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1. Turbulent heating in an inhomogeneous, magnetised plasma slab

Author

Barnes, M., Abiuso, P., and Dorland, W.

Subjects
Plasma Physics (physics.plasm-ph), Physics::Plasma Physics, FOS: Physical sciences, Physics - Plasma Physics
Abstract

Observational evidence in space and astrophysical plasmas with long collisional mean free path suggests that more massive charged particles may be preferentially heated. One possible mechanism for this is the turbulent cascade of energy from injection to dissipation scales, where the energy is converted to heat. Here we consider a simple system consisting of a magnetized plasma slab of electrons and a single ion species with a cross-field density gradient. We show that such a system is subject to an electron drift wave instability, known as the universal instability, which is stabilized only when the electron and ion thermal speeds are equal. For unequal thermal speeds, we find that the instability gives rise to turbulent energy exchange between ions and electrons that acts to equalize the thermal speeds. Consequently, this turbulent heating tends to equalize the component temperatures of pair plasmas and to heat ions to much higher temperatures than electrons for conventional mass-ratio plasmas., Comment: 11 pages, 3 figures, submitted to the Journal of Plasma Physics

Published
2018
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3. A model of turbulence in magnetized plasmas: Implications for the dissipation range in the solar wind

Author

Howes, G, Cowley, S, Dorland, W, Hammett, G, Quataert, E, and Schekochihin, A

Subjects
Physics::Plasma Physics, Astrophysics (astro-ph), Physics::Space Physics, FOS: Physical sciences, Astrophysics
Abstract

This paper studies the turbulent cascade of magnetic energy in weakly collisional magnetized plasmas. A cascade model is presented, based on the assumptions of local nonlinear energy transfer in wavenumber space, critical balance between linear propagation and nonlinear interaction times, and the applicability of linear dissipation rates for the nonlinearly turbulent plasma. The model follows the nonlinear cascade of energy from the driving scale in the MHD regime, through the transition at the ion Larmor radius into the kinetic Alfven wave regime, in which the turbulence is dissipated by kinetic processes. The turbulent fluctuations remain at frequencies below the ion cyclotron frequency due to the strong anisotropy of the turbulent fluctuations, k_parallel << k_perp (implied by critical balance). In this limit, the turbulence is optimally described by gyrokinetics; it is shown that the gyrokinetic approximation is well satisfied for typical slow solar wind parameters. Wave phase velocity measurements are consistent with a kinetic Alfven wave cascade and not the onset of ion cyclotron damping. The conditions under which the gyrokinetic cascade reaches the ion cyclotron frequency are established. Cascade model solutions imply that collisionless damping provides a natural explanation for the observed range of spectral indices in the dissipation range of the solar wind. The dissipation range spectrum is predicted to be an exponential fall off; the power-law behavior apparent in observations may be an artifact of limited instrumental sensitivity. The cascade model is motivated by a programme of gyrokinetic simulations of turbulence and particle heating in the solar wind., 29 pages, 14 figures

Published
2016

4. Considering Fluctuation Energy as a Measure of Gyrokinetic Turbulence

Author

Plunk, G. G., Tatsuno, T., and Dorland, W.

Subjects
Plasma Physics (physics.plasm-ph), FOS: Physical sciences, Physics - Plasma Physics
Abstract

In gyrokinetic theory there are two quadratic measures of fluctuation energy, left invariant under nonlinear interactions, that constrain the turbulence. The recent work of Plunk and Tatsuno [Phys. Rev. Lett. 106, 165003 (2011)] reported on the novel consequences that this constraint has on the direction and locality of spectral energy transfer. This paper builds on that work. We provide detailed analysis in support of the results of Plunk and Tatsuno but also significantly broaden the scope and use additional methods to address the problem of energy transfer. The perspective taken here is that the fluctuation energies are not merely formal invariants of an idealized model (two-dimensional gyrokinetics) but are general measures of gyrokinetic turbulence, i.e. quantities that can be used to predict the behavior of the turbulence. Though many open questions remain, this paper collects evidence in favor of this perspective by demonstrating in several contexts that constrained spectral energy transfer governs the dynamics., Comment: Final version as published. Some cosmetic changes and update of references

