Cometary H2+ and solar wind He2+ dynamics across the Halley cometopause
- 1 June 1988
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 15 (6) , 549-552
- https://doi.org/10.1029/gl015i006p00549
Abstract
Two Mass/Charge (M/Q) ≈ 2 distributions were observed by the Giotto Ion Mass Spectrometer/High Energy Range Spectrometer (IMS/HERS) during the encounter with comet Halley. The first, present throughout the encounter, is identified as solar wind He2+. The second, detectable only within ∼6 × 105 km of the nucleus, is identified as H2+ (produced primarily by dissociation and ionization of cometary H2O). When these two distributions are separated, distinct differences in their dynamics are apparent, particularly in the density and velocity profiles near the “cometopause”.This publication has 5 references indexed in Scilit:
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