The ~150 day quasi-periodicity in interplanetary and solar phenomena during cycle 23

Details The ~150 day quasi-periodicity in interplanetary and solar phenomena during cycle 23 The ~150 day quasi-periodicity in interplanetary and solar phenomena during cycle 23

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005georl..3202104r&link_type=abstract

Geophysical Research Letters, Volume 32, Issue 2, CiteID L02104

Physics

16

Interplanetary Physics: Coronal Mass Ejections (7513), Interplanetary Physics: Ejecta, Driver Gases, And Magnetic Clouds, Interplanetary Physics: Energetic Particles (7514), Interplanetary Physics: Solar Cycle Variations (7536), Interplanetary Physics: Interplanetary Magnetic Fields

Scientific paper

An intermittent quasi-periodicity of ~150 days in various solar and interplanetary phenomena has been reported in earlier solar cycles. We suggest that variations in the occurrence of solar energetic particle events, interplanetary coronal mass ejections, and geomagnetic storm sudden commencements during solar cycle 23 show evidence of this quasi-periodicity, which is also present in the sunspot number, in particular in the northern solar hemisphere. It is not, however, prominent in the interplanetary magnetic field strength.

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