Turbulent drifts of impurity ions as an explanation for anomalous radial transport in the far-SOL of DIII-D

Successful fusion reactor operation relies on minimal core contamination by impurities, otherwise too much power may be radiated and harm performance. This requires reliable predictions of impurity transport from the scrape-off layer (SOL) into the core, beyond the traditional ‘anomalous’ diffusion...

Full description

Saved in:
Bibliographic Details
Main Authors: S.A. Zamperini, T.N. Bernard, D.L Rudakov, J.A Boedo
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:Nuclear Fusion
Subjects:
Online Access:https://doi.org/10.1088/1741-4326/ad4c78
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1841525390999289856
author S.A. Zamperini
T.N. Bernard
D.L Rudakov
J.A Boedo
author_facet S.A. Zamperini
T.N. Bernard
D.L Rudakov
J.A Boedo
author_sort S.A. Zamperini
collection DOAJ
description Successful fusion reactor operation relies on minimal core contamination by impurities, otherwise too much power may be radiated and harm performance. This requires reliable predictions of impurity transport from the scrape-off layer (SOL) into the core, beyond the traditional ‘anomalous’ diffusion approach. We report a set of far-SOL tungsten transport simulations that demonstrate the role of turbulent drifts on radial impurity transport. A turbulent plasma background is simulated using the gyrokinetic SOL code Gkeyll. Tungsten ions are followed within the plasma background using only their drifts. We find that tungsten tends to travel radially outwards with velocities between v _r = 300–1200 m s ^−1 primarily due to polarization drift. We also extract an anomalous radial diffusion coefficient that varies from $D_{\text{r}}^{{\text{anom}}}$ = 5–20 m ^2 s ^−1 . These results are compared to and agree with previous interpretive modeling results. We also show how the turbulent polarization drift can transport some tungsten ions from the wall inwards with effective pinch velocities up to 10 000 m s ^−1 . We conclude that turbulent drifts are a likely explanation for historically anomalous radial impurity transport.
format Article
id doaj-art-905b46080537431eb173928299943c0f
institution Kabale University
issn 0029-5515
language English
publishDate 2024-01-01
publisher IOP Publishing
record_format Article
series Nuclear Fusion
spelling doaj-art-905b46080537431eb173928299943c0f2025-01-17T12:52:39ZengIOP PublishingNuclear Fusion0029-55152024-01-0164707400210.1088/1741-4326/ad4c78Turbulent drifts of impurity ions as an explanation for anomalous radial transport in the far-SOL of DIII-DS.A. Zamperini0https://orcid.org/0000-0001-6896-6686T.N. Bernard1https://orcid.org/0000-0002-7331-9704D.L Rudakov2https://orcid.org/0000-0002-5266-4269J.A Boedo3https://orcid.org/0000-0003-2230-4112General Atomics , San Diego, CA, United States of AmericaGeneral Atomics , San Diego, CA, United States of AmericaUniversity of California , San Diego, CA, United States of AmericaUniversity of California , San Diego, CA, United States of AmericaSuccessful fusion reactor operation relies on minimal core contamination by impurities, otherwise too much power may be radiated and harm performance. This requires reliable predictions of impurity transport from the scrape-off layer (SOL) into the core, beyond the traditional ‘anomalous’ diffusion approach. We report a set of far-SOL tungsten transport simulations that demonstrate the role of turbulent drifts on radial impurity transport. A turbulent plasma background is simulated using the gyrokinetic SOL code Gkeyll. Tungsten ions are followed within the plasma background using only their drifts. We find that tungsten tends to travel radially outwards with velocities between v _r = 300–1200 m s ^−1 primarily due to polarization drift. We also extract an anomalous radial diffusion coefficient that varies from $D_{\text{r}}^{{\text{anom}}}$ = 5–20 m ^2 s ^−1 . These results are compared to and agree with previous interpretive modeling results. We also show how the turbulent polarization drift can transport some tungsten ions from the wall inwards with effective pinch velocities up to 10 000 m s ^−1 . We conclude that turbulent drifts are a likely explanation for historically anomalous radial impurity transport.https://doi.org/10.1088/1741-4326/ad4c78impurity transportSOLDIII-Dturbulence
spellingShingle S.A. Zamperini
T.N. Bernard
D.L Rudakov
J.A Boedo
Turbulent drifts of impurity ions as an explanation for anomalous radial transport in the far-SOL of DIII-D
Nuclear Fusion
impurity transport
SOL
DIII-D
turbulence
title Turbulent drifts of impurity ions as an explanation for anomalous radial transport in the far-SOL of DIII-D
title_full Turbulent drifts of impurity ions as an explanation for anomalous radial transport in the far-SOL of DIII-D
title_fullStr Turbulent drifts of impurity ions as an explanation for anomalous radial transport in the far-SOL of DIII-D
title_full_unstemmed Turbulent drifts of impurity ions as an explanation for anomalous radial transport in the far-SOL of DIII-D
title_short Turbulent drifts of impurity ions as an explanation for anomalous radial transport in the far-SOL of DIII-D
title_sort turbulent drifts of impurity ions as an explanation for anomalous radial transport in the far sol of diii d
topic impurity transport
SOL
DIII-D
turbulence
url https://doi.org/10.1088/1741-4326/ad4c78
work_keys_str_mv AT sazamperini turbulentdriftsofimpurityionsasanexplanationforanomalousradialtransportinthefarsolofdiiid
AT tnbernard turbulentdriftsofimpurityionsasanexplanationforanomalousradialtransportinthefarsolofdiiid
AT dlrudakov turbulentdriftsofimpurityionsasanexplanationforanomalousradialtransportinthefarsolofdiiid
AT jaboedo turbulentdriftsofimpurityionsasanexplanationforanomalousradialtransportinthefarsolofdiiid