Reply to Comments by Tsurutani et al. on 'Modeling Extreme 'Carrington-Type' Space Weather Events Using Three-Dimensional Global MHD Simulations'

Chigomezyo M. Ngwira; Antti Pulkkinen; Maria M. KuznetsovaAlex Glocer

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Reply to Comments by Tsurutani et al. on 'Modeling Extreme 'Carrington-Type' Space Weather Events Using Three-Dimensional Global MHD Simulations'

机译：回复评论Tsurutani等人在“建模极端的Carrington-Type空间天气事件使用三维全球磁流体动力模拟”

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In this response, we address the three main comments by Tsurutani et al. (2018, http://doi.org/10.1002/2017JA024779) namely, unusually high plasma density, interplanetary magnetic field intensity, and fast storm recovery phase. The authors agree that there is room to improve the modeling by taking into account these comments and other aspects that were not fully explored during our initial work. We are already in the process of undertaking a more comprehensive modeling project.

机译：在这个反应中,我们解决三个主要的评论by Tsurutani et al . (2018),http://doi.org/10.1002/2017JA024779)即异常高的等离子体密度,星际磁场强度,风暴和快速复苏阶段。提高建模通过考虑这些评论和其他方面还不完全探索在我们最初的工作。在进行的过程中全面的建模项目。

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来源
《Journal of Geophysical Research, A. Space Physics: JGR》 |2018年第2期|1393-1395|共3页
作者
Chigomezyo M. Ngwira; Antti Pulkkinen; Maria M. KuznetsovaAlex Glocer;
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作者单位

Department of Physics, Catholic University of America, Washington, DC, USA;

NASA Goddard Space Flight Center, Space Weather Laboratory, Greenbelt, MD, USA;

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正文语种英语
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关键词
space weather; plasma density; aluminiumComment;

机译：空间天气,等离子体密度;aluminiumComment;

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Reply to Comments by Tsurutani et al. on 'Modeling Extreme 'Carrington-Type' Space Weather Events Using Three-Dimensional Global MHD Simulations'

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