A semi-kinetic model of wave-ion interaction in the solar corona

Geophysical Research Letters

Volumn 28, Issue 10, 2001, Pages 1917-1920

  Vocks, C ^a   Marsch, E ^a  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

MAGNETIC FIELDS; NUMERICAL ANALYSIS; SOLAR SYSTEM; SPECTRUM ANALYSIS; VELOCITY;

WAVEPARTICLE INTERACTIONS;

GEOPHYSICS;

CORONA; SOLAR ACTIVITY;

EID: 0035874415     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2000GL012764     Document Type: Article

References (15)

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2. Spectroscopic constraints on models of ion cyclotron resonance heating in the polar solar corona and high-speed solar wind
3. Nonlinear cyclotron resonant wave-particle interaction in a nonuniform magnetic field
4. The anisotropy of the solar wind
5. Plasma properties in coronal funnels
6. A fast solar wind model with anisotropic proton temperature
7. The kinetic shell model of coronal heating and acceleration by ion-cyclotron waves. 1. Outward-propagating waves
8. Generation of solar wind proton tails and double beams by Coulomb collisions
9. Calculation of the electron velocity distribution function in a plasma slab with large temperature and density gradient
10. Closure of multi-fluid and kinetic equations for cyclotron-resonant interactions of solar wind ions with Alfvén waves
11. The effects of Coulomb collisions on solar wind ion velocity distributions
12. Wave heating and acceleration of solar wind ions by cyclotron resonance
13. Kinetic evolution and acceleration of solar wind
14. The solar corona above polar coronal holes as seen by SUMER on SOHO