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AGU: Geophysical Research Letters

 

Index Terms

  • Interplanetary Physics: Interplanetary shocks
  • Interplanetary Physics: Energetic particles

Abstract

The effect of the shock of 15:43 UT March 23, 1991 on 50 keV to 5 MeV ions at Ulysses

T. P. Armstrong

University of Kansas

T. H. Choo

University of Kansas

E. C. Roelof

Johns Hopkins University/Applied Physics Laboratory

G. M. Simnett

University of Birmingham

E. T. Sarris

Democritos University

The intensities, angular distributions, and energy spectra of 50 keV to 5 MeV ions are examined in the several hour time interval when an interplanetary shock passed the Ulysses spacecraft. The increase in intensity, evolution of pitch angle distribution from upstream flow away from the shock to a post‐shock “pancake” distribution, the earlier arrival of more energetic particles, and the presence of non‐gyrotropic effects at the time of shock passage all can be understood in terms of kinematical behavior of the particles crossing the shock.

Received 31 January 1992; accepted 16 March 1992; .

Citation: Armstrong, T. P., T. H. Choo, E. C. Roelof, G. M. Simnett, and E. T. Sarris (1992), The effect of the shock of 15:43 UT March 23, 1991 on 50 keV to 5 MeV ions at Ulysses, Geophys. Res. Lett., 19(12), 1247–1250.

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