Correlation between the He/H ratios in upstream particle events and in the solar wind

The ratio of helium to proton differential intensities at a fixed energy per charge in the diffuse ion population during long-lived upstream particle events is compared with the simultaneously measured solar wind He/H ratio. It is found that the He/H intensity ratio at about 30 keV in upstream events is highly correlated with and on the average directly proportional to the He/H ratio in the solar wind, and larger than the He/H ratio in the solar wind by an average factor of 1.6. It is concluded that the solar wind is the parent population for the diffuse ions. The He abundance in the diffuse component is on average observed to be larger than in the solar wind. The observations are consistent with the predictions of Fermi acceleration models for a seed particle population drawn from the solar wind with little compositional bias and moderately enhanced in He during the acceleration process.