HR: 13:55h
AN: SH23A-02    [Abstracts]
TI: What did we Learn About CMEs From the ISEE-3 Mission (of Relevance to the Stereo Mission)
AU: * Sanderson, T R
EM: trevor.sanderson@esa.int
AF: RSSD of ESA, Estec, Noordwijk, 2200AG Netherlands
AB: ISEE-3 was launched in 1978 into a halo orbit around the L1 point. It was subsequently renamed ICE and sent on a journey around the Sun ahead of the earth in an orbit similar to that which one of the Stereo spacecraft will follow. ISEE-3 contained a comprehensive particles and fields instrumentation package, in many ways resembling the particles and fields packages of the Stereo mission. In this paper we discuss some results from the particle experiments which may have relevance to the upcoming Stereo mission. We will show observations of such aspects as particle time-intensity profiles, spectra, and anisotropies. We will discuss the relation with shock characteristics and also wave-particle interactions for the different type of particle events observed. We discuss the implications for the forthcoming Stereo mission.
DE: 7509 Corona
DE: 7513 Coronal mass ejections
DE: 7549 Ultraviolet emissions
DE: 2100 INTERPLANETARY PHYSICS
DE: 2194 Instruments and techniques
SC: SPA-Solar and Heliospheric Physics [SH]
MN: 2004 AGU Fall Meeting