Number of the records: 1  

Study of secondary instability of precursor magnetic island in COMPASS density limit disruptions

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    SYSNO ASEP0531034
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleStudy of secondary instability of precursor magnetic island in COMPASS density limit disruptions
    Author(s) Salzedas, F. (PT)
    Shah, S. I.W. (PK)
    Havlíček, Josef (UFP-V) RID, ORCID
    Stöckel, Jan (UFP-V) RID
    Háček, Pavel (UFP-V) RID, ORCID
    Varju, Jozef (UFP-V) ORCID
    Havránek, Aleš (UFP-V) ORCID
    Pánek, Radomír (UFP-V) RID
    Silva, C. (PT)
    Number of authors9
    Article number022515
    Source TitlePhysics of Plasmas - ISSN 1070-664X
    Roč. 27, č. 2 (2020)
    Number of pages6 s.
    Languageeng - English
    CountryUS - United States
    KeywordsCOMPASS ; magnetic island
    Subject RIVBL - Plasma and Gas Discharge Physics
    OECD categoryFluids and plasma physics (including surface physics)
    R&D ProjectsLM2015045 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    EF16_019/0000768 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    Method of publishingOpen access
    Institutional supportUFP-V - RVO:61389021
    UT WOS000519635100002
    EID SCOPUS85081113431
    DOI10.1063/1.5123677
    AnnotationA 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).
    WorkplaceInstitute of Plasma Physics
    ContactVladimíra Kebza, kebza@ipp.cas.cz, Tel.: 266 052 975
    Year of Publishing2021
    Electronic addresshttps://aip.scitation.org/doi/10.1063/1.5123677
Number of the records: 1  

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