AMPTE/CCE observations of shell-like He(2+) and O(6+) distributions in the magnetosheath

Details AMPTE/CCE observations of shell-like He(2+) and O(6+) distributions in the magnetosheath AMPTE/CCE observations of shell-like He(2+) and O(6+) distributions in the magnetosheath

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988georl..15.1333f&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 15, Nov. 1988, p. 1333-1336.

Computer Science

Sound

28

Helium, Magnetosheath, Oxygen, Plasma Composition, Solar Wind, Ampte (Satellites), Satellite Sounding

Scientific paper

Simultaneous observations of solar wind He(2+) and O(6+) shell-like distributions in the magnetosheath were obtained by the AMPTE CCE on November 1, 1984. It is found that the present distributions are centered on the downstream H(+) bulk velocity and have radii proportional to the mass/charge ratio. The results support an electrostatic cross-shock potential model.

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