Using Energetic Particles to Probe the Magnetic Topology of Ejecta
Open Access
- 18 March 2013
- book chapter
- Published by Wiley
- p. 189-196
- https://doi.org/10.1029/gm099p0189
Abstract
No abstract availableKeywords
This publication has 27 references indexed in Scilit:
- Helios 1 and 2 observations of particle decreases, ejecta, and magnetic cloudsJournal of Geophysical Research, 1997
- Cosmic ray decreases: 1964–1994Journal of Geophysical Research, 1996
- The Ulysses south polar pass: Transient fluxes of energetic ionsGeophysical Research Letters, 1995
- Cosmic ray decreases and shock structure: A multispacecraft studyJournal of Geophysical Research, 1994
- Observation by Ulysses of hot (∼270 keV) coronal particles at 32° south heliolatitude and 4.6 AUGeophysical Research Letters, 1994
- Simultaneous observations of solar MeV particles in a magnetic cloud and in the Earth's northern tail lobe: Implications for the global field line topology of magnetic clouds and for the entry of solar particles into the magnetosphere during cloud passageJournal of Geophysical Research, 1993
- A study of an expanding interplanetary magnetic cloud and its interaction with the Earth's magnetosphere: The interplanetary aspectJournal of Geophysical Research, 1993
- A bubblelike coronal mass ejection flux rope in the solar windPublished by Wiley ,1990
- The role of interplanetary shocks in the longitude distribution of solar energetic particlesJournal of Geophysical Research, 1988
- Magnetic loop behind an interplanetary shock: Voyager, Helios, and IMP 8 observationsJournal of Geophysical Research, 1981