Energetic Water Group Ion Fluxes (E H 2O >60 KEV) in a Quasiperpendicular and a Quasiparallel Shock Front as Observed Durlng the Giotto-Halley Encounter.-Reference-Cited by-同舟云学术

Energetic Water Group Ion Fluxes (E H 2O >60 KEV) in a Quasiperpendicular and a Quasiparallel Shock Front as Observed Durlng the Giotto-Halley Encounter.

Published:2013-03-26 Issue: Volume: Page:357-364
ISSN:2328-8779
Container-title:Cometary Plasma Processes
language:
Short-container-title:

Author:

Kirsch E.,McKenna-Lawlor S.,Daly P. W.,Neubauer F. M.,Coates A.,Thompson A.,O'Sullivan D.,Wenzel K.-P.

Publisher

American Geophysical Union

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1029/GM061p0357/fullpdf

Reference26 articles.

1. Energization of positive ions in the cometary foreshock region;Amata;Planet Space Sci.,1985

2. The upstream region, foreshock and bowshock wave at comet P/Halley from plasma electron measurements;anderson;Astron. Astrophys.,1987

3. Shock drift acceleration

4. Giotto measurements of cometary and solar wind plasma at the Comet Halley bow shock;Coates;Nature,1987

5. Bulk properties and velocity distributions of water group ions at comet Halley: Giotto Measurements;Coates;J. Geophys. Res.,1990

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Energetic particle data recorded onboard Giotto during the first encounter of an observing spacecraft coming from deep space with Planet Earth;Planetary and Space Science;2001-11

2. A flux enhancement measured in energetic particles(E ∼ 60–100 keV) by the epona instrument aboard Giotto close to P⧸Grigg-Skjellerup, and its interpretationas the signature of a companion comet;Planetary and Space Science;1999-04

3. Particle Acceleration At Comet Related Shock Surfaces;Plasma Astrophysics And Space Physics;1999