Abstract
There have been recent suggestions that large fluxes of solar energetic particles may produce their own turbulence. To verify this argument it becomes essential to find out whether these flows cause changes in the interplanetary magnetic field (IMF) fluctuations. In the present work, power and helicity spectra of the IMF before, during and after eight Helios observed solar proton events in the range 0.3–1 AU are analysed. To detect proton self generated waves, the time evolution of spectra is followed.
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