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摘要:
Standing oscillations with multiple periods have been found in a number of atmospheric structures on the Sun.The ratio of the period of the fundamental to twice the one of its first overtone,P1/2P2,is important in applications of solar magneto-seismology.We examine how field-aligned flows impact P1/2P2 of standing modes in solar magnetic cylinders.For coronal loops,the flow effects are significant for both fast kink and sausage modes.For kink modes,they reduce P1/2P2 by up to 17% relative to the static case even when the density contrast between the loop and its surroundings approaches infinity.For sausage modes,the reduction in P1/2P2 due to flow is typically (~<) 5.5% compared with the static case.However,the threshold aspect ratio,only above which can trapped sausage modes be supported,may increase dramatically with the flow magnitude.For photospheric tubes,the flow effect on P1/2P2 is not as strong.However,when applied to sausage modes,introducing field-aligned flows offers more possibilities in interpreting the multiple periods that have recently been measured.We conclude that field-aligned flows should be taken into account to help better understand what causes the departure of P1/2P2 from unity.
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篇名 Period ratios for standing kink and sausage modes in magnetized structures with siphon flow on the Sun
来源期刊 天文和天体物理学研究 学科
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年,卷(期) 2016,(6) 所属期刊栏目
研究方向 页码范围 69-84
页数 16页 分类号
字数 语种 英文
DOI 10.1088/1674-4527/16/6/092
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天文和天体物理学研究
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1674-4527
11-5721/P
北京朝阳区大屯路甲20号国家天文台 RAA编辑部
eng
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