1 V.A. Soukhanovskii/IAEA-FEC/Oct. 2014 Developing Physics Basis for the Radiative Snowflake Divertor at DIII-D by V.A. Soukhanovskii 1, with S.L. Allen.

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Presentation transcript:

1 V.A. Soukhanovskii/IAEA-FEC/Oct Developing Physics Basis for the Radiative Snowflake Divertor at DIII-D by V.A. Soukhanovskii 1, with S.L. Allen 1, M.E. Fenstermacher 1, C.J. Lasnier1, M.A. Makowski 1, A.G. McLean 1, W.H. Meyer 1, D.D. Ryutov 1, E. Kolemen 2, R.J. Groebner 3, A.W. Hyatt 3, A.W. Leonard 3, T.H. Osborne 3, T.W. Petrie 3, J. Watkins 4, 1 Lawrence Livermore National Laboratory 2 Princeton University 3 General Atomics, 4 Sandia National Laboratory Presented at the 25 th IAEA Fusion Energy Conference Saint Petersburg, Russia October 13–18, 2014

2 V.A. Soukhanovskii/IAEA-FEC/Oct Snowflake Divertor Configuration is Studied in DIII-D as a Tokamak Divertor Power Exhaust Concept Divertor power exhaust challenge – Steady-state heat flux Technological limit q peak ≤ 5-15 MW/m 2 DEMO: Unmitigated, q peak ≤ 150 MW/m 2 – ELM energy, target peak temperature Melting limit MJ/m 2 DEMO: Unmitigated, ≥ 10 MJ/m 2 Snowflake divertor with 2nd-order null – ∇ B p ~ 0 Large region of low B p – Very large A wet possibility Experiments in TCV, NSTX, EAST, DIII-D D. D. Ryutov, PoP 14, ; PPCF 54, (2012)

3 V.A. Soukhanovskii/IAEA-FEC/Oct Large Region of Low B p Around Second-order Null in Snowflake Divertor is Predicted to Modify Power Exhaust Geometry properties Criterion: d XX ≤ a ( q /a) 1/3 – Higher edge magnetic shear – Larger plasma wetted-area A wet (f exp ) – Larger parallel connection length L || – Larger effective divertor volume V div Transport properties Criterion: d XX ≤ D*~a (a  pm / R) 1/3 – High convection zone with radius D* – Power sharing over four strike points – Enhanced radial transport (larger q ) “Laboratory for divertor physics” d SF ≤ a ( q /a) 1/3 d SF ≤D* Snowflake Standard Low B p contour: 0.1 B p /B p mid

4 V.A. Soukhanovskii/IAEA-FEC/Oct Outline of talk Comparisons between snowflake and standard divertor encouraging – Compatibility with good core and pedestal performance – Confirmed geometry properties A wet and L II – Initial confirmation of transport properties Radiative Snowflake Divertor Experiments in DIII-D Suggest Strong Effects on Power Exhaust Standard Snowflake Broader divertor radiation distribution Reduced inter-ELM peak heat flux q peak Reduced ELM energy, T peak and q peak Control of steady-state snowflake configurations in DIII-D with existing coils E. Kolemen et.al., next talk

5 V.A. Soukhanovskii/IAEA-FEC/Oct Increased Plasma-wetted Area Leads to q peak Reduction In Snowflake Divertor Snowflake with d XX < 10 cm Core plasma unaffected – 5 MW NBI H-mode – Stored energy and density constant Divertor power balance unaffected In outer divertor, q peak reduced by 30% Standard Snowflake

6 V.A. Soukhanovskii/IAEA-FEC/Oct q peak Reduction in Snowflake Divertor Partly Due to Increased A wet and L || Flux expansion increased ~20% – Depends on configuration, can be up to X3 L || increased by 20-60% over SOL width Divertor heat flux reduced ~30% Parallel heat flux reduced ~20% SOL width Standard Snowflake Strike point

