Cyclotron resonance in coronal holes: 1. Heating and acceleration of protons, O5+, and Mg9+
- 1 November 1999
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 104 (A11) , 24781-24791
- https://doi.org/10.1029/1999ja900300
Abstract
No abstract availableKeywords
This publication has 39 references indexed in Scilit:
- Ion‐cyclotron wave dissipation channel for Alfvén wavesGeophysical Research Letters, 1999
- A study of solar wind acceleration based on gyrotropic transport equationsJournal of Geophysical Research, 1999
- Heating and Acceleration of the Solar Wind via Gravity Damping of Alfven WavesThe Astrophysical Journal, 1999
- Heating and cooling of protons by turbulence‐driven ion cyclotron waves in the fast solar windJournal of Geophysical Research, 1999
- Potential wells, the cyclotron resonance, and ion heating in coronal holesJournal of Geophysical Research, 1999
- A study of density fluctuations in the solar wind acceleration regionJournal of Geophysical Research, 1998
- Observational constraints on the dynamics of the interplanetary magnetic field dissipation rangeJournal of Geophysical Research, 1998
- The fast solar windGeophysical Research Letters, 1997
- Interaction between Alfvén waves and a multicomponent plasma with differential ion streamingJournal of Geophysical Research, 1994
- Why fast solar wind originates from slowly expanding coronal flux tubesThe Astrophysical Journal, 1991