Physics – Plasma Physics
Scientific paper
Jun 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..669..812r&link_type=abstract
PLASMA PHYSICS: 11th International Congress on Plasma Physics: ICPP2002. AIP Conference Proceedings, Volume 669, pp. 812-815 (2
Physics
Plasma Physics
Magnetohydrodynamics And Plasmas, Particle Emission, Solar Wind
Scientific paper
Valuable information on active solar sites can be obtained from particle abundances as measured in situ by satellites. Energization processes in the strongly magnetized and dense solar corona or in the weakly magnetized and dilute interplanetary medium form a convenient prototype of laboratories for stellar and galactic plasma processes. Coronal energization is due to resonant interaction of a subset of coronal elements and isotopes with electromagnetic waves, which are excited during a major reconfiguration of the flaring magnetic field. These resonant processes together with the intense, less frequent gradual acceleration by interplanetary shocks forms a new heliospheric baseline abundances of minority elements during active periods. Similar process may enrich the planetary nebulae with 3He, solving partly the ``astrophysical 3He problem'', with important implications for the stellar and galactic evolution.
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