Measurement and modeling of aluminum sputtering and ionization in the DIII-D divertor including magnetic pre-sheath effects. (8th August 2018)

• Record Type: Journal Article
• Authors: Chrobak, C.P.; Stangeby, P.C.; Hollmann, E.; Rudakov, D.L.; Abrams, T.; Ding, R.; Elder, J.D.; Guterl, J.; Hinson, E.; Guo, H.Y.; Thomas, D.M.; Skinner, C.H.; McLean, A.G.; Wampler, W.R.; Buchenauer, D.A.; Doerner, R.P.; Tynan, G.R.
• Is Part Of: Nuclear fusion. Volume 58:Number 10(2018:Oct.)
• Publication Date: 2018-08-08
• Subjects: divertor -- sheath -- low-Z -- erosion -- ionization -- angular distribution -- sputtering; Nuclear fusion -- Periodicals; 621.48405
• DOI: 10.1088/1741-4326/aad4c9
• Languages: English
• ISSNs: 0029-5515

Abstract

Abstract: We present analysis and modeling of Al sputtering and ionization in attached, low-power L-mode plasmas near the outer divertor strike point of the DIII-D tokamak. Al serves as a useful proxy for Be, the low-Z main wall material for ITER and JET that will undergo significant divertor plasma contact upon migrating from the first wall to the divertor. Al is easily distinguishable from background sources in DIII-D (namely C and B), has a high physical sputtering yield similar to Be, and has a long ionization mean free path compared to its gyro radius ( ). Using neutral Al emission imaging techniques, we measured a toroidal and radial asymmetry in the shape of the photo-emission plumes of sputtered neutral Al that was consistent with previously observed asymmetry in the distribution of redeposited Al in these experiments. We propose that the main cause of the emission and redeposition asymmetry is due to a sputtering anisotropy caused by near-grazing angle incident ions. The observed emission asymmetry was reproduced using a simple emission/ionization model that included full angular distributions of sputtering yield and energy calculated by SDTRIM.SP, but not when symmetric, mono-energetic cosine sputtering distributions were assumed. We used an ion orbit tracking model to calculate the distributions of ion impact energies through the potential gradient in the magnetic pre-sheath and Debye sheath. We found that with the magnetic field pitch angle (1.5°–2° with respect to the surface plane), the majority of ions strike the surface at <15° with respect to the surface plane, leading to angular sputtering yield and energy distributions with significant forward-scattering bias. We also observed surface microstructure consistent with directional sputtering and ion flux shadowing expected from the calculated ion incidence angles.