Simulation on Collision between a Magnetic Flux Tube and Shock Waves in Solar Plasmas
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概要
- 論文の詳細を見る
Recent observations show that small-scale magnetic flux tubes in the quiet photospheric network are the subject of a complex dynamics with flux emerging from belos, fragmentation and merging. Furusawa et al. (1999) showed that there appear shock waves during collision of two magnetic flux tubes with weak electric currents. We present by using 3-D neutral MHD simulation code that during collision between a shock and a magnetic flux tube with weak current, the surface Alfven waves can be generated and propagate upwards along the flux tube. These processes could play important roles for solar coronal heating.
- 理論物理学刊行会の論文
- 2000-04-28
著者
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Sakai J
Toyama Univ. Toyama
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Sakai Jun-ichi
Laboratory For Plasma Astrophysics Faculty Of Engineering Toyama University
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Furusawa Kyoko
Faculty Of Engineering Toyama University
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SAKAI Jun-ichi
Faculty of Science and Engineering, Ritsumeikan University
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KAWATA Tsutomu
Faculty of Engineering, Toyama University
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YOSHIDA Kazuhiro
Faculty of Engineering, Toyama University
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CRAMER Neil
School of Physics, The University of Sydney
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Cramer Neil
School Of Physics The University Of Sydney
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Kawata Tsutomu
Faculty Of Engineering Toyama University
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Kawata Tsutomu
Department Of Information Processing Faculty Of Engineering Toyama University
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Sakai Jun-ichi
Faculty Of Engineering Toyama University
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Yoshida Kazuhiro
Faculty Of Engineering Toyama University
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SAKAI Jun-Ichi
Faculty of Engineering, Toyama University
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YOSHIDA Kazuhiro
Department of Physics, Faculty of Science, Chiba University
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