Physics
Scientific paper
Jun 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.confq..98v&link_type=abstract
Uttar Pradesh State Observatory, International Solar Wind 8 Conference, p. 98
Physics
Solar Wind, High Speed, Power Spectra, Time Measurement, Periodic Variations, Coronal Holes, Solar Physics, Time Series Analysis, Astronomical Catalogs, Spectrum Analysis
Scientific paper
We have investigated the rate of occurrence of solar wind phenomena observed between 1972-1984 using power spectrum analysis. The data have been taken from the high speed solar wind (HSSW) streams catalogue published by Mavromichalaki et al. (1988). The power spectrum analysis of HSSW events indicate that HSSW stream events have a periodicity of 9 days. This periodicity of HSSW events is 1/3 of the 27 days period of coronal holes which are the major source of solar wind events. In our opinion the 9 days period may be the energy build up time to produce the HSSW stream events.
Joshi Girish C.
Verma V. K.
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