A MECHANISM FOR THE NON-GYROTROPIC DISTRIBUTION OF THE SOLAR WIND PARTICLES

TU Chuanyi; LI Chunqiang

doi:10.11728/cjss1997.02.184

Volume 17 Issue 2

Apr. 1997

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Article Navigation > Chinese Journal of Space Science > 1997 > 17(2): 184-188

TU Chuanyi, LI Chunqiang. A MECHANISM FOR THE NON-GYROTROPIC DISTRIBUTION OF THE SOLAR WIND PARTICLES[J]. Chinese Journal of Space Science, 1997, 17(2): 184-188. doi: 10.11728/cjss1997.02.184

Citation:

TU Chuanyi, LI Chunqiang. A MECHANISM FOR THE NON-GYROTROPIC DISTRIBUTION OF THE SOLAR WIND PARTICLES[J]. Chinese Journal of Space Science, 1997, 17(2): 184-188. doi: 10.11728/cjss1997.02.184

TU Chuanyi, LI Chunqiang. A MECHANISM FOR THE NON-GYROTROPIC DISTRIBUTION OF THE SOLAR WIND PARTICLES[J]. Chinese Journal of Space Science, 1997, 17(2): 184-188. doi: 10.11728/cjss1997.02.184

Citation:

TU Chuanyi, LI Chunqiang. A MECHANISM FOR THE NON-GYROTROPIC DISTRIBUTION OF THE SOLAR WIND PARTICLES[J]. Chinese Journal of Space Science, 1997, 17(2): 184-188. doi: 10.11728/cjss1997.02.184

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A MECHANISM FOR THE NON-GYROTROPIC DISTRIBUTION OF THE SOLAR WIND PARTICLES

doi: 10.11728/cjss1997.02.184 cstr: 32142.14.cjss1997.02.184

Department of Geophysics, Peking University, Beijing 100871

Received Date: 1996-06-20
Rev Recd Date: 1996-12-25
Publish Date: 1997-04-24

Abstract

Abstract

It is suggested in this paper that the non-gyrotropic particle velocity distributions may not represent the real distribution of the particles. It may be resulted by a sudden changes of density during the sampling period of the plasma analyar for a single velocity distribution. Simulation results based on this idea are qualitatively agree with the observations.
- Solar wind,
- Particle