Periodicities in Solar Coronal Mass Ejections

Details Periodicities in Solar Coronal Mass Ejections Periodicities in Solar Coronal Mass Ejections

2003-07-14

arxiv.org/abs/astro-ph/0307277v1

Mon.Not.Roy.Astron.Soc.345:809,2003

Astronomy and Astrophysics

Astrophysics

Accepted by MNRAS, 6 figures

Scientific paper

10.1046/j.1365-8711.2003.06993.x

Mid-term quasi-periodicities in solar coronal mass ejections (CMEs) during the most recent solar maximum cycle 23 are reported here for the first time using the four-year data (February 5, 1999 to February 10, 2003) of the Large Angle Spectrometric Coronagraph (LASCO) onboard the Solar and Heliospheric Observatory (SOHO). In parallel, mid-term quasi-periodicities in solar X-ray flares (class >M5.0) from the Geosynchronous Operational Environment Satellites (GOES) and in daily averages of Ap index for geomagnetic disturbances from the World Data Center (WDC) at the International Association for Geomagnetism and Aeronomy (IAGA) are also examined for the same four-year time span. Several conceptual aspects of possible equatorially trapped Rossby-type waves at and beneath the solar photosphere are discussed.

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