Published
2012
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5. Gyrokinetic simulation of entropy cascade in two-dimensional electrostatic turbulence

Author

Tatsuno, T, Barnes, M, Cowley, SC, Dorland, W, Howes, GG, Numata, R, Plunk, GG, and Schekochihin, AA

Subjects
Plasma Physics (physics.plasm-ph), Astrophysics - Solar and Stellar Astrophysics, Physics::Plasma Physics, Physics::Space Physics, Fluid Dynamics (physics.flu-dyn), FOS: Physical sciences, Physics - Fluid Dynamics, Computational Physics (physics.comp-ph), Physics - Computational Physics, Physics - Plasma Physics, Solar and Stellar Astrophysics (astro-ph.SR)
Abstract

Two-dimensional electrostatic turbulence in magnetized weakly-collisional plasmas exhibits a cascade of entropy in phase space [Phys. Rev. Lett. 103, 015003 (2009)]. At scales smaller than the gyroradius, this cascade is characterized by the dimensionless ratio D of the collision time to the eddy turnover time measured at the scale of the thermal Larmor radius. When D >> 1, a broad spectrum of fluctuations at sub-Larmor scales is found in both position and velocity space. The distribution function develops structure as a function of v_{perp}, the velocity coordinate perpendicular to the local magnetic field. The cascade shows a local-scale nonlinear interaction in both position and velocity spaces, and Kolmogorov's scaling theory can be extended into phase space., 8 pages, 10 figures, Conference paper presented at 2009 Asia-Pacific Plasma Theory Conference. Ver.2 includes corrected typos & updated references

Published
2010
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6. Dimits Shift in Realistic Gyrokinetic Plasma-Turbulence Simulations

Author

D. R. Mikkelsen and Dorland W

Subjects
Physics, Tokamak, Turbulence, General Physics and Astronomy, Plasma, Electron, Collisionality, Instability, Computational physics, law.invention, Heat flux, Physics::Plasma Physics, law, Quantum mechanics, Physics::Space Physics, Adiabatic process
Abstract

In simulations of turbulent plasma transport due to long wavelength (k{sub perpendicular}){rho}{sub i}{

Published
2008
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7. Model Collision Operators for Numerical Gyrokinetics

Author

Abel, I. G., Barnes, M., Cowley, S. C., Dorland, W., Gregory Hammett, Schekochihin, A. A., Tatsuno, T., Garbet, X., Sauter, O., and Sindoni, E.

Subjects
Physics, Conservation law, Operator (computer programming), Physics::Plasma Physics, Numerical analysis, Gyrokinetics, Code (cryptography), Statistical physics, K-omega turbulence model, Dissipation, Collision
Abstract

We motivate the need to include collisional dissipation in gyrokinetic turbulence simulations, and construct criteria for a physically valid model of such dissipation. A new analytically manageable operator satisfying those criteria is presented and transformed into gyrokinetic variables. The form of conservation laws for collision operators in gyrokinetic variables is explained. The numerical implementation of our new operator in the code GS2 is outlined and successful tests from this code presented.

Published
2008
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8. Fast and slow nonlinear tearing mode reconnection

Author

Loureiro, N. F., Cowley, S. C., Dorland, W. D., Haines, M. G., and Schekochihin, A. A.

