating space. Now, at the end of the day, you can’t be 100 percent sustainable. But I think it’s fair to say today that we have enough evidence that we can actually deliver sustainable economic development. We’re saying that people and the planet can go hand-in-hand. There is therefore not, in the strictest sense, a limit to growth.

e360: Is the vision of a stable Anthropocene dependent on technologies that have yet to be developed?

Rockström: Well, yes and no. To me, a good Anthropocene is that we stay within Holocene-like conditions. Technologies will play a fundamental role in allowing a transformation to a zero-carbon future. I don’t believe, though, that that transition will easily be accomplished through large-scale geoengineering. It’s rather about innovations in the energy system, in mobility, in energy efficiencies, construction. And also, fundamentally, in the way we produce goods and services. So I think the innovation towards circular economic models is absolutely fundamental and, in particular, for the food system to produce food in sustainable ways that can deliver to nine, ten billion people. But I wouldn’t exclude some large-scale technological innovations to help us. For example, carbon storage and capture, or a breakthrough in fuel cell technology that can go to scale in ways that we do not see today. You can think of next-generation nuclear power, which we haven’t seen yet. So, technologies will, and do already, play a very important role. Just five years back you couldn’t say that renewable energy could be delivered to scale. Today we can with solar and wind, which is quite remarkable.
But technology alone will not do the job. It will require behavioral change and new values. We need a mind shift. We need to reconnect our human societies with biospheres, and we need to work with nature, not against it.

e360: Are there strategies that you would encourage that could expedite such a mind shift?

Rockström: We need to work with the humanistic dimension of ethics, of responsibility, of thinking inter-generationally and, quite frankly, to nurture the love of our planet, the beauty in nature. At one point in this book we say that we don’t believe that any human being wakes up in the morning with a deliberate attempt to destroy the planet. It’s simply that we are stuck in a logic, where, despite our love for our planet, we destroy her anyway, because we are stuck in a path that, just to live our lives, we cannot be fully sustainable. And the mind shift is really about putting the planet first, and then evolving from there to allow us to be much smarter about resolving these current conflicts between sustainability and development. It’s not a journey where we are backing into the caves. It’s a journey of high technology, good health, of better democracy, and huge, multiple benefits. It’s really about a high-tech — what I call a Tesla — future. It’s a future that is techier, cooler, desirable, healthier, and therefore a very exciting journey.

e360: When President Obama visited Alaska recently to sound the alarm about climate change, critics pointed to the irony of that trip, considering his decision to allow Shell to drill for oil in the Arctic. In response, the President’s senior adviser on science and technology said, quote, “We might wish for an instantaneous transformation that was drastically less reliant on oil and gas. But we don’t live in a magical world.” What’s your reaction to that?

Rockström: There is of course, a fundamental contradiction here. And the contradiction is so blatant because, on the one hand, both [Secretary of State] John Kerry and President Obama point out very clearly that the climate risks in the world are not only urgent, they’re potentially catastrophic, and things are moving too slowly because we need a transformation to an essentially zero-carbon world economy by 2050, 2070. And then secondly, they like to point out that this is not a journey of sacrifice, it’s a journey of opportunity. But then Kerry says, “Oops, we cannot phase out oil in the short term, because we simply need a transitional phase, and we don’t have this magic wand that would enable us to abruptly shift out of oil.” And that to me is problematic because either you ride on the risk analysis and on the description of this huge opportunity arising, or you ride on the argument that, in fact, these renewable technologies are not scalable. So because we need cheap energy, we need to continue on oil.
And I think the reason why you’re hearing these contradictory arguments is that we are in a very exciting transitional phase right now. Just three, four years back, the argument that we needed cheap energy, fossil fuel energy systems, because we cannot scale novel technologies, was correct when solar was 0.2, 0.3, or up to 1 percent of the energy mix. Today that’s not true at all. China, Germany, parts of the U.S., Denmark are going to scale with wind and solar and biomass in ways that were impossible to predict. In fact they’ve gone totally through the roof compared to any optimistic assessment just three, four years back. So now we’re in a transitional phase where, for the first time, we can say, “Yes, we have the largest planet risk ever, and yes, we have a solution that is scalable.”
So I think he [President Obama] is making a cold calculation that, “I cannot domestically go head-on with all of my desired arguments on a phase-out of fossil fuels — I have to make some compromise.” What he has decided is to allow for exploration. And then count on, in three or four years, oil will not be very attractive. I mean, with current oil prices, there’s no way at all that any oil will be taken out of the Arctic, which is now under sea ice.

e360: Later this month, the U.N. will meet to formally adopt 17 sustainable development goals that will address a wide range of issues. Do you see the concept of planetary boundaries being taken into account in those goals?

