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AGU: Geophysical Research Letters

 

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  • Planetology: Comets and Small Bodies: Interactions with solar wind plasma and fields

Abstract

GEOPHYSICAL RESEARCH LETTERS, VOL. 13, NO. 8, PP. 853-856, 1986
doi:10.1029/GL013i008p00853

Energetic ion properties observed near the periphery of the mass‐loaded flow region surrounding comet P/Giacobini‐Zinner

C. Tranquille

Space Science Department of ESA, ESTEC, Noordwijk, NL

I. G. Richardson

Blackett Laboratory, Imperial College, London, UK

S. W. H. Cowley

Blackett Laboratory, Imperial College, London, UK

T. R. Sanderson

Space Science Department of ESA, ESTEC, Noordwijk, NL

K.‐P. Wenzel

Space Science Department of ESA, ESTEC, Noordwijk, NL

R. J. Hynds

Blackett Laboratory, Imperial College, London, UK

Measurements made by the Energetic Particle Anisotropy Spectrometer (EPAS) on the International Cometary Explorer (ICE) spacecraft show that relatively abrupt changes occur in energetic heavy ion properties near the periphery of the mass‐loaded flow region surrounding comet P/Giacobini‐Zinner. Corresponding features are observed both inbound and outbound from the comet. As the distance to the comet decreases, a change in the ion distribution takes place over approximately 5 minutes, indicative of flow deflection away from the comet‐sun axis. Shortly afterwards, the ion angular distribution broadens over a further 6 minutes, indicative of a slowing of the ion bulk flow by about 100 km s−1. Taken together with magnetic field and plasma data, these observations are suggestive of a shock wave standing in the flow.

Received 9 April 1986; accepted 11 July 1986; .

Citation: Tranquille, C., I. G. Richardson, S. W. H. Cowley, T. R. Sanderson, K.‐P. Wenzel, and R. J. Hynds (1986), Energetic ion properties observed near the periphery of the mass‐loaded flow region surrounding comet P/Giacobini‐Zinner, Geophys. Res. Lett., 13(8), 853–856, doi:10.1029/GL013i008p00853.

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