磁侵蚀如何影响快速冠状体质量喷射的基于拖动的动力学
Sotiris Stamkos1, Spiros Patsourakos1, Angelos Vourlidas2
1Department of Physics, University of Ioannina, Ioannina, Greece.
概括
磁性侵蚀通过减缓它们到达地球,显著影响冠状质量喷射 (CMEs). 在这种过程中,CME会失去质量和磁流,这可能会延迟它们的行程长达三小时.
科学领域:
- 空间物理 空间物理
- 太阳物理 太阳物理
- 等离子体物理学的物理学
背景情况:
- 冠状质量喷射 (CME) 是动态的太阳事件,影响太空天气.
- 了解通过磁化太阳风传播的CME传播对于太空天气预测至关重要.
- 空气动力阻力是影响快速CME的已知力,但对磁效应的理解较少.
研究的目的:
- 研究磁性侵蚀对CME阻力和传播动态的影响.
- 量化磁再连接对1AU的CME到达时间和速度的影响.
- 探索CME运动中可变质量和磁流保存的作用.
主要方法:
- 开发了CME物理参数 (质量,磁流) 的经验关系.
- 模拟CME传播使用一个包含虚拟质量效应的可变质量系统.
- 实现磁再连接以模拟CME磁流量和质量的侵蚀.
主要成果:
- 磁性侵蚀显著改变了CME阻力,可能将到达1AU的时间推迟到3小时.
- 侵蚀的CME可以经历大量的质量减少,这表明侵蚀的开始超出了冠状图视图.
- 磁侵蚀的强度与CME传播的延迟直接相关.
结论:
- 磁侵蚀是影响快速CME传播和到达时间预测的关键因素.
- 观察到的冠状体质量减少的缺乏表明,侵蚀开始于更远的太阳距离.
- 准确的太空天气预报需要将磁性侵蚀纳入CME模型.
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