Abundances and charge states of particles in the solar wind
- 1 May 2000
- journal article
- Published by American Geophysical Union (AGU) in Reviews of Geophysics
- Vol. 38 (2) , 247-266
- https://doi.org/10.1029/1999rg000063
Abstract
No abstract availableKeywords
This publication has 55 references indexed in Scilit:
- Enhanced solar wind ³He2+ associated with coronal mass ejectionsGeophysical Research Letters, 2000
- On the bulk isotopic composition of magnesium and silicon during the May 1998 CME: ACE/SWIMSGeophysical Research Letters, 1999
- Unusual composition of the solar wind in the 2–3 May 1998 CME observed with SWICS on ACEGeophysical Research Letters, 1999
- Kinetic properties of solar wind minor ions and protons measured with SOHO/CELIASJournal of Geophysical Research, 1998
- First determination of the silicon isotopic composition of the solar wind: WIND/MASS resultsJournal of Geophysical Research, 1998
- Meteoritic Evidence for the Infall of Large Interstellar Dust Aggregates during the Formation of the Solar SystemThe Astrophysical Journal, 1998
- Isotopic composition of solar wind neon measured by CELIAS/MTOF on board SOHOJournal of Geophysical Research, 1997
- Diagnostics of Closed Magnetic Structures in the Solar Corona Using Charge States of Helium and of Minor IonsThe Astrophysical Journal, 1996
- Subthreshold stochastic diffusion with application to selective acceleration of He-3 in solar flaresThe Astrophysical Journal, 1991
- Singly‐ionized helium in the driver gas of an interplanetary shock waveGeophysical Research Letters, 1980