Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3339n&link_type=abstract
Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I
Physics
Scientific paper
Our model shows that in large solar energetic particle (SEP) events, streaming protons amplify interplanetary (IP) Alfv´n waves by orders of magnitude near e the Sun. The wave intensity varies strongly and non-monotonically in wavenumb er, time, and space. It falls steeply with distance and may be difficult to observe at 1 AU. Wave amplification dynamically modifies the rigidity and radial dependence of SEP scattering and throttles SEP transport. It is essential in understanding the time and energy variations of SEP elemental abundances.
Ng Chee K.
Reames Donald. V.
Tylka Allan J.
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