globalchange  > 气候减缓与适应
DOI: 10.1002/2017JA024779
Scopus记录号: 2-s2.0-85042532948
论文题名:
Comment on “Modeling Extreme “Carrington-Type” Space Weather Events Using Three-Dimensional Global MHD Simulations” by C. M. Ngwira, A. Pulkkinen, M. M. Kuznetsova, and A. Glocer”
作者: Tsurutani B.T.; Lakhina G.S.; Echer E.; Hajra R.; Nayak C.; Mannucci A.J.; Meng X.
刊名: Journal of Geophysical Research: Space Physics
ISSN: 21699380
出版年: 2018
卷: 123, 期:2
起始页码: 1388
结束页码: 1392
语种: 英语
英文关键词: Carrington storm ; magnetic field intensities ; modeling ; solar wind densities ; space weather
英文摘要: An alternative scenario to the Ngwira et al. (2014, https://doi.org/10.1002/2013JA019661) high sheath densities is proposed for modeling the Carrington magnetic storm. Typical slow solar wind densities (~5 cm−3) and lower interplanetary magnetic cloud magnetic field intensities (~90 nT) can be used to explain the observed initial and main phase storm features. A second point is that the fast storm recovery may be explained by ring current losses due to electromagnetic ion cyclotron wave scattering. ©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/114634
Appears in Collections:气候减缓与适应

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作者单位: Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States; Indian Institute of Geomagnetism, Navi Mumbai, India; INPE, São José dos Campos, Brazil; LPC2E, CNRS, Orléans, France; Department of Physics and Astronomy, George Mason University, Fairfax, VA, United States

Recommended Citation:
Tsurutani B.T.,Lakhina G.S.,Echer E.,等. Comment on “Modeling Extreme “Carrington-Type” Space Weather Events Using Three-Dimensional Global MHD Simulations” by C. M. Ngwira, A. Pulkkinen, M. M. Kuznetsova, and A. Glocer”[J]. Journal of Geophysical Research: Space Physics,2018-01-01,123(2)
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