ISEE 3 observations of low-energy proton bidirectional events and their relation to isolated interplanetary magnetic structures

Details ISEE 3 observations of low-energy proton bidirectional events and their relation to isolated interplanetary magnetic structures ISEE 3 observations of low-energy proton bidirectional events and their relation to isolated interplanetary magnetic structures

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987jgr....9211009m&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 92, Oct. 1, 1987, p. 11009-11019.

Physics

95

Interplanetary Magnetic Fields, Satellite Observation, Signature Analysis, Solar Protons, Magnetic Signatures, Magnetometers, Solar Corona, Solar Flares, Solar Wind

Scientific paper

The paper represents the results of a comprehensive survey of low-energy proton bidirectional anisotropies and associated transient magnetic structures as observed in the 35-1600 keV energy range on ISEE-3 during the last solar maximum. The majority of observed bidirectional flow (BDF) events (more than 70 percent) are associated with isolated magnetic structures which are postulated to be an interplanetary manifestation of coronal mass ejection (CME) events. The observed BDF events can be qualitatively grouped into five classes depending on the field signature of the related magnetic structure and the association (or lack of association) with an interplanetary shock. Concerning the topology of the CME-related magnetic structures, the observations are interpreted as being consistent with a detached bubble, comprising closed loops or tightly wound helices.

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