Comment on 'Comparison of small-scale flux rope magnetic properties to large-scale magnetic clouds: Evidence for reconnection across the HCS'? by M. L. Cartwright and M. B. Moldwin

H. Q. Feng; D. J. Wu; J. K. Chao

首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Comment on 'Comparison of small-scale flux rope magnetic properties to large-scale magnetic clouds: Evidence for reconnection across the HCS'? by M. L. Cartwright and M. B. Moldwin

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Comment on 'Comparison of small-scale flux rope magnetic properties to large-scale magnetic clouds: Evidence for reconnection across the HCS'? by M. L. Cartwright and M. B. Moldwin

机译：评论“比较小规模的通量绳大型磁磁性云:重新连接到的证据高碳钢”?

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Recently Cartwright and Moldwin 2008 developed a newly semiautomated routine to identify interplanetary small-scale symmetric force-free flux ropes. Using the semi-automated routine, they examined the solar wind magnetic field and plasma data measured by Wind during 1995-2005, and identified 68 small-scale flux ropes. They presented comprehensive survey of these small-scale flux ropes, and compared them with previously published small-scale flux rope surveys and interplanetary coronal mass ejection (ICME)/magnetic cloud databases. Cartwright and Moldwin 2008 found that the size distribution of flux ropes in the solar wind appears to be bimodal, with majority of the events having durations of 4 h or less whereas the magnetic cloud distribution peaks between 12 and 16 h. So they suggest different source mechanisms for small- and large-scale flux ropes, respectively and attribute small flux ropes to recon-nection occurring in the solar wind.

机译：最近卡特赖特和Moldwin[2008]了新半自动的例程来识别星际小规模对称的自由通量绳。他们检查了太阳风磁场和等离子体风在1995 - 2005年期间,测量的数据并确定了68小规模通量绳。提出了全面的调查小规模的通量绳和比较以前公布的小规模的通量绳调查和星际日冕物质抛射(ICME) /磁云数据库。Moldwin[2008]发现大小分布太阳风的通量绳似乎双峰,多数的事件持续时间4小时或更少而磁性云分布峰值12到16 h。所以他们认为不同的源的机制小型和大型通量绳,分别小通量绳recon-nection和属性发生在太阳风。

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来源
《Journal of Geophysical Research, A. Space Physics: JGR》 |2010年第10期|A10109:1-A10109:4|共4页
作者
H. Q. Feng; D. J. Wu; J. K. Chao;
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作者单位

Institute of Space Science, National Central University, Jhongli, Taiwan;

College of Physics and Electronics Science, Luoyang Normal University, Luoyang, China;

Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China;

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正文语种英语
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small flow; solar wind; magnetic cloudsComment;

机译：小流量;太阳能风;磁云注释;

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1. W. D. D'haeseleer, W. N. G. Hitchon, J. D. Callen, J. L. Shohet: Flux Coordinates and Magnetic Field Structure — A Guide to a Fundamental Tool of the Plasma Theory. Edited by R. Glowinski, M. Holt, P. Hut, H. B. Keller, J. Killeen, S. A. Orszag and V. V. Rusanov. Springer Series in Computational Physics, Springer Verlag Berlin 1991 [J] . D. Sünder contributions to plasma physics . 1991,第6期

机译：W. D. D'haeseleer, W. N. G. Hitchon, J. D. Callen, J. L. Shohet: Flux Coordinates and Magnetic Field Structure — A Guide to a Fundamental Tool of the Plasma Theory. Edited by R. Glowinski, M. Holt, P. Hut, H. B. Keller, J. Killeen, S. A. Orszag and V. V. Rusanov. Springer Series in Computational Physics, Springer Verlag Berlin 1991
2. Reply to comment by M. Lockwood and M. J. Owens on "What causes the flux excess in the heliospheric magnetic field?" [J] . Smith Edward J. Journal of geophysical research . 2013,第5期

机译：Reply to comment by M. Lockwood and M. J. Owens on "What causes the flux excess in the heliospheric magnetic field?"
3. Evidence for the core field polarity of magnetic flux ropes against the reconnection guide field [J] . Teh W. -L., Abdullah M., Hasbi A. M. Journal of geophysical research . 2014,第11期

机译：Evidence for the core field polarity of magnetic flux ropes against the reconnection guide field

Comment on 'Comparison of small-scale flux rope magnetic properties to large-scale magnetic clouds: Evidence for reconnection across the HCS'? by M. L. Cartwright and M. B. Moldwin

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