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ITER NEWSLINE 55
In order to keep our schedule, the ITER Organization and the Domestic Agencies need to integrate better. The new tool called "Integrated Product Teams" (IPT) is an important approach in this respect. In its meeting last week, the Management Advisory Committee (MAC) strongly encouraged the IO and the DAs to proceed this way and to implement IPTs as soon as possible.
At this stage, establishing a better way of working together is crucial for the success of this project. Out of the 26 Procurement Arrangements that were scheduled to be signed by end of this year, so far only seven have been signed. So, immediate action to recover the delay is necessary.
As for this coming Council meeting starting on 19 November here in Cadarache, there are some critical subjects on the agenda. The budgets for the following years need to be discussed and IO expects the one for 2009 to be fixed. The long-term accumulative resource estimates for construction period has been subject to an independent review by the panel led by Dr. Frank Briscoe.
It is now also only a few weeks away that our Headquarters will be moving to the new office building on the ITER site. The Council Members will be invited to the inauguration upon their arrival on the first day of its meeting. They will thus see for themselves the impressive progress that has been made on site thanks to our host Agence ITER France. The message is — ITER is on its way.
The ITER VV is a double wall box structure and the space between the inner and outer shells of the VV is filled with pre-assembled or modular blocks. These blocks are called "in-wall shielding". There are two types of IWS: primary IWS provides an effective neutron shielding, while ferromagnetic inserts provide neutron shielding and reduce the toroidal field ripple.
The Indian DA will fabricate and deliver more than 6000 shielding blocks for installation into the VV sectors in Korea and the EU, while yet more blocks will be delivered to ITER for installation in the field joints regions when the VV sectors are assembled at Cadarache. The weight of each neutron shielding plate can vary between 50 and 500 kg depending on its location.
The space between the inner and outer shells of the VV is also used for cooling and so the IWS will be exposed to water. Understandably there was concern regarding corrosion and the radiation levels of the cooling water. Other topics included interfaces with the IWS, electromagnetic loading and ferromagnetic material distribution.
The deadline for the completion of the PA is 20 November, followed by signature by the Indian DA by the end of December 2008.
"This is a landmark experimental paper demonstrating the efficacy of using resonant magnetic field perturbations (RMPs) for the suppression of large amplitude edge localized modes (Type I ELMs); a critical issue for ITER and other reactor grade machines because of the erosion of the divertor target that would occur if ELMs are not controlled", writes the publisher. "This demonstration of ELM suppression without a reduction in H-mode global confinement performance has stimulated much subsequent work in the field, both experimental and theoretical, and encouraged the proposal that a similar RMP coil set be included in the design for ITER. The experiment was based on the expectation that ergodization of the edge magnetic fields could reduce the pressure gradient that drives MHD instability to trigger ELMs. The paper examined the extent to which this is borne out by experiment and raised plasma physics issues which are currently subject to intense examination."
As a service to the nuclear fusion research community, the winning paper will be freely available to read until the end of March 2009 at http://www.iop.org/.
An IO-DA workshop on HAZard and OPerability analysis (HAZOP) took place last week. Together with more that 15 representatives from all seven Domestic Agencies, the ITER Tritium Group and a US consultant went through a first general presentation of the analysis that will be required for all ITER systems wetted by tritium. The HAZOP studies will help to define a safe system design and acceptance criteria for ITER equipment. The method will thus be used to help design all tritium loops within ITER. The two-day training was an initiative of US ITER together with the ITER Tritium group. As a conclusion, the usefulness of this approach was recognized and the implementation plan discussed.
Click here to read the press release...
Even in the event of only a slight injury, you should immediately call the Rescue Team (CEA FLS), by dialling 18 (or cell phone 04 42 25 22 18 — or using the emergency call button). CEA FLS is authorised to look after injured people and to transport them to the Medical Centre; before the arrival of the FLS, the ITER First Aid Team is here to secure the area and carry out first emergency actions.
An Indian-built launcher carrying the one-and-a-half-tonne satellite blasted off from Satish Dhawan Space Centre in Sriharikota, an island off the coast of Andhra Pradesh, at about 06:20 local time (00:50 GMT) last Wednesday 22nd October.
One key objective is to search for surface or sub-surface water-ice on the Moon, especially at the poles.
Another is to detect Helium 3, an isotope which is rare on Earth, but is sought to power nuclear fusion and could be a valuable source of energy in future.
Read more here...
Although the ITER site still looks like a sandy plain with lots of machines working to level the platform, some people within the ITER organization think ahead, way ahead... about 10 years to be exact, when ITER will be up and running!
Didier van Houtte's primary responsibility, as Senior Project Coordinator for RAMI in Project Office, is to make sure that all the systems of the ITER machine will be reliable during the operation phase and maintain their performance under operational conditions with the best possible availability.
The RAMI process, which is based on a functional analysis and a FMECA (Failure Mode Effects and Criticality Analysis) approach, aims to ensure that at all times, the ITER machine is
Failure of only one small function might result in the machine being halted for long periods of time and result in high costs for repairs and replacements. It is therefore important that every system undergoes a risk-analysis to evaluate WHAT can go wrong, WHERE and WHEN, and to recommend spare components, back-up systems, increased frequency maintenance schedules, systems design optimization etc, to reduce the risk level of a main function breakdown to a minimum.
The RAMI approach allows small expenditure on a critical function failure, instead of large expenditure on a unreliable component of a not very important function, while achieving the same result in term of machine availability.
The analysis of all these systems must of course primarily be carried out in the design and procurement phase of the project to make sure RAMI requirements are taken into account when the systems and their critical spare parts are manufactured.
So these are busy times for Didier, soon to be assisted by additional staff for RAMI. He also works with contractors and DAs on some of these specific issues.
Before coming to ITER, Didier worked for Tore Supra where he started in 1986, and was the Head of Operations for 10 years. "One of the fascinating parts of my job here is that I get to work in all the technical fields with all the departments and all the Domestic Agencies. I really enjoy having the opportunity to think ahead to failures that could occur during ITER operation, after having been constrained to do many repairs on certain subsystems of Tore Supra during their operation and construction." he says" which gives me a very broad and interesting perspective on the future operation of the ITER machine."
"Experimenting with toroidal configurations started in the mid 1950s, remembers Vladimir Mukhovatov, now a Senior Scientific Officer with the IO, then a 23 year old researcher, freshly out of Moscow State University. Our 'Sector-44', within the Laboratory of Measuring Apparatus of Academy of Science — the future Kurchatov Institute — was building machines at a very fast pace. When I arrived in 1956 for my graduation thesis, there was a small toroidal device called TMP, originally equipped with a porcelain chamber which was soon improved by adding metal spirals within the chamber. Later two small devices with copper walls and insulating gaps were built."
By "late 1957", according to Mukhovatov's recollection, these devices were succeeded by T-1 which was somewhat larger and marks the "symbolic beginning" of the tokamak adventure. T-1 was the first device to have a stainless steel liner inside a copper vacuum chamber.
Finding a name for this new toroidal concept was to take some time and quite a bit of discussion. "Igor Golovin, then vice-director of the Laboratory, came up with an acronym: 'Tokamak' for Toroidalnaya Kamera i Magnitnaya Katushka (Toroidal Chamber and Magnetic Coil). A combination of "Tok" for electric current and "Mag" for magnetic field, with a connective vowel 'o', which gave "tokomag" or "tokomak" after replacing "G" with "K" for harmony, was also circulated..."
Whether it was 'Tokomag', or 'Tokamak', Lev Artsimovitch, head of Department of Plasma Research, was initially sceptical about the concept. Vladimir Mukhovatov remembers the man "liked to use strong, spectacular, sentences. When engaging in polemics, he would say that 'achieving fusion with a tokamak was the same as trying to create a cigarette out of cigarette smoke'. It's only after experiments on T-2, TM-2 and especially T-3 that he became a strong proponent of tokamaks. And in a way, this led to ITER."
It was even more so in the late 1920s, when the French National Service for Scientific Research decided to create a new observatory to complement the one in Paris, where fog, urban lights and ground vibrations were making observations more and more difficult.
Site studies lasted for several years and in 1936, a wooded plateau, close to the village of Saint-Michel, 12 km to the south-east of Forcalquier, was eventually chosen to host the installation.
For more than a half-century, observing stars and comets, galaxies and asteroids, the Observatoire de Haute-Provence (OHP), was to contribute to the understanding of the Universe.
But in the world of astronomy things were changing fast: new challenges required more powerful instruments, which, in turn, demanded ever more transparent skies and a stable atmosphere. 8 or 10 metre mirrors were becoming the norm, positioned at ever higher altitudes. With its 1.93 metre telescope, peering at the stars from a hilltop a mere 600 metres high, the OHP, once among the leading observatories in Europe, was under threat.
By the mid 1990's, the place was scheduled to close. At this point, two astronomers from Observatoire de Genève, Switzerland, using a high performance spectrometer coupled to the old "193", made an historical discovery: a planet orbiting a distant star, 48 light-years from the Earth, the first proof that the solar system was not unique in the Universe.
The discovery of this "hot Jupiter" orbiting star 51 Pegasi was to be followed by scores of others. Searching for exoplanets is now one of the observatory's fields of excellence: More than 300 have been discovered to this day, some 30 of them at the OHP.
Needless to say, no one talks about closing the old Provençal observatory anymore.
Researchers at the University of California, Los Angeles, have shown that simply peeling ordinary sticky tape in a vacuum can generate enough X-rays to take an image. The researchers suggest that the high charge density generated by peeling the tape could be great enough to trigger nuclear fusion.