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高速太阳风中质子的随机湍动加热
引用本文:韩继岭. 高速太阳风中质子的随机湍动加热[J]. 北京师范大学学报(自然科学版), 1999, 35(1): 42-45
作者姓名:韩继岭
作者单位:北京师范大学物理学系,100875,北京
摘    要:在高速太阳风中,Alfven波在传播过程中其能量可能转移给快磁声波,当磁场强度和Alfven波速度趋于零时,快磁声波将转变为离子声波。通过对质子的随机湍动加热,而导致高速太阳风中质子平均温度高于电子的平均温度。

关 键 词:高速太阳风  离子声波  质子的随机湍动加热
修稿时间:1998-07-134

STOCHASTIC TURBULENCE HEATING FOR PROTONS IN HIGH-SPEED SOLAR WIND
HanJiling. STOCHASTIC TURBULENCE HEATING FOR PROTONS IN HIGH-SPEED SOLAR WIND[J]. Journal of Beijing Normal University(Natural Science), 1999, 35(1): 42-45
Authors:HanJiling
Affiliation:HanJiling(Department of Physics,Beijing Normal University,100875,Beijing,China)
Abstract:During a propagating process of Alfven waves in high-speed solar wind,Alfvenwave energy can be transferred into fast magnetosonic waves.When both magnetic field andalfven wave velocity approach zero,fast magnetosonic waves will be transferred into ion-acoustic waves.As the phase velocity of ion-- acoustic waves is slightly greater than the thermalvelocity of protons,the turbulence energy of ion- acoustic waves can largely be absorbed byprotons. Thus the mean temperature of protons ingeater than one of electrons by stochastieturbulence heating of ion-acoustic waves for protons.
Keywords:high--speed solar wind  ion--acoustic waves  stochastic turbulence heating forprotons
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