Acceleration of heavy ions in the solar wind
Technical Report
·
OSTI ID:6590703
The preferential acceleration and heating of solar wind heavy ions by the resonant cyclotron interaction were studied. It is concluded that this interaction is incapable of producing the observed differential speeds for reasonable solar wind parameters.
- Research Organization:
- New Hampshire Univ., Durham (USA)
- OSTI ID:
- 6590703
- Report Number(s):
- N-84-13118
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640104* -- Astrophysics & Cosmology-- Solar Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ACCELERATION
ACCELERATORS
CHARGED PARTICLES
CYCLIC ACCELERATORS
CYCLOTRON RESONANCE
CYCLOTRONS
ENERGY TRANSFER
HEATING
HEAVY IONS
INTERACTIONS
IONS
PARTICLE INTERACTIONS
RESONANCE
SOLAR ACTIVITY
SOLAR WIND
STELLAR WINDS
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ACCELERATION
ACCELERATORS
CHARGED PARTICLES
CYCLIC ACCELERATORS
CYCLOTRON RESONANCE
CYCLOTRONS
ENERGY TRANSFER
HEATING
HEAVY IONS
INTERACTIONS
IONS
PARTICLE INTERACTIONS
RESONANCE
SOLAR ACTIVITY
SOLAR WIND
STELLAR WINDS