OBSERVATION OF HIGH IRON CHARGE STATES AT LOW ENERGIES IN SOLAR ENERGETIC PARTICLE EVENTS

The ionic charge states of solar energetic particles (SEPs) provide direct information about the source plasma, the acceleration environment, and their transport. Recent studies report that both gradual and impulsive SEP events show mean iron charge states < Q(Fe)> similar to 10-14 at low energies E <= 0.1 MeV nuc (1), consistent with their origin from typical corona material at temperatures 1-2 MK. Observed increases of < Q(Fe)> up to 20 at energies 0.1-0.5 MeV nuc(-1) in impulsive SEPs are attributed to stripping during acceleration. However, Q(Fe) > 16 is occasionally found in the solar wind, particularly coming from active regions, in contrast to the exclusively reported < Q(Fe)> <= 14 for low energy SEPs. Here we report results from a survey of all 89 SEP events observed with Advanced Composition Explorer Solar Energetic Particle Ionic Charge Analyzer (SEPICA) in 1998-2000 for iron charge states augmented at low energy with Solar and Heliospheric Observatory CELIAS suprathermal time-of-flight (STOF). Nine SEP events with < Q(Fe)> >= 14 throughout the entire SEPICA and STOF energy range have been identified. Four of the nine events are impulsive events identified through velocity dispersion that are consistent with source temperatures >= 2 MK up to similar to 4 MK. The other five events show evidence of interplanetary acceleration. Four of them involve re-acceleration of impulsive material, whose original energy dependent charge states appear re-distributed to varying extent bringing higher charge states to lower energy. One event, which shows flat but elevated < Q(Fe)> similar to 14.2 over the entire energy range, can be associated with interplanetary acceleration of high temperature material. This event may exemplify a rare situation when a second shock plows through high temperature coronal mass ejection material.