Physics
Scientific paper
May 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsh41b..01m&link_type=abstract
American Geophysical Union, Spring Meeting 2008, abstract #SH41B-01
Physics
2102 Corotating Streams, 7511 Coronal Holes, 7514 Energetic Particles (2114), 7536 Solar Activity Cycle (2162)
Scientific paper
Using instruments on the ACE spacecraft, we have surveyed the heavy ion spectra and composition over the range He-Fe for 41 Corotating Interaction Regions (CIRs) during 1998-2007. Below ~1 MeV/nucleon the spectra are power laws in kinetic energy/nucleon with average spectral index 2.51 +/- 0.10, rolling over above ~1 MeV/nucleon to power law spectra with average index 4.47+/- 0.17. The spectral shape for different species are similar, leading to relative abundances that are constant over our energy range even though the intensities cover up to 8 orders of magnitude. Except for an overabundance of 4He and Ne, the abundances relative to Oxygen are quite close to the abundance of the fast solar wind. We have found 3He/4He ratios to be enhanced over solar wind values in ~40% of the CIRs. The Fe/O ratio in individual CIRs is observed to vary over a factor of ~10, and is strongly correlated with the solar wind Fe/O ratio measured 2-4 days preceding each CIR. Taken together with previous studies showing the presence of pick-up He+ in CIRs, the observational data provides evidence that CIR energetic particles are accelerated out of a suprathermal ion pool that includes heated solar wind ions, pick-up ions, and remnant suprathermals from impulsive solar energetic particle events.
Cohen M. C.
Desai Mihir I.
Dwyer Joesph R.
Gold Robert E.
Krimigis Stamatios M.
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