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Upstream energetic ions and electrons: Bow shock--associated or magnetospheric origin

Journal Article · · J. Geophys. Res.; (United States)
We have analyzed 35 proton bursts observed with the Max-Planck-Institut/University of Maryland sensor system on ISEE 3 far upstream of the earth's bow shock. These upstream bursts fall into two distinctive groups: the first group is accompanied by energetic electrons (> or approx. =75 kev) and the proton spectrum extends up to energies > or approx. =300 kev and higher and bends over towards lower energies (< or approx. =30 keV). The second group, which is unaccompanied by energetic electron bursts, exhibits spectra which can be represented very well by exponentials in energy with a mean e-folding energy of approx.15 keV. We have supplemented these data with measurements obtained with an identical sensor system on ISEE 1 close to the bow shock or within the geomagnetic tail. Whenever ISEE 1 is upstream of the bow shock and ISEE 3 observes a burst of group 2, ISEE 1 observes diffuse upstream ions. When ISEE 3 observes bursts of group 1, ISEE 1 observes either no bursts, diffuse ions, or highly anisotropic distributions. It is suggested that group 1 is of magnetospheric origin, while group 2 is bow shock--associated.
Research Organization:
Max-Planck-Institut fuer Physik und Astrophysik, Institut fuer extraterrestrische Physik, 8046 Garching, Federal Republic of Germany
OSTI ID:
5958641
Journal Information:
J. Geophys. Res.; (United States), Journal Name: J. Geophys. Res.; (United States) Vol. 86:A11; ISSN JGREA
Country of Publication:
United States
Language:
English