Henrik Bindslev has been appointed today as the new Director of the European Joint Undertaking for ITER and the Development of Fusion Energy (Fusion for Energy). He is currently the Vice Dean for Research at Aarhus University, Faculty of Science and Technology.
Stuart Ward, Chair of the Fusion for Energy Governing Board, took the opportunity to congratulate Henrik Bindslev on his new position and thanked all members of the Board for their collaboration taking together this important decision. 

"I am honoured to have been appointed Director of Fusion for Energy at a time that Europe’s contribution to ITER enters a decisive stage and rapid progress will be made on all fronts. It is the moment to engage actively with Europe’s industry and fusion community to honour our commitment to this prestigious international project" said Bindslev.

Henrik Bindslev has been engaged in energy research for more than 20 years and has considerable experience in research management, both in Denmark and internationally. He is currently Vice Dean for research at Aarhus University, Faculty of Science and Technology and past Chair of the European Energy Research Alliance (EERA). He is a delegate to the European Strategy Forum on Research Infrastructures (ESFRI) and Chairman of ESFRI’s Energy Strategy Working Group. Previously, he was the Director of Risø DTU, the Danish National Laboratory for Sustainable Energy, managing 700 members of staff. 
He was educated at Denmark’s Technical University and completed a DPhil in Plasma Physics at the University of Oxford. He worked as a fusion researcher at different facilities including ten years at the Joint European Torus (JET), Europe’s biggest fusion research device, and has published more than 150 papers.

The Director is appointed by Fusion for Energy’s Governing Board for a period of five years, once renewable up to five years. The appointment is made on the basis of a list of candidates proposed by the European Commission after an open competition, following a publication in the Official Journal of the European Communities.

Source: F4E

One of the most interesting refurbishment tasks for JET this year is costing over half a million euros, extending the lifetime of JET and reducing operating costs.

The original construction of JET’s site cooling water system was carried out under two separate contracts. The pipework in the immediate area of the cooling towers passed its original design lifetime long ago and continued to work successfully. However, for the last four or five years it has been plagued with a series of chronic water leaks. This has not been enough to interrupt operations, but it was certainly sufficient to have a noticeable impact on running costs. Water leaking from the system has to be replaced with fresh water, which has to be specially treated before it can be used.

Remarkably, the pipes around the rest of the site are still in good condition, thanks to the choice of cast iron as opposed to mild steel in the corroded sections. It was originally hoped that the leaking pipes could be repaired using ‘trenchless technology’ where a leak-tight lining is installed inside the pipes without disturbing the ground. Several companies expressed an interest in the task, but in the end none of them tendered. Consequently a contract has been placed with a company to design, fabricate install and test about 200m of pipe as large as 700mm in diameter. Since August, trenches have been dug and much of the old pipework has been removed. It is being replaced by new pipes of the same material, carbon steel with a bitumen coating. These are likely to be serviceable for at least 20 years. This large operation has progressed according to plan, and by early November the task should be complete, pressure tests will have been carried out, and the performance of the system demonstrated against benchmark measurements that were taken on the old system.

Source: EFDA

In the high-stakes race to realize fusion energy, a smaller lab may be putting the squeeze on the big boys. Worldwide efforts to harness fusion—the power source of the sun and stars—for energy on Earth currently focus on two multibillion dollar facilities: the ITER fusion reactor in France and the National Ignition Facility (NIF) in California. But other, cheaper approaches exist—and one of them may have a chance to be the first to reach “break-even,” a key milestone in which a process produces more energy than needed to trigger the fusion reaction.

Researchers at the Sandia National Laboratory in Albuquerque, New Mexico, will announce in a Physical Review Letters (PRL) paper accepted for publication that their process, known as magnetized liner inertial fusion (MagLIF) and first proposed 2 years ago, has passed the first of three tests, putting it on track for an attempt at the coveted break-even. Tests of the remaining components of the process will continue next year, and the team expects to take its first shot at fusion before the end of 2013.

