On the Differences in Composition between Solar Energetic Particles and Solar Wind

Details On the Differences in Composition between Solar Energetic Particles and Solar Wind On the Differences in Composition between Solar Energetic Particles and Solar Wind

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ssrv..130..207m&link_type=abstract

Space Science Reviews, Volume 130, Issue 1-4, pp. 207-219

Other

14

Sun: Particle Emission, Sun: Solar Wind, Sun: Coronal Mass Ejections (Cmes), Sun: Abundances, Sun: Flares, Acceleration Of Particles

Scientific paper

Although the average composition of solar energetic particles (SEPs) and the bulk solar wind are similar in a number of ways, there are key differences which imply that solar wind is not the principal seed population for SEPs accelerated by coronal mass ejection (CME) driven shocks. This paper reviews these composition differences and considers the composition of other possible seed populations, including coronal material, impulsive flare material, and interplanetary CME material.

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