SIMULATION OF MAGNETIC CLOUD PROPAGATION IN THREE DIMENSIONS

机译：三维中磁云的传播模拟

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Magnetohydrodynamic simulation is used to study evolution and propagation of loop-like magnetic clouds through interplanetary space in three dimensions. Results show that a flux rope becomes highly deformed; for instance, a spacecraft located at 1 AU would observe two times the same flux rope when the flux rope has a low inclination to the ecliptic plane. Initially circular cross section of the flux rope becomes very prolate at 1 AU.

机译：磁流体动力学模拟用于研究环状磁云通过行星际空间在三个维度上的演化和传播。结果表明，助焊剂钢丝变形严重。例如，当通量绳相对于黄道的倾斜度较小时，位于1 AU的航天器将观察到两倍的通量绳。最初，助焊剂绳的圆形横截面在1 AU时变得非常平坦。

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来源
《Second Solar Cycle and Space Weather Euroconference Sep 24-29, 2001 Vico Equense, Italy》|2001年|p.293-296|共4页
会议地点 Vico Equense(IT);Vico Equense(IT)
作者
M. Vandas; D. Odstrcil; S. Watari;
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作者单位

Astronomical Institute, Academy of Sciences, Bocni Ⅱ1401, 141 31 Praha 4, Czech Republic;

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会议组织
原文格式 PDF
正文语种 eng
中图分类天文学;
关键词
magnetic clouds; numerical simulations; space weather;

机译：磁云;数值模拟;空间天气;

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4. SIMULATION OF MAGNETIC CLOUD PROPAGATION IN THREE DIMENSIONS [C] . M. Vandas, D. Odstrcil, S. Watari, Solar cycle and space weather euroconference . 2002

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SIMULATION OF MAGNETIC CLOUD PROPAGATION IN THREE DIMENSIONS

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