Preferential acceleration of heavy ions in multi-component plasmas

Geophysical Research Letters

Volumn 28, Issue 16, 2001, Pages 3099-3102

  Mizuta, T ^a   Hoshino, M ^a  

^a UNIVERSITY OF TOKYO   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

ELEMENTARY PARTICLES; HEAVY IONS; MAGNETOHYDRODYNAMICS; PARTICLE ACCELERATORS; ALPHA PARTICLES; ELECTRON CYCLOTRON RESONANCE; KINETIC THEORY; PARTICLE INTERACTIONS; WAVE PLASMA INTERACTIONS;

PHASE VELOCITY;

PLASMAS; MAGNETOPLASMA;

MAGNETOHYDRODYNAMICS; PLASMA;

LARGE AMPLITUDE; LONG WAVES; MAGNETOHYDRODYNAMIC WAVES; MULTICOMPONENTS; N-WAVES; TEST PARTICLES; WAVE-PARTICLE INTERACTIONS;

EID: 0035880429     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2001GL012957     Document Type: Article

References (17)

1. Response of thermal ions to electro magnetic ion cyclotron waves
2. UVCS/SOHO: The first two years
3. Constraints on high-speed solar wind structure near its coronal base: A Ulysses perspective
4. Alpha/proton magnetosonic instability in the solar wind
5. A four-fluid turbulence-driven solar wind model for preferential acceleration and heating of heavy ions
6. Heating of coronal holes and generation of the solar wind by ion-cyclotron resonance
7. Stochastic ion heating by a lower hybrid wave
8. Liner and nonlinear properties of ULF waves driven by ring-beam distribution functions
9. Heating and acceleration of protons and minor ions by fast shocks in the solar corona
10. + in association with auroral electromagnetic ion cyclotron waves
11. Solar wind helium ions: Observations of the Helios solar probes between 0.3 and IAU
12. Nonlinear whistler-mode interaction and triggered emissions in the magnetosphere: A review
13. Ulysses observations of differential alphaproton streaming in the solar wind
14. Upstream waves at Mars: Phobos observations
15. Differential flow between solar wind protons and alpha particles: First WIND observations
16. 3He-rich flares by electromagnetic hydrogen cyclotron waves
17. A new look at the nature of comet Halley's LF electromagnetic waves: Giotto observations