Subjects
Plasma Physics (physics.plasm-ph), Physics - Space Physics, FOS: Physical sciences, Physics - Plasma Physics, Space Physics (physics.space-ph)
Abstract

This is a brief account of our numerical study of the tearing mode reconnection. We demonstrate two main points. First, we show that, given sufficiently small resistivity, the Rutherford regime always exists; larger values of Delta' require smaller values of resistivity. Rutherford's negligible-inertia assumption is validated and the asymptotically linear dependence of the time derivative of the island width on the resistivity and Delta' is confirmed. Second, we find that, at large Delta', the Rutherford regime is followed by a nonlinear stage of fast growth linked to X-point collapse and formation of a current sheet. This causes the reconnection to become Sweet-Parke (SP) like. The signature resistivity^{1/2} scaling of the effective island growth rate is, indeed, found in this nonlinear stage. The SP stage culminates in the saturation of the mode, which can, thus, be achieved much faster than via Rutherford regime., Comment: latex, 4 pages, 8 figures; Paper 4-208, Proceedings of the 31st EPS Conference on Plasma Physics, London 28 June - 2 July 2004

Published
2004
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12. Overview of MAST results

Author

Chapman, I. T., Adamek, J., Akers, R. J., Allan, S., Appel, L., Asunta, O., Barnes, M., Ben Ayed, N., Bigelow, T., Boeglin, W., Bradley, J., Bruenner, J., Cahyna, P., Carr, M., Caughman, J., Cecconello, M., Challis, C., Chapman, S., Chorley, J., Colyer, G., Conway, N., Cooper, W. A., Cox, M., Crocker, N., Crowley, B., Cunningham, G., Danilov, A., Darrow, D., Dendy, R., Diallo, A., Dickinson, D., Diem, S., Dorland, W., Dudson, B., Dunai, D., Easy, L., Elmore, S., Field, A., Fishpool, G., Fox, M., Fredrickson, E., Freethy, S., Garzotti, L., Ghim, Y. C., Gibson, K., Graves, J., Gurl, C., Guttenfelder, W., Ham, C., Harrison, J., Harting, D., Havlickova, E., Hawke, J., Hawkes, N., Hender, T., Henderson, S., Highcock, E., Hillesheim, J., Hnat, B., Holgate, J., Horacek, J., Howard, J., Huang, B., Imada, K., Jones, O., Kaye, S., Keeling, D., Kirk, A., Klimek, I., Kocan, M., Leggate, H., Lilley, M., Lipschultz, B., Lisgo, S., Liu, Y. Q., Lloyd, B., Lomanowski, B., Lupelli, I., Maddison, G., Mailloux, J., Martin, R., Mcardle, G., Mcclements, K., Mcmillan, B., Meakins, A., Meyer, H., Michael, C., Militello, F., Milnes, J., Morris, A. W., Motojima, G., Muir, D., Nardon, E., Naulin, V., Naylor, G., Nielsen, A., O'Brien, M., O'Gorman, T., Ono, Y., Oliver, H., Pamela, S., Pangione, L., Parra, F., Patel, A., Peebles, W., Peng, M., Perez, R., Pinches, S., Piron, L., Podesta, M., Price, M., Reinke, M., Ren, Y., Roach, C., Robinson, J., Romanelli, M., Rozhansky, V., Saarelma, S., Sangaroon, S., Saveliev, A., Scannell, R., Schekochihin, A., Sharapov, S., Sharples, R., Shevchenko, V., Silburn, S., Simpson, J., Storrs, J., Takase, Y., Tanabe, H., Tanaka, H., Taylor, D., Taylor, G., Thomas, D., Thomas-Davies, N., Thornton, A., Turnyanskiy, M., Valovic, M., Vann, R., Walkden, N., Wilson, H., Wyk, L. V., Yamada, T., Zoletnik, S., MAST Team, and MAST Upgrade Team

Subjects
high confinement operation, Physics::Plasma Physics, MAST, numerical modelling, RMPs
Abstract

