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THE MATERIAL MOTION IN A “POST”-FLARE LOOP PROMINENCE

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【作者】 顾啸马李伯殊李秋莎丁有济许敖敖丁久平唐玉华

【Author】 GU XIAOMA;LI BOSHU;LI QIUSHA;DING YOUJI;XU AOAO;DING JIUPING;TANG YUHUA Yunnan Observatory, Academia Sinica Department of Astronomy, Nanjing University

【机构】 Yunnan ObservatoryAcademia Sinica Department of AstronomyNanjing UniversityNanjing University

【摘要】 <正> The velocity fields of a "post" - flare loop prominence taken in different times by thespectra- spectroheliograph are measured by the 3CS densitometer. According to the fundamentalfeatures of the observed velocity fields, we consider that the plasma matter within the loopprominence, which is formed by the magnetic reconnection after flares, would flow down fromthe top of loops along the helical magnetic lines under the action of the gravity of the Sun andthe magnetic stress in the loop prominence. The theoretical distributive chart of the velocityfields of the loop prominence is basically in accordance with the observations.

【Abstract】 The velocity fields of a "post" - flare loop prominence taken in different times by thespectra- spectroheliograph are measured by the 3CS densitometer. According to the fundamentalfeatures of the observed velocity fields, we consider that the plasma matter within the loopprominence, which is formed by the magnetic reconnection after flares, would flow down fromthe top of loops along the helical magnetic lines under the action of the gravity of the Sun andthe magnetic stress in the loop prominence. The theoretical distributive chart of the velocityfields of the loop prominence is basically in accordance with the observations.

【关键词】 POSTaccordancebasicallygravityhelicalestabribbonchartvioletabsolutely
  • 【文献出处】 Science in China,Ser.A ,中国科学A辑(英文版) , 编辑部邮箱 ,1984年09期
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