PROTO-SPHERA experiment ISTW2015 | Princeton, 3-6 November

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PROTO-SPHERA experiment ISTW2015 | Princeton, 3-6 November
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PROTO-SPHERA experiment ISTW2015 | Princeton, 3-6 November Perspectives of the PROTO-SPHERA experiment P. Micozzi, F. Alladio, A. Lampasi, G. Maffia ISTW2015 | Princeton, 3-6 November

ISTW2015 | Princeton, 3-6 November Spherical Tokamaks allow to obtain: High plasma current Ip with low BT, high β and more compact devices But, for a reactor/CTF extrapolation: • No space for central solenoid (Current Drive requirement more severe) • No neutrons shield for central stack (no superconductor/high dissipation) Intriguing possibility ⇒ substitute central rod with Screw Pinch plasma (ITF → Ie) Potentially two problems solved: • Simply connected configuration (no conductors inside) • Ip driven by Ie (Helicity Injection from SP to ST) Flux Core Spheromak (FCS) Theory: Taylor & Turner, Nucl. Fusion 29, 219 (1989) Experiment: TS-3; N. Amemiya, et al., JPSJ 63, 1552 (1993) 2 ISTW2015 | Princeton, 3-6 November 2

ISTW2015 | Princeton, 3-6 November But Flux Core Spheromaks are: • injected by plasma guns • formed by ~10 kV voltage on electrodes • high pressure prefilled • with ST safety factor q≤1 New configuration proposed (Alladio F. et al. 2006 Nucl. Fusion 46 S613): PROTO-SPHERA “Flux Core Spherical Tokamak” (FCST), rather than FCS Disk-shaped electrode driven Screw Pinch plasma (SP) Prolated low aspect ratio ST (A=R/a≥1.2, κ=b/a~2.3) to get a Tokamak-like safety factor (q0≥1, qedge~3) SP electrode current Ie=60 kA ST toroidal current Ip=120÷240 kA ST diameter Rsph=0.7 m ⇓ Stability should be improved and helicity drive may be less disruptive than in conventional Flux-Core-Spheromak ISTW2015 | Princeton, 3-6 November 3

ISTW2015 | Princeton, 3-6 November PROTO-SPHERA formation follows TS-3 scheme (SP kink instability) Tunnelling (ST formation) ST compression (Ip/Ie↑, A ↓ ) T0 Ie=8.5 kA T3 Ip=30 kA A=1.8 T4 Ip=60 kA A=1.5 T5 Ip=120 kA A=1.3 T6 Ip=180 kA A=1.25 TF Ip=240 kA A=1.2 Ie 8.5→60 kA Formation time scale: Alfvén MHD growth time τ A~ 0.5 ms Resistive diffusion time τ R~ 70 ms (τR τ A)1/2~ 1 ms for IST=120 kA (2xIe) Courtesy by Farengo (ISTW2008 - Frascati) Smoke-ring-like formation ISTW2015 | Princeton, 3-6 November 4

Key points of proto-sphera design • Stable Screw Pinch formed at Tokamak pressures (10-3÷10-2 mbar) and with low voltage break-down (100-200 V) • Ip/Ie ratio relevant parameter (strong energy dissipation in SP) • MHD equilibria computed both with monotonic as well as reversal safety factor profiles ⇓ magnetic configutation is quite robust Some level of low n resistive instability needed (reconnections to inject helicity from SP to ST) but SP+ST must be ideally stable at any time slice ⇓ Ideal MHD analisys to assess Ip/Ie & β limits (Micozzi P. et al., 2010 Nucl. Fusion 50 095004) • Stable at β 21÷26% for Ip/Ie=0.5, down to 14÷16% for Ip/Ie=4 Comparing with the conventional Spherical Tokamak with central rod: βT0=28÷29% for Ip/Ie=0.5 to βT0=72÷84% for Ip/Ie=4 • Spherical Torus elongation κ plays a key role in increasing Ip/Ie • Comparison with TS-3 experimental results: disk-shaped SP plasma important for the configuration stability ISTW2015 | Princeton, 3-6 November 5

ISTW2015 | Princeton, 3-6 November Critical points of PROTO-SPHERA Helicity injection to sustain the plasma torus: driven relaxation of Plasma Central Column forms & sustains the ST Anode • IST= 240 kA (4xIe) really achievable? • Can it be sustained by H.I. for at least τR~ 70 ms? • Resistive MHD stability & confinement? “Smoke-ring like self-organization” Beluga… Cathode Volcano… Crab Nebula: magnetized configuration produced by Supernova explosion ISTW2015 | Princeton, 3-6 November 6

ISTW2015 | Princeton, 3-6 November Proto-Sphera Phase1 (Multi-Pinch) Aims: 1) Breakdown 2) Stable formation of plasma ‘mushrooms’ 3) Stable (≈1 s) achievement of Ie = 8.5 kA Proto-Sphera (All parts will be reused) By adding: 5 pair of new PF coils New power supplies Full amount of Tungsten wires (324 Vs 54) on the direcltly heated cathode now only partially filled ISTW2015 | Princeton, 3-6 November 7

