Short-Term Periodicities in Sunspot Activity and Flare Index Data during Solar Cycle 23

Kilic H.

SOLAR PHYSICS, vol.255, no.1, pp.155-162, 2009 (SCI-Expanded) identifier identifier

  • Publication Type: Article / Article
  • Volume: 255 Issue: 1
  • Publication Date: 2009
  • Doi Number: 10.1007/s11207-008-9310-9
  • Journal Name: SOLAR PHYSICS
  • Journal Indexes: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Page Numbers: pp.155-162
  • Keywords: Flares, Short periodicities, Sunspot activity, TIME-SERIES, SOLAR-CYCLE-23, EVOLUTION, PHASE, WIND
  • Akdeniz University Affiliated: No

Abstract

The short-term periodicities in sunspot numbers, sunspot areas, and flare index data are investigated in detail using the Date Compensated Discrete Fourier Transform (DCDFT) for the full disk of the Sun separately over the rising, the maximum, and the declining portions of solar cycle 23 (1996 -aEuro parts per thousand 2006). While sunspot numbers and areas show several significant periodicities in a wide range between 23.1 and 36.4 days, the flare index data do not exhibit any significant periodicity. The earlier conclusion of Pap, Tobiska, and Bouwer (1990, Solar Phys. 129, 165) and Kane (2003, J. Atmos. Solar-Terr. Phys. 65, 1169), that the 27-day periodicity is more pronounced in the declining portion of a solar cycle than in the rising and maximum ones, seems to be true for sunspot numbers and sunspot area data analyzed here during solar cycle 23.