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2. Robust Chauvenet Outlier Rejection

Author

M. L. Paggen, R. E. Joyner, M. Maples, A. S. Trotter, J. R. Martin, Travis A. Berger, D. A. Dutton, C. P. Salemi, N. C. Konz, and Daniel E. Reichart

Subjects
FOS: Computer and information sciences, Physics, Central tendency, Sample (material), FOS: Physical sciences, Sigma, Astronomy and Astrophysics, Chauvenet's criterion, 01 natural sciences, Statistics - Computation, Standard deviation, 010104 statistics & probability, Clipping (photography), Space and Planetary Science, 0103 physical sciences, Statistics, Outlier, Fraction (mathematics), 0101 mathematics, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, Computation (stat.CO)
Abstract

Sigma clipping is commonly used in astronomy for outlier rejection, but the number of standard deviations beyond which one should clip data from a sample ultimately depends on the size of the sample. Chauvenet rejection is one of the oldest, and simplest, ways to account for this, but, like sigma clipping, depends on the sample's mean and standard deviation, neither of which are robust quantities: Both are easily contaminated by the very outliers they are being used to reject. Many, more robust measures of central tendency, and of sample deviation, exist, but each has a tradeoff with precision. Here, we demonstrate that outlier rejection can be both very robust and very precise if decreasingly robust but increasingly precise techniques are applied in sequence. To this end, we present a variation on Chauvenet rejection that we call "robust" Chauvenet rejection (RCR), which uses three decreasingly robust/increasingly precise measures of central tendency, and four decreasingly robust/increasingly precise measures of sample deviation. We show this sequential approach to be very effective for a wide variety of contaminant types, even when a significant -- even dominant -- fraction of the sample is contaminated, and especially when the contaminants are strong. Furthermore, we have developed a bulk-rejection variant, to significantly decrease computing times, and RCR can be applied both to weighted data, and when fitting parameterized models to data. We present aperture photometry in a contaminated, crowded field as an example. RCR may be used by anyone at https://skynet.unc.edu/rcr, and source code is available there as well., 62 pages, 48 figures, 7 tables, accepted for publication in ApJS

Published
2018

3. Easy use of high performance computers for fusion simulations

Author

F. Imbeaux, C. Konz, D. P. Coster, B. Guillerminet, Y. Frauel, Bruce D. Scott, M. Plociennik, M. Owsiak, Pär Strand, and A. Jackson

Subjects
Fusion, Tokamak, Computer science, End user, Mechanical Engineering, Distributed computing, Grid, Supercomputer, law.invention, Plasma edge, Nuclear Energy and Engineering, Physics::Plasma Physics, law, General Materials Science, Civil and Structural Engineering
Abstract

Fusion Modelling and Simulation are very challenging and the high performance computing issues are addressed here. Based on the framework developed by the European Integrated Tokamak Modelling project and on the EUFORIA infrastructure, a tool solving nicely these difficulties has been developed for the end users and applied to several fusion simulation cases. The first part recalls the issues with GRID and high performance computing, while the second part presents the solutions and the tool for developing easily a GRID/HPC actor. The last part reports the use of this tool in MHD equilibrium and plasma edge simulations.

Published
2012
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4. Amplitude, frequency, and timbre with the French horn

Author

Michael J. Ruiz and N. C. Konz

Subjects
Auditory perception, Science instruction, 05 social sciences, 050301 education, General Physics and Astronomy, 01 natural sciences, Linguistics, Education, Amplitude, 0103 physical sciences, Intonation (music), Video technology, 010306 general physics, 0503 education, Timbre
Published
2018
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5. Fecal Containment in Bedridden Patients: Economic Impact of 2 Commercial Bowel Catheter Systems

Author

Barbara Barnett, Mary DeSane, Sara Jane Salstrom, Elizabeth C. Konz, John W. Mah, Bruce Potenza, Areta Kowal-Vern, Mary Majewski, Michael Koenig, Michael Tan, Malford E. Cullum, Elizabeth Stokes, Michelle Ferrari, Linda L. Morris, Jan Powers, Shirley Ambutas, Kathleen Casey, Kathy Berry, Cindy Zaletel, Stathis Poulakidas, Michael R. Riemer, Deborah L. Conway, Jayne Stein, and Daniel Culver

Subjects
medicine.medical_specialty, Critical Care, Cost-Benefit Analysis, Urinary system, Pilot Projects, Critical Care Nursing, Observational period, Catheterization, law.invention, law, medicine, Humans, In patient, Feces, Aged, Pressure Ulcer, Cross Infection, business.industry, Incidence (epidemiology), General Medicine, Intensive care unit, Surgery, Catheter, Urinary Tract Infections, Cost of care, business, Fecal Incontinence
Abstract

Background Fecal contamination is a major challenge in patients in acute/critical care settings that is associated with increased cost of care and supplies and with development of pressure ulcers, incontinence dermatitis, skin and soft tissue infections, and urinary tract infections. Objectives To assess the economic impact of fecal containment in bedridden patients using 2 different indwelling bowel catheters and to compare infection rates between groups. Methods A multicenter, observational study was done at 12 US sites (7 that use catheter A, 5 that use catheter B). Patients were followed from insertion of an indwelling bowel catheter system until the patient left the acute/critical care unit or until 29 days after enrollment, whichever came first. Demographic data, frequency of bedding/dressing changes, incidence of infection, and Braden scores (risk of pressure ulcers) were recorded. Results The study included 146 bedridden patients (76 with catheter A, 70 with catheter B) who had similar Braden scores at enrollment. The rate of bedding/dressing changes per day differed significantly between groups (1.20 for catheter A vs 1.71 for catheter B; P = .004). According to a formula that accounted for personnel resources and laundry cycle costs, catheter A cost $13.94 less per patient per day to use than did catheter B. Catheter A was less likely than was catheter B to be removed during the observational period (P = .03). Observed infection rates were low. Conclusion Catheter A may be more cost-effective than catheter B because it requires fewer unscheduled linen changes per patient day.

Published
2009
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6. Progress in edge plasma transport modeling on JET

Author

G. Corrigan, Anders Nielsen, W. Fundamenski, Markus Airila, Detlev Reiter, Volker Naulin, Xavier Bonnin, D. P. Coster, J. Juul Rasmussen, T. T. Ribeiro, J. D. Strachan, M. Wischmeier, A. V. Chankin, E. Tsitrone, B. Gulejova, S.K. Erents, S. Glowacz, Fabio Subba, R. Zagórski, Odd Erik Garcia, Vladislav Kotov, C. Konz, S. Wiesen, R.A. Pitts, Bruce D. Scott, David Tskhakaya, A. Kirschner, Efda Jet Contributors, P. Belo, and G. Kirnev

Subjects
Physics, Nuclear physics, modelling, Jet (fluid), Web of science, SOL, Divertor, divertor, ELM, Plasma, Edge (geometry), Condensed Matter Physics
Abstract

Recent progress in edge plasma modeling on the JET tokamak is briefly, and somewhat selectively, reviewed. This ongoing modeling activity is aimed at developing a predictive capability for ITER based on numerical models verified and validated upon JET experimental data. Topics include both steady‐state and transient particle and power exhaust, the effect of edge/SOL turbulence and edge localized modes, and first wall material migration.

Published
2008
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7. Discrepancy between modelled and measured radial electric fields in the scrape-off layer of divertor tokamaks: a challenge for 2D fluid codes?

Author

Michael Kaufmann, S.K. Erents, A. V. Chankin, W. Fundamenski, Xavier Bonnin, D. P. Coster, Garrard Conway, C. Konz, H. W. Müller, K. Lackner, M. Wischmeier, J. Neuhauser, A. Kallenbach, G. Corrigan, Nobuyuki Asakura, R.A. Pitts, and J. Horacek

Subjects
Physics, Nuclear and High Energy Physics, Debye sheath, Jet (fluid), Tokamak, Divertor, Collisionality, Condensed Matter Physics, Computational physics, law.invention, symbols.namesake, ASDEX Upgrade, JET, Physics::Plasma Physics, law, symbols, Langmuir probe, Plasma diagnostics, Atomic physics
Abstract

Examination of radial electric field (E,.) profiles in the scrape-off layer (SOL) of ASDEX Upgrade (AUG) and JET revealed large discrepancies between 2D fluid edge modelling and experiment. Experimental profiles of plasma potential (V-p) in the outer (low field) side of the plasma, obtained with reciprocating Langmuir probes, decay radially with electron temperature, T-e, with the -eE(r)/del T-e ratio being > 1.5. In contrast, code simulated E-r are fairly low in most of the SOL (compared with -del T-e/e). Modelling with kinetic treatment of neutrals and drifts was performed using the SOLPS code for AUG cases and EDGE2D-Nimbus for JET cases. Mismatches between modelled and experimental E-r may be caused by the recently established tendency for the SOLPS code to underestimate T-e in the divertor of AUG. It was attributed to non-locality of parallel transport of supra-thermal, heat-carrying electrons originating upstream of the divertor, which are usually only weakly collisional and can penetrate, with few collisions, to the target. Ratios -eE(r)/del T-e obtained from the probe measurements in JET are of order 1.6, while in AUG, JT-60U and TCV they are of order 3. Such high values point to the possibility of fast electrons contributing, apart from target heat fluxes, also to the formation of the Debye sheath. The problem of the underestimation of E-r. in the codes must be closely related with the well-known problem of the underestimation of those parts of parallel ion flows in the SOL that are influenced by the toroidal field direction. It was demonstrated earlier that parallel ion flow at the outer midplane is dominated by the ion Pfirsch-Schluter flow, which in turn is partly driven by the radial electric field. The T-e and E-r discrepancies, as well as discrepancies between simulated and experimental parallel ion flows, raise a question of the validity of fluid codes for the plasma edge modelling and prompt the inclusion of kinetic effects into present-day 2D fluid codes which assume strong collisionality.

Published
2007
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8. SOLPS modelling of ASDEX upgrade H-mode plasma

Author

R. Pugno, C. F. Maggi, L. D. Horton, A. V. Chankin, H. W. Müller, G. Haas, Wolf-Dieter Schneider, A. Herrmann, J. Neuhauser, M. Reich, C. Konz, R. Dux, Ch. Fuchs, Michael Kaufmann, K. Lackner, A. Kallenbach, and D. P. Coster

Subjects
Physics, Divertor, Magnetic confinement fusion, Flux, Plasma, Collisionality, Effective radiated power, Condensed Matter Physics, Computational physics, Nuclear Energy and Engineering, ASDEX Upgrade, Physics::Plasma Physics, Electron temperature, Atomic physics
Abstract

A low density H-mode plasma has been selected for detailed inter-ELM modelling by the SOLPS code package, with the coupled treatment of its plasma (fluid code B2) and neutral (Monte-Carlo code Eirene) parts. Good quality measured midplane density and temperature profiles, covering the pedestal region and stretching far into the SOL, as well as several other parameters and profiles measured in the divertor, have enabled testing the consistency of code solutions with experiment. Once the upstream, midplane profiles have been fitted, and the global parameters (e.g. input power into the computational grid, radiated power) matched, the code reproduces experimental profiles and control parameters in the divertor with an accuracy within a factor of 2. Deviations of modelled parameters from the experiment were found around the strike point position where most of the power was deposited on the target. The deviations are consistent among themselves and all point to one common problem with the modelling: the predicted divertor electron temperature is too low and the density too high, compared with the experiment. The largest inconsistency between the code and experiment was in the magnitude of the peak Hα radiation in the outer divertor, which was larger by a factor of 2 in the code simulations. In addition, the code predicts a somewhat higher sub-divertor neutral flux but lower carbon impurity content in the edge plasma than in the experiment, as well as lower CIII emission. The discrepancy between Hα profiles can to a large degree be attributed to profile effects: the simulated Hα emission profiles are narrower than in the experiment, reflecting the tendency of the neutral–plasma mix to congregate excessively around the strike point in the modelling. At the same time, the integrated Hα emission matches very well with the experiment.Extensive sensitivity studies of the influence of variations in input parameters and assumptions of the code on the modelled divertor conditions have been conducted. They have not resulted in an identification of any SOLPS input/control parameters capable of removing the main disagreement between the code output and experiment. A possibility of parallel transport effects related to low collisionality to increase the effective plasma temperature near the strike point position or of increased perpendicular transport by neutrals (due to some missing reactions in Eirene) to widen the target profiles, will be explored in the future.

Published
2006
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9. Overview of ASDEX Upgrade results—development of integrated operating scenarios for ITER

Author

F. Serra, R. Pugno, S. Klose, A. Herrmann, B. Kurzan, K. Mank, R. Narayanan, Garrard Conway, E. Würsching, O. Gehre, Q. Yu, P. Merkel, U. Seidel, R. Kochergov, T. Eich, K. Krieger, A. Bergmann, M. G. Pacco-Düchs, F. Ryter, C. F. Maggi, M. Balden, P. Martin, R. Riedl, Philipp Lauber, Frank Jenko, I. Radivojevic, L. Giannone, M. Maraschek, B. Zaniol, G. Haas, A. Mück, Gerhard Raupp, C. Tichmann, R. Merkel, H. F. Meyer, E. Strumberger, Martin Jakobi, D. Zasche, G. Becker, M. Garcia Munoz, K. Lackner, Y.P. Chen, W. Sandmann, O. J. W. F. Kardaun, K.-H. Steuer, Analiza M. Silva, F. Braun, A. G. Peeters, O. Gruber, F. Leuterer, A. Lyssoivan, W. Suttrop, A. Kallenbach, V. Mertens, K. K. Kirov, Bruce D. Scott, F. Wesner, Y.-S. Na, M. Münich, E. Quigley, C. Angioni, R. Lorenzini, Ivan Bizyukov, Michael Kaufmann, S. Kálvin, H. P. Zehrfeld, K.H. Behringer, W. Becker, Yasutaro Nishimura, A. Carlson, Daisuke Nishijima, M. Mayer, Hajime Urano, S. Cirant, A. Manini, T. Ribeiro, D. Borba, K. Engelhardt, B. Streibl, Junghee Kim, K. Dimova, H. Meister, M. Troppmann, S. Saarelma, Ursel Fantz, J. Hobirk, S. D. Pinches, F. Monaco, Emanuele Poli, Sheena Menmuir, Marco Brambilla, W. Kraus, A. Geier, H. Maier, S. Schweizer, G. Schramm, D. Merkl, S. W. Yoon, R. Neu, E. Speth, R. Bilato, A. V. Chankin, Thomas Zehetbauer, M. Tsalas, Julia Fuchs, M. Huart, J. Gafert, Fernando Meo, Alexander Kendl, T. Bolzonella, R. Drube, R. Dux, G. Tardini, K. Borrass, B. Heger, G. Pautasso, H. D. Murmann, Th. Pütterich, J. Chen, D. Meisel, K. Behler, J. Schirmer, V. Rohde, Wolf-Dieter Schneider, A. Lohs, G. Gantenbein, K. F. Mast, C. V. Atanasiu, G. Schall, A. Stäbler, A. Buhler, H. W. Müller, P. Varela, D. Strintzi, V. Bobkov, K. Gal, A. C. C. Sips, A. Jacchia, H. Kollotzek, Peter Lang, J. M. Santos, W. Treutterer, M. Apostoliceanu, M. Zilker, J. Neuhauser, M. Reich, P. Franzen, Tilman Dannert, J. Roth, H.-U. Fahrbach, Bernd Heinemann, M. E. Manso, D. A. Hartmann, C. Sihler, J. Stober, L. Fattorini, Isabel L. Nunes, H. Zohm, M. Kick, D. Wagner, A. Keller, Martin Laux, Jari Likonen, Taina Kurki-Suonio, E. Posthumus-Wolfrum, D. P. Coster, J. Schweinzer, G. Kocsis, M. Y. Ye, H. Hohenöcker, H. B. Schilling, C. Konz, P. Mantica, V. Igochine, G. Neu, Sibylle Günter, G. V. Pereverzev, L. D. Horton, Patrick J. McCarthy, M. Foley, A. Lorenz, and J.-M. Noterdaeme

Subjects
Nuclear and High Energy Physics, Materials science, Tokamak, Nuclear engineering, Automatic frequency control, fusion reactors, Electron, Parameter space, 7. Clean energy, 01 natural sciences, Particle transport, Electron cyclotron resonance, 010305 fluids & plasmas, ASDEX Upgrade, ITER, 0103 physical sciences, 010306 general physics, plasma, Magnetic confinement fusion, Condensed Matter Physics, fusion energy, ___, JET, Atomic physics, Control methods
Abstract

Significant progress has been made on ASDEX Upgrade during the last two years in the basic understanding of transport, in the extension of the improved H-mode in parameter space and towards an integrated operating scenario and in the development of control methods for major performance limiting instabilities. The important features were the understanding of particle transport and the control of impurity accumulation based on it, the satisfactory operation with predominantly tungsten-clad walls, the improved H-mode operation over density ranges and for temperature ratios covering (non-simultaneously) the ITER requirements on ν*, n/nGW and Te/Ti, the ELM frequency control by pellet injection and the optimization of NTM suppression by DC-ECCD through variation of the launching angle. From these experiments an integrated scenario has emerged which extrapolates to a 50% improvement in n T τ or a 30% reduction of the required current when compared with the ITER base-line assumptions, with moderately peaked electron and controllable high-Z density profiles.

