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Evidence for confinement of low-energy cosmic rays ahead of interplanetary shock waves
Authors:R. A. R. Palmeira  F. R. Allum
Affiliation:(1) The University of Texas at Dallas, Dallas, Tex., U.S.A.;(2) Present address: Instituto de Pesquisas Espaciais, S. Jose dos Campos, Caixa Postal 515 S. Paulo, Brazil
Abstract:Short-lived (sim 15 min), low-energy proton increases associated with the passage of interplanetary shock waves have been previously reported. In the present paper, we have examined in a fine time scale (sim 1 min) the concurrent particle and magnetic field data, taken by detectors on Explorer 34, for four of these events which occurred on 30 May 1967, 5 June 1967, 29 November 1967, and 11 January 1968. Our results further support the view that these impulsive events are due to confinement of the solar cosmic-ray particles in the region just ahead (sim 106 km) of the advancing shock front. Data from the Pioneer 7 spacecraft for a similar event on 30 August 1966, when this spacecraft was 1.9 × 106 km from the Earth, are shown to be consistent with this interpretation.
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