7 V.A. Soukhanovskii/IAEA-FEC/Oct Convective Plasma Mixing Driven by Null-region Instabilities May Modify Particle and Heat Transport Flute-like, ballooning and electrostatic modes are predicted in the low B p region –  p =P k /P m = 8  P k /B p 2 >> 1 –Loss of poloidal equilibrium –Fast convective plasma redistribution –Especially efficient during ELMs when P k is large Estimated size of convective zone –Standard: 1cm –Snowflake: 6-8 cm D. D. Ryutov, IAEA 2012; Phys. Scripta 89 (2014) Divertor null-region  p measured by divertor Thomson Scattering – In snowflake, broad region of higher  p >>1 – Higher X10 during ELMs q

8 V.A. Soukhanovskii/IAEA-FEC/Oct Heat and Particle Fluxes Shared Among Strike Points in Snowflake Divertor q SP3 / q SP1 < 0.5 P SP3 / P SP1 < 0.3 Sharing fraction maximized at low d XX  SP3 q SP3 q SP1 Standard Snowflake

9 V.A. Soukhanovskii/IAEA-FEC/Oct Fit q || profile with Gaussian (S) and Exp. ( SOL ) functions (Eich PRL 107 (2011) ) Increased q may imply increased transport – Increased radial spreading due to L || – SOL transport affected by null-region mixing – Enhanced dissipation may also play role Broader q || Profiles in Snowflake Divertor May Imply Increased Radial Transport q = 2.40 mm q = 3.20 mm Standard Snowflake

10 V.A. Soukhanovskii/IAEA-FEC/Oct Divertor Radiation More Broadly Distributed in Snowflake for Radiative Divertor, q peak Reduced by x5 Standard Snowflake Detached radiative divertor produced by D 2 injection with intrinsic carbon radiation In radiative snowflake nearly complete power detachment at P SOL ~3 MW P SOL = 3-4 MW

11 V.A. Soukhanovskii/IAEA-FEC/Oct SF Divertor Weakly Affects Pedestal Magnetic and Kinetic Characteristics, Peeling-balooning Stability in DIII-D At lower n e, H-mode performance unchanged with snowflake divertor – Similar P ped, W ped – H98(y,2) ~ ,  N ~2 – Plasma profiles only weakly affected Peeling-ballooning stability unaffected – Shear 95, q 95 increased by up to 30% – Medium-size type I ELMs – ELM frequency weakly reduced – ELM size weakly reduced Standard Snowflake

12 V.A. Soukhanovskii/IAEA-FEC/Oct ELM Power Loss Scales with Collisionality, Reduced in H-modes with Snowflake Divertor Increased collisionality with snowflake * ped =  Rq 95 / ee Both  W ELM and  W ELM /W ped weakly reduced Mostly for  W ELM /W ped < 0.10 Standard Snowflake Small ELMs removed for clarity Standard Snowflake

13 V.A. Soukhanovskii/IAEA-FEC/Oct Peak ELM Target Temperature and ELM Heat Flux Reduced in Snowflake Divertor Snowfl ake Type I ELM power deposition correlates with  ELM In radiative snowflake, ELM peak heat flux reduced by % Similar effect in NSTX In snowflake divertor –  T surf ~E ELM /(A wet  ELM ) 1/2 – Increased  ELM =L II /c s,ped – Weakly reduced E ELM – A wet ELM similar S. L. Allen et. al., IAEA 2012 Standard Snowflake

14 V.A. Soukhanovskii/IAEA-FEC/Oct SF divertor configurations compatible with high H-mode confinement and high pressure pedestal Snowflake geometry may offer multiple benefits for inter-ELM and ELM heat flux mitigation – Geometry enables divertor inter-ELM heat flux spreading over larger plasma-wetted area, multiple strike points – Broader parallel heat fluxes may imply increased radial transport – ELM divertor peak target temperature and heat flux reduction, especially in radiative snowflake configurations Developing the Snowflake Divertor Physics Basis For High-power Density Tokamaks