Please use this identifier to cite or link to this item: https://hdl.handle.net/10216/126201
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dc.contributor.otherJozef Varju
dc.contributor.otherRadomír Pánek
dc.contributor.otherCarlos A. Silva
dc.creatorFrancisco Salzedas
dc.creatorSyed I. W. Shah
dc.creatorJosef Havlícek
dc.creatorJuliane Stöckel
dc.creatorP. Hácek
dc.creatorAleš Havránek
dc.date.accessioned2021-02-26T00:11:34Z-
dc.date.available2021-02-26T00:11:34Z-
dc.date.issued2020-02-19
dc.identifier.othersigarra:385946
dc.identifier.urihttps://hdl.handle.net/10216/126201-
dc.description.abstractA systematic study of COMPASS density limit disruptions (DLDs) was carried out to analyze the relation between the precursor magnetic island and its secondary instability (SI). In all of these plasmas, the SI was always found present at the onset of energy confinement erosion. The duration of this erosion was shorter for precursor quasi-locked island than for rotating island, and the larger the island amplitude, the shorter the duration. It was also found, at the onset of the erosion of energy confinement, an inverse relation between the magnetic island amplitude and its rotation frequency, showing that erosion can start at different values of precursor island amplitude, depending on what is its rotation frequency. DLDs occur either with smaller precursor island rotating faster or larger island rotating slower (quasi-locked). (c) 2020 Author(s).
dc.language.isoeng
dc.rightsopenAccess
dc.subjectFísica, Física
dc.subjectPhysics, Physical sciences
dc.titleStudy of secondary instability of precursor magnetic island in COMPASS density limit disruptions
dc.typeArtigo em Revista Científica Internacional
dc.contributor.uportoFaculdade de Engenharia
dc.identifier.doi10.1063/1.5123677
dc.subject.fosCiências exactas e naturais::Física
dc.subject.fosNatural sciences::Physical sciences
Appears in Collections:FEUP - Artigo em Revista Científica Internacional

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