Published
2005
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10. Characterization of the H-mode edge barrier at ASDEX Upgrade

Author

L.D Horton, A.V Chankin, Y.P Chen, G.D Conway, D.P Coster, T Eich, E Kaveeva, C Konz, B Kurzan, J Neuhauser, I Nunes, M Reich, V Rozhansky, S Saarelma, J Schirmer, J Schweinzer, S Voskoboynikov, E Wolfrum, and the ASDEX Upgrade Team

Subjects
Nuclear and High Energy Physics, Tokamak, Materials science, Magnetic confinement fusion, Plasma, Condensed Matter Physics, law.invention, ASDEX Upgrade, Physics::Plasma Physics, law, Electron temperature, Plasma diagnostics, Magnetohydrodynamics, Atomic physics, Pressure gradient
Abstract

The scaling of the edge transport barrier (ETB) that sustains H-mode plasmas is crucial for the performance of next step tokamaks. At ASDEX Upgrade, the suite of edge diagnostics has been significantly improved to address this issue. High spatial resolution profiles of most of the key edge plasma parameters necessary to determine the magneto hydrodynamic (MHD) stability are now available. New high temporal resolution measurements give clear indications of the nonlinear evolution of the ELM crash. The correlation lengths of edge turbulence have been shown to be correlated with the edge radial electric field shear using a new correlation Doppler reflectometer system. The measured pressure gradient in the ETB is found to be consistent with ideal MHD stability limits, both for Type I and II ELMs. In addition, the edge electron temperature and density gradient lengths are found to be strongly correlated, leaving only the ETB width as a free parameter. In ASDEX Upgrade, the ETB width does not vary significantly over the entire H-mode edge database. Modelling of the transport of comparison discharges in hydrogen and deuterium shows that the expected mass effect on neutral penetration is largely compensated by more efficient heating of deuterium neutrals but requires a transport barrier in both the energy and particle channels in order to reproduce the measured edge temperature and density profiles.

Published
2005
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11. Plasma-neutral gas simulations of reconnection events in cometary tails

Author

C. Konz, Harald Lesch, and G. T. Birk

Subjects
Physics, Comet, Interplanetary medium, Astronomy and Astrophysics, Magnetic reconnection, Astrophysics, Plasma, Solar wind, Physics::Plasma Physics, Space and Planetary Science, Physics::Space Physics, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Heliospheric current sheet, Heliosphere, Excitation
Abstract

The formation and dynamical evolution of cometary plasma tails and magnetic boundary layers is studied by the first numerical plasma-neutral gas simulations. It is shown that collisional interaction between the cometary neutral envelope and the solar wind plasma leads to the formation of a magnetic barrier that separates the entire cometary body from the solar wind. The overall dynamics, in particular, of the magnetotail are governed by magnetic reconnection. Multiple reconnection events are initiated by the localized excitation of anomalous resistivity modeled by η(j). If the comet encounters a heliospheric current sheet, strong disconnection events characterize the cometary plasma tail. But even in the case of homogeneous solar wind conditions, partial disruption of the tail is triggered by dayside reconnection.

Published
2004
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12. Geometric absorption of electromagnetic angular momentum

Author

C. Konz and Gregory Benford

Subjects
Physics, Angular momentum, business.industry, Rotational transition, Atomic and Molecular Physics, and Optics, Electronic, Optical and Magnetic Materials, Optics, Total angular momentum quantum number, Angular momentum of light, Angular momentum coupling, Orbital angular momentum multiplexing, Orbital angular momentum of light, Electrical and Electronic Engineering, Physical and Theoretical Chemistry, Angular momentum operator, business
Abstract

Circularly polarized electromagnetic fields carry both energy and angular momentum. We investigate the conditions under which a circularly polarized wave field transfers angular momentum to a perfectly conducting macroscopic object, using exact electromagnetic wave theory in a steady-state calculation. We find that axisymmetric perfect conductors cannot absorb or radiate angular momentum when illuminated. However, any asymmetry allows absorption. A rigorous, steady-state solution of the boundary value problem for the reflection from a perfectly conducting infinite wedge shows that waves convey angular momentum at the edges of asymmetries. Conductors can also radiate angular momentum, so their geometric absorption coefficient for angular momentum can be negative. Such absorption or radiation depends solely on the specific geometry of the conductor. The geometric absorption coefficient can be as high as 0.8, and the coefficient for radiation can be −0.4, larger than typical material absorption coefficients. We apply the results to recent experiments which spun roof-shaped aluminum sheets with polarized microwave beams. Applications of geometric, instead of material, absorption can be quite varied. Though experiments testing these ideas will be simpler at microwavelengths, the ideas work for optical ones as well.

Published
2003
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13. Rosiglitazone amplifies the benefits of lifestyle intervention measures in long-standing type 2 diabetes mellitus

Author

L. R. Reynolds, Robert C Frederich, James W. Anderson, and Elizabeth C. Konz

Subjects
medicine.medical_specialty, Endocrinology, Diabetes and Metabolism, Blood Pressure, Type 2 diabetes, Placebo, Body Mass Index, law.invention, Placebos, Rosiglitazone, Endocrinology, Randomized controlled trial, law, Weight loss, Internal medicine, Diabetes mellitus, Weight Loss, Diabetes Mellitus, Internal Medicine, medicine, Humans, Hypoglycemic Agents, Obesity, Life Style, Triglycerides, Glycated Hemoglobin, business.industry, Type 2 Diabetes Mellitus, medicine.disease, Thiazoles, Cholesterol, Diabetes Mellitus, Type 2, Physical therapy, Body Constitution, Thiazolidinediones, medicine.symptom, business, Body mass index, Biomarkers
Abstract

Aims: To evaluate the efficacy of a lifestyle intervention programme including meal replacements and increased physical activity upon body weight, diabetes control and other cardiovascular risk factors in obese, poorly controlled, insulin-treated, type-2-diabetic individuals and to assess the impact of concomitant rosiglitazone (RSG) therapy. Methods: This 6-month intervention study included 21 patients with type 2 diabetes mellitus (DM) requiring insulin therapy with haemoglobin A1c (HbA1c) > 7% and with a body mass index (b.m.i.) > 27. All subjects were enrolled in a 6-month lifestyle intervention programme and randomized to placebo or RSG 4 mg/day. Participation in the lifestyle programme included meal replacements, increased intake of fruits and vegetables and increased daily physical activity. Measured end-points included body weight, waist circumference, blood pressure, HbA1c and serum lipids, before entry into the study. Results: The baseline mean b.m.i. was 36.4 and the mean HbA1c was 9.0%. The greatest weight losses occurred during the first 12 weeks (19 lbs for RSG, 13.4 lbs for placebo) with a greater weight loss at each point for the group receiving RSG. Waist circumference declined by 2.8 and 4.0 inches for the placebo and RSG groups. Systolic BP declined 16.2 mmHg in the placebo group and 14.3 mmHg in the RSG group. Diastolic blood pressure decreased by 12.8 mmHg in the placebo group. HbA1c was reduced significantly by 1.3% for the placebo group and 1.1% in the RSG group. Discussion: This study demonstrates the benefits of lifestyle intervention using meal replacements and increased physical activity with resultant modest weight loss in long-standing, poorly controlled type 2 diabetes. RSG did not impede weight loss and, in fact, amplified some of the positive benefits of lifestyle intervention.

Published
2002
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14. Obesity and Disease Management: Effects of Weight Loss on Comorbid Conditions

Author

James W. Anderson and Elizabeth C. Konz

Subjects
Male, medicine.medical_specialty, Endocrinology, Diabetes and Metabolism, Medicine (miscellaneous), Blood Pressure, Coronary Disease, Overweight, Weight Gain, Body Mass Index, chemistry.chemical_compound, Endocrinology, Risk Factors, Weight loss, Internal medicine, Weight Loss, Diabetes Mellitus, medicine, Humans, Obesity, Cholesterol, business.industry, Public Health, Environmental and Occupational Health, medicine.disease, Lipids, Blood pressure, chemistry, Relative risk, Female, medicine.symptom, business, Body mass index, Weight gain, Food Science
Abstract

ANDERSON, JAMES W. AND ELIZABETH C. KONZ. Obesity and disease management: effects of weight loss on comorbid conditions. Obes Res. 2001;9:326S‐334S. Objective: This review is designed to quantitate the effects of obesity and weight gain on risk for coronary heart disease (CHD) and to review the effects of weight loss on CHD risk factors. Research Methods and Procedures: After a comprehensive review of the literature related to body weight and weight gain on CHD risk, the relative risks (RRs) were tabulated. Values were averaged and meta-analysis techniques were used to estimate the variance-adjusted RR. Results: Young persons with higher body mass index values have a significantly higher risk for CHD than do slender young people. For every 1% above a desirable body mass index, the risk for CHD increases by 3.3% for women and by 3.6% for men. Every kilogram of weight gain after high school increases risk for CHD by 5.7% for women and 3.1% for men. Weight loss significantly decreases major CHD risk factors. For every kilogram of weight loss the following favorable changes occur: fasting serum cholesterol, 21.0%; low-density lipoprotein cholesterol, 20.7%; triglycerides, 21.9%; high-density lipoprotein cholesterol, 10.2%; systolic blood pressure, 20.5%; diastolic blood pressure, 20.4%; and blood glucose, 20.2 mM. Discussion: Obesity and/or weight gain are associated with major risk for CHD. Weight loss significantly improves serum lipid parameters, blood pressure, and fasting blood glucose values. Effective treatment approaches are available for most overweight or obese individuals but a major challenge is to enable these individuals to engage in these programs. Professional and consumer education is essential for advancing effective intervention strategies for overweight individuals.

Published
2001
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15. Long-term weight-loss maintenance: a meta-analysis of US studies

Author

Elizabeth C. Konz, James W. Anderson, Robert C Frederich, and Constance L. Wood

Subjects
Adult, Male, Gerontology, Diet, Reducing, MEDLINE, food.diet, Medicine (miscellaneous), Body weight, Design studies, food, Animal science, Primary outcome, Weight loss, Weight Loss, medicine, Humans, Longitudinal Studies, Obesity, Exercise, Nutrition and Dietetics, Kilogram, business.industry, Body Weight, Middle Aged, Anthropometry, United States, Very low calorie diet, Treatment Outcome, Meta-analysis, Female, medicine.symptom, Energy Intake, business, Follow-Up Studies
Abstract

BACKGROUND Current perception is that participants of a structured weight-loss program regain all of their weight loss within 5 y. OBJECTIVE The objective was to examine the long-term weight-loss maintenance of individuals completing a structured weight-loss program. DESIGN Studies were required to 1) have been conducted in the United States, 2) have included participants in a structured weight-loss program, 3) have provided follow-up data with variance estimates for > or =2 y. Primary outcome variables were weight-loss maintenance in kilograms, weight-loss maintenance as a percentage of initial weight loss, and weight loss as a percentage of initial body weight (reduced weight). RESULTS Twenty-nine studies met the inclusion criteria. Successful very-low-energy diets (VLEDs) were associated with significantly greater weight-loss maintenance than were successful hypoenergetic balanced diets (HBDs) at all years of follow-up. The percentage of individuals at 4 or 5 y of follow-up for VLEDs and HBDs were 55.4% and 79.7%, respectively. The results for VLEDs and HBDs, respectively, were as follows: weight-loss maintenance, 7.1 kg (95% CI: 6.1, 8.1 kg) and 2.0 (1.5, 2.5) kg; percentage weight-loss maintenance, 29% (25%, 33%) and 17% (13%, 22%); and reduced weight, 6.6% (5.7%, 7.5%) and 2.1% (1.6%, 2.7%). Weight-loss maintenance did not differ significantly between women and men. Six studies reported that groups who exercised more had significantly greater weight-loss maintenance than did those who exercised less. CONCLUSIONS Five years after completing structured weight-loss programs, the average individual maintained a weight loss of >3 kg and a reduced weight of >3% of initial body weight. After VLEDs or weight loss of > or =20 kg, individuals maintained significantly more weight loss than after HBDs or weight losses of

Published
2001
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16. The Critical Velocity Effect as a Cause for the Hα Emission from the Magellanic Stream

Author

C. Konz, Harald Lesch, G. T. Birk, and H. Wiechen

Subjects
Physics, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Plasma, Critical ionization velocity, Galactic halo, Space and Planetary Science, Ionization, Magellanic Stream, Yield (chemistry), H-alpha, Physics::Atomic Physics, Astrophysics::Galaxy Astrophysics
Abstract

Observations show significant H\alpha-emissions in the Galactic halo near the edges of cold gas clouds of the Magellanic Stream. The source for the ionization of the cold gas is still a widely open question. In our paper we discuss the critical velocity effect as a possible explanation for the observed H\alpha-emission. The critical velocity effect can yield a fast ionization of cold gas if this neutral gas passes through a magnetized plasma under suitable conditions. We show that for parameters that are typical for the Magellanic Stream the critical velocity effect has to be considered as a possible ionization source of high relevance., Comment: 9 pages, 2 figures. accepted, to appear in The Astrophysical Journal

Published
2001
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18. Feasibility Study of Economics and Performance of Solar Photovoltaics at the Crazy Horse Landfill Site in Salinas, California. A Study Prepared in Partnership with the Environmental Protection Agency for the RE-Powering America's Land Initiative: Siting Renewable Energy on Potentially Contaminated Land and Mine Sites

Author

B. Stoltenberg, G. Mosey, and C. Konz

Subjects
Engineering, Brownfield, business.industry, Environmental protection, General partnership, Market transformation, business, Superfund, Solar energy, Net metering, Renewable energy, Contaminated land
Published
2013
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19. Overview of ASDEX Upgrade results

Author

A. Kallenbach, J. Adamek, L. Aho-Mantila, S. Äkäslompolo, C. Angioni, C.V. Atanasiu, M. Balden, K. Behler, E. Belonohy, A. Bergmann, M. Bernert, R. Bilato, V. Bobkov, J. Boom, A. Bottino, F. Braun, M. Brüdgam, A. Buhler, A. Burckhart, A. Chankin, I.G.J. Classen, G.D. Conway, D.P. Coster, P. de Marné, R. D'Inca, R. Drube, R. Dux, T. Eich, N. Endstrasser, K. Engelhardt, B. Esposito, E. Fable, H.-U. Fahrbach, L. Fattorini, R. Fischer, A. Flaws, H. Fünfgelder, J.C. Fuchs, K. Gál, M. García Muñoz, B. Geiger, M. Gemisic Adamov, L. Giannone, C. Giroud, T. Görler, S. da Graca, H. Greuner, O. Gruber, A. Gude, S. Günter, G. Haas, A.H. Hakola, D. Hangan, T. Happel, T. Hauff, B. Heinemann, A. Herrmann, N. Hicks, J. Hobirk, H. Höhnle, M. Hölzl, C. Hopf, L. Horton, M. Huart, V. Igochine, C. Ionita, A. Janzer, F. Jenko, C.-P. Käsemann, S. Kálvin, O. Kardaun, M. Kaufmann, A. Kirk, H.-J. Klingshirn, M. Kocan, G. Kocsis, H. Kollotzek, C. Konz, R. Koslowski, K. Krieger, T. Kurki-Suonio, B. Kurzan, K. Lackner, P.T. Lang, P. Lauber, M. Laux, F. Leipold, F. Leuterer, A. Lohs, N.C. Luhmann, T. Lunt, A. Lyssoivan, H. Maier, C. Maggi, K. Mank, M.-E. Manso, M. Maraschek, P. Martin, M. Mayer, P.J. McCarthy, R. McDermott, H. Meister, L. Menchero, F. Meo, P. Merkel, R. Merkel, V. Mertens, F. Merz, A. Mlynek, F. Monaco, H.W. Müller, M. Münich, H. Murmann, G. Neu, R. Neu, B. Nold, J.-M. Noterdaeme, H.K. Park, G. Pautasso, G. Pereverzev, Y. Podoba, F. Pompon, E. Poli, K. Polochiy, S. Potzel, M. Prechtl, M.J. Püschel, T. Pütterich, S.K. Rathgeber, G. Raupp, M. Reich, B. Reiter, T. Ribeiro, R. Riedl, V. Rohde, J. Roth, M. Rott, F. Ryter, W. Sandmann, J. Santos, K. Sassenberg, P. Sauter, A. Scarabosio, G. Schall, K. Schmid, P.A. Schneider, W. Schneider, G. Schramm, R. Schrittwieser, J. Schweinzer, B. Scott, M. Sempf, F. Serra, M. Sertoli, M. Siccinio, A. Sigalov, A. Silva, A.C.C. Sips, F. Sommer, A. Stäbler, J. Stober, B. Streibl, E. Strumberger, K. Sugiyama, W. Suttrop, T. Szepesi, G. Tardini, C. Tichmann, D. Told, W. Treutterer, L. Urso, P. Varela, J. Vincente, N. Vianello, T. Vierle, E. Viezzer, C. Vorpahl, D. Wagner, A. Weller, R. Wenninger, B. Wieland, C. Wigger, M. Willensdorfer, M. Wischmeier, E. Wolfrum, E. Würsching, D. Yadikin, Q. Yu, I. Zammuto, D. Zasche, T. Zehetbauer, Y. Zhang, M. Zilker, H. Zohm, and Science and Technology of Nuclear Fusion