Rockström: Yes, I do. The Sustainable Development Goals say that we want world development within quantitative, scientifically defined, global environmental goals. And four of the 17 goals are planetary boundaries.

What keeps me awake at night is the slow pace of change, and that we win one, and then lose one.’
There is a climate goal, a freshwater goal, a biodiversity goal, and an ocean goal.
But actually all the other five boundaries are inside the sustainable development goals. We’re really in a dire state in terms of both social and environmental risks in the world, and we need a new logic where people and planet operate in harmony, and if you translate that to the goals, it’s clear that it’s a world that develops within a safe operating space. It is a shift toward a logic that aligns itself with the planetary boundary framework.

e360:
With climate negotiations set to begin in Paris in about three months, you’ve said that we’ve reached a “Montreal moment in climate.” What do you mean by that?

Rockström:
In 1987, the world agreed to come back to the safe operating space on one of the nine boundaries, namely the depletion of the stratospheric ozone layer — the layer that protects us from dangerous ultraviolet radiation from the sun. Scientists identified the risks from chlorofluorocarbons from refrigerators and cooling systems. And the Montreal Protocol was a phenomenal success. The world actually took itself from a danger zone back into the safe operating space. How did this happen? Well, the industry actually had technologies that it went to scale with and, moreover, actually delivered not only a safer future, but cheaper and more advanced technology. And when you analyze that success, you find that three criteria were in place. One, the science was established, and policy makers and industry believed in the science. The second is that technology was available, and industry was ready to move. And third, you had policy makers that were ready to act.
For climate, these criteria have never been fulfilled. So you’ve had debates on science. You have never been able to talk convincingly about solutions. They’ve never been scalable. Shell and BP will say, “We trust the science, but we are forced to drill for oil, because it’s the only way to power the world economy.” And third, we haven’t had a kind of an alignment in terms of policy. And now, in 2015, for the first time, you actually see that we’ve seen a Montreal moment on climate. Because the science is now so well established, and the technologies are available and scalable. And we have a completely new policy and business recognition that this is not only a risk we need to solve but it’s an opportunity that we can grasp. And that was not there just a few years back.

e360:
Your book has quite an optimistic tone. By your estimation, though, we’ve got a decade to accomplish the mind shift and begin operating within the planetary boundaries. You’ve also said that if bold decisions are taken this year, you’re optimistic that the future will be bright. But what keeps you up at night?

Rockström:
I’m convinced that the world has crossed a social tipping point. We’ve tipped over to a logic where it’s clear that sustainability is the future for humanity. But what keeps me awake at night is the slow pace of change, and that we win one, and then lose one. We see Australia investing in coalmines. We see Canada being a slow mover. We see India with an uncertain position. We see a world that is in a very nervous state with regards to terrorism, fundamentalist Islamic movements, and the economy.
So with all of this social, geopolitical turbulence and ups and downs, when it comes to really moving forward on solving the climate challenge and grasping the opportunities, will we really be able to turn the tide in five to ten years? Will we be able to avoid the earth system pushing these hard-wired “on” buttons that will take us irreversibly in the wrong direction? So it’s a very interesting moment right now. There’s never been a reason to be so nervous as today, but never has there been so much reason for hope as today. And the question is where will we take it.
POSTED ON 23 Sep 2015 IN Biodiversity Business & Innovation Climate Climate Energy Policy & Politics Sustainability Africa Europe
 

http://e360.yale.edu/feature/one_scientists_hopeful_view_on_how_to_repair_the_planet/2913/

Muum’s D Cafe in Turkey is a flexible daylit space wrapped in recycled metal plates

 

D Cafe in Kocaeli Province in Turkey, a corporate campus for automotive importer Dogus Automotive AS, is an innovative cafe space wrapped in layers ofrecycled metal plates. Combined with large glass-to-ceiling windows, the metal skin frames a user-friendly social space where the company employees can interact and socialize. Istanbul-based design firm Muum designed the building as a flexible space that blends the border between inside and outside, to give employees a dose of nature while relaxing.

Through the use of an integrated design approach, the architects created a consistent visual and formal language that makes the facade and the volume of the building appear as a unified whole. One of the most notable design elements is the building’s transparency, which draws natural lighting into the interior and provides a direct connection with the outside.

Related: Inspiring LOSEV center in Turkey teaches visitors how to lead sustainable lives

Perforated anthracite metal plates were arranged in a rhythmic composition and frame the volume of the building, the interior of which looks like it extends into the landscape and the green space in front of the structure. Simple and striking, D Cafe dominates its surroundings and functions as an essentially extroverted space in its more subdued surroundings.

+ Muum

Photos by Anday Bodur

http://inhabitat.com/muums-d-cafe-in-turkey-is-a-flexible-daylit-space-wrapped-in-recycled-metal-plates/