EXCESS HEATING OF HE-4(2+) AND O6+ RELATIVE TO H+ DOWNSTREAM OF INTERPLANETARY SHOCKS

Using observations made by the solar wind ion composition spectrometer on sses during its trip in the ecliptic plane to Jupiter, we examined the temperature ratios T(He-4(2+)/T(H+) and T(O6(+))/T(H+) across 15 shocks, including forward and reverse shock pairs as well as isolated shocks. The mean value over the whole set of downstream data studied w as 7+/-3 for the T(He-4(2+))T/(H+). Appreciable differentiated heating downstream of a shock occurred for an upstream ratio T(He-4(2+))/T(H)<4.5. Downstream in the shock regions, characterized by a quasisteady plasma flux, values of T(He-4(2+)/T(H+) and T(O6(+))/T(H+) are observ ed in the range 4.6 to 10.8 and 19 to 48, respectively. Downstream of the shock, extra-heated ions heavier than H+ added a mean 13+/-6% to t he ions' plasma pressure. (This is in addition to the pressure calcula ted using the common assumption of a temperature scaling with the ion masses in heliospheric collisionless plasma.) The extra heating of He- 4(2+) relative to H+ was larger for a smaller plasma beta, agreeing wi th the prediction of the magnetohydrodynamic calculations by Zhao et a l. [1991], although they appeared to underestimate the amount of added heating by a factor of 1.25 to 2.