The Mega Ampere Spherical Tokamak (MAST) programme is strongly focused on addressing key physics issues in preparation for operation of ITER as well as providing solutions for DEMO design choices. In this regard, MAST has provided key results in understanding and optimizing H-mode confinement, operating with smaller edge localized modes (ELMs), predicting and handling plasma exhaust and tailoring auxiliary current drive. In all cases, the high-resolution diagnostic capability on MAST is complemented by sophisticated numerical modelling to facilitate a deeper understanding. Mitigation of ELMs with resonant magnetic perturbations (RMPs) with toroidal mode number n(RMP) = 2, 3, 4, 6 has been demonstrated: at high and low collisionality; for the first ELM following the transition to high confinement operation; during the current ramp-up; and with rotating n(RMP) = 3 RMPs. n(RMP) = 4, 6 fields cause less rotation braking whilst the power to access H-mode is less with n(RMP) = 4 than n(RMP) = 3, 6. Refuelling with gas or pellets gives plasmas with mitigated ELMs and reduced peak heat flux at the same time as achieving good confinement. A synergy exists between pellet fuelling and RMPs, since mitigated ELMs remove fewer particles. Inter-ELM instabilities observed with Doppler backscattering are consistent with gyrokinetic simulations of micro-tearing modes in the pedestal. Meanwhile, ELM precursors have been strikingly observed with beam emission spectroscopy (BES) measurements. A scan in beta at the L-H transition shows that pedestal height scales strongly with core pressure. Gyro-Bohm normalized turbulent ion heat flux (as estimated from the BES data) is observed to decrease with increasing tilt of the turbulent eddies. Fast ion redistribution by energetic particle modes depends on density, and access to a quiescent domain with 'classical' fast ion transport is found above a critical density. Highly efficient electron Bernstein wave current drive (1 A W-1) has been achieved in solenoid-free start-up. A new proton detector has characterized escaping fusion products. Langmuir probes and a high-speed camera suggest filaments play a role in particle transport in the private flux region whilst coherence imaging has measured scrape-off layer (SOL) flows. BOUT++ simulations show that fluxes due to filaments are strongly dependent on resistivity and magnetic geometry of the SOL, with higher radial fluxes at higher resistivity. Finally, MAST Upgrade is due to begin operation in 2016 to support ITER preparation and importantly to operate with a Super-X divertor to test extended leg concepts for particle and power exhaust.

14. Physics of high performance deuterium-tritium plasmas in TFTR

Author

Mcguire, Km, Barnes, Cw, Batha, Sh, Beer, Ma, Bell, Mg, Bell, Re, Belov, A., Berk, Hl, Bernabei, S., Bitter, M., Breizman, Bn, Bretz, Nl, Budny, Rv, Bush, Ce, Callen, Jd, Cauffman, S., Chang, Cs, Chang, Z., Cheng, Cz, Cottrell, Ga, Darrow, Ds, Dendy, Ro, Dorland, W., Duong, H., Efthimion, Pc, Ernst, D., Evenson, H., Fisch, Nj, Fisher, R., Fonck, Rj, Forest, Cb, Fredrickson, Ed, Fu, Gy, Furth, Hp, Goloborod Ko, Vy, Gorelenkov, Nn, Grek, B., Grisham, Lr, Hammett, Gw, Hanson, Gr, Hawryluk, Rj, Heidbrink, Ww, Herrmann, Hw, Herrmann, M., Hill, Kw, Hogan, J., Hooper, B., Hosea, Jc, Houlberg, Wa, Hughes, M., Hulse, Ra, Jassby, Dl, Jobes, Fc, Johnson, Dw, Kaita, R., Kaye, Sm, Kesner, J., Kim, Js, Kissick, M., Krasilnikov, Av, Kugel, Hw, Kumar, A., Lam, Nt, Lamarche, P., Leblanc, B., Levinton, Fm, Ludescher, C., Machuzak, J., Majeski, R., Manickam, J., Mansfield, Dk, Mauel, Me, Mazzucato, E., Mcchesney, J., Mccune, Dc, Mckee, G., Meade, Dm, Medley, Ss, Mika, R., Mikkelsen, Dr, Mirnov, Sv, Mueller, D., Nagayama, Y., Navratil, Ga, Nazikian, R., Okabayashi, M., Owens, Dk, Park, Hk, Park, W., Parks, P., Paul, Sf, Petrov, Mp, Phillips, Ck, Phillips, M., Phillips, P., Ramsey, At, Redi, Mh, Rewoldt, G., Reznik, S., Rogers, Jh, Roquemore, Al, Ruskov, E., Sabbagh, Sa, Sasao, M., Schilling, G., Schivell, J., Schmidt, Gl, Scott, Sd, Semenov, Ib, Senko, T., Sesnic, S., Skinner, Ch, Stevenson, T., Stodiek, W., Strachan, Jd, Strait, Ej, Stratton, Bc, Synakowski, Ej, Takahashi, H., Tang, Wm, Taylor, G., Terry, Jl, Thompson, Me, Goeler, S., Halle, A., Walters, Rt, Wang, S., White, Rb, Wieland, Rm, Williams, M., Wilson, Jr, Wong, Kl, Glen Wurden, Yamada, M., Yavorski, V., Young, Km, Zakharov, Le, Zarnstorff, Mc, Zweben, Sj, and INT ATOMIC ENERGY AGCY

