Effect of electron resonant heating on the kinetic evolution and acceleration of the solar wind

Geophysical Research Letters

Volumn 28, Issue 7, 2001, Pages 1351-1354

  Tam, S W Y ^a   Chang, T ^a  

^a MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

CYCLOTRONS; ELECTRIC FIELDS; ELECTRON RESONANCE; ELECTRONS; HEATING; PROTONS; WIND; ELECTRIC LINES; IONS; KINETICS; PARTICLE INTERACTIONS; PLASMA HEATING; SOLAR WIND; WAVE PLASMA INTERACTIONS;

SOLAR WIND;

GEOPHYSICS; HEATING;

SOLAR WIND;

AMBIPOLAR ELECTRIC FIELDS; ELECTRON CYCLOTRONS; INHOMOGENEOUS FIELDS; PARTICLE DISTRIBUTIONS; PREFERENTIAL HEATING; QUALITATIVE FEATURES; SOLAR WIND VELOCITY; WAVE-PARTICLE INTERACTIONS;

EID: 0035302437     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2000GL012508     Document Type: Article

References (15)

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5. A kinetic model of the solar wind with Kappa distribution functions in the corona
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7. Solar wind protons: Three-dimensional velocity distributions and derived plasma parameters measured between 0.3 and I AU
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11. A theory of local and global processes which affect solar wind electrons: 1. The origin of typical 1 AU velocity distribution functions -- Steady state theory
12. Differential flow between solar wind protons and alpha particles: First WIND observations
13. Kinetic evolution and acceleration of the solar wind
14. Self-consistent kinetic photoelectron effects on the polar wind
15. Further development in theory/data closure of the photoelectron-driven polar wind and day-night transition of the outflow