The Structure of the Global Heliosphere as Seen by In-Situ Ions from the Voyagers and Remotely Sensed ENAs from Cassini
K. Dialynas(Academy of Athens), A. Czechowski(Centrum Badań Kosmicznych), M. Hilchenbach(Max Planck Society), S. M. Krimigis(Johns Hopkins University), R. B. Decker(Johns Hopkins University Applied Physics Laboratory), D. G. Mitchell(Max Planck Society), Ke Chiang Hsieh(University of Arizona), M. E. Hill(Johns Hopkins University Applied Physics Laboratory)
Cited by 37
Related Papers
The MESSENGER mission to Mercury: scientific objectives and implementation
|Planetary and Space Science|2001|408
Magnetosphere Imaging Instrument (MIMI) on the Cassini Mission to Saturn/Titan
|Space Science Reviews|2004|399
Structure of the tail plasma/current sheet at ∼11 <i>R<sub>E</sub></i> and its changes in the course of a substorm
|Journal of Geophysical Research Atmospheres|1993|308
CELIAS - Charge, Element and Isotope Analysis System for SOHO
|Solar Physics|1995|295
An extended study of the low‐latitude boundary layer on the dawn and dusk flanks of the magnetosphere
|Journal of Geophysical Research Atmospheres|1987|287