15. ICRF results in D-T plasmas in JET and TFTR and implications for ITER

Author

Adams, JM, Ageladarakis, P, Alper, B, Altmann, H, Amasov, V, Arshad, S, Andrew, P, Andrew, Y, Bailey, D, Bainbridge, N, Balet, B, Baranov, Y, Barker, P, Barnsley, R, Baronian, M, Bartlett, DV, Bell, AC, Bertalot, L, Bertolini, E, Bhatnagar, V, Bickley, AJ, Bindslev, H, Blackler, K, Bond, D, Bonicelli, T, Borba, D, Brandon, M, Breger, P, Brelen, H, Brennan, P, Brewerton, WJ, Browne, ML, Budd, T, Budny, R, Burt, A, Businaro, T, Buzio, M, Caldwell-Nicholls, C, Campling, D, Card, P, Challis, CD, Chankin, AV, Chiron, D, Christiansen, J, Chuilon, P, Ciric, D, Claesen, R, Clarke, HE, Clement, S, Coad, JP, Coffey, I, Conroy, S, Conway, G, Cooper, S, Cordey, JG, Corrigan, G, Cottrell, G, Cox, M, Cox, SJ, Cusack, R, Davies, N, Davies, SJ, Davis, JJ, de Benedetti, M, de Esch, H, de Haas, J, Deksnis, E, Deliyanakis, N, Dines, A, Dmitrenko, SL, Dobbing, J, Dolgetta, N, Dorling, SE, Doyle, PG, Duquenoy, H, Edwards, AM, Edwards, AW, Egedal, J, Ehrenberg, J, Ekedahl, A, Elevant, T, Ellis, J, Endler, M, Erents, SK, Ericsson, G, Esposito, B, Eriksson, LG, Falter, H, Farthing, JW, Fichtmuller, M, Fishpool, G, Fullard, K, Gadeberg, M, Galbiati, L, Gibson, A, Gill, RD, Godden, D, Gondhalekar, A, Goodall, D, Gormezano, C, Gowers, C, Groth, M, Guenther, K, Guo, H, Haigh, A, Haist, B, Hancock, CJ, Harbour, PJ, Hawkes, NC, Hawkes, NP, Hemmerich, JL, Hender, T, Hoekzema, J, Horton, L, Howman, A, Huart, M, Hughes, TP, Hurd, F, Huysmans, G, Ingesson, C, Ingram, B, Irving, M, Jacquinot, J, Jaeckel, H, Jaeger, JF, Jarvis, ON, Johnson, M, Jones, EM, Jones, TTC, Junger, JF, Junique, F, Jupen, C, Kallne, J, Kaye, A, Keen, BE, Keilhacker, M, Kerner, W, Kidd, NG, Knipe, S, Konig, R, Korotkov, A, Krasilnikov, A, Krom, JG, Kupschus, P, Lasser, R, Last, JR, Lauro-Taroni, L, Lawson, K, Lennholm, M, Lingertat, J, Litaudon, X, Loarer, T, Lomas, PJ, Loughlin, M, Lowry, C, Maas, AC, Macklin, B, Maggi, CF, Mantsinen, M, Marchese, V, Marcus, F, Mart, J, Martin, D, Matthews, G, McBryan, H, McCracken, G, McCullen, PA, Meigs, A, Middleton, R, Miele, P, Milani, F, Mills, J, Mohanti, R, Monk, R, Morgan, P, Murphy, G, Nave, F, Newbert, G, Nielsen, P, Noll, P, Obert, W, O'Brien, D, O'Mullane, M, Oord, E, Ostrom, R, Papastergiou, S, Parail, VV, Parkinson, R, Parsons, W, Patel, B, Paynter, A, Perevezentsev, A, Peacock, A, Pearce, RJH, Pick, MA, Plancoulaine, J, Pogutse, O, Prentice, R, Puppin, S, Radford, G, Reichle, R, Riccardo, V, Rimini, F, Rochard, F, Rolfe, A, Roquemore, AL, Ross, RT, Rossi, A, Sadler, G, Saibene, G, Santaguistina, A, Sartori, R, Saunders, R, Schild, P, Schmid, M, Schmidt, V, Schokker, B, Schunke, B, Scott, SM, Sharapov, S, Sibley, A, Simon, M, Simonini, R, Sips, ACC, Smeulders, P, Smith, P, Smith, R, Soldner, F, Spence, J, Springman, E, Stagg, R, Stamp, M, Stangeby, P, Start, DF, Stork, D, Stott, PE, Strachan, JD, Stubberfield, P, Summers, D, Svensson, L, Svensson, P, Tabasso, A, Tabellini, M, Tait, J, Tanga, A, Taroni, A, Terella, C, Thomas, PR, Thomsen, K, Traneus, E, Tubbing, B, Twyman, P, Vadgama, A, van Belle, P, Vlases, GC, von Hellermann, M, Wade, T, Walton, R, Ward, D, Watkins, ML, Watkins, N, Watson, MJ, Wheatley, M, Wilson, D, Winkel, T, Young, D, Young, ID, Yu, Q, Zastrow, KD, Zwingmann, W, McGuire, KM, Barnes, CW, Batha, SH, Beer, MA, Bell, MG, Bell, RE, Belov, A, Berk, HL, Bernabei, S, Bitter, M, Breizman, BN, Bretz, NL, Budny, RV, Bush, CE, Callen, JD, Cauffman, S, Chang, CS, Chang, Z, Cheng, CZ, Cottell, GA, Darrow, DS, Dendy, RO, Dorland, W, Duong, H, Efthimion, PC, Ernst, D, Evenson, H, Fisch, NJ, Fisher, R, Fonck, RJ, Forest, CB, Fredrickson, ED, Fu, GY, Furth, HP, Goloborod'ko, VY, Gorelenkov, NN, Grek, B, Grisham, LR, Hammett, GW, Hanson, GR, Hawryluk, RJ, Heidbrink, WW, Herrmann, HW, Herrmann, M, Hill, KW, Hogan, J, Hooper, B, Hosea, JC, Houlberg, WA, Hughes, M, Hulse, RA, Jassby, DL, Jobes, FC, Johnson, DW, Kaita, R, Kaye, SM, Kesner, J, Kim, JS, Kissick, M, Krasilnikov, AV, Kugel, HW, Kumar, A, Lam, NT, LaMarche, P, LeBlanc, B, Levinton, FM, Ludescher, C, Machuzak, J, Majeski, R, Manickam, J, Mansfield, DK, Mauel, ME, Mazzucato, E, McChesney, J, McCune, DC, McKee, G, Meade, DM, Medley, SS, Mika, R, Mikkelsen, DR, Mirnov, SV, Mueller, D, Nagayama, Y, Navratil, GA, Nazikian, R, Okabayashi, M, Owens, DK, Park, HK, Park, W, Parks, P, Paul, SF, Petrov, MP, Phillips, CK, Phillips, M, Phillips, P, Ramsey, AT, Redi, MH, Rewoldt, G, Reznik, S, Rogers, JH, Ruskov, E, Sabbagh, SA, Sasao, M, Schilling, G, Schivell, J, Schmidt, GL, Scott, SD, Senenov, IB, Senko, T, Sesnic, S, Skinner, CH, Stevenson, T, Stodiek, W, Strait, EJ, Stratton, BC, Synakowski, EJ, Takahashi, H, Tang, WM, Taylor, G, Terry, JL, Thompson, ME, Von Goeler, S, Von Halle, A, Walters, RT, Wang, S, White, RB, Wieland, RM, Williams, M, Wilson, JR, Wong, KL, Wurden, GA, Yamada, M, Yavorski, V, Young, KM, Zakharov, LE, Zarnstorff, MC, Zweben, SJ, Team, JET, and Team, TFTR

