Occurrence Rates and Heating Effects of Tangential and Rotational Discontinuities as Obtained from T

来源 :The Fourteenth International Solar Wind Conference (第十四届国际太阳 | 被引量 : 0次 | 上传用户：www_acafa_com

【摘要】

：

【作者】

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L Zhang JS He CY Tu LP Yang X Wang E Marsch LH Wang

【机构】

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School of Earth and Space Sciences,Peking University,Beijing,China,100871

【出处】

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The Fourteenth International Solar Wind Conference (第十四届国际太阳

【发表日期】

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2015年5期

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In solar wind,magnetohydrodynamic(MHD) discontinuities are ubiquitous and often found to be at the origin of turbulence intermittency.They may also play a key role in the turbulence dissipation and heating of the solar wind.The tangential(TD) and rotational(RD) discontinuities are the two most important types of discontinuities.Recently,the connection between turbulence intermittency and proton thermodynamics has been being investigated observationally.

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Occurrence Rates and Heating Effects of Tangential and Rotational Discontinuities as Obtained from T

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