Number of the records: 1  

Predicting minima and maxima of solar cycles based on prominences and emission corona

  1. TitlePredicting minima and maxima of solar cycles based on prominences and emission corona
    Author Minarovjech Milan SAVASTRO - Astronomický ústav SAV
    Co-authors Rušin Vojtech 1942- SAVASTRO - Astronomický ústav SAV    SCOPUS    RID    ORCID

    Saniga Metod 1959- SAVASTRO - Astronomický ústav SAV    SCOPUS    RID    ORCID

    Source document Contributions of the Astronomical Observatory Skalnaté Pleso. Vol. 41, no. 2 (2011), p. 175-182
    Languageeng - English
    CountrySK - Slovak Republic
    Document kindrozpis článkov z periodík (rbx)
    CitationsDUDIK, J. - AULANIER, G. - SCHMIEDER, B. - ZAPIOR, M. - HEINZEL, P. Magnetic topology of bubbles in quiescent prominences. In ASTROPHYSICAL JOURNAL, 2012, vol. 761, no. 1, article no. 9, p. 1-13.
    KONG, D. F. - QU, Z. N. - GUO, Q. L. Revisiting the question: Does high-latitude solar activity lead low-latitude solar activity in time phase? In ASTRONOMICAL JOURNAL, 2014, vol. 147, no. 5, article no. 97, p. 1-7.
    SVOREŇ, J. Distribution of the activity of the Sun during an average solar cycle. In CONTRIBUTIONS OF THE ASTRONOMICAL OBSERVATORY SKALNATE PLESO, 2015, vol. 45, no. 2, p. 131-136.
    CategoryADNA - Scientific papers in domestic impacted journals registered in Web of Sciences or Scopus
    Category of document (from 2022)V3 - Vedecký výstup publikačnej činnosti z časopisu
    Type of documentčlánok
    Year2011
    Registered inWOS
    Registered inSCOPUS
    article

    article

    rokCCIFIF Q (best)JCR Av Jour IF PercSJRSJR Q (best)CiteScore
    N
    rok vydaniarok metrikyIFIF Q (best)SJRSJR Q (best)
    201120100.296Q40.186Q4
Number of the records: 1  

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