16. Review of deuterium-tritium results from the Tokamak Fusion Test Reactor

Author

Mcguire, K. M., Adler, H., Alling, P., Ancher, C., Anderson, H., Anderson, J. L., Anderson, J. W., Arunasalam, V., Ascione, G., Ashcroft, D., Barnes, C. W., Barnes, G., Batha, S., Bateman, G., Beer, M., Bell, M. G., Bell, R., Bitter, M., Blanchard, W., Bretz, N. L., Brunkhorst, C., Budny, R., Bush, C. E., Camp, R., Caorlin, M., Carnevale, H., Cauffman, S., Chang, Z., Chang, C. S., Cheng, C. Z., Chrzanowski, J., Collins, J., Coward, G., Cropper, M., Darrow, D. S., Daugert, R., Delooper, J., Dendy, R., Dorland, W., Dudek, L., Duong, H., Durst, R., Efthimion, P. C., Ernst, D., Evenson, H., Fisch, N. J., Fisher, R., Fonck, R. J., Fredd, E., Fredrickson, E., Fromm, N., Fu, G. Y., Fujita, T., Furth, H. P., Garzotto, V., Gentile, C., Gilbert, J., Gioia, J., Gorelenkov, N., Grek, B., Grisham, L. R., Hammett, G., Hanson, G. R., Hawryluk, R. J., Heidbrink, W., Herrmann, H. W., Hill, K. W., Hosea, J., Hsuan, H., Hughes, M., Hulse, R., Janos, A., Jassby, D. L., Jobes, F. C., Johnson, D. W., Johnson, L. C., Kalish, M., Kamperschroer, J., Kesner, J., Kugel, H., Labik, G., Lam, N. T., Lamarche, P. H., Lawson, E., Leblanc, B., Levine, J., Levinton, F. M., Loesser, D., Long, D., Loughlin, M. J., Machuzak, J., Majeski, R., Mansfield, D. K., Marmar, E. S., Marsala, R., Martin, A., Martin, G., Mazzucato, E., Mauel, M., Mccarthy, M. P., Mcchesney, J., Mccormack, B., Mccune, D. C., Mckee, G., Meade, D. M., Medley, S. S., Mikkelsen, D. R., Mirnov, S. V., Mueller, D., Murakami, M., Murphy, J. A., Nagy, A., Navratil, G. A., Nazikian, R., Newman, R., Norris, M., Oconnor, T., Oldaker, M., Ongena, J., Osakabe, M., Owens, D. K., Park, H., Park, W., Parks, P., Paul, S. F., Pearson, G., Perry, E., Persing, R., Petrov, M., Phillips, C. K., Phillips, M., Pitcher, S., Pysher, R., Qualls, A. L., Raftopoulos, S., Ramakrishnan, S., Ramsey, A., Rasmussen, D. A., Redi, M. H., Renda, G., Rewoldt, G., Roberts, D., Rogers, J., Rossmassler, R., Roquemore, A. L., Ruskov, E., Sabbagh, S. A., Sasao, M., Schilling, G., Schivell, J., Schmidt, G. L., Scillia, R., Scott, S. D., Semenov, I., Senko, T., Sesnic, S., Sissingh, R., Skinner, C. H., Snipes, J., Stencel, J., Stevens, J., Stevenson, T., Stratton, B. C., Strachan, J. D., Stodiek, W., Swanson, J., Synakowski, E., Takahashi, H., Tang, W., Taylor, G., Terry, J., Thompson, M. E., Tighe, W., Timberlake, J. R., Tobita, K., Towner, H. H., Tuszewski, M., Vonhalle, A., Vannoy, C., Viola, M., Vongoeler, S., Voorhees, D., Walters, R. T., Wester, R., White, R., Wieland, R., Wilgen, J. B., William Dorland, Wilson, J. R., Winston, J., Wright, K., Wong, K. L., Woskov, P., Wurden, G. A., Yamada, M., Yoshikawa, S., Young, K. M., Zarnstorff, M. C., Zavereev, V., and Zweben, S. J.

