Ion AccelerationE ~ ED

Energies up to ? 1 MeV/nucleon

3He / 4He and[Ne, Mg, Si, Fe] / [C, N, O] enhanced when E / ED ? 0.35 – 0.4

Can have Lyman a red wing enhancement, Ha polarization, but no standard g-ray lines

Holman (1995)

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Responsible NASA Official:  Gordon D. Holman Web Design:  Merrick Berg, Brian Dennis, Gordon Holman, & Gilbert Prevost Heliophysics Science Division NASA/Goddard Space Flight Center Laboratory for Solar Physics/ Code 671 Greenbelt, MD, 20771, USA Gordon.D.Holman@nasa.gov

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