CHARGE-STATE MEASUREMENTS OF SOLAR ENERGETIC PARTICLES OBSERVED WITH SAMPEX

We have measured the ionization states of major elements accelerated i n two large solar energetic particle events by use of the geomagnetic cutoff technique. The observations were made in 1992 October/November using instrumentation on the SAMPEX satellite, which is in an 82 degre es inclination low Earth orbit. We calibrate the geomagnetic cutoff ri gidity by assuming that protons and He observed on SAMPEX are fully st ripped. The mean charge states of the heavier elements are then determ ined from their measured cutoffs, along with this calibrated scale. Ou r results cover the energy range similar to 0.5-5 MeV nucleon(-1) and are in good agreement with earlier studies by Luhn et al. (1985) near similar to 1 MeV nucleon-l in all cases except for Fe. We find a mean charge state of 11.04 +/- 0.22 for Fe, while the average from Luhn is 14.09 +/- 0.09. The lower ionization state of Fe reported here appears to be consistent with the general range of values recently measured i n solar wind Fe on the Ulysses deep space probe. Although the observat ional picture is still incomplete, overall the present results confirm and extend previous evidence that the solar energetic particles in la rge events are accelerated from the coronal or solar wind material.