Development of a measuring technique based on JET second D-T campaign (DTE2) experience for assessing fusion power at ITER during D-T operation using the radial gamma-ray spectrometer.


Journal

The Review of scientific instruments
ISSN: 1089-7623
Titre abrégé: Rev Sci Instrum
Pays: United States
ID NLM: 0405571

Informations de publication

Date de publication:
01 Aug 2024
Historique:
received: 06 05 2024
accepted: 13 07 2024
medline: 5 8 2024
pubmed: 5 8 2024
entrez: 5 8 2024
Statut: ppublish

Résumé

The ITER Radial Gamma-Ray Spectrometer (RGRS) consists of three gamma-ray detectors observing the plasma through three collimated, coplanar, radial lines of sight (LoS). The system was initially designed to monitor the runaway electron emission and the alpha-particle density profile [Nocente et al., Nucl. Fusion 57, 076016 (2017)]. This work presents a novel technique for measuring the fusion power during D-T operation using the RGRS. This method is based on the absolute measurement of the 17 MeV fusion gamma-rays and a semi-analytical computation of their transport from the plasma source to the detectors. This approach was initially developed and tested at JET during the second D-T campaign (DTE2) on a single LoS diagnostic [Dal Molin et al., Phys. Rev. Lett. (submitted) (2024); Rebai et al., Phys. Rev. C (submitted) (2024); and Marcer et al., Nucl. Fusion (unpublished) (2024)]. This work exploits the multiple LoS of the RGRS to create a combined virtual diagnostic whose detected fraction of the total plasma emission is less affected by variations in the plasma emission profile, reducing systematic uncertainties on the estimated total emission, compared to the individual detectors.

Identifiants

pubmed: 39101791
pii: 3306482
doi: 10.1063/5.0217677
pii:
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Informations de copyright

© 2024 Author(s). Published under an exclusive license by AIP Publishing.

Auteurs

G Marcer (G)

Department of Physics, University of Milan-Bicocca, Milan, Italy.

F Scioscioli (F)

Department of Physics, University of Milan-Bicocca, Milan, Italy.
Institute for Plasma Science and Technology, CNR, Milan, Italy.

G Croci (G)

Department of Physics, University of Milan-Bicocca, Milan, Italy.

A Dal Molin (A)

Institute for Plasma Science and Technology, CNR, Milan, Italy.

G Gorini (G)

Department of Physics, University of Milan-Bicocca, Milan, Italy.
Institute for Plasma Science and Technology, CNR, Milan, Italy.

A Muraro (A)

Institute for Plasma Science and Technology, CNR, Milan, Italy.

M Nocente (M)

Department of Physics, University of Milan-Bicocca, Milan, Italy.
Institute for Plasma Science and Technology, CNR, Milan, Italy.

E Perelli Cippo (E)

Institute for Plasma Science and Technology, CNR, Milan, Italy.

M Rebai (M)

Institute for Plasma Science and Technology, CNR, Milan, Italy.

D Rigamonti (D)

Institute for Plasma Science and Technology, CNR, Milan, Italy.

B Coriton (B)

Diagnostic Program, ITER Organization, Saint Paul-lez-Durance, France.

A Kovalev (A)

Diagnostic Program, ITER Organization, Saint Paul-lez-Durance, France.

A Polevoi (A)

Diagnostic Program, ITER Organization, Saint Paul-lez-Durance, France.

E Khilkevitch (E)

Independent researcher, St. Petersburg, Russian Federation.

A Shevelev (A)

Independent researcher, St. Petersburg, Russian Federation.

A Bracco (A)

Department of Physics, University of Milan, Milan, Italy.

F Camera (F)

Department of Physics, University of Milan, Milan, Italy.

C Cazzaniga (C)

UKRI-STFC, Rutherford Appleton Laboratory, Didcot, United Kingdom.

M Tardocchi (M)

Institute for Plasma Science and Technology, CNR, Milan, Italy.

Classifications MeSH