Ions Preheated in 3He-Rich Solar Particle Events
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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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Cite this article:
WANG De-Yu. Ions Preheated in 3He-Rich Solar Particle Events[J]. Chin. Phys. Lett., 2003, 20(10): 1891-1894.
WANG De-Yu. Ions Preheated in 3He-Rich Solar Particle Events[J]. Chin. Phys. Lett., 2003, 20(10): 1891-1894.
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WANG De-Yu. Ions Preheated in 3He-Rich Solar Particle Events[J]. Chin. Phys. Lett., 2003, 20(10): 1891-1894.
WANG De-Yu. Ions Preheated in 3He-Rich Solar Particle Events[J]. Chin. Phys. Lett., 2003, 20(10): 1891-1894.
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