ISTW2015 | Princeton, 3-6 November Assembly of the anular anode on the machine (May 2015) Cathode feeder bars and return plasma current rods ISTW2015 | Princeton, 3-6 November 8

ISTW2015 | Princeton, 3-6 November Proto-Sphera Phase1 preliminary results (Much more details on F. Alladio presentation) Anodic plasma  Ie≈ 3 kA for about 300 ms  More than 500 shots without any damage on cathode W filaments But there is a problem… wrong path on the external part of vacuum vessel Plasma Central column Cathodic plasma ISTW2015 | Princeton, 3-6 November 9

ISTW2015 | Princeton, 3-6 November Proto-Sphera Phase1 preliminary results (See F. Alladio presentation) Anode (no plasma filaments) The major risk… Anodic anchoring of arc discharges On the contrary in PROTO-SPHERA… due to favourable E x B effect… Cathodic plasma filaments disappear going towards anode Cathode (18 plasma filaments from emitters) ISTW2015 | Princeton, 3-6 November 10

ISTW2015 | Princeton, 3-6 November PROTO-SPHERA Poloidal Field coils Group A: ST compression coils (connected in series) Not installed on Multi-Pinch Characteristics:  High voltage (∼20 kV) insulation Thin Inconel casings to allow for fast B diffusion Cost ≈ 0.5M$ Group B: SP shaping coils (connected in series) Already installed on Multi-Pinch Three new Power Supplies: “Group A” (no on Multi-Pinch) “Cathode” (reduced on Multi-Pinch) implementation cost ≈ 0.2M$ “Screw Pinch” (reduced on Multi-Pinch) ISTW2015 | Princeton, 3-6 November 11

ISTW2015 | Princeton, 3-6 November Proto-Sphera power supplies: SuperCapacitors will be used Screw Pinch PF coils ‘A’ 60 kA 200 μs Ie 1200 A 10 ms qPinch=0.45 SC based P.S. 40 kA 800 A qPinch=0.98 Same simulation results with very different arc V/I characteristics Lcoils = 14.2 mH Rcoils = 70 mΩ 400 A 20 kA qPinch=2.08 Existing P.S. 0 kA Maxwel Technologies SC (C=63 F , V=125 V) Advantages:  No connection to 20 kV substation and no the step-down transformers  Standard SCR Controller (no thyristor bridges)  Very reduced cost! For the “PF coils A” P.S. a small conventional capacitor bank (Ducati) must be added Multi-Pinch Multi-Pinch Reference: G. Maffia et al., EEEIC 2015, Rome ISTW2015 | Princeton, 3-6 November Cost ≈ 0.6M$ Cost: less than 0.1M$ 12

ISTW2015 | Princeton, 3-6 November Conclusions Proto-Sphera Phase1 already solved the major concern: no anode arc anchoring! The progress in SuperCondenser solves the major “technological” concern If Central plasma column & Spherical Torus formation are successful Proto-Sphera will allow to assess if magnetic configurations • simply connected (construction advantages!) • with high plasma beta (minimal geometrical size) • sustained by helicity injection can have further developments… Proto-Sphera can develop this program: at very modest costs (≈1.5M$); in a flexible way (easy to add-up new machine components) ISTW2015 | Princeton, 3-6 November 13

ISTW2015 | Princeton, 3-6 November Further developments… "Open" structure of the magnetic field & simply connected configurations: Magnetic well inside the plasma at β≈1 Confinement system with two "ends" : easy refueling/exhausting of plasma Emerging field lines ease the control of the electric potential within the plasma Recover from disruptions (plasma rebuilds from the open ends if there are electrodes) A simply connected configuration is also more suitable for channeling particle jets and transforming fusion power into propulsive power (for space thrusters) From University of Washington Star Thrust Experiment (STX) ISTW2015 | Princeton, 3-6 November 14

ISTW2015 | Princeton, 3-6 November Further developments… CKF configuration is a possible evolution of the Proto-Sphera concept It has found to be ideally MHD stable up to β=1 (same code of Proto-Sphera) …promising for space thrusters But how to drive the ST current? In a D-He3 reactor the fast particle losses could produce the “right” current on the surrounding discharge… This mechanism could also help in producing the SP current (Ie) in a D-T reactor based upon the “standard” Proto-Sphera configuration (β≈0.2): SP dissipation is a crucial point… ISTW2015 | Princeton, 3-6 November 15

ISTW2015 | Princeton, 3-6 November Further developments… Proto-Sphera load assembly could in principle accommodate a CKF, with some changes, in order to investigate formation, stability and β level before the resistive decay A pair of new coils, same electrodes: smaller but hotter? Same coils, new electrodes: bigger but colder? ISTW2015 | Princeton, 3-6 November 16