Subjects
PHYSICS, Nuclear and High Energy Physics, 0103 physical sciences, TOKAMAK, 010306 general physics, Condensed Matter Physics, 7. Clean energy, 01 natural sciences, 010305 fluids & plasmas, REFLECTOMETRY
Abstract

The ASDEX Upgrade programme is directed towards physics input to critical elements of the ITER design and the preparation of ITER operation, as well as addressing physics issues for a future DEMO design. After the finalization of the tungsten coating of the plasma facing components, the re-availability of all flywheel-generators allowed high-power operation with up to 20 MW heating power at I p up to 1.2 MA. Implementation of alternative ECRH schemes (140 GHz O2- and X3-mode) facilitated central heating above n e = 1.2 × 1020 m−3 and low q 95 operation at B t = 1.8 T. Central O2-mode heating was successfully used in high P/R discharges with 20 MW total heating power and divertor load control with nitrogen seeding. Improved energy confinement is obtained with nitrogen seeding both for type-I and type-III ELMy conditions. The main contributor is increased plasma temperature, no significant changes in the density profile have been observed. This behaviour may be explained by higher pedestal temperatures caused by ion dilution in combination with a pressure limited pedestal and hollow nitrogen profiles. Core particle transport simulations with gyrokinetic calculations have been benchmarked by dedicated discharges using variations of the ECRH deposition location. The reaction of normalized electron density gradients to variations of temperature gradients and the T e/T i ratio could be well reproduced. Doppler reflectometry studies at the L–H transition allowed the disentanglement of the interplay between the oscillatory geodesic acoustic modes, turbulent fluctuations and the mean equilibrium E × B flow in the edge negative E r well region just inside the separatrix. Improved pedestal diagnostics revealed also a refined picture of the pedestal transport in the fully developed H-mode type-I ELM cycle. Impurity ion transport turned out to be neoclassical in between ELMs. Electron and energy transport remain anomalous, but exhibit different recovery time scales after an ELM. After recovery of the pre-ELM profiles, strong fluctuations develop in the gradients of n e and T e. The occurrence of the next ELM cannot be explained by the local current diffusion time scale, since this turns out to be too short. Fast ion losses induced by shear Alfvén eigenmodes have been investigated by time-resolved energy and pitch angle measurements. This allowed the separation of the convective and diffusive loss mechanisms.

Published
2011
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20. Lessons learned from jointly using HTC- and HPC-driven e-Science infrastructures in fusion science

Author

C. Konz, David Tskhakaya, Achim Streit, M.S. Memon, Th. Lippert, A.S. Memon, Morris Riedel, Marcin Plociennik, Felix Wolf, and Michal Owsiak

Subjects
business.industry, Computer science, Interoperability, computer.software_genre, Grid, Workflow, Grid computing, Open standard, Middleware (distributed applications), e-Science, Operating system, High-throughput computing, Software engineering, business, computer
Abstract

The interoperability of e-Science infrastructures like DEISA/PRACE and EGEE/EGI is an increasing demand for a wide variety of cross-Grid applications, but interoperability based on common open standards adopted by Grid middleware is only starting to emerge and is not broadly provided today. In earlier work, we have shown how refined open standards form a reference model, which is based on careful academic analysis of lessons learned obtained from production cross-Grid applications that require access to both, High Throughput Computing (HTC) resources as well as High Performance Computing (HPC) resources. This paper provides insights in several concepts of this reference model with a particular focus on the finding of using HPC and HTC resources with the fusion applications BIT1 and a cross-infrastructure workflow based on the HELENA and ILSA fusion applications. Based on lessons learned over years gained with production interoperability setups and experimental interoperability work between production Grids like EGEE, DEISA, and NorduGrid, we illustrate how open Grid standards (e.g. OGSA-BES, JSDL, GLUE2, etc) can be used to overcome several limitations of the production architecture of the EUFORIA framework paving the way to a more standards-based and thus more maintainable and efficient solution.

Published
2010
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21. Addendum to papers from Axially Symmetric Divertor Experiment (ASDEX) Upgrade Team, published in Review of Scientific Instruments

Author

T. Eich, D. Yadikin, P. de Marne, Piero Martin, C. Tichmann, T. Lunt, K. Behler, A. Kammel, E. Strumberger, G. Tardini, K.H. Behringer, G. D. Conway, Bill Scott, F. Monaco, M. Rott, Manfred Zilker, A. Stäbler, K. Krieger, Taina Kurki-Suonio, G. Haas, G. Koscis, B. Streibl, R. Merkel, M. Mantsinen, L. Urso, B. Langer, A. Gude, A. Kirk, J. Stober, H. Doerk-Bendig, T. Hauff, M. Gemisic Adamov, G. Schall, H. Zohm, H.-J. Klingshirn, Karl Schmid, J. M. Santos, Emanuele Poli, K. McCormick, J. Neuhauser, A. Kagarmanov, J. Hobirk, D. Wagner, D. Zasche, Fernando Meo, A. Herrmann, Michael Kaufmann, W. Suttrop, E. Würsching, M. Reich, C. Angioni, G. Pautasso, N. Hicks, G. Antar, C. Wigger, B. Kurzan, H. Meister, Wolf-Dieter Schneider, V. Rohde, C. Vorpahl, Martin Laux, A. Lohs, Jari Likonen, M. Sertoli, D. P. Coster, P. Varela, O. J. W. F. Kardaun, J. Schweinzer, A. Lyssoivan, C. Konz, M. Püschel, M. Manso, L. Fattorini, S. Kálvin, K. Gal, H. Greuner, S. da Graca, Analiza M. Silva, Marco Brambilla, E. Wolfrum, K. Sassenberg, R. Bilato, M. Huart, R. Fischer, M. Münich, K. Mank, V. Mertens, H. Kollotzek, P. Merkel, L. Giannone, H. D. Murmann, N. Hammer, M. Sempf, M. Hölzl, M. Maraschek, Peter Lang, B. Reiter, Sibylle Günter, J. Roth, Lin Liu, H.-U. Fahrbach, Bernd Heinemann, P. Sauter, W. Treutterer, C. V. Atanasiu, I. Classen, U. Seidel, G. V. Pereverzev, Roman Schrittwieser, O. Gruber, R. Riedl, Cary Forest, Patrick J. McCarthy, A. Bergmann, Julia Fuchs, Philipp Lauber, V. Igochine, J. Adamek, F. Ryter, S. Potzel, Tobias Görler, M. Janzer, H. W. Müller, M. Brüdgam, F. Merz, E. Speth, A. Mlynek, M. Garcia-Munoz, F. Serra, E. Vainonen-Ahlgren, M. Balden, J.-M. Noterdaeme, M. Kick, H. F. Meyer, N. Endstrasser, A. V. Chankin, Gerhard Raupp, Mattia Siccinio, Frank Jenko, K.-H. Steuer, Alberto Bottino, K. Engelhardt, T. Pütterich, Q. Yu, R. Drube, R. Dux, A. Sigalov, K. Lackner, Christian Hopf, W. Sandmann, A. Scarabosio, A. Buhler, A. Kallenbach, Thomas Zehetbauer, T. Ribeiro, R. Neu, R. M. McDermott, M. Mayer, R. D’Inca, D. Holtum, F. Braun, G. Neu, B. Nold, J. E. Boom, D. Dodt, R. Stadler, S. Gori, V. Bobkov, M. Wischmeier, F. Leuterer, Peter Schneider, and W. Becker

Subjects
Scientific instrument, Physics, ASDEX Upgrade, Divertor, Nuclear engineering, Addendum, Axial symmetry, Instrumentation, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries)
Abstract

This addendum applies to papers authored by contributors from the Axially Symmetric Divertor Experiment (ASDEX) Upgrade Team published in Review of Scientific Instruments. This addendum provides the full list of ASDEX Upgrade Team contributors and their affiliations.

Published
2010
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22. Cladding Performance of High-Rise Buildings in the Houston CBD during Hurricane Ike

Author

Rolando E. Vega and Robert C. Konz

Subjects
Cladding (construction), Engineering, Glazing, Meteorology, business.industry, Wind gust, business, Central business district, High rise
Abstract

In 1983, Hurricane Alicia caused extensive glazing damage to high-rise buildings in the Central Business District (CBD) of Houston with fastest-mile winds reaching 80 mph (∼94 mph 3-second gust). Twenty five years later, Hurricane Ike also passed near the Houston CBD causing significant glazing damage despite 15–20% lower wind speeds. Straightforward kinetic energy calculations of hurricane Alicia and Ike show that Ike can cause comparable or even more damage than Alicia if cladding components start failing at 60 mph (1-min) winds. While both hurricanes followed virtually identical headings, Alicia passed west of the CBD and Ike to the east, providing a unique opportunity to understand extreme wind environments in an urban area for different angles of attack. This paper discusses post-Ike glazing and rooftop appurtenance damage observed in sixteen high-rise buildings within the Houston CBD, including those affected during Alicia

Published
2009
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23. Pedestal stability comparison and ITER pedestal prediction

Author

A. Kirk, G. Saibene, J. Lönnroth, Alexei Pankin, C. F. Maggi, R. Maingi, P. B. Snyder, Hajime Urano, R. J. Groebner, Naoyuki Oyama, G.T.A. Huysmans, J. L. Terry, M.N.A. Beurskens, A. E. Hubbard, L. D. Horton, S. Saarelma, N. Aiba, H. R. Wilson, J. W. Hughes, C. Konz, T. H. Osborne, Y. Kamada, Anthony Leonard, and Applied Physics and Science Education

Subjects
Physics, Nuclear and High Energy Physics, Fusion, Tokamak, business.industry, Magnetic confinement fusion, Mechanics, Edge (geometry), Condensed Matter Physics, Stability (probability), law.invention, Wavelength, Pedestal, Optics, law, Physics::Plasma Physics, Magnetohydrodynamics, business
Abstract

The pressure at the top of the edge transport barrier (or ‘pedestal height’) strongly impacts fusion performance, while large edge localized modes (ELMs), driven by the free energy in the pedestal region, can constrain material lifetimes. Accurately predicting the pedestal height and ELM behavior in ITER is an essential element of prediction and optimization of fusion performance. Investigation of intermediate wavelength MHD modes (or ‘peeling–ballooning’ modes) has led to an improved understanding of important constraints on the pedestal height and the mechanism for ELMs. The combination of high-resolution pedestal diagnostics, including substantial recent improvements, and a suite of highly efficient stability codes, has made edge stability analysis routine on several major tokamaks, contributing both to understanding, and to experimental planning and performance optimization. Here we present extensive comparisons of observations to predicted edge stability boundaries on several tokamaks, both for the standard (Type I) ELM regime, and for small ELM and ELM-free regimes. We further discuss a new predictive model for the pedestal height and width (EPED1), developed by self-consistently combining a simple width model with peeling–ballooning stability calculations. This model is tested against experimental measurements, and used in initial predictions of the pedestal height for ITER.

Published
2009
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25. Plasma wall interaction and its implication in an all tungsten divertor tokamak

Author

Emanuele Poli, Y. R. Martin, L. Fattorini, Fernando Meo, M. Sertoli, G. Tardini, M. Garcia Munoz, T T Ribeiro, Qiang Yu, E. Vainonen-Ahlgren, Laure Vermare, G. Haas, K. Lackner, W. Sandmann, O. J. W. F. Kardaun, M. Rott, R. Merkel, K.-H. Steuer, Piero Martin, A. Kallenbach, P. de Marne, K. Gál, Alberto Bottino, N. Hicks, M. Gemisic-Adamov, Michael Kaufmann, Bruce D. Scott, A. Gude, J. Stober, H. Zohm, V. Mertens, H. D. Murmann, C. V. Atanasiu, K.H. Behringer, D. Wagner, V. Igochine, J.-M. Noterdaeme, Th. Pütterich, K. Sassenberg, A. Flaws, M. Püschel, F. Serra, G. Neu, H. Kollotzek, A. Bergmann, R. Pugno, H. W. Müller, W. Schustereder, K. McCormick, H. Meister, H. Greuner, R. Bilato, M. Huart, Wolf-Dieter Schneider, A. Lohs, R. Schrittwieser, W. Becker, F. Ryter, F. Merz, V. Bobkov, H. F. Meyer, M. Mlynek, Julia Fuchs, M. Mayer, C. F. Maggi, D. Holtum, F. Braun, Peter Lang, J. Hobirk, Taina Kurki-Suonio, A. C. C. Sips, S. da Graca, W. Suttrop, M. Balden, Marco Brambilla, T. Eich, H. Maier, J. M. Santos, M. Wischmeier, C. Tröster, Garrard Conway, E. Würsching, B. Nold, T. Bertoncelli, B. Reiter, M. Zilker, Ana Elisa Bauer de Camargo Silva, Ch. Hopf, C. Angioni, Sibylle Günter, A. Stäbler, R. Riedl, E. Speth, G. Kocsis, Thomas Zehetbauer, Philipp Lauber, S. Kálvin, J. Schirmer, G. V. Pereverzev, K. Engelhardt, C. Tichmann, E. Wolfrum, P. Varela, A. Manini, Patrick J. McCarthy, J. Harhausen, J. Roth, S. Gori, H.-U. Fahrbach, A. Scarabosio, Bernd Heinemann, L. D. Horton, M. E. Manso, Lin Liu, A. Schmid, P. Merkel, Rudolf Neu, D. Yadikin, L. Giannone, C. Konz, M. Maraschek, F. Monaco, E. Strumberger, R. Fischer, J. Fink, K. Mank, S. Dietrich, G. Pautasso, R. Drube, R. Dux, V. Rohde, A. Sigalov, A. Buhler, Martin Laux, Jari Likonen, D. P. Coster, J. Schweinzer, L. Urso, G. Schall, D. Zasche, Ursel Fantz, G. Schramm, A. V. Chankin, K. Behler, Gerhard Raupp, K. Krieger, O. Gruber, K. Dimova, S. Schweizer, J. Neuhauser, A. Herrmann, M. Reich, B. Kurzan, P. Franzen, U. Seidel, M. Kick, and W. Treutterer

Subjects
Tokamak, Materials science, Divertor, Facing Components, Transport, chemistry.chemical_element, Flux, Plasma, Effective radiated power, Tungsten, Condensed Matter Physics, law.invention, Nuclear Energy and Engineering, Alcator C-Mod, chemistry, ASDEX Upgrade, Erosion, law, Iter-Like Wall, Atomic physics, Asdex Upgrade Divertor, Operation
Abstract

ASDEX Upgrade has recently finished its transition towards an all-W divertor tokamak, by the exchange of the last remaining graphite tiles to W-coated ones. The plasma start-up was performed without prior boronization. It was found that the large He content in the plasma, resulting from DC glow discharges for conditioning, leads to a confinement reduction. After the change to D glow for inter-shot conditioning, the He content quickly dropped and, in parallel, the usual H-Mode confinement with H factors close to one was achieved. After the initial conditioning phase, oxygen concentrations similar to that in previous campaigns with boronizations could be achieved. Despite the removal of all macroscopic carbon sources, no strong change in C influxes and C content could be observed so far. The W concentrations are similar to the ones measured previously in discharges with old boronization and only partial coverage of the surfaces with W. Concomitantly it is found that although the W erosion flux in the divertor is larger than the W sources in the main chamber in most of the scenarios, it plays only a minor role for the W content in the main plasma. For large antenna distances and strong gas puffing, ICRH power coupling could be optimized to reduce the W influxes. This allowed a similar increase of stored energy as yielded with comparable beam power. However, a strong increase of radiated power and a loss of H-Mode was observed for conditions with high temperature edge plasma close to the antennas. The use of ECRH allowed keeping the central peaking of the W concentration low and even phases of improved H-modes have already been achieved.

