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Ions Preheated in 3He-Rich Solar Particle Events |
WANG De-Yu1,2 |
1Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008
2National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 |
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Cite this article: |
WANG De-Yu 2003 Chin. Phys. Lett. 20 1891-1894 |
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Abstract A wave-particle resonance absorption model in the two-ion plasma is suggested in explanation to the coronal ions preheating in 3He-rich solar particle events. It is found that 3He and Fe ions are preferably preheated by the ion-ion hybrid waves at their fundamental and second harmonic ion cyclotron frequencies, respectively.
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Keywords:
96.60.Rd
96.60.Fs
52.35.Hr
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Published: 01 October 2003
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PACS: |
96.60.Rd
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96.60.Fs
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(Composition)
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52.35.Hr
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(Electromagnetic waves (e.g., electron-cyclotron, Whistler, Bernstein, upper hybrid, lower hybrid))
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Abstract
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