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5. Kinetic simulation of slow magnetosonic waves and intermittent outflows in the solar corona

Kinetic simulation of slow magnetosonic waves and intermittent outflows in the solar corona

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：tangroo

【摘 要】

：

Quasi-periodic intensity disturbances are frequently observed in the corona.These disturbances propagate upward along the magnetic field line with speeds of～100 km/s.

【作 者】

：

Wenzhi Ruan Jiansen He Lei Zhang Christian Vocks Chuanyi Tu Eckart Marsch Linghua Wang 

【机 构】

：

School of Earth and Space Sciences,Peking University,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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Quasi-periodic intensity disturbances are frequently observed in the corona.These disturbances propagate upward along the magnetic field line with speeds of～100 km/s.

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