Published
2007
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26. Tearing instabilities in multiple current sheets for current-dependent resistivity models

Author

Antonius Otto, C. Konz, and G. T. Birk

Subjects
Physics, Resistive touchscreen, Electrical resistivity and conductivity, Physics::Space Physics, Tearing, Astrophysics::Solar and Stellar Astrophysics, Microturbulence, Mechanics, Dissipation, Condensed Matter Physics, Joule heating, Instability, Magnetic flux
Abstract

A generalized analytical treatment of the resistive tearing mode in multiple current sheets for current-dependent electrical resistivities is given. This generalization allows for taking into account anomalous dissipation caused by current-driven microturbulence. The growth rates of the mode are found to be larger than the growth rates for constant resistivity. Numerical simulations show the linear and nonlinear development of the instability, where, in particular, the assumption of periodic configurations necessary in the analytical treatment can be relaxed. The results indicate that reconnection in neighboring magnetic flux systems mainly results in Ohmic heating and small tongue outflow rather than plasmoid-like eruptions.

Published
1997
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27. Dynamical Evolution of High Velocity Clouds in the Galactic Halo

Author

H. Lesch, C. Konz, and G. T. Birk

Subjects
Galactic halo, Physics, Dark matter halo, Ionization, Galactic habitable zone, Thermal, Galactic corona, Plasma, Astrophysics, Galactic tide, Astrophysics::Galaxy Astrophysics
Abstract

The stability of cold relatively dense weakly ionized high-velocity clouds in hot galactic halo plasmas is a highly interesting question of interstellar physics. The question of the dynamical and thermal stabilization of a neutral cloud in a thin ambient plasma is numerically investigated by three-dimensional plasma-neutral gas simulations. The results show the dynamical formation of a magnetic barrier which exerts a stabilizing pressure on the cloud and thus offers a solution to the lifetime puzzle.

Published
2005
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29. Contributor contact details

Author

B.M. Popkin, Camilla Verdich, Karine Clément, Thorkild I.A. Sorensen, Med Sci, Arne Astrup, Klaas R. Westerterp, M.I. Goran, C.P. Herman, C. de Graaf, B.J. Rolls, S. Whybrow, Manny Noakes, Karen Teff, P. Clifton, R.D. Mattes, Julie Miller Jones, G. Harvey Anderson, Kjeld Rahbek Ryttig, Hans C.M. van Trijp, Monika Leonhardt, James W. Anderson, Elizabeth C. Konz, Hollie Raynor, R.R. Wing, S.I. Barr, C. Bell, M.S. Westerterp-Plantenga, and David J. Mela

Published
2005
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30. Solar wind induced magnetic field around the unmagnetized Earth

Author

C. Konz, Harald Lesch, and G. T. Birk

Subjects
Physics, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics (astro-ph), FOS: Physical sciences, Astronomy and Astrophysics, Cosmic ray, Astrophysics, Magnetic field, Physics::Geophysics, Atmosphere, Solar wind, Space and Planetary Science, Dynamo theory, Physics::Space Physics, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Ionosphere, Magnetic dipole, Dynamo
Abstract

The Earth is a planet with a dipolar magnetic field which is agitated by a magnetized plasma wind streaming from the Sun. The magnetic field shields the Earth's surface from penetrating high energy solar wind particles, as well as interstellar cosmic rays. The magnetic dipole has reversed sign some hundreds of times over the last 400 million years. These polarity reversals correspond to drastic breakdowns of the dynamo action. The question arises what the consequences for the Earth's atmosphere, climate, and, in particular, biosphere are. It is shown by kinematic estimates and three-dimensional plasma-neutral gas simulations that the solar wind can induce very fast a magnetic field in the previously completely unmagnetized Earth's ionosphere that is strong enough to protect Earth from cosmic radiations comparable to the case of an intact magnetic dynamo., Comment: 4pages, accepted

Published
2004
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31. Cell proliferation and apoptosis are altered in mice deficient in the NF-kappaB p50 subunit after treatment with the peroxisome proliferator ciprofibrate

Author

Howard P. Glauert, Aaron B. Owens, Aysegul Nalca, Elizabeth C. Konz, Leila Ghabrial, Brett T. Spear, and Job C. Tharappel

Subjects
Male, medicine.medical_specialty, Programmed cell death, Ratón, JUNB, Proto-Oncogene Proteins c-jun, Blotting, Western, Administration, Oral, Apoptosis, Mice, Inbred Strains, Biology, Toxicology, Clofibric Acid, Mice, Internal medicine, medicine, In Situ Nick-End Labeling, Animals, RNA, Messenger, Mice, Knockout, Cell growth, Fibric Acids, NF-kappa B, NF-kappa B p50 Subunit, Diet, medicine.anatomical_structure, Endocrinology, Liver, Hepatocyte, Hepatic stellate cell, Peroxisome Proliferators, Ciprofibrate, Cell Division, medicine.drug
Abstract

We previously showed that the peroxisome proliferator ciprofibrate increases hepatic NF-κB DNA binding activity in rats, mice, and hepatoma cell lines. Here, we analyzed the response to ciprofibrate in mice that lack the NF-κB p50 gene (p50 -/- ). Wild-type and p50 -/- mice were fed a diet with or without 0.01% ciprofibrate for 10 days. NF-κB DNA binding activity was present and increased after ciprofibrate treatment in wild-type mice, but was not detected in p50 -/- mice. The untreated p50 -/- mice had a higher level of hepatic cell proliferation, as measured by BrdU labeling, than did untreated wild-type mice. However, the increase in proliferation was greater in ciprofibrate-fed wild-type mice than in ciprofibrate-fed p50 -/- mice. The apoptotic index was low in wild-type mice in the presence or absence of ciprofibrate. Apoptosis was increased in untreated p50 -/- mice compared to wild-type mice; apoptosis was reduced in p50 -/- mice after ciprofibrate feeding. The c-Jun and JunB mRNA levels were higher in untreated p50 -/- mice than in untreated control mice; c-Jun mRNA levels increased, whereas JunB mRNA levels decreased in both groups after ciprofibrate treatment. The c-Jun and JunB protein levels were the same in untreated wild-type and p50 -/- mice and increased in both groups after ciprofibrate treatment. Several apoptosis-related mRNAs were higher in untreated p50 -/- mice compared to untreated control mice; expression of these genes increased in both groups after ciprofibrate treatment. These data indicate that NF-κB contributes to the proliferative and apoptotic changes that occur in the liver in response to ciprofibrate.

Published
2003

33. Dynamical evolution of high velocity clouds in the intergalactic medium

Author

C. Konz, G. T. Birk, and C. Brüns

Subjects
Physics, Astrophysics (astro-ph), FOS: Physical sciences, Astronomy and Astrophysics, Field strength, Plasma, Astrophysics, Galactic halo, Space and Planetary Science, Magellanic Stream, Thermal, Intergalactic travel, Magnetohydrodynamic drive, Halo, Astrophysics::Galaxy Astrophysics
Abstract

HI observations of high-velocity clouds (HVCs) indicate, that they are interacting with their ambient medium. Even clouds located in the very outer Galactic halo or the intergalactic space seem to interact with their ambient medium. In this paper, we investigate the dynamical evolution of high velocity neutral gas clouds moving through a hot magnetized ambient plasma by means of two-dimensional magnetohydrodynamic plasma-neutral gas simulations. This situation is representative for the fast moving dense neutral gas cloudlets in the Magellanic Stream as well as for high velocity clouds in general. The question on the dynamical and thermal stabilization of a cold dense neutral cloud in a hot thin ambient halo plasma is numerically investigated. The simulations show the formation of a comet-like head-tail structure combined with a magnetic barrier of increased field strength which exerts a stabilizing pressure on the cloud and hinders hot plasma from diffusing into the cloud. The simulations can explain both the survival times in the intergalactic medium and the existence of head-tail high velocity clouds., Comment: 11 pages, 19 figures

Published
2002
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34. Corrigendum: The European Integrated Tokamak Modelling (ITM) effort: achievements and first physics results (2014Nucl. Fusion54 043018)

Author

S. Nowak, C. Konz, H.-J. Klingshirn, I. Voitsekhovitch, D. P. Coster, Ph. Huynh, R. Reimer, A. Figueiredo, Denis Kalupin, Olivier Sauter, Irena Ivanova-Stanik, Daniela Farina, E. Westerhof, G. Falchetto, Michal Owsiak, V. Basiuk, W. Zwingmann, A. Kus, Bruce D. Scott, Jorge Ferreira, Luís L Alves, Emanuele Poli, R. Coelho, G. V. Pereverzev, J. Signoret, Lorenzo Figini, Andreas Dinklage, João P. S. Bizarro, P. Strand, Jet-Efda Contributors, Y. Peysson, R. Stankiewicz, Eric Nardon, T. Jonsson, Tomasz Zok, Itm-Tf Contributors, Cédric Boulbe, Nikolai B. Marushchenko, Blaise Faugeras, J.F. Artaud, Frederic Imbeaux, ITM-TF Contributors, ASDEX Upgrade Team, Max Planck Institute for Plasma Physics, Max Planck Society, and JET-EFDA Contributors

Subjects
Nuclear and High Energy Physics, Tokamak, Web of science, Plasma instability, law, Systems engineering, Iter tokamak, Plasma confinement, Magnetic confinement fusion, Condensed Matter Physics, law.invention
Abstract

Reference EPFL-ARTICLE-202347doi:10.1088/0029-5515/54/9/099501View record in Web of Science Record created on 2014-10-23, modified on 2017-05-12

Published
2014
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35. Factors Influencing Bond Strength of Adhesive Anchors

Author

Ronald A. Cook and Robert C. Konz

Subjects
Test series, business.product_category, Materials science, business.industry, Bond strength, Building and Construction, Structural engineering, Fastener, Adhesion strength, Test program, Adhesive, business, Curing (chemistry), Civil and Structural Engineering
Abstract

This paper presents results of a comprehensive test program that investigated various factors with the potential to influence the bond strength of polymer-based adhesive anchors. 20 products from 12 manufacturers were included in the program for a total of 765 tests. To establish a reference bond strength, baseline tests were performed at room temperature for anchors installed in cleaned, dry holes. Individual factors were isolated through separate test series that maintained baseline conditions, except for the variable under consideration. The variables that were investigated included those that could be anticipated to occur during and after installation. Factors occurring during installation included the condition of the drilled hole, differences in the concrete strength, and differences in concrete aggregate. Factors occurring after installation included a short-term adhesive curing period and loading at an elevated temperature. This research demonstrates that reliable predictions of adhesive anchor performance are only practical by product-specific and condition-specific testing.

Published
2001
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36. Shear-Flow Driven Current Filamentation: Two-Dimensional Magnetohydrodynamic Simulations

Author

C. Konz, H. Wiechen, and Harald Lesch

Subjects
Physics, Magnetic energy, Astrophysics (astro-ph), FOS: Physical sciences, Magnetic reconnection, Mechanics, Astrophysics, Dissipation, Condensed Matter Physics, Filamentation, Dissipative system, Magnetohydrodynamic drive, Magnetohydrodynamics, Shear flow
Abstract

The process of current filamentation in permanently externally driven, initially globally ideal plasmas is investigated by means of two-dimensional Magnetohydrodynamic (MHD)-simulations. This situation is typical for astrophysical systems like jets, the interstellar and intergalactic medium where the dynamics is dominated by external forces. Two different cases are studied. In one case, the system is ideal permanently and dissipative processes are excluded. In the second case, a system with a current density dependent resistivity is considered. This resistivity is switched on self-consistently in current filaments and allows for local dissipation due to magnetic reconnection. Thus one finds tearing of current filaments and, besides, merging of filaments due to coalescence instabilities. Energy input and dissipation finally balance each other and the system reaches a state of constant magnetic energy in time., 32 Pages, 13 Figures. accepted, to appear in Physics of Plasmas (049012)

Published
2000

37. Health advantages and disadvantages of weight-reducing diets: a computer analysis and critical review

Author

David J.A. Jenkins, James W. Anderson, and Elizabeth C. Konz

Subjects
medicine.medical_specialty, Diet, Reducing, Medicine (miscellaneous), Nutritional Status, Healthy eating, Coronary Disease, Nutrition Policy, Cholesterol, Dietary, Computer analysis, Weight loss, Risk Factors, Internal medicine, Environmental health, Weight Loss, Medicine, Humans, Obesity, Nutrition and Dietetics, business.industry, Food pyramid, Diet Fads, Nutritional Requirements, medicine.disease, Coronary heart disease, Endocrinology, Cholesterol, Saturated fatty acid, medicine.symptom, business, Reducing Diets
Abstract

Some weight-loss diets are nutritionally sound and consistent with recommendations for healthy eating while others are "fad" diets encouraging irrational and, sometimes, unsafe practices.The purpose of the study was to compare several weight loss diets and assess their potential long-term effects.Eight popular weight-loss diets were selected (Atkins, Protein Power, Sugar Busters, Zone, ADA Exchange, High-Fiber Fitness, Pritikin and Omish) to be non-clinically analyzed by means of a computer to predict their relative benefits/potential harm. A summary description, menu plan and recommended snacks were developed for each diet. The nutrient composition of each diet was determined using computer software, and a Food Pyramid Score was calculated to compare diets. The Mensink, Hegsted and other formulae were applied to estimate coronary heart disease risk factors.Higher fat diets are higher in saturated fats and cholesterol than current dietary guidelines and their long-term use would increase serum cholesterol levels and risk for CHD. Diets restricted in sugar intake would lower serum cholesterol levels and long-term risk for CHD; however, higher carbohydrate, higher fiber, lower fat diets would have the greatest effect in decreasing serum cholesterol concentrations and risk of CHD.While high fat diets may promote short-term weight loss, the potential hazards for worsening risk for progression of atherosclerosis override the short-term benefits. Individuals derive the greatest health benefits from diets low in saturated fat and high in carbohydrate and fiber: these increase sensitivity to insulin and lower risk for CHD.

Published
2000

38. Pedestal and core confinement of hybrid scenario in ASDEX Upgrade and DIII-D

Author

R. E. Waltz, T. Hein, P. B. Snyder, R. J. Groebner, C. Angioni, C.F. Maggi, Jeff Candy, L. D. Horton, C. Konz, A.W. Leonard, A.C.C. Sips, C.C. Petty, and Diii-D Teams

Subjects
Physics, Nuclear and High Energy Physics, Tokamak, DIII-D, Magnetic confinement fusion, Condensed Matter Physics, law.invention, Pedestal, ASDEX Upgrade, law, Beta (plasma physics), Magnetohydrodynamics, Atomic physics, Pressure gradient
Abstract

Pedestal and core confinement of hybrid discharges in ASDEX Upgrade (AUG) and DIII-D are studied in dedicated power scan experiments. The H98(y,2) confinement factor increases with total ?N in both tokamaks and it is higher in DIII-D with higher ? plasma shape at a given ?N. The pedestal beta, , increases linearly with total beta in AUG hybrid discharges, while it is roughly constant with ?N at fixed shape in the DIII-D power scans. The confinement enhancement with power observed with respect to the IPB98(y,2) scaling is due to an increase in pedestal confinement in AUG hybrid discharges and to an increase in core confinement in the DIII-D hybrid power scans. The increase in pedestal pressure with power in AUG hybrid discharges is primarily due to an increase in the width of the edge transport barrier at constant pressure gradient. In the DIII-D discharges the widths of the Te and ne pedestals, and , are consistent with a scaling. In the AUG hybrid power scans a dependence of on ?pol,PED cannot be excluded, while shows no dependence on ?pol,PED In both machines increases with ?. The maximum pedestal pressure achieved in the experiment prior to the onset of type I ELMs is consistent with predictions from ideal MHD; however, a physics model explaining the increase in the pedestal width with ? is still missing. The increase in with ? in the core of DIII-D is consistent with predictions by linear gyrokinetic simulations. In the plasma core, E ? B shearing rate stabilization of the ITG modes is significant in both machines as beta is increased. Inclusion of electromagnetic effects in the gyrokinetic calculations provides additional stabilization at ?N values achieved in the experiment. In AUG, proximity to the kinetic ballooning threshold and/or a stronger reduction in normalized ion heat flux with increasing input power are possible explanations for the constancy of at mid-radius as beta is increased.

