Physics
Scientific paper
Jun 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.conf...83v&link_type=abstract
Universidad Nacional Autonoma de Mexico, International Solar Wind 8 Conference, p. 83
Physics
Solar Protons, Interplanetary Magnetic Fields, Energetic Particles, Solar Flux, Solar Wind, Plasma Turbulence, Magnetohydrodynamic Waves, Power Spectra, Helios Satellites
Scientific paper
There have been recent suggestions that large fluxes during solar energetic particle events may produce their own turbulence. To verify this argument it becomes essential to find out whether these flows cause an enhancement of interplanetary magnetic field fluctuations. In the present work, power and helicity spectra of the IMF before, during and after 8 Helios-observed solar proton events in the range 0.3 - 1 AU are analyzed. In order to detect proton self generated waves, the time evolution of spectra are followed.
Alexander Paul
Otaola J. A.
Valdezgalicia J. F.
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