globalchange  > 气候减缓与适应
DOI: 10.1002/2017JA024928
Scopus记录号: 2-s2.0-85042529930
论文题名:
Reply to Comments by Tsurutani et al. on “Modeling Extreme ‘Carrington-Type’ Space Weather Events Using Three-Dimensional Global MHD Simulations”
作者: Ngwira C.M.; Pulkkinen A.; Kuznetsova M.M.; Glocer A.
刊名: Journal of Geophysical Research: Space Physics
ISSN: 21699380
出版年: 2018
卷: 123, 期:2
起始页码: 1393
结束页码: 1395
语种: 英语
英文关键词: Carrinton-type storm ; extreme space weather ; fast storm recovery phase ; high solar wind density ; interplanetary magnetic field intensity
英文摘要: 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. ©2018. American Geophysical Union. All Rights Reserved.
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资源类型: 期刊论文
标识符: http://119.78.100.158/handle/2HF3EXSE/114578
Appears in Collections:气候减缓与适应

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作者单位: Department of Physics, Catholic University of America, Washington, DC, United States; NASA Goddard Space Flight Center, Space Weather Laboratory, Greenbelt, MD, United States

Recommended Citation:
Ngwira C.M.,Pulkkinen A.,Kuznetsova M.M.,et al. Reply to Comments by Tsurutani et al. on “Modeling Extreme ‘Carrington-Type’ Space Weather Events Using Three-Dimensional Global MHD Simulations”[J]. Journal of Geophysical Research: Space Physics,2018-01-01,123(2)
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