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5. Heating of Solar Wind Protons in the Interplanetary Turbulence

Heating of Solar Wind Protons in the Interplanetary Turbulence

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：dluflonline

【摘 要】

：

The Solar wind is observed to expand outward non-adiabatically.The energy source for the non-adiabatic behavior is commonly attributed to the solar wind turbulence.

【作 者】

：

Jiansen He Chuanyi Tu Eckart Marsch Linghua Wang Zhongtian Pei Lei Zhang Xin Wang 

【机 构】

：

School of Earth and Space Sciences,PekingUniversity,100871,Beijing,China

【出 处】

：

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

【发表日期】

：

2015年5期

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The Solar wind is observed to expand outward non-adiabatically.The energy source for the non-adiabatic behavior is commonly attributed to the solar wind turbulence.

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