Physics
Scientific paper
Aug 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...3e...6m&link_type=abstract
Solar Active Regions and 3D Magnetic Structure, 26th meeting of the IAU, Joint Discussion 3, 16-17 August, 2006, Prague, Czech R
Physics
Scientific paper
The modulation effects of the solar ejecta over the solar energetic particle evens (0.5-100 MeV) have recently been highlighted. Especially important is the behaviour of these fluxes inside MCs where, in spite of the low magnetic field intensities of these interplanetary structures (about 30 nT), a decrease in the population of the energetic particles is observed. The experimental data from ACE, SAMPEX, SOHO, Ulysses and WIND satellites are presented, both from MC coincident with Solar particles evens (left figure) and not coincident (right figure). A simple model is proposed to explain this phenomenon. This work is performed inside COST Action 724.
Hidalgo M. A.
Medina Julieta
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