• Title of article

    Gnevyshev gap effects in solar energetic particle activity Original Research Article

  • Author/Authors

    G.A. Bazilevskaya، نويسنده , , V.S. Makhmutov، نويسنده , , A.I. Sladkova، نويسنده ,

  • Issue Information
    دوهفته نامه با شماره پیاپی سال 2006
  • Pages
    5
  • From page
    484
  • To page
    488
  • Abstract
    Time dependence of many solar activity factors and related phenomena has a double-peak structure around the maximum phase of the 11-year cycle. A distinctive minimum between peaks was named the Gnevyshev gap. This paper deals with Gnevyshev gap effects in solar energetic particle activity during the last four solar cycles. A hypothesis that the Gnevyshev gap structure is a result of superposition of quasi-biennial and 11-year oscillation is examined. The occurrence rate of solar energetic particle events does not contradict the hypothesis given all the events with the peak proton intensity J(>10 MeV) > 1 cm−2 s−1 sr−1 are considered. However, the most powerful solar energetic particle events (ground level enhancements) demonstrate pronounced peak and valley structure which is sometimes not synchronous with quasi-biennial oscillations in other solar indices.
  • Journal title
    Advances in Space Research
  • Serial Year
    2006
  • Journal title
    Advances in Space Research
  • Record number

    1131001