http://www.cnr.it/ontology/cnr/individuo/prodotto/ID253297
Non-axisymmetric perturbation of the plasma surface in RFX: analysis of magnetic data versus CCD images of plasma-wall interaction (Articolo in rivista)
- Type
- Label
- Non-axisymmetric perturbation of the plasma surface in RFX: analysis of magnetic data versus CCD images of plasma-wall interaction (Articolo in rivista) (literal)
- Anno
- 2001-01-01T00:00:00+01:00 (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
- 10.1016/S0022-3115(00)00474-8 (literal)
- Alternative label
P. Zanca; D. Bettella; S. Martini; M. Valisa (2001)
Non-axisymmetric perturbation of the plasma surface in RFX: analysis of magnetic data versus CCD images of plasma-wall interaction
in Journal of nuclear materials; ELSEVIER SCIENCE BV, PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS, AMSTERDAM (Paesi Bassi)
(literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
- P. Zanca; D. Bettella; S. Martini; M. Valisa (literal)
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- E-ISSN: 1873-4820 (literal)
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- http://www.sciencedirect.com/science/article/pii/S0022311500004748# (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
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- ISI Web of Science (WOS) (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
- Consorzio RFX, Associazione ENEA-Euratom sulla Fusione. 35127 Padova (literal)
- Titolo
- Non-axisymmetric perturbation of the plasma surface in RFX: analysis of magnetic data versus CCD images of plasma-wall interaction (literal)
- Abstract
- In the RFX experiment, as in other reversed field pinches, the sustainment of the configuration in standard conditions entails the presence of a relatively wide spectrum of internally resonant tearing modes with saturated amplitude. Such modes cause a non-axisymmetric perturbation of the magnetic configuration. In this paper a detailed comparison of the perturbed magnetic surface with the footprint of enhanced plasma wall interaction evidenced by CCD camera images of the RFX graphite first wall is presented. The comparison confirms the accuracy of the magnetic reconstruction algorithm, which computes peak-to peak perturbation of the plasma surface as large as 5 cm in some cases and a contribution from m=0 modes which can be comparable to that of m=1 modes, particularly at low currents. (literal)
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