In:
Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 124, No. 3 ( 2019-03), p. 1568-1581
Abstract:
Numerical experiments suggest that an IMF strength near or below 0.1 nT is consistent with New Horizons data High plasma beta in the wake adequately explains the broad heavy ion tail that was observed The shell distribution of interplanetary pickup ions is important for understanding Pluto's plasma wake
Type of Medium:
Online Resource
ISSN:
2169-9380
,
2169-9402
DOI:
10.1029/2018JA026083
Language:
English
Publisher:
American Geophysical Union (AGU)
Publication Date:
2019
detail.hit.zdb_id:
2033040-6
detail.hit.zdb_id:
161665-1
detail.hit.zdb_id:
3094181-7
SSG:
16,13
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