18. Isotope scaling of heating and confinement in multiple regimes of TFTR

Author

Scott, Sd, Hammett, Gw, Phillips, Ck, Synakowski, Ej, Batha, Sh, Beer, Ma, Bell, Mg, Bell, Re, Budny, Rv, Bush, Ce, Dorland, W., Philip Efthimion, Ernst, D., Fredrickson, Ed, Hosea, Jc, Kaye, Sm, Kotschenreuther, M., Levinton, Fm, Liu, Qp, Majeski, R., Mccune, Dc, Mikkelsen, Dr, Park, Hk, Ramsey, At, Rogers, Jh, Sabbagh, Sa, Schilling, G., Skinner, Ch, Taylor, G., Goeler, S., Waltz, Re, Wilson, Jr, and Zarnstorff, Mc

19. Report of the FESAC panel on a burning plasma program strategy to advance fusion energy

Author

Prager, S., Baker, C., Baldwin, D., Berk, H., Betti, R., Callen, J., Chan, V., Coppi, B., Dahlburg, J., Dean, S., Dorland, W., Drake, J., Freidberg, J., Goldston, R., Hawryluk, R., Hazeltine, R., Bickford Hooper, E., Hubbard, A., Jarboe, T., Johnson, J., Lampe, M., Lindl, J., Logan, G., Marmar, E., Michael Mauel, Mccarthy, K., Mccurdy, W., Meade, D., Meier, W., Milora, S., Morales, G., Najmabadi, F., Navratil, G., Nevins, W., Newman, D., Parker, R., Perkins, F., Phillips, C., Porkolab, M., Rosenbluth, M., Sauthoff, N., Schoenberg, K., Sheffield, J., Stambaugh, R., Synakowski, E., Tynan, G., and Uckan, N.

22. Validation of 1-D transport and sawtooth models for ITER

Author

Connor, Jw, Alexander, M., Attenberger, Se, Bateman, G., Boucher, D., Chudnovskij, N., Dnestrovskij, Yn, Dorland, W., Fukuyama, A., Hoang, Gt, Hogeweij, Dmg, Houlberg, Wa, Kaye, Sm, Kinsey, Je, Konings, Ja, Kotschenreuther, M., Kritz, Ah, Leonov, Vm, Marinucci, M., Mikkelsen, Dr, Ongena, J., Polevoj, Ar, Romanelli, F., Schissel, Dp, Shirai, H., Stubberfield, Pm, Takizuka, T., Taroni, A., Turner, Mf, Gregorio Vlad, Waltz, Re, and Weiland, J.

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