Recurrences of interplanetary interaction regions at southern solar latitudes and approximate harmonics

Details Recurrences of interplanetary interaction regions at southern solar latitudes and approximate harmonics Recurrences of interplanetary interaction regions at southern solar latitudes and approximate harmonics

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..20..103t&link_type=abstract

Advances in Space Research, vol. 20, p. 103

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Interplanetary Magnetic Fields, Solar Protons, Elementary Particle Interactions, Ulysses Mission, Particle Energy, Spectrum Analysis, Helium, Iron, Cyano Compounds

Scientific paper

Spectral analyses have been conducted of the time series of the fluxes of protons, He, CNO, and Fe group ions in each of two energy intervals measured during a series of low energy interplanetary particle enhancements by the HI-SCALE instrument aboard Ulysses during much of 1993. The fundamental rotation rate for the nearest Fe enhancement was about 26.5 days; several other shorter periods were found. In all cases, rotation rates were shorter than those of the IMF and the solar source field at the time.

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