Fusion reactors heat and squeeze a plasma—an ionized gas—composed of the hydrogen isotopes deuterium and tritium, compressing the isotopes until their nuclei overcome their mutual repulsion and fuse together. Out of this pressure-cooker emerge helium nuclei, neutrons, and a lot of energy. The temperature required for fusion is more than 100 million°C—so you have to put a lot of energy in before you start to get anything out. ITER and NIF are planning to attack this problem in different ways. ITER, which will be finished in 2019 or 2020, will attempt fusion by containing a plasma with enormous magnetic fields and heating it with particle beams and radio waves. NIF, in contrast, takes a tiny capsule filled with hydrogen fuel and crushes it with a powerful laser pulse. NIF has been operating for a few years but has yet to achieve break-even.

Sandia’s MagLIF technique is similar to NIF’s in that it rapidly crushes its fuel—a process known as inertial confinement fusion. But to do it, MagLIF uses a magnetic pulse rather than lasers. The target in MagLIF is a tiny cylinder about 7 millimeters in diameter; it’s made of beryllium and filled with deuterium and tritium. The cylinder, known as a liner, is connected to Sandia’s vast electrical pulse generator (called the Z machine), which can deliver 26 million amps in a pulse lasting milliseconds or less. That much current passing down the walls of the cylinder creates a magnetic field that exerts an inward force on the liner’s walls, instantly crushing it—and compressing and heating the fusion fuel.

Researchers have known about this technique of crushing a liner to heat the fusion fuel for some time. But the MagLIF-Z machine setup on its own didn’t produce quite enough heat; something extra was needed to make the process capable of reaching break-even. Sandia researcher Steve Slutz led a team that investigated various enhancements through computer simulations of the process. In a paper published in Physics of Plasmas in 2010, the team predicted that break-even could be reached with three enhancements.

First, they needed to apply the current pulse much more quickly, in just 100 nanoseconds, to increase the implosion velocity. They would also preheat the hydrogen fuel inside the liner with a laser pulse just before the Z machine kicks in. And finally, they would position two electrical coils around the liner, one at each end. These coils produce a magnetic field that links the two coils, wrapping the liner in a magnetic blanket. The magnetic blanket prevents charged particles, such as electrons and helium nuclei, from escaping and cooling the plasma—so the temperature stays hot.

Sandia plasma physicist Ryan McBride is leading the effort to see if the simulations are correct. The first item on the list is testing the rapid compression of the liner. One critical parameter is the thickness of the liner wall: The thinner the wall, the faster it will be accelerated by the magnetic pulse. But the wall material also starts to evaporate away during the pulse, and if it breaks up too early, it will spoil the compression. On the other hand, if the wall is too thick, it won’t reach a high enough velocity. “There’s a sweet spot in the middle where it stays intact and you still get a pretty good implosion velocity,” McBride says.

To test the predicted sweet spot, McBride and his team set up an elaborate imaging system that involved blasting a sample of manganese with a high-powered laser (actually a NIF prototype moved to Sandia) to produce x-rays. By shining the x-rays through the liner at various stages in its implosion, the researchers could image what was going on. They found that at the sweet-spot thickness, the liner held its shape right through the implosion. “It performed as predicted,” McBride says. The team aims to test the other two enhancements—the laser preheating and the magnetic blanket—in the coming year, and then put it all together to take a shot at break-even before the end of 2013.

Earlier this year, Slutz and his team published other simulations in PRL that showed that if a more powerful pulse generator was built to produce higher currents—say, 60 million amps—the system could achieve not just break-even, but high gain. In other words, the MagLIF could produce the kind of energy needed for a commercial fusion power plant.

“I am excited about Sandia discovering that magnetized target fusion … is a pathway to significant gain on the Z machine. We agree, and hope that their experiments get a chance to try it out,” says Glen Wurden, the magnetized plasma team leader at Los Alamos National Laboratory in New Mexico.

Daniel Clery, ScienceNOW

For more information visit: www.wired.com

Ignition research continues at the giant laser facility, but the end of the calendar year looks like a more significant date than that set by Congress.

Staff at the National Ignition Facility (NIF) say that work to generate inertial confinement fusion with energy gain will continue as planned, despite the end of the official “ignition campaign” last week.

September 30 saw the expiration of an arbitrary “deadline” for achieving ignition that was set by US Congress, prompting speculation about the future of the laboratory, whose primary function is to simulate the physics of nuclear weapons, but for which fusion energy has become another long-term development target.

Just before that date, which marked the end of the US government’s financial year rather than anything of more scientific significance, a New York Times article suggested that the failure to meet the ignition goal could have “serious repercussions” for not only the giant Lawrence Livermore National Laboratory project (estimated cost so far: $5 billion), but federal financing of “big science” in general. A follow-up editorial in the same newspaper added that Congress would need to look hard at whether either of the “stockpile stewardship” or long-term energy goals could be pursued on a smaller budget.

NIF officials have long expressed their confidence that the system will eventually succeed in “bringing star power to Earth”, as a giant banner at the facility puts it, and told optics.org earlier this year that it was “tantalizingly close” to that goal. But others, including those working on the rival magnetic confinement approach to fusion, are more skeptical, doubting that the laser technique will ever work on a scale that makes for a practical energy source.

A memorandum to the Department of Energy dated July 19 added fuel to that skepticism, even though advisor and memo author David Crandall wrote that the functionality of the laser, its diagnostics, optics and targets – as well as the laser operations performed by the NIF team - were all “outstanding”.

The problem was that the same memo also noted that “considerable hurdles” must still be overcome to reach the ignition goal, or to observe unequivocally the phenomenon of alpha heating – a key element of the fusion process. Given those issues, Crandall and his fellow reviewers said that the probability of demonstrating ignition before the end of this year was now “extremely low”, and that even the less ambitious goal of showing unambiguous alpha heating would be “challenging”.

“While no reviewer thought ignition likely before December 31, 2012, some thought the intermediate goal of measurable alpha heating (increasing the neutron yield) might be achieved within that time, and several expressed optimism about achieving ignition at NIF within a few years,” concluded the memo.

Model problems
According to the same document, the reason has nothing to do with NIF not working to its specifications – on the contrary, the 192-beam system is actually outperforming expectations in many areas. The key problem seems to be that the “hohlraum” ignition target and its interaction with the laser is not behaving in the way that physical models had predicted.

“The coupling of the laser through the radiation inside the hohlraum to the capsule is less efficient than expected and the physical ablation process is somewhat different than expected - resulting in a lower implosion velocity than is predicted to be required for ignition,” the review panel wrote.

NIF told optics.org that it was working to resolve what it called the “remaining few issues” towards achieving ignition in its current campaign. According to officials, that campaign has so far been able to demonstrate the fundamental conditions required to achieve ignition – though, crucially, not all at the same time.

“Achieving ignition conditions requires four things,” the lab explained. “An implosion velocity of 370 km/second, creating a symmetrical hot spot at the center of the target, proper plasma mix and uniform compression.”

On the question of alpha heating, NIF says that alpha particles have been produced from fusion reactions, and have compressed fuel to a sufficient density to re-deposit energy.

However, the lab concedes that its experiments have not yet produced the kind of results that had been predicted in its models, and said that it was continually refining these as more experimental data was collected. It is also working to produce even higher laser energy pulses (of 2 MJ, compared with the 1.8 MJ thought to be sufficient) as one way to overcome the less efficient coupling between the laser and hohlraum than was initially expected.

In demand

“September 30 marked the end of the National Ignition Campaign, but does not mark the end of ignition research or an expiration of the value of the facility,” said officials. Highlighting the scientific value of the system, they added: “As a measure of its success, there are now requests from its user communities for more than 500 experiment days in 2013, about twice the NIF capacity. Requests for use of NIF extend for many years into the future.”

As things stand, NIF will be able to continue operations as planned through fiscal year 2013, though its funding beyond that remains to be determined by future government budget cycles.

Responding to the reaction to the expiration of the Congress “deadline” in some quarters, the lab stressed the unpredictable nature of the work, saying: “Ignition experiments on NIF are continuing steps in a well-managed and deliberate scientific program, not the ‘pass/fail’ event that it has become - and one that should be tied to the process of discovery science and the expansion of knowledge, not fiscal year boundaries.”

In fact, it looks like the end of this calendar year could turn out to be a much more significant date than September 30, in terms of NIF’s future direction and the ambitious goal of harnessing “star power” on Earth. Crandall’s memo raises the prospect that NIF will take on a quite different role if experimental results and computer models for ignition continue to contradict each other.

The memo states that if alpha heating and “further substantial progress” towards ignition is not demonstrated before the end of December, the ignition program should be redirected to a “broader and more balanced research program” – suggesting that the pursuit of fusion power will take a back seat.

Mike Hatcher

Editor in Chief of optics.org

For more information visit: www.optics.org

Good news, denizens of Earth: If the findings from two premier research labs are to be believed, commercial nuclear fusion is feasible — and could arrive sooner than expected.

The first breakthrough comes from Sandia National Laboratories (the same engineers who brought us the fanless heatsink). At SNL, a research team has been working on a new way of creating fusion called magnetized liner inertial fusion (MagLIF). This approach is quite similar to the National Ignition Facility at the LLNL in California, where they fuse deuterium and tritium (hydrogen isotopes) by crushing and heating the fuel with 500 trillion watts of laser power. Instead of lasers, MagLIF uses a massive magnetic pulse (26 million amps), created by Sandia’s Z Machine (a huge X-ray generator), to crush a small cylinder containing the hydrogen fuel. Through various optimizations, the researchers discovered a MagLIF setup that almost breaks even (i.e. it almost produces more thermal energy than the electrical energy required to begin the fusion reaction).

Probably more significant is news from the Joint European Torus (JET), a magnetic confinement fusion facility in the UK. JET is very similar to the ITER nuclear fusion reactor, an international project which is being built in the south of France. Whereas NIF and Sandia create an instantaneous fusion reaction using heat and pressure, ITER and JET confine the fusing plasma for a much longer duration using strong magnetic fields, and are thus more inclined towards the steady production of electricity. JET’s breakthrough was the installation of a new beryllium-lined wall and tungsten floor inside the tokamak — the doughnut-shaped inner vessel that confines 11-million-degrees-Celsius plasma (pictured above).

Carbon is the conventional tokamak lining (and the lining that had been chosen for the first iteration of ITER) but now it seems the beryllium-tungsten combo significantly improves the quality of the plasma. Hopefully this information will allow ITER to skip the carbon tokamak and jump straight to beryllium-tungsten, shaving years and millions of dollars off the project.

Moving forward, JET will actually try full-blown fusion with the optimum mix of deuterium and tritium (16 megawatts, for less than a second). At this point, JET is practically an ITER testbed, so its results from the next year or two will have a large impact on the construction of ITER’s tokamak, which should be completed by 2019.

Before today, magnetic confinement fusion was generally considered to be more mature and efficient than inertial confinement fusion — but Sandia’s new approach might change that. ITER is one of the world’s largest ongoing engineering projects (it’s expected to cost around $20 billion), and yet critics are quick to point out that we still don’t know if it will actually work. ITER isn’t expected to fuse D-T fuel until 2027 (producing 500 megawatts for up to 1,000 seconds) — and an awful lot can happen in 15 years. Still, the main thing is that we’re actually working on fusion power — when we’re talking about limitless, clean power, it’s probably worth investing a few billion dollars, even if it doesn’t work out.

Fusion reactors are some of the most beautiful constructions you’ll ever see, so be sure to check out our galleries of the National Ignition Facility and the Princeton Plasma Physics Lab.

For more information visit: www.peakoil.com