On the importance of investigating CME complexity evolution during interplanetary propagation

On the importance of investigating CME complexity evolution during interplanetary propagation
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DOI:
10.3389/fspas.2022.1064175
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发表时间:
2022-12
期刊:
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影响因子:
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通讯作者:
R. Winslow;C. Scolini;L. Jian;T. Nieves-chinchilla;M. Temmer;F. Carcaboso;B. Schmieder;S. Poedts;B. Lynch;B. Wood;E. Palmerio;N. Lugaz;C. Farrugia;Christina O. Lee;E. Davies;F. Regnault;T. Salman;T. Török;N. Al-Haddad;A. Vourlidas;W. Manchester;M. Jin;B. Lavraud;A. Galvin
R. Winslow;C. Scolini;L. Jian;T. Nieves-chinchilla;M. Temmer;F. Carcaboso;B. Schmieder;S. Poedts;B. Lynch;B. Wood;E. Palmerio;N. Lugaz;C. Farrugia;Christina O. Lee;E. Davies;F. Regnault;T. Salman;T. Török;N. Al-Haddad;A. Vourlidas;W. Manchester;M. Jin;B. Lavraud;A. Galvin
中科院分区:
其他
文献类型:
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作者:
R. Winslow;C. Scolini;L. Jian;T. Nieves-chinchilla;M. Temmer;F. Carcaboso;B. Schmieder;S. Poedts;B. Lynch;B. Wood;E. Palmerio;N. Lugaz;C. Farrugia;Christina O. Lee;E. Davies;F. Regnault;T. Salman;T. Török;N. Al-Haddad;A. Vourlidas;W. Manchester;M. Jin;B. Lavraud;A. Galvin

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这篇透视性论文揭示了对行星际日冕物质抛射(ICME)在传播过程中复杂性演化进行全面研究的必要性。到目前为止,关于ICME复杂性的研究很少。在这里,我们定义了ICME复杂性和相关的复杂性变化,描述了最近的工作及其局限性,并概述了需要解决的关键科学问题。对ICME复杂性从日冕到1AU及以上变化的基础研究对于我们从物理上理解内日光层瞬变的演化和相互作用是至关重要的。此外,需要全面了解这种变化,以了解国际海洋和海洋生态系统对不同日球层位置的空间气象影响,并改进预测空间气象模型。
This perspective paper brings to light the need for comprehensive studies on the evolution of interplanetary coronal mass ejection (ICME) complexity during propagation. To date, few studies of ICME complexity exist. Here, we define ICME complexity and associated changes in complexity, describe recent works and their limitations, and outline key science questions that need to be tackled. Fundamental research on ICME complexity changes from the solar corona to 1 AU and beyond is critical to our physical understanding of the evolution and interaction of transients in the inner heliosphere. Furthermore, a comprehensive understanding of such changes is required to understand the space weather impact of ICMEs at different heliospheric locations and to improve on predictive space weather models.