Published
2010
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39. Benefits and risks of antiobesity agents

Author

James W. Anderson and Elizabeth C. Konz

Subjects
Nutrition and Dietetics, Anti-Obesity Agents, Weight loss, business.industry, medicine, Medicine (miscellaneous), ANTIOBESITY AGENTS, medicine.symptom, Bioinformatics, business, medicine.disease, Obesity
Published
2000
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40. Disruption studies in ASDEX Upgrade in view of ITER

Author

Xavier Bonnin, D. P. Coster, M Marascheck, G. Pautasso, T. Eich, Julia Fuchs, K. Lackner, T. Lunt, A. Gude, Yi Zhang, B. Reiter, G Prausner, A. Herrmann, B. Kurzan, O. Gruber, M. Beck, C. Konz, V. Igochine, A. Mlynek, and V. Rohde

Subjects
Electron density, Tokamak, Materials science, chemistry.chemical_element, Plasma, Electron, Condensed Matter Physics, Critical value, law.invention, Nuclear physics, Neon, Nuclear Energy and Engineering, chemistry, ASDEX Upgrade, Physics::Plasma Physics, law, Order of magnitude
Abstract

Experiments on ASDEX Upgrade and other tokamaks have shown that the magnitude of mechanical forces and thermal loads during disruptions can be significantly reduced by raising the plasma density with massive injection of noble gases. This method should be applicable to ITER too. Nevertheless, the suppression of the runaway electron (RE) avalanche requires a much larger (two order of magnitude) density rise. This paper reports on recent experiments aimed at increasing the plasma density towards the critical value, needed for the collisional suppression of REs. An effective electron density equal to 24% of the critical density has been reached after injection of 3.3?bar?l of neon. However, the resultant large plasma density is very poloidally and toroidally asymmetric; this implies that several valves distributed around the plasma periphery become necessary at this level of massive gas injection to ensure a homogeneous density distribution.

Published
2009
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41. Interaction of Hot and Cold Space Plasmas

Author

G. T. Birk, Harald Lesch, and C. Konz

Subjects
Physics, Astrophysics::High Energy Astrophysical Phenomena, Magnetic reconnection, Astrophysics, Dipole model of the Earth's magnetic field, Condensed Matter Physics, Atomic and Molecular Physics, and Optics, L-shell, Solar wind, Physics::Plasma Physics, Physics::Space Physics, Astrophysical plasma, Interplanetary magnetic field, Mercury's magnetic field, Magnetic dipole, Astrophysics::Galaxy Astrophysics, Mathematical Physics
Abstract

Cosmic plasma phenomena are often characterized by the interaction of hot and cold plasma components. Magnetic fields prove to be of particular importance in the dynamics of such plasmas. As an example, three different cosmic objects are studied by means of two- and three-dimensional plasma-neutral gas fluid simulations. It is shown that magnetic fields can be responsible for the dynamical stabilization of neutral gas clouds in the Galactic halo. Disconnection events in cometary tails can be caused by magnetic reconnection. The interaction of the solar wind with the Earth during periods of a vanishing dipole field can lead to the generation of a magnetic field in the ionosphere thereby protecting the biosphere against cosmic rays.

Published
2004
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42. Overview of JET results

Author

F. Romanelli, F. Laxaback, I. Abel, V. Afanesyev, G. Agarici, K. M. Aggarwal, M. Airila, R. Akers, T.h. Alarcon, A. Alexeev, A. Alfier, P. Allan, S. Almaviva, A. Alonso, M. Alonso, B. Alper, H. Altmann, D. Alves, V. Amosov, G. Anda, F. Andersson, E. Andersson Sund́en, V. Andreev, Y. Andrew, M. Angelone, M. Anghel, A. Anghel, C. Angioni, G. Apruzzese, N. Arcis, P. Arena, A. Argouarch, M. Ariola, A. Armitano, R. Armstrong, G. Arnoux, S. Arshad, G. Artaserse, J. F. Artaud, A. Ash, E. Asp, O. Asunta, C. V. Atanasiu, G. Atkins, M. D. Axton, C. Ayres, A. Baciero, V. Bailescu, B. Baiocchi, R. A. Baker, I. Balboa, C. Balorin, N. Balshaw, J. W. Banks, Y. F. Baranov, D. Barbier, I. L. Barlow, M. A. Barnard, R. Barnsley, L. Barrena, L. Barrera, M. Baruzzo, V. Basiuk, G. Bateman, P. Batistoni, N. Baumgarten, L. Baylor, B. Bazylev, P. S. Beaumont, K. Beausang, M. B́ecoulet, N. Bekris, M. Beldishevski, A. C. Bell, F. Belli, M. Bellinger, P. S. A. Belo, ́.E. Belonohy, P. E. Bennett, N. A. Benterman, G. Berger By, H. Bergsåker, H. Berk, J. Bernardo, B. Bertrand, M. N. A. Beurskens, B. Bieg, B. Bienkowska, T. Biewer, T. M. Biewer, M. Bigi, R. Bilato, J. Bird, J. Bizarro, T. R. Blackman, P. Blanchard, E. Blanco, J. Blum, V. Bobkov, A. Boboc, D. Boilson, I. Bolshakova, T. Bolzonella, L. Boncagni, G. Bonheure, X. Bonnin, D. Borba, A. Borthwick, A. Botrugno, C. Boulbe, F. Bouquey, C. Bourdelle, K. v. Bovert, M. Bowden, T. Boyce, H. J. Boyer, A. Bozhenkov, R. J. Brade, J. M. A. Bradshaw, J. Braet, V. Braic, G. C. Braithwaite, C. Brault, H. Braune, B. Breizman, S. Bremond, P. D. Brennan, A. Brett, J. Breue, S. Brezinsek, M. D. J. Bright, F. Briscoe, M. Brix, M. Brombin, B. C. Brown, D. P. D. Brown, A. Bruschi, J. Brzozowski, J. Bucalossi, M. A. Buckley, T. Budd, R. Budny, R. V. Budny, P. Bunting, P. Buratti, G. Burcea, P. R. Butcher, R. J. Buttery, R. Caç̃ao, G. Calabr`o, C. P. Callaghan, J. P. Caminade, P. G. Camp, D. C. Campling, J. Canik, B. Cannas, A. J. Capel, P. J. Card, A. Cardinali, T. Carlstrom, P. Carman, D. Carralero, L. Carraro, T. Carter, B. B. Carvalho, P. Carvalho, A. Casati, C. Castaldo, J. Caughman, R. Cavazzana, M. Cavinato, M. Cecconello, F. E. Cecil, A. Cenedese, C. Centioli, R. Cesario, C. D. Challis, M. Chandler, C. Chang, A. Chankin, I. T. Chapman, D. J. Child, P. Chiru, G. Chitarin, I. Chugonov, I. Chugunov, D. Ciric, F. Clairet, R. H. Clarke, R. Clay, M. Clever, J. P. Coad, P. A. Coates, V. Cocilovo, S. Coda, R. Coelho, J. Coenen, I. Coffey, L. Colas, M. Cole, S. Collins, S. Combs, J. Compan, J. E. Conboy, S. Conroy, N. Cook, S. P. Cook, D. Coombs, S. R. Cooper, Y. Corre, G. Corrigan, S. Cortes, D. Coster, G. F. Counsell, X. Courtois, M. Cox, T. Craciunescu, S. Cramp, F. Crisanti, O. Croft, K. Crombe, B. J. Crowley, N. Cruz, L. Cupido, M. Curuia, R. A. Cusack, A. Czarnecka, S. Dalley, E. T. Daly, A. Dalziel, D. Darrow, O. David, N. Davies, J. J. Davis, I. E. Day, C. Day, R. De Angelis, G. deArcas, M. R. de Baar, E. delaCal, E. de la Luna, J. L. de Pablos, G. De Temmerman, P. C. de Vries, F. Degli Agostini, E. Delabie, D. del Castillo Negrete, L. Delpech, G. Denisov, A. J. Denyer, R. F. Denyer, S. Devaux, P. Devynck, L. Di Matteo, L. DiPace, P. J. Dirken, A. Dnestrovskiy, D. Dodt, K. Dominiczak, S. E. Dorling, D. Douai, A. P. Down, P. T. Doyle, J. R. Drake, T. Dreischuh, V. Drozdov, P. Dumortier, D. Dunai, I. Duran, F. Durodíe, K. Dylst, R. Eaton, T. Edlington, A. M. Edwards, D. T. Edwards, P. K. Edwards, T.h. Eich, A. Ekedahl, T. Elevant, A. Elfimov, B. Ellingboe, C. G. Elsmore, B. Emmoth, G. Ericsson, L. G. Eriksson, A. Eriksson, B. Esposito, H. G. Esser, T. Estrada, E. A. Evangelidis, G. E. Evans, G. D. Ewart, D. T. Ewers, G. Falchetto, D. Falie, J. G. A. Fanthome, D. Farina, J. W. Farthing, A. Fasoli, B. Faugeras, N. Fedorczak, R. C. Felton, C. Fenzi, H. Fernandes, J. A. Ferreira, J. Ferreira, J. Ferron, J. A. Fessey, L. Figini, A. Figueiredo, J. Figueiredo, P. Finburg, K. H. Finken, U. Fischer, N. Fitzgerald, J. Flanagan, C. Fleming, A. Fonseca, A. D. Forbes, O. Ford, A. Formisano, D. Fraboulet, R. J. Francis, L. Frassinetti, R. Fresa, J. P. Friconneau, D. Frigione, J. C. Fuchs, K. Fullard, W. Fundamenski, M. Furno Palumbo, J. Gafert, K. Ǵal, R. Galṽao, S. Garavaglia, X. Garbet, J. Garcia, M. Gar cia Munoz, W. Gardner, P. Garibaldi, D. Garnier, L. Garzotti, M. Gatu Johnson, P. Gaudio, E. Gauthier, J. W. Gaze, D. F. Gear, J. Gedney, S. J. Gee, M. Gelfusa, E. Genangeli, S. Gerasimov, A. Geraud, T. Gerbaud, M. Gherendi, N. Ghirelli, J. C. Giacalone, L. Giacomelli, C. S. Gibson, C. Gil, S. J. Gilligan, C. G. Gimblett, D. Gin, E. Giovannozzi, C. Giroud, G. Giruzzi, S. Glowacz, J. Godwin, J. K. Goff, P. Gohil, V. Goloborod’ko, B. Gonçalves, M. Goniche, S. Gonzales, S. M. Gonźalezde Vicente, A. Goodyear, N. Gorelenkov, G. Gorini, R. Goulding, B. Graham, D. Graham, M. E. Graham, G. Granucci, J. Graves, N. R. Green, H. Greuner, E. Grigore, F. S. Griph, C. Grisolia, G. Gros, G. Grossetti, M. Groth, S. Gr̈unhagen, M. P. Gryaznevich, R. Guirlet, B. Gulejova, J. Gunn, A. Gupta, P. Guzdar, P. Hacek, L. J. Hackett, S. Hacquin, B. Haist, A. Hakola, S. J. Hall, S. P. HallworthCook, D. T. Hamilton, H. Han, R. C. Handley, S. Harding, J. D. W. Harling, D. Harting, M. J. Harvey, T. D. V. Haupt, E. Havlickova, N. C. Hawkes, R. Hawryluk, J. H. Hay, N. Hayashi, P. W. Haydon, I. R. Hayward, S. Hazel, P. J. L. Heesterman, W. Heidbrink, J. Heikkinen, C. Hellesen, T. Hellsten, O. N. Hemming, T. C. Hender, M. Henderson, C. Hennig, V. Hennion, C. Hidalgo, S. Higashijima, J. W. Hill, M. Hill, K. Hill, J. Hillairet, D. Hillis, T. Hirai, M. Hitchin, J. Hobirk, C. Hogan, C. H. A. Hogben, G. M. D. Hogeweij, I. C. Hollingham, R. Holyaka, D. A. Homfray, G. Honeyands, S. H. Hong, C. Hopf, B. A. Horn, A. R. Horton, L. D. Horton, S. P. Hotchin, M. R. Hough, W. Houlberg, D. F. Howell, M. Hron, A. Huber, T. M. Huddleston, Z. Hudson, M. Hughes, M. Ḧuhnerbein, C. C. Hume, A. J. Hunt, C. L. Hunter, T. S. Hutchinson, S. Huygen, G. Huysmans, V. Hyn̈onen, S. Ide, R. Igreja, C. Illescas, F. Imbeaux, D. Ivanova, E. Ivings, S. Jachmich, G. Jackson, P. Jacquet, K. Jakubowska, M. Jakubowski, P. V. James, R. J. E. Jaspers, S. Jednorog, I. Jenkins, M. A. C. Jennison, C. Jeskins, O. Jin Kwon, E. Joffrin, M. F. Johnson, R. Johnson, T. Johnson, D. Jolovic, V. Jonauskas, E. M. Jones, G. Jones, H. D. Jones, T. T. C. Jones, M. Jouvet, C. Juṕen, I. Kachtchouk, J. Kaczmarczyk, A. Kallenbach, J. K̈allne, D. Kalupin, S. Ḱalvin, G. Kamelander, R. Kamendje, A. Kappatou, S. Karttunen, W. Kasparek, I. Katramados, M. Kaufmann, G. Kaveney, A. S. Kaye, M. J. Kear, D. L. Keeling, D. Kelliher, M. Kempenaars, P. Khilar, N. G. Kidd, M. Kiisk, K. M. Kim, R. F. King, D. J. Kinna, V. Kiptily, G. Kirnev, N. Kirneva, K. Kirov, A. Kirschner, R. Kisielius, D. Kislov, G. Kiss, T. Kiviniemi, G. Kizane, A. Klein, A. Klix, M. Knaup, K. Kneuper, H. Kneupner, P. J. Knight, S. J. Knipe, M. Kocan, F. K̈ochl, G. Kocsis, C. Konz, T. Koppitz, A. Korotkov, H. R. Koslowski, V. Kotov, M. D. Kovari, K. Kovarik, G. Kramer, A. Krasilnikov, V. Krasilnikov, S. Kraus, A. Kreter, K. Krieger, A. Kritz, Y. Krivchenkov, U. Kruezi, M. Krychowiak, S. Krylov, I. Ksiazek, M. Kubic, S. Kuhn, W. K̈uhnlein, T. Kurki Suonio, A. Kurowski, B. Kuteev, A. Kuyanov, R. La Haye, M. Laan, C. Labate, A. Lachichi, N. Lam, P. Lang, M. T. Large, I. Lassiwe, J. R. Last, K. D. Lawson, M. Laxåback, R. A. Layne, E. Lazzaro, F. LeGuern, B. LeBlanc, H. J. Leggate, M. Lehnen, M. Leigheb, I. Lengar, M. Lennholm, E. Lerche, C. N. Lescure, Y. Li, A. Li Puma, Y. Liang, J. Likonen, Y. Lin, J. Linke, S. A. Linstead, B. Lipshultz, X. Litaudon, A. G. Litvak, Y. Liu, T. Loarer, A. Loarte, R. C. Lobel, P. J. Lomas, F. D. Long, J. L̈onnroth, D. J. Looker, J. Lopez, P.h. Lotte, M. J. Loughlin, A. B. Loving, C. Lowry, T. Luce, R. M. A. Lucock, A. Lukanitsa, A. M. Lungu, C. P. Lungu, A. Lyssoivan, P. Macheta, A. S. Mackenzie, M. Macrae, G. Maddaluno, G. P. Maddison, J. Madsen, P. Maget, C. Maggi, H. Maier, J. Mailloux, M. Makowski, C. J. Manning, M. Mansfield, M. E. Manso, P. Mantica, M. Mantsinen, M. Maraschek, C. Marchetto, M. A. Marchitti, M. Mardenfeld, J. L. Marechal, M. Marinelli, A. Marinoni, M. Marinucci, J. M̈arki, D. Marocco, C. A. Marren, D. Martin, D. L. Martin, G. Martin, Y. Martin, J. R. Mart́ın Soĺıs, K. Masaki, A. Masiello, M. Maslov, C. Maszl, A. Matilal, M. Mattei, G. F. Matthews, F. Maviglia, C. R. May, M. Mayer, M. L. Mayoral, D. Mazon, C. Mazzotta, E. Mazzucato, P. McCarthy, K. G. McClements, K. McCormick, P. A. McCullen, D. McCune, D. C. McDonald, R. Mcgregor, J. P. Mckivitt, A. Meakins, F. Medina, A. G. Meigs, M. Menard, L. Meneses, S. Menmuir, I. R. Merrigan, P.h. Mertens, A. Messiaen, H. Meyer, M. Miele, P. Migliucci, A. G. Miller, S. F. Mills, J. J. Milnes, K. Min Kim, T. Mindham, F. Mirizzi, E. Mirones, M. Mironov, R. Mitteau, J. Mlynar, P. Mollard, I. Monakhov, P. Monier Garbet, R. Mooney, S. Moradi, D. Moreau, P.h. Moreau, L. Moreira, A. Morgan, P. D. Morgan, C. Morlock, A. Moro, A. W. Morris, G. L. Mort, C. Mrozek, A. Mueck, H. W. M̈uller, M. Murakami, A. Murari, I. Mustata, F. Nabais, E. Nardon, G. Nash, V. Naulin, M. F. F. Nave, R. Nazikian, I. Nedzelski, C. R. Negus, J. D. Neilson, A. Neto, R. Neu, O. Neubauer, G. J. Newbert, M. Newman, K. J. Nicholls, A. Nicolai, L. Nicolas, P. Nieckchen, P. Nielsen, A. H. Nielsen, S. K. Nielsen, G. Nielson, J. Nieto, M. P. S. Nightingale, C. Noble, M. Nocente, M. Nora, H. Nordman, M. Norman, J. M. Noterdaeme, S. Nowak, I. Nunes, F. Ognissanto, T. O’Gorman, S. Olariu, A. Oleynikov, M. O’Mullane, J. Ongena, F. Orsitto, O. I. Oswuigwe, M. Ottaviani, N. Oyama, D. Pacella, K. Paget, S. Palazzo, J. Pamela, S. Pamela, R. Panek, L. Pangione, A. Panin, T.h. Panis, A. Pankin, A. Pantea, V. Parail, T.h. Parisot, A. Parkin, A. Parsloe, B. T. Parsons, R. Pasqualotto, P. Pastor, R. Paterson, M. K. Paul, D. Peach, R. J. H. Pearce, B. J. Pearson, I. J. Pearson, L. C. Pedrick, M. A. Pedrosa, B. Pegourie, R. Pereira, E. Perelli Cippo, G. Pereverzev, A. Perevezentsev, C.h. PerezvonThun, V. Pericoli Ridolfini, A. Perona, Y. Perrot, S. Peruzzo, S. Peschanyy, G. Petravich, L. Petrizzi, V. Petrov, V. Petrzilka, V. Philipps, G. Piazza, F. Piccolo, A. Pietropaolo, M. Pillon, S. D. Pinches, T. Pinna, G. Pintsuk, P. Piovesan, F. Pisano, R. Pitts, B. Plaum, V. Plyusnin, M. Polasik, F. M. Poli, N. Pomaro, O. Pompilian, L. Poncet, P. J. Pool, S. Popovichev, F. Porcelli, M. T. Porfiri, C. Portafaix, A. Pospieszczyk, G. Possnert, G. Prestopino, P. Prior, R. Prokopowicz, I. Proverbio, R. Pugno, M. E. Puiatti, K. Purahoo, V. Pustovitov, T.h. P̈utterich, D. P̈uttmann Kneupner, E. Rachlew, R. Rademaker, T. Rafiq, M. S. J. Rainford, G. Ramogida, K. Rantam̈aki, J. Rapp, J. J. Rasmussen, G. Ratt́a, G. Ravera, M. Reich, R. Reichle, D. Reiser, R. Reiss, D. Reiter, D. Rendell, C. Reux, G. Rewoldt, T. T. Ribeiro, V. Riccardo, D. Richards, F. Rigollet, F. G. Rimini, L. Rios, M. Riva, J. E. C. Roberts, R. J. Robins, D. S. Robinson, S. A. Robinson, D. W. Robson, H. Roche, M. R̈odig, N. Rodionov, V. Rohde, A. Rolfe, M. Romanelli, A. Romano, J. Romero, E. Ronchi, S. Rosanvallon, C.h. Roux, S. Rowe, M. Rubel, L. Ruchko, M. Ruiz, C. Ruset, M. Russell, A. Ruth, L. Ryc, A. Rydzy, F. Ryter, J. Rzadkiewicz, S. Saarelma, F. Sabathier, R. Sabot, S. Sadakov, P. Sagar, G. Saibene, A. Saille, F. Saint Laurent, A. Salmi, R. Salomaa, F. Salzedas, U. Samm, P. Sanchez, S. Sanders, S. G. Sanders, G. Sandford, K. Sandland, P. Sandquist, D. E. G. Sands, M. I. K. Santala, F. Sartori, R. Sartori, O. Sauter, A. Savelyev, A. Savtchkov, S. C. Scales, A. Scarabosio, N. Schaefer, C.h. Schlatter, V. Schmidt, A. Schmidt, O. Schmitz, S. Schmuck, M. Schneider, M. Scholz, K. Scḧopf, B. Schweer, J. Schweinzer, B. Scott, M. Seki, L. Semeraro, A. Semerok, G. Sergienko, F. Serra, M. Sertoli, M. M. J. Shannon, S. E. Sharapov, S. R. Shaw, A. Shevelev, R. Sievering, C. A. Silva, P. A. Simmons, A. Simonetto, D. Simpson, S. Sipila, A. C. C. Sips, A. Sirinelli, H. Sj̈ostrand, D. Skopintsev, K. S.l.a.b.k.o.w.s.k.a., P. G. Smith, J. Snipes, L. Snoj, S. Snyder, S. Soare, E. R. Solano, S. Soldatov, A. Soleto, W. Solomon, C. Soltane, P. Sonato, A. Sopplesa, A. Sorrentino, J. Sousa, C. B. C. Sowden, C. Sozzi, P. Sp̈ah, T. Spelzini, J. Spence, F. Spineanu, P. Spuig, A. Sẗabler, R. D. Stagg, M. F. Stamp, V. Stancalie, P. Stangeby, C. Stan Sion, D. E. Starkey, M. J. Stead, A. V. Stephen, A. L. Stevens, J. Stober, R. B. Stokes, D. Stork, D. Stoyanov, J. Strachan, P. Strand, M. Stransky, D. Strauss, D. Strintzi, W. Studholme, Y. SuNa, F. Subba, H. P. Summers, Y. Sun, C. Surdu Bob, E. Surrey, D. J. Sutton, J. Svensson, D. Swain, B. D. Syme, I. D. Symonds, T. Szepesi, A. Szydlowski, F. Tabares, V. Takalo, H. Takenaga, T. Tala, A. R. Talbot, C. Taliercio, C. Tame, G. Tardini, M. Tardocchi, L. Taroni, G. Telesca, A. Terra, A. O. Terrington, D. Testa, J. M. Theis, J. D. Thomas, P. D. Thomas, P. R. Thomas, V. K. Thompson, H. Thomsen, C. Thomser, A. Thyagaraja, P. A. Tigwell, I. Tiseanu, R. Tivey, J. M. Todd, T. N. Todd, M. Z. Tokar, S. Tosti, P. Trabuc, J. M. Travere, W. Treutterer, P. Trimble, A. Trkov, E. Trukhina, M. Tsalas, H. Tsige Tamirat, E. Tsitrone, D. Tskhakaya jun, O. Tudisco, S. Tugarinov, M. M. Turner, G. Turri, S. G. J. Tyrrell, N. Umeda, B. Unterberg, H. Urano, A. J. Urquhart, I. Uytdenhouwen, A. Vaccaro, A. P. Vadgama, G. Vagliasindi, D. Valcarcel, M. Valisa, J. Vallory, M. Valovic, D. Van Eester, B. van Milligen, G. J. van Rooij, C. A. F. Varandas, S. Vartanian, V. Vdovin, J. Vega, G. Verdoolaege, J. M. Verger, L. Vermare, C. Verona, T.h. Versloot, M. Vervier, J. Vicente, S. Villari, E. Villedieu, F. Villone, J. E. Vince, G. J. Vine, B. Viola, E. Vitale, R. Vitelli, M. Vlad, I. Voitsekhovitch, M. Vrancken, K. Vulliez, C. W. F. Waldon, M. Walker, M. J. Walsh, J. Waterhouse, M. L. Watkins, M. J. Watson, T. Wauters, M. W. Way, C. R. Webb, J. Weiland, H. Weisen, M. Weiszflog, R. Wenninger, A. T. West, J. M. Weulersse, B. Weyssow, M. R. Wheatley, A. D. Whiteford, A. M. Whitehead, A. G. Whitehurst, A. M. Widdowson, R. C. Wieggers, C. Wiegmann, S. Wiesen, A. Wilson, D. Wilson, D. J. Wilson, H. R. Wilson, M. Wischmeier, D. M. Witts, R. C. Wolf, J. Wolowski, P. Woscov, G. M. Wright, J. Wright, G. S. Xu, V. Yavorskij, V. Yerashok, J. Yorkshades, C. Young, D. Young, I. D. Young, X. Yuhong, L. Zabeo, A. Zabolotsky, L. Zaccarian, R. Zagorski, F. S. Zaitsev, S. Zajac, L. Zakharov, R. Zanino, V. Zaroschi, K. D. Zastrow, I. Zatz, B. Zefran, W. Zeidner, M. Zerbini, T. Zhang, Y. Zhu, E. Zilli, O. Zimmermann, V. Zoita, S. Zoletnik, W. Zwingman, JET EFDA Contributors, ALBANESE, Raffaele, AMBROSINO, GIUSEPPE, BELLIZIO, TERESA, CARANNANTE, GIUSEPPE, COCCORESE, VINCENZO, DE TOMMASI, GIANMARIA, MIANO, GIOVANNI, PIRONTI, ALFREDO, QUERCIA, ANTONIO, RUBINACCI, GUGLIELMO, J., Pamela, EMILIA R., Solano, AND JET EFDA, Contributor, J. M., Adam, G., Agarici, M., Agarici, H., Akhter, Albanese, Raffaele, Romanelli, F., Laxaback, F., Abel, I., Afanesyev, V., Agarici, G., Aggarwal, K. M., Airila, M., Akers, R., Alarcon, T. h., Alexeev, A., Alfier, A., Allan, P., Almaviva, S., Alonso, A., Alonso, M., Alper, B., Altmann, H., Alves, D., Ambrosino, Giuseppe, Amosov, V., Anda, G., Andersson, F., Andersson Sund́en, E., Andreev, V., Andrew, Y., Angelone, M., Anghel, M., Anghel, A., Angioni, C., Apruzzese, G., Arcis, N., Arena, P., Argouarch, A., Ariola, M., Armitano, A., Armstrong, R., Arnoux, G., Arshad, S., Artaserse, G., Artaud, J. F., Ash, A., Asp, E., Asunta, O., Atanasiu, C. V., Atkins, G., Axton, M. D., Ayres, C., Baciero, A., Bailescu, V., Baiocchi, B., Baker, R. A., Balboa, I., Balorin, C., Balshaw, N., Banks, J. W., Baranov, Y. F., Barbier, D., Barlow, I. L., Barnard, M. A., Barnsley, R., Barrena, L., Barrera, L., Baruzzo, M., Basiuk, V., Bateman, G., Batistoni, P., Baumgarten, N., Baylor, L., Bazylev, B., Beaumont, P. S., Beausang, K., B́ecoulet, M., Bekris, N., Beldishevski, M., Bell, A. C., Belli, F., Bellinger, M., Bellizio, Teresa, Belo, P. S. A., Belonohy, ́. E., Bennett, P. E., Benterman, N. A., Berger By, G., Bergsåker, H., Berk, H., Bernardo, J., Bertrand, B., Beurskens, M. N. A., Bieg, B., Bienkowska, B., Biewer, T., Biewer, T. M., Bigi, M., Bilato, R., Bird, J., Bizarro, J., Blackman, T. R., Blanchard, P., Blanco, E., Blum, J., Bobkov, V., Boboc, A., Boilson, D., Bolshakova, I., Bolzonella, T., Boncagni, L., Bonheure, G., Bonnin, X., Borba, D., Borthwick, A., Botrugno, A., Boulbe, C., Bouquey, F., Bourdelle, C., Bovert, K. v., Bowden, M., Boyce, T., Boyer, H. J., Bozhenkov, A., Brade, R. J., Bradshaw, J. M. A., Braet, J., Braic, V., Braithwaite, G. C., Brault, C., Braune, H., Breizman, B., Bremond, S., Brennan, P. D., Brett, A., Breue, J., Brezinsek, S., Bright, M. D. J., Briscoe, F., Brix, M., Brombin, M., Brown, B. C., Brown, D. P. D., Bruschi, A., Brzozowski, J., Bucalossi, J., Buckley, M. A., Budd, T., Budny, R., Budny, R. V., Bunting, P., Buratti, P., Burcea, G., Butcher, P. R., Buttery, R. J., Caç̃ao, R., Calabr`o, G., Callaghan, C. P., Caminade, J. P., Camp, P. G., Campling, D. C., Canik, J., Cannas, B., Capel, A. J., Carannante, Giuseppe, Card, P. J., Cardinali, A., Carlstrom, T., Carman, P., Carralero, D., Carraro, L., Carter, T., Carvalho, B. B., Carvalho, P., Casati, A., Castaldo, C., Caughman, J., Cavazzana, R., Cavinato, M., Cecconello, M., Cecil, F. E., Cenedese, A., Centioli, C., Cesario, R., Challis, C. D., Chandler, M., Chang, C., Chankin, A., Chapman, I. T., Child, D. J., Chiru, P., Chitarin, G., Chugonov, I., Chugunov, I., Ciric, D., Clairet, F., Clarke, R. H., Clay, R., Clever, M., Coad, J. P., Coates, P. A., Coccorese, Vincenzo, Cocilovo, V., Coda, S., Coelho, R., Coenen, J., Coffey, I., Colas, L., Cole, M., Collins, S., Combs, S., Compan, J., Conboy, J. E., Conroy, S., Cook, N., Cook, S. P., Coombs, D., Cooper, S. R., Corre, Y., Corrigan, G., Cortes, S., Coster, D., Counsell, G. F., Courtois, X., Cox, M., Craciunescu, T., Cramp, S., Crisanti, F., Croft, O., Crombe, K., Crowley, B. J., Cruz, N., Cupido, L., Curuia, M., Cusack, R. A., Czarnecka, A., Dalley, S., Daly, E. T., Dalziel, A., Darrow, D., David, O., Davies, N., Davis, J. J., Day, I. E., Day, C., De Angelis, R., Dearcas, G., de Baar, M. R., Delacal, E., de la Luna, E., de Pablos, J. L., De Temmerman, G., DE TOMMASI, Gianmaria, de Vries, P. C., Degli Agostini, F., Delabie, E., del Castillo Negrete, D., Delpech, L., Denisov, G., Denyer, A. J., Denyer, R. F., Devaux, S., Devynck, P., Di Matteo, L., Dipace, L., Dirken, P. J., Dnestrovskiy, A., Dodt, D., Dominiczak, K., Dorling, S. E., Douai, D., Down, A. P., Doyle, P. T., Drake, J. R., Dreischuh, T., Drozdov, V., Dumortier, P., Dunai, D., Duran, I., Durodíe, F., Dylst, K., Eaton, R., Edlington, T., Edwards, A. M., Edwards, D. T., Edwards, P. K., Eich, T. h., Ekedahl, A., Elevant, T., Elfimov, A., Ellingboe, B., Elsmore, C. G., Emmoth, B., Ericsson, G., Eriksson, L. G., Eriksson, A., Esposito, B., Esser, H. G., Estrada, T., Evangelidis, E. A., Evans, G. E., Ewart, G. D., Ewers, D. T., Falchetto, G., Falie, D., Fanthome, J. G. A., Farina, D., Farthing, J. W., Fasoli, A., Faugeras, B., Fedorczak, N., Felton, R. C., Fenzi, C., Fernandes, H., Ferreira, J. A., Ferreira, J., Ferron, J., Fessey, J. A., Figini, L., Figueiredo, A., Figueiredo, J., Finburg, P., Finken, K. H., Fischer, U., Fitzgerald, N., Flanagan, J., Fleming, C., Fonseca, A., Forbes, A. D., Ford, O., Formisano, A., Fraboulet, D., Francis, R. J., Frassinetti, L., Fresa, R., Friconneau, J. P., Frigione, D., Fuchs, J. C., Fullard, K., Fundamenski, W., Furno Palumbo, M., Gafert, J., Ǵal, K., Galṽao, R., Garavaglia, S., Garbet, X., Garcia, J., Gar cia Munoz, M., Gardner, W., Garibaldi, P., Garnier, D., Garzotti, L., Gatu Johnson, M., Gaudio, P., Gauthier, E., Gaze, J. W., Gear, D. F., Gedney, J., Gee, S. J., Gelfusa, M., Genangeli, E., Gerasimov, S., Geraud, A., Gerbaud, T., Gherendi, M., Ghirelli, N., Giacalone, J. C., Giacomelli, L., Gibson, C. S., Gil, C., Gilligan, S. J., Gimblett, C. G., Gin, D., Giovannozzi, E., Giroud, C., Giruzzi, G., Glowacz, S., Godwin, J., Goff, J. K., Gohil, P., Goloborod’Ko, V., Gonçalves, B., Goniche, M., Gonzales, S., Gonźalezde Vicente, S. M., Goodyear, A., Gorelenkov, N., Gorini, G., Goulding, R., Graham, B., Graham, D., Graham, M. E., Granucci, G., Graves, J., Green, N. R., Greuner, H., Grigore, E., Griph, F. S., Grisolia, C., Gros, G., Grossetti, G., Groth, M., Gr̈unhagen, S., Gryaznevich, M. P., Guirlet, R., Gulejova, B., Gunn, J., Gupta, A., Guzdar, P., Hacek, P., Hackett, L. J., Hacquin, S., Haist, B., Hakola, A., Hall, S. J., Hallworthcook, S. P., Hamilton, D. T., Han, H., Handley, R. C., Harding, S., Harling, J. D. W., Harting, D., Harvey, M. J., Haupt, T. D. V., Havlickova, E., Hawkes, N. C., Hawryluk, R., Hay, J. H., Hayashi, N., Haydon, P. W., Hayward, I. R., Hazel, S., Heesterman, P. J. L., Heidbrink, W., Heikkinen, J., Hellesen, C., Hellsten, T., Hemming, O. N., Hender, T. C., Henderson, M., Hennig, C., Hennion, V., Hidalgo, C., Higashijima, S., Hill, J. W., Hill, M., Hill, K., Hillairet, J., Hillis, D., Hirai, T., Hitchin, M., Hobirk, J., Hogan, C., Hogben, C. H. A., Hogeweij, G. M. D., Hollingham, I. C., Holyaka, R., Homfray, D. A., Honeyands, G., Hong, S. H., Hopf, C., Horn, B. A., Horton, A. R., Horton, L. D., Hotchin, S. P., Hough, M. R., Houlberg, W., Howell, D. F., Hron, M., Huber, A., Huddleston, T. M., Hudson, Z., Hughes, M., Ḧuhnerbein, M., Hume, C. C., Hunt, A. J., Hunter, C. L., Hutchinson, T. S., Huygen, S., Huysmans, G., Hyn̈onen, V., Ide, S., Igreja, R., Illescas, C., Imbeaux, F., Ivanova, D., Ivings, E., Jachmich, S., Jackson, G., Jacquet, P., Jakubowska, K., Jakubowski, M., James, P. V., Jaspers, R. J. E., Jednorog, S., Jenkins, I., Jennison, M. A. C., Jeskins, C., Jin Kwon, O., Joffrin, E., Johnson, M. F., Johnson, R., Johnson, T., Jolovic, D., Jonauskas, V., Jones, E. M., Jones, G., Jones, H. D., Jones, T. T. C., Jouvet, M., Juṕen, C., Kachtchouk, I., Kaczmarczyk, J., Kallenbach, A., K̈allne, J., Kalupin, D., Ḱalvin, S., Kamelander, G., Kamendje, R., Kappatou, A., Karttunen, S., Kasparek, W., Katramados, I., Kaufmann, M., Kaveney, G., Kaye, A. S., Kear, M. J., Keeling, D. L., Kelliher, D., Kempenaars, M., Khilar, P., Kidd, N. G., Kiisk, M., Kim, K. M., King, R. F., Kinna, D. J., Kiptily, V., Kirnev, G., Kirneva, N., Kirov, K., Kirschner, A., Kisielius, R., Kislov, D., Kiss, G., Kiviniemi, T., Kizane, G., Klein, A., Klix, A., Knaup, M., Kneuper, K., Kneupner, H., Knight, P. J., Knipe, S. J., Kocan, M., K̈ochl, F., Kocsis, G., Konz, C., Koppitz, T., Korotkov, A., Koslowski, H. R., Kotov, V., Kovari, M. D., Kovarik, K., Kramer, G., Krasilnikov, A., Krasilnikov, V., Kraus, S., Kreter, A., Krieger, K., Kritz, A., Krivchenkov, Y., Kruezi, U., Krychowiak, M., Krylov, S., Ksiazek, I., Kubic, M., Kuhn, S., K̈uhnlein, W., Kurki Suonio, T., Kurowski, A., Kuteev, B., Kuyanov, A., La Haye, R., Laan, M., Labate, C., Lachichi, A., Lam, N., Lang, P., Large, M. T., Lassiwe, I., Last, J. R., Lawson, K. D., Laxåback, M., Layne, R. A., Lazzaro, E., Leguern, F., Leblanc, B., Leggate, H. J., Lehnen, M., Leigheb, M., Lengar, I., Lennholm, M., Lerche, E., Lescure, C. N., Li, Y., Li Puma, A., Liang, Y., Likonen, J., Lin, Y., Linke, J., Linstead, S. A., Lipshultz, B., Litaudon, X., Litvak, A. G., Liu, Y., Loarer, T., Loarte, A., Lobel, R. C., Lomas, P. J., Long, F. D., L̈onnroth, J., Looker, D. J., Lopez, J., Lotte, P. h., Loughlin, M. J., Loving, A. B., Lowry, C., Luce, T., Lucock, R. M. A., Lukanitsa, A., Lungu, A. M., Lungu, C. P., Lyssoivan, A., Macheta, P., Mackenzie, A. S., Macrae, M., Maddaluno, G., Maddison, G. P., Madsen, J., Maget, P., Maggi, C., Maier, H., Mailloux, J., Makowski, M., Manning, C. J., Mansfield, M., Manso, M. E., Mantica, P., Mantsinen, M., Maraschek, M., Marchetto, C., Marchitti, M. A., Mardenfeld, M., Marechal, J. L., Marinelli, M., Marinoni, A., Marinucci, M., M̈arki, J., Marocco, D., Marren, C. A., Martin, D., Martin, D. L., Martin, G., Martin, Y., Mart́ın Soĺıs, J. R., Masaki, K., Masiello, A., Maslov, M., Maszl, C., Matilal, A., Mattei, M., Matthews, G. F., Maviglia, F., May, C. R., Mayer, M., Mayoral, M. L., Mazon, D., Mazzotta, C., Mazzucato, E., Mccarthy, P., Mcclements, K. G., Mccormick, K., Mccullen, P. A., Mccune, D., Mcdonald, D. C., Mcgregor, R., Mckivitt, J. P., Meakins, A., Medina, F., Meigs, A. G., Menard, M., Meneses, L., Menmuir, S., Merrigan, I. R., Mertens, P. h., Messiaen, A., Meyer, H., Miano, Giovanni, Miele, M., Migliucci, P., Miller, A. G., Mills, S. F., Milnes, J. J., Min Kim, K., Mindham, T., Mirizzi, F., Mirones, E., Mironov, M., Mitteau, R., Mlynar, J., Mollard, P., Monakhov, I., Monier Garbet, P., Mooney, R., Moradi, S., Moreau, D., Moreau, P. h., Moreira, L., Morgan, A., Morgan, P. D., Morlock, C., Moro, A., Morris, A. W., Mort, G. L., Mrozek, C., Mueck, A., M̈uller, H. W., Murakami, M., Murari, A., Mustata, I., Nabais, F., Nardon, E., Nash, G., Naulin, V., Nave, M. F. F., Nazikian, R., Nedzelski, I., Negus, C. R., Neilson, J. D., Neto, A., Neu, R., Neubauer, O., Newbert, G. J., Newman, M., Nicholls, K. J., Nicolai, A., Nicolas, L., Nieckchen, P., Nielsen, P., Nielsen, A. H., Nielsen, S. K., Nielson, G., Nieto, J., Nightingale, M. P. S., Noble, C., Nocente, M., Nora, M., Nordman, H., Norman, M., Noterdaeme, J. M., Nowak, S., Nunes, I., Ognissanto, F., O’Gorman, T., Olariu, S., Oleynikov, A., O’Mullane, M., Ongena, J., Orsitto, F., Oswuigwe, O. I., Ottaviani, M., Oyama, N., Pacella, D., Paget, K., Palazzo, S., Pamela, J., Pamela, S., Panek, R., Pangione, L., Panin, A., Panis, T. h., Pankin, A., Pantea, A., Parail, V., Parisot, T. h., Parkin, A., Parsloe, A., Parsons, B. T., Pasqualotto, R., Pastor, P., Paterson, R., Paul, M. K., Peach, D., Pearce, R. J. H., Pearson, B. J., Pearson, I. J., Pedrick, L. C., Pedrosa, M. A., Pegourie, B., Pereira, R., Perelli Cippo, E., Pereverzev, G., Perevezentsev, A., Perezvonthun, C. h., Pericoli Ridolfini, V., Perona, A., Perrot, Y., Peruzzo, S., Peschanyy, S., Petravich, G., Petrizzi, L., Petrov, V., Petrzilka, V., Philipps, V., Piazza, G., Piccolo, F., Pietropaolo, A., Pillon, M., Pinches, S. D., Pinna, T., Pintsuk, G., Piovesan, P., Pironti, Alfredo, Pisano, F., Pitts, R., Plaum, B., Plyusnin, V., Polasik, M., Poli, F. M., Pomaro, N., Pompilian, O., Poncet, L., Pool, P. J., Popovichev, S., Porcelli, F., Porfiri, M. T., Portafaix, C., Pospieszczyk, A., Possnert, G., Prestopino, G., Prior, P., Prokopowicz, R., Proverbio, I., Pugno, R., Puiatti, M. E., Purahoo, K., Pustovitov, V., P̈utterich, T. h., P̈uttmann Kneupner, D., Quercia, Antonio, Rachlew, E., Rademaker, R., Rafiq, T., Rainford, M. S. J., Ramogida, G., Rantam̈aki, K., Rapp, J., Rasmussen, J. J., Ratt́a, G., Ravera, G., Reich, M., Reichle, R., Reiser, D., Reiss, R., Reiter, D., Rendell, D., Reux, C., Rewoldt, G., Ribeiro, T. T., Riccardo, V., Richards, D., Rigollet, F., Rimini, F. G., Rios, L., Riva, M., Roberts, J. E. C., Robins, R. J., Robinson, D. S., Robinson, S. A., Robson, D. W., Roche, H., R̈odig, M., Rodionov, N., Rohde, V., Rolfe, A., Romanelli, M., Romano, A., Romero, J., Ronchi, E., Rosanvallon, S., Roux, C. h., Rowe, S., Rubel, M., Rubinacci, Guglielmo, Ruchko, L., Ruiz, M., Ruset, C., Russell, M., Ruth, A., Ryc, L., Rydzy, A., Ryter, F., Rzadkiewicz, J., Saarelma, S., Sabathier, F., Sabot, R., Sadakov, S., Sagar, P., Saibene, G., Saille, A., Saint Laurent, F., Salmi, A., Salomaa, R., Salzedas, F., Samm, U., Sanchez, P., Sanders, S., Sanders, S. G., Sandford, G., Sandland, K., Sandquist, P., Sands, D. E. G., Santala, M. I. K., Sartori, F., Sartori, R., Sauter, O., Savelyev, A., Savtchkov, A., Scales, S. C., Scarabosio, A., Schaefer, N., Schlatter, C. h., Schmidt, V., Schmidt, A., Schmitz, O., Schmuck, S., Schneider, M., Scholz, M., Scḧopf, K., Schweer, B., Schweinzer, J., Scott, B., Seki, M., Semeraro, L., Semerok, A., Sergienko, G., Serra, F., Sertoli, M., Shannon, M. M. J., Sharapov, S. E., Shaw, S. R., Shevelev, A., Sievering, R., Silva, C. A., Simmons, P. A., Simonetto, A., Simpson, D., Sipila, S., Sips, A. C. C., Sirinelli, A., Sj̈ostrand, H., Skopintsev, D., K. S. l. a. b. k. o. w. s. k. a., Smith, P. G., Snipes, J., Snoj, L., Snyder, S., Soare, S., Solano, E. R., Soldatov, S., Soleto, A., Solomon, W., Soltane, C., Sonato, P., Sopplesa, A., Sorrentino, A., Sousa, J., Sowden, C. B. C., Sozzi, C., Sp̈ah, P., Spelzini, T., Spence, J., Spineanu, F., Spuig, P., Sẗabler, A., Stagg, R. D., Stamp, M. F., Stancalie, V., Stangeby, P., Stan Sion, C., Starkey, D. E., Stead, M. J., Stephen, A. V., Stevens, A. L., Stober, J., Stokes, R. B., Stork, D., Stoyanov, D., Strachan, J., Strand, P., Stransky, M., Strauss, D., Strintzi, D., Studholme, W., Suna, Y., Subba, F., Summers, H. P., Sun, Y., Surdu Bob, C., Surrey, E., Sutton, D. J., Svensson, J., Swain, D., Syme, B. D., Symonds, I. D., Szepesi, T., Szydlowski, A., Tabares, F., Takalo, V., Takenaga, H., Tala, T., Talbot, A. R., Taliercio, C., Tame, C., Tardini, G., Tardocchi, M., Taroni, L., Telesca, G., Terra, A., Terrington, A. O., Testa, D., Theis, J. M., Thomas, J. D., Thomas, P. D., Thomas, P. R., Thompson, V. K., Thomsen, H., Thomser, C., Thyagaraja, A., Tigwell, P. A., Tiseanu, I., Tivey, R., Todd, J. M., Todd, T. N., Tokar, M. Z., Tosti, S., Trabuc, P., Travere, J. M., Treutterer, W., Trimble, P., Trkov, A., Trukhina, E., Tsalas, M., Tsige Tamirat, H., Tsitrone, E., Tskhakaya jun, D., Tudisco, O., Tugarinov, S., Turner, M. M., Turri, G., Tyrrell, S. G. J., Umeda, N., Unterberg, B., Urano, H., Urquhart, A. J., Uytdenhouwen, I., Vaccaro, A., Vadgama, A. P., Vagliasindi, G., Valcarcel, D., Valisa, M., Vallory, J., Valovic, M., Van Eester, D., van Milligen, B., van Rooij, G. J., Varandas, C. A. F., Vartanian, S., Vdovin, V., Vega, J., Verdoolaege, G., Verger, J. M., Vermare, L., Verona, C., Versloot, T. h., Vervier, M., Vicente, J., Villari, S., Villedieu, E., Villone, F., Vince, J. E., Vine, G. J., Viola, B., Vitale, E., Vitelli, R., Vlad, M., Voitsekhovitch, I., Vrancken, M., Vulliez, K., Waldon, C. W. F., Walker, M., Walsh, M. J., Waterhouse, J., Watkins, M. L., Watson, M. J., Wauters, T., Way, M. W., Webb, C. R., Weiland, J., Weisen, H., Weiszflog, M., Wenninger, R., West, A. T., Weulersse, J. M., Weyssow, B., Wheatley, M. R., Whiteford, A. D., Whitehead, A. M., Whitehurst, A. G., Widdowson, A. M., Wieggers, R. C., Wiegmann, C., Wiesen, S., Wilson, A., Wilson, D., Wilson, D. J., Wilson, H. R., Wischmeier, M., Witts, D. M., Wolf, R. C., Wolowski, J., Woscov, P., Wright, G. M., Wright, J., G. S., Xu, Yavorskij, V., Yerashok, V., Yorkshades, J., Young, C., Young, D., Young, I. D., Yuhong, X., Zabeo, L., Zabolotsky, A., Zaccarian, L., Zagorski, R., Zaitsev, F. S., Zajac, S., Zakharov, L., Zanino, R., Zaroschi, V., Zastrow, K. D., Zatz, I., Zefran, B., Zeidner, W., Zerbini, M., Zhang, T., Zhu, Y., Zilli, E., Zimmermann, O., Zoita, V., Zoletnik, S., Zwingman, W., JET EFDA Contributors, Romanelli, F, Laxaback, M, Abel, I, Afanesyev, V, Agarici, G, Aggarwal, K, Airila, M, Akers, R, Alarcon, T, Albanese, R, Alexeev, A, Alfier, A, Allan, P, Almaviva, S, Alonso, A, Alonso, M, Alper, B, Altmann, H, Alves, D, Ambrosino, G, Amosov, V, Anda, G, Andersson, F, Andersson Sunden, E, Andreev, V, Andrew, Y, Angelone, M, Anghel, M, Anghel, A, Angioni, C, Apruzzese, G, Arcis, N, Arena, P, Argouarch, A, Ariola, M, Armitano, A, Armstrong, R, Arnoux, G, Arshad, S, Artaserse, G, Artaud, J, Ash, A, Asp, E, Asunta, O, Atanasiu, C, Atkins, G, Axton, M, Ayres, C, Baciero, A, Bailescu, V, Baiocchi, B, Baker, R, Balboa, I, Balorin, C, Balshaw, N, Banks, J, Baranov, Y, Barbier, D, Barlow, I, Barnard, M, Barnsley, R, Barrena, L, Barrera, L, Baruzzo, M, Basiuk, V, Bateman, G, Batiston, P, Baumgarten, N, Baylor, L, Bazylev, B, Beaumont, P, Beausang, K, Becoulet, M, Bekris, N, Beldishevski, M, Bell, A, Belli, F, Bellinger, M, Bellizio, T, Belo, P, Belonohy, E, Bennett, P, Benterman, N, Berger By, G, Bergsaker, H, Berk, H, Bernardo, J, Bertrand, B, Beurskens, M, Bieg, B, Bienkowska, B, Biewer, T, Bigi, M, Bilato, R, Bird, J, Bizarro, J, Blackman, T, Blanchard, P, Blanco, E, Blum, J, Bobkov, V, Boboc, A, Boilson, D, Bolshakova, I, Bolzonella, T, Boncagni, L, Bonheure, G, Bonnin, X, Borba, D, Borthwick, A, Botrugno, A, Boulbe, C, Bouquey, F, Bourdelle, C, Bovert, K, Bowden, M, Boyce, T, Boyer, H, Bozhenkov, A, Brade, R, Bradshaw, J, Braet, J, Braic, V, Braithwaite, G, Brault, C, Braune, H, Breizman, B, Bremond, S, Brennan, P, Brett, A, Breue, J, Brezinsek, S, Bright, M, Briscoe, F, Brix, M, Brombin, M, Brown, B, Brown, D, Bruschi, A, Brzozowski, J, Bucalossi, J, Buckley, M, Budd, T, Budny, R, Bunting, P, Buratti, P, Burcea, G, Butcher, P, Buttery, R, Cacao, R, Calabro, G, Callaghan, C, Caminade, J, Camp, P, Campling, D, Canik, J, Cannas, B, Capel, A, Carannante, G, Card, P, Cardinali, A, Carlstrom, T, Carman, P, Carralero, D, Carraro, L, Carter, T, Carvalho, B, Carvalho, P, Casati, A, Castaldo, C, Caughman, J, Cavazzana, R, Cavinato, M, Cecconello, M, Cecil, F, Cenedese, A, Centioli, C, Cesario, R, Challis, C, Chandler, M, Chang, C, Chankin, A, Chapman, I, Child, D, Chiru, P, Chitarin, G, Chugonov, I, Ciric, D, Clairet, F, Clarke, R, Clay, R, Clever, M, Coad, J, Coates, P, Coccorese, V, Cocilovo, V, Coda, S, Coelho, R, Coenen, J, Coffey, I, Colas, L, Cole, M, Collins, S, Combs, S, Compan, J, Conboy, J, Conroy, S, Cook, N, Cook, S, Coombs, D, Cooper, S, Corre, Y, Corrigan, G, Cortes, S, Coster, D, Counsell, G, Courtois, X, Cox, M, Craciunescu, T, Cramp, S, Crisanti, F, Croft, O, Crombe, K, Crowley, B, Cruz, N, Cupido, L, Curuia, M, Cusack, R, Czarnecka, A, Dalley, S, Daly, E, Dalziel, A, Darrow, D, David, O, Davies, N, Davis, J, Day, I, Day, C, De Angelis, R, de Arcas, G, de Baar, M, de la Cal, E, de la Luna, E, de Pablos, J, De Temmerman, G, De Tommasi, G, de Vries, P, Degli Agostini, F, Delabie, E, del Castillo Negrete, D, Delpech, L, Denisov, G, Denyer, A, Denyer, R, Devaux, S, Devynck, P, Di Matteo, L, Di Pace, L, Dirken, P, Dnestrovskiy, A, Dodt, D, Dominiczak, K, Dorling, S, Douai, D, Down, A, Doyle, P, Drake, J, Dreischuh, T, Drozdov, V, Dumortier, P, Dunai, D, Duran, I, Durodie, F, Dylst, K, Eaton, R, Edlington, T, Edwards, A, Edwards, D, Edwards, P, Eich, T, Ekedahl, A, Elevant, T, Elfimov, A, Ellingboe, B, Elsmore, C, Emmoth, B, Ericsson, G, Eriksson, L, Eriksson, A, Esposito, B, Esser, H, Estrada, T, Evangelidis, E, Evans, G, Ewart, G, Ewers, D, Falchetto, G, Falie, D, Fanthome, J, Farina, D, Farthing, J, Fasoli, A, Faugeras, B, Fedorczak, N, Felton, R, Fenzi, C, Fernandes, H, Ferreira, J, Ferron, J, Fessey, J, Figini, L, Figueiredo, A, Figueiredo, J, Finburg, P, Finken, K, Fischer, U, Fitzgerald, N, Flanagan, J, Fleming, C, Fonseca, A, Forbes, A, Ford, O, Formisano, A, Fraboulet, D, Francis, R, Frassinetti, L, Fresa, R, Friconneau, J, Frigione, D, Fuchs, J, Fullard, K, Fundamenski, W, Furno Palumbo, M, Gafert, J, Gal, K, Galvao, R, Garavaglia, S, Garbet, X, Garcia, J, Garcia Munoz, M, Gardner, W, Garibaldi, P, Garnier, D, Garzotti, L, Gatu Johnson, M, Gaudio, P, Gauthier, E, Gaze, J, Gear, D, Gedney, J, Gee, S, Gelfusa, M, Genangeli, E, Gerasimov, S, Geraud, A, Gerbaud, T, Gherendi, M, Ghirelli, N, Giacalone, J, Giacomelli, L, Gibson, C, Gil, C, Gilligan, S, Gimblett, C, Gin, D, Giovannozzi, E, Giroud, C, Giruzzi, G, Glowacz, S, Godwin, J, Goff, J, Gohil, P, Goloborod'Ko, V, Goncalves, B, Goniche, M, Gonzales, S, Gonzales de Vicente, S, Goodyear, A, Gorelenkov, N, Gorini, G, Goulding, R, Graham, B, Graham, D, Graham, M, Granucci, G, Graves, J, Green, N, Greuner, H, Grigore, E, Griph, F, Grisolia, C, Gros, G, Grossetti, G, Groth, M, Gruenhagen, S, Gryaznevich, M, Guirlet, R, Gulejova, B, Gunn, J, Gupta, A, Guzdar, P, Hacek, P, Hackett, L, Hacquin, S, Haist, B, Hakola, A, Hall, S, Hallworth Cook, S, Hamilton, D, Han, H, Handley, R, Harding, S, Harling, J, Harting, D, Harvey, M, Haupt, T, Havlickova, E, Hawkes, N, Hawryluk, R, Hay, J, Hayashi, N, Haydon, P, Hayward, I, Hazel, S, Heesterman, P, Heidbrink, W, Heikkinen, J, Hellesen, C, Hellsten, T, Hemming, O, Hender, T, Henderson, M, Hennig, C, Hennion, V, Hidalgo, C, Higashijima, S, Hill, J, Hill, M, Hill, K, Hillairet, J, Hillis, D, Hirai, T, Hitchin, M, Hobirk, J, Hogan, C, Hogben, C, Hogeweij, G, Hollingham, I, Holyaka, R, Homfray, D, Honeyands, G, Hong, S, Hopf, C, Horn, B, Horton, A, Horton, L, Hotchin, S, Hough, M, Houlberg, W, Howell, D, Hron, M, Huber, A, Huddleston, T, Hudson, Z, Hughes, M, Huehnerbein, M, Hume, C, Hunt, A, Hunter, C, Hutchinson, T, Huygen, S, Huysmans, G, Hynoenen, V, Ide, S, Igreja, R, Illescas, C, Imbeaux, F, Ivanova, D, Ivings, E, Jachmich, S, Jackson, G, Jacquet, P, Jakubowska, K, Jakubowski, M, James, P, Jaspers, R, Jednorog, S, Jenkins, I, Jennison, M, Jeskins, C, Jin Kwon, O, Joffrin, E, Johnson, M, Johnson, R, Johnson, T, Jolovic, D, Jonauskas, V, Jones, E, Jones, G, Jones, H, Jones, T, Jouvet, M, Jupen, C, Kachtchouk, I, Kaczmarczyk, J, Kallenbach, A, Kaellne, J, Kalupin, D, Kalvin, S, Kamelander, G, Kamendje, R, Kappatou, A, Karttunen, S, Kasparek, W, Katramados, I, Kaufmann, M, Kaveney, G, Kaye, A, Kear, M, Keeling, D, Kelliher, D, Kempenaars, M, Khilar, P, Kidd, N, Kiisk, M, Kim, K, King, R, Kinna, D, Kiptily, V, Kirnev, G, Kirneva, N, Kirov, K, Kirschner, A, Kisielius, R, Kislov, D, Kiss, G, Kiviniemi, T, Kizane, G, Klein, A, Klix, A, Knaup, M, Kneuper, K, Kneupner, H, Knight, P, Knipe, S, Kocan, M, Koechl, F, Kocsis, G, Konz, C, Koppitz, T, Korotkov, A, Koslowski, H, Kotov, V, Kovari, M, Kovarik, K, Kramer, G, Krasilnikov, A, Krasilnikov, V, Kraus, S, Kreter, A, Krieger, K, Kritz, A, Krivchenkov, Y, Kruezi, U, Krychowiak, M, Krylov, S, Ksiazek, I, Kubic, M, Kuhn, S, Kuehnlein, W, Kurki Suonio, T, Kurowski, A, Kuteev, B, Kuyanov, A, La Haye, R, Laan, M, Labate, C, Lachichi, A, Lam, N, Lang, P, Large, M, Lassiwe, I, Last, J, Lawson, K, Layne, R, Lazzaro, E, Le Guern, F, Leblanc, B, Leggate, H, Lehnen, M, Leigheb, M, Lengar, I, Lennholm, M, Lerche, E, Lescure, C, Li, Y, Li Puma, A, Liang, Y, Likonen, J, Lin, Y, Linke, J, Linstead, S, Lipshultz, B, Litaudon, X, Litvak, A, Liu, Y, Loarer, T, Loarte, A, Lobel, R, Lomas, P, Long, F, Loennroth, J, Looker, D, Lopez, J, Lotte, P, Loughlin, M, Loving, A, Lowry, C, Luce, T, Lucock, R, Lukanitsa, A, Lungu, A, Lungu, C, Lyssoivan, A, Macheta, P, Mackenzie, A, Macrae, M, Maddaluno, G, Maddison, G, Madsen, J, Maget, P, Maggi, C, Maier, H, Mailloux, J, Makowski, M, Manning, C, Mansfield, M, Manso, M, Mantica, P, Mantsinen, M, Maraschek, M, Marchetto, C, Marchitti, M, Mardenfeld, M, Marechal, J, Marinelli, M, Marinoni, A, Marinucci, M, Maerki, J, Marocco, D, Marren, C, Martin, D, Martin, G, Martin, Y, Martin Solis, J, Masaki, K, Masiello, A, Maslov, M, Maszl, C, Matilal, A, Mattei, M, Matthews, G, Maviglia, F, May, C, Mayer, M, Mayoral, M, Mazon, D, Mazzotta, C, Mazzucato, E, Mccarthy, P, Mcclements, K, Mccormick, K, Mccullen, P, Mccune, D, Mcdonald, D, Mcgregor, R, Mckivitt, J, Meakins, A, Medina, F, Meigs, A, Menard, M, Meneses, L, Menmuir, S, Merrigan, I, Mertens, P, Messiaen, A, Meyer, H, Miano, G, Miele, M, Migliucci, P, Miller, A, Mills, S, Milnes, J, Min Kim, K, Mindham, T, Mirizzi, F, Mirones, E, Mironov, M, Mitteau, R, Mlynar, J, Mollard, P, Monakhov, I, Monier Garbet, P, Mooney, R, Moradi, S, Moreau, D, Moreau, P, Moreira, L, Morgan, A, Morgan, P, Morlock, C, Moro, A, Morris, A, Mort, G, Mrozek, C, Mueck, A, Mueller, H, Murakami, M, Murari, A, Mustata, I, Nabais, F, Nardon, E, Nash, G, Naulin, V, Nave, M, Nazikian, R, Nedzelski, I, Negus, C, Neilson, J, Neto, A, Neu, R, Neubauer, O, Newbert, G, Newman, M, Nicholls, K, Nicolai, A, Nicolas, L, Nieckchen, P, Nielsen, P, Nielsen, A, Nielsen, S, Nielson, G, Nieto, J, Nightingale, M, Noble, C, Nocente, M, Nora, M, Nordman, H, Norman, M, Noterdaeme, J, Nowak, S, Nunes, I, Ognissanto, F, O'Gorman, T, Olariu, S, Oleynikov, A, O'Mullane, M, Ongena, J, Orsitto, F, Oswuigwe, O, Ottaviani, M, Oyama, N, Pacella, D, Paget, K, Palazzo, S, Pamela, J, Pamela, S, Panek, R, Pangione, L, Panin, A, Panis, T, Pankin, A, Pantea, A, Parail, V, Parisot, T, Parkin, A, Parsloe, A, Parsons, B, Pasqualotto, R, Pastor, P, Paterson, R, Paul, M, Peach, D, Pearce, R, Pearson, B, Pearson, I, Pedrick, L, Pedrosa, M, Pegourie, B, Pereira, R, Perelli Cippo, E, Pereverzev, G, Perevezentsev, A, Perez von Thun, C, Pericoli Ridolfini, V, Perona, A, Perrot, Y, Peruzzo, S, Peschanyy, S, Petravich, G, Petrizzi, L, Petrov, V, Petrzilka, V, Philipps, V, Piazza, G, Piccolo, F, Pietropaolo, A, Pillon, M, Pinches, S, Pinna, T, Pintsuk, G, Piovesan, P, Pironti, A, Pisano, F, Pitts, R, Plaum, B, Plyusnin, V, Polasik, M, Poli, F, Pomaro, N, Pompilian, O, Poncet, L, Pool, P, Popovichev, S, Porcelli, F, Porfiri, 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Subjects
Nuclear and High Energy Physics, 52.55.Fa Tokamaks, spherical tokamak, Materials science, Tokamak, Physics and Astronomy (all), Condensed Matter Physics, Física [Ciências exactas e naturais], Cyclotron, law.invention, Bootstrap current, Physical sciences [Natural sciences], law, Physics::Plasma Physics, ITER, divertor, FIS/03 - FISICA DELLA MATERIA, Nuclear and High Energy Physic, Jet (fluid), Safety factor, Divertor, 52.50.Qt Plasma heating by radio-frequency field, Settore FIS/01 - Fisica Sperimentale, magnetic confinement, Magnetic confinement fusion, Física, 52.55.Rk Power exhaust, JET, overview, Settore FIS/07 - Fisica Applicata(Beni Culturali, Ambientali, Biol.e Medicin), Computational physics, Physical sciences, ICR, ICP, helicons, ___, JET, Beta (plasma physics), Atomic physics, tokamaks
Abstract

Since the last IAEA conference, the scientific programme of JET has focused on the qualification of the integrated operating scenarios for ITER and on physics issues essential for the consolidation of design choices and the efficient exploitation of ITER. Particular attention has been given to the characterization of the edge plasma, pedestal energy and edge localized modes (ELMs), and their impact on plasma facing components (PFCs). Various ELM mitigation techniques have been assessed for all ITER operating scenarios using active methods such as resonant magnetic field perturbation, rapid variation of the radial field and pellet pacing. In particular, the amplitude and frequency of type I ELMs have been actively controlled over a wide parameter range (q(95) = 3-4.8, beta(N)

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