Potential wells, the cyclotron resonance, and ion heating in coronal holes
- 1 January 1999
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 104 (A1) , 505-520
- https://doi.org/10.1029/98ja02826
Abstract
No abstract availableKeywords
This publication has 44 references indexed in Scilit:
- Observational constraints on the dynamics of the interplanetary magnetic field dissipation rangeJournal of Geophysical Research, 1998
- Experimental constraints on pulsed and steady state models of the solar wind near the SunJournal of Geophysical Research, 1997
- Finest Filamentary Structures of the Corona in the Slow and Fast Solar WindThe Astrophysical Journal, 1997
- Measurement of Hydrogen Velocity Distributions in the Extended Solar CoronaThe Astrophysical Journal, 1996
- Ponderomotive acceleration of ions by circularly polarized electromagnetic wavesGeophysical Research Letters, 1996
- Interaction between Alfvén waves and a multicomponent plasma with differential ion streamingJournal of Geophysical Research, 1994
- Acceleration and heating of two-fluid solar wind by Alfven wavesThe Astrophysical Journal, 1994
- Alfvenically driven slow shocks in the solar chromosphere and coronaThe Astrophysical Journal, 1992
- Heating of the corona and solar wind by switch-on shocksThe Astrophysical Journal, 1982
- Heat Conductivity, Plasma Instabilities, and Radio-Star - Lations in the Solar WindThe Astrophysical Journal, 1973