Heavy-Element Abundances in Solar Energetic Particle Events

We survey the relative abundances of elements with 1 < Z < 82 in solar energetic particle (SEP) events observed at 2-10 MeV amu super(-1) during nearly 9 years aboard the Wind spacecraft, with special emphasis on enhanced abundances of elements with Z => 34. Abundances of Fe/O again show a bimodal distribution with distinct contributions from impulsive and gradual SEP events, as seen in earlier solar cycles. Periods with greatly enhanced abundances of (50 < Z < 56)/O, just as those with enhanced super(3)He/ super( 4)He, fall prominently in the Fe-rich population of the impulsive SEP events. In a sample of the 39 largest impulsive events, 25 have measurable enhancements in (50 < Z < 56)/O and (76 < Z < 82)/O, relative to coronal values, ranging from [approx]100 to 10,000. By contrast, in a sample of 45 large gradual events the corresponding enhancements vary from [approx]0.2 to 20. However, the magnitude of the heavy- element enhancements in impulsive events is less striking than their strong correlation with the Fe spectral index and flare size, with the largest enhancements occurring in flares with the steepest Fe spectra, the smallest Fe fluence, and the lowest X-ray intensity, as reported here for the first time. Thus, it seems that small events with low energy input can produce only steep spectra of the dominant species but accelerate rare heavy elements with great efficiency, probably by selective absorption of resonant waves in the flare plasma. With increased energy input, enhancements diminish as heavy ions are depleted, and spectra of the dominant species harden.