On resonant interactions of ions with plasma waves in a reduced quasi-linear theory

Nonlinear Processes in Geophysics

Volumn 9, Issue 2, 2002, Pages 69-74

  Marsch, E ^a  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

PLASMA; SOLAR WIND;

EID: 0036218649     PISSN: 10235809     EISSN: None     Source Type: Journal    
DOI: 10.5194/npg-9-69-2002     Document Type: Article

References (17)

1. Spectroscopic constraints on models of ion cyclotron resonance heating in the polar solar corona and high-speed solar wind
2. Determination of wave growth from measured distribution functions and transport theory
3. Velocity space diffusion from weak plasma turbulence in a magnetic field
4. First results from the SOHO ultra violet coronagraph spectrometer
5. Linear mode analysis in multi-ion plasmas
6. Kinetic physics of the solar wind
7. Closure of multifluid and kinetic equations for cyclotron-resonant interactions of solar wind ions with Alfvén waves
8. The effects of Coulomb collisions on solar wind ion velocity distributions
9. Heating and acceleration of coronal ions interacting with plasma waves through cyclotron and Landau resonance
10. Evidence for pitch-angle diffusion of solar wind protons in resonance with cyclotron waves
11. Ion temperatures in a solar polar coronal hole observed by SUMER on SOHO
12. A semi-kinetic model of wave-ion interaction in the solar corona
13. Kinetic properties of heavy ions in the solar wind from SWICS/Ulysses
14. The solar corona above polar coronal holes